This is only a preview of the August 2008 issue of Silicon Chip. You can view 33 of the 104 pages in the full issue, including the advertisments. For full access, purchase the issue for $10.00 or subscribe for access to the latest issues. Items relevant to "Ultra-LD Mk.2 200W Power Amplifier Module":
Items relevant to "Planet Jupiter Receiver":
Items relevant to "LED Strobe & Contactless Tachometer":
Items relevant to "DSP Musicolour Light Show; Pt.3":
Purchase a printed copy of this issue for $10.00. |
SILICON
CHIP
AUGUST 2008
ISSN 1030-2662
08
9 771030 266001
PRINT POST APPROVED
- PP255003/01272
8
$ 50* NZ $ 9 90
INC GST
ALL-NEW 200W AMP MODULE
INC GST
Astonishingly low distortion
State-of-the-art design
Uses new 5-pin ThermalTrak
transistors
BELIEVE IT OR NOT . . .
This 3D heart model was printed,
in colour, on an inkjet printer!
See the full story inside . . .
LISTEN IN TO JUPITER!
BUILD THIS RECEIVER FOR
NASA’S RADIO JOVE PROJECT
siliconchip.com.au
(It’s
much
cheaper than
the US import kit!)
August 2008 1
EVERYTHING FOR THE
ELECTRONICS ENTHUSIAST
Wireless Fun
RC Mini M*A*S*H Helicopter
This is our smallest readyto-fly infrared remote
control helicopter. It is
made of durable plastic
and is ideal for indoor use.
• 20 min charge time
for 8 min flying time
• Requires 6 x AA batteries
• Helicopter 135mm long
• Suitable for 8yrs+
$
29
95
Cat: GT-3260
RC 1:43 Scale Turbo
Mercedes C-Class DTM
This little wonder is a 1/43rd
scale factory endorsed
replica of one of the
most stylish vehicles
available. It features
full functioning controls
including forward, back, left, right & turbo.
• Requires 6 x AA batteries
See in-store or on-line for our full
range of remote controlled cars.
$
ENTERTAINMENT
AM/FM World Band Receiver
A truly portable world radio that is designed for functionality
and ease of use. It covers the standard AM/FM bands as
well as the short wave bands from 2,300kHz to
22,000kHz. The tuner uses phase locked
loop (PPL) technology which
ensures rock-steady, drift
free reception. This is an
excellent radio that will
perform well for years to
come.
• Approx 190mm wide
• Requires 2 x AA
$
95
batteries
Cat: AR-1745
See our website for a full list of features
49
3.6V Cordless Screwdriver
with Pivoting Handle
22 95
Cat: GT-3294
V8 Alarm Clock
Wake up to the realistic V8 engine-sounding alarm.
Easy to use and attractive in design, it
is sure to be a hit with any
motoring enthusiast young or old.
• Realistic pedals for demo
and clock controls
• Spinning brake disc when
the alarm is activated
$
95
• Clock 120mm dia.
Cat: AR-1769
• Requires 3 x AA batteries
24
Nothing beats the convenience of
a cordless screwdriver. This one
is even better because of its
pivoting handle which folds
from straight to an angle
position for better grip.
Includes charger.
• 230RPM
• 6 torque settings
This pre-programmed remote operates the
main functions of your TV and features large,
easily read buttons. The unit is great for
people with big hands or who find tiny
buttons & small writing difficult to cope with.
• Requires 2 x AAA batteries
• 130mm long
$
14 95
Cat: AR-1703
Solar Mobile Phone Charger
Simply charge the internal battery via the
sun, USB port or mains adaptor for truly
portable energy that allows you to charge
your phone and other digital devices
wherever you are! Keep the battery topped
up using free power from the sun.
• Li-ion battery
$
95
• 1000mAh capacity
• Suits most phones
Cat: MB-3588
• Folded size - 120(L) x
17(W) x 62(H)mm
Was $69.95
$15
54
$
11 95
Cat: TD-2495
Single RCD (Safety Switch) Outlet
Non-Contact AC Voltage
Tester with Torch
This non-contact tester detects voltages from 100 600VAC in mains outlets, power boards or insulated
wiring etc. It also has an LED torch and a handy pocket
clip. 180mm long.
$
Pre-Programmed Smart TV Remote
17 95
Cat: QP-2271
RCDs (residual current devices) are
designed to cut the power in a
fraction of a second in the event of a
fault condition. Use this handy
portable one if your house doesn't
have RCDs fitted.
• Test function
• Reset button
• 10A 240V rated
$
24 95
Cat: MS-4013
300pc QC Crimp Connector Pack
Finally, a Quick-Connector pack for regular everyday use.
We have hand selected
the contents of this pack
$
95
to ensure it contains
Cat: PT-4536
300pcs of the most
commonly-used quick
connectors from our range
of separately sold QC
connectors.
29
12V Auto Work Light
Ideal for use in caravans, boats, 4WDs and cars. This
Auto work lamp draws a little over an amp and is
supplied with 4.5m power cord with a cigarette lighter
socket for easy connection.
$
14
95
Cat: ST-3032
Digital Tyre Pressure Gauge
This simple device lets you keep track of
tyre pressure and avoid pressure related
problems. Includes an integrated torch for
night use.
• Range: 5 - 100PSI
• 156mm long
$
19 95
Cat: QP-2293
Illuminated Gooseneck Magnifier
I-Sight Magnifier with LED
A handy little magnifying glass with a built-in LED light.
Perfect for reading a menu in a dark restaurant, mapreading, hobbies etc.
Battery and lanyard
included. 65mm long
$
This handy hobbyist's magnifyer has a 2 x main magnifier
lens with a 5 x insert lens and 2 LED lights, all mounted on
a flexible arm. Can be free-standing or
clamped to a surface up to 38mm thick.
• Lens 110mm (dia.)
• Requires 3 x AAA batteries
$
9 95
29 95
Cat: QM-3532
Cat: ST-3197
Mini Bench Vice
Shed/Garage/Boat Security Alarm
The valuable tools and equipment stored in your
garage or garden shed are an easy target
for would be thieves. Protect them with
this easily installed alarm. The self
contained system includes a PIR, piezo
siren, and reed switch. Simple plug &
play installation.
$
95
• 120mm high
Cat: LA-5400
Was $39.95
29
This strong lightweight aluminium
vice will clamp to surfaces up
to 1" thick and hold
material up to 2" thick.
Great for hobby work or
for repairs on the go.
$10
$
14 95
Free Call: 1800 022 888 for orders! www.jaycar.com.au
Cat: TH-1764
Contents
Vol.21, No.8; August 2008
SILICON
CHIP
www.siliconchip.com.au
Features
12 Printing In The Third Dimension
Imagine an inkjet colour printer that outputs images not just in two dimensions
(ie, width and depth) but adds the third dimension, height, as well to give 3D
objects. The technology is here now – by Ross Tester
Printing In The Third Dimension
– Page 12.
18 Review: TekTronix DPO3034 Digital Oscilloscope
The new 300MHz DPO3034 features a wide “digital phosphor” LCD screen,
has an excellent user interface and boasts an impressive list of features – by
Mauro Grassi
Pro jects To Build
24 Ultra-LD Mk.2 200W Power Amplifier Module
It uses On Semiconductor’s new ThermalTrak power transistors for superlative
performance and delivers 200W into 4-ohms or 135W into 8-ohms with ultralow distortion. It’s also very easy to build – by Leo Simpson & John Clarke
32 Planet Jupiter Receiver
Like to try some basic radio astronomy by listening to noise bursts originating
from the planet Jupiter? This AM shortwave receiver lets you join in NASA’s
world-wide Radio Jove project – by Jim Rowe
62 LED Strobe & Contactless Tachometer
This LED strobe & tachometer project is ideal for measuring the speed of
rotating machinery. It can do strobe measurements or you can trigger the
tachometer using an optical pickup or photo-interruptor – by John Clarke
Ultra-LD Mk.2 200W Power
Amplifier Module – Page 24.
78 DSP Musicolour Light Show; Pt.3
Third article gives the final testing, troubleshooting and operating details and
describes the firmware operation – by Mauro Grassi
Special Columns
44 Serviceman’s Log
She was just what I’d always fancied – by the TV Serviceman
57 Circuit Notebook
(1) Charging Controller For 12V Lead-Acid Batteries; (2) Random Direction
Control For A Model Railway Layout; (3) Antenna Resonance Indicator; (4)
Balanced Supply Rails From A 12V Battery; (5) Universal IR Remote Control
Repeater
Planet Jupiter
Receiver– Page 32.
88 Vintage Radio
The incredible 1925 RCA 26 portable superhet – by Rodney Champness
Departments
2
4
17
96
Publisher’s Letter
Mailbag
Order Form
Product Showcase
siliconchip.com.au
97 Ask Silicon Chip
100 Notes & Errata
101 Market Centre
LED Strobe &
Tachometer –
Page 62.
August 2008 1
SILICON
CHIP
www.siliconchip.com.au
Publisher & Editor-in-Chief
Leo Simpson, B.Bus., FAICD
Production Manager
Greg Swain, B.Sc.(Hons.)
Technical Editor
John Clarke, B.E.(Elec.)
Technical Staff
Ross Tester
Jim Rowe, B.A., B.Sc, VK2ZLO
Mauro Grassi, B.Sc.(Hons.)
Photography
Ross Tester
Reader Services
Ann Morris
Advertising Enquiries
Glyn Smith
Phone (02) 9939 3295
Mobile 0431 792 293
glyn<at>siliconchip.com.au
Regular Contributors
Brendan Akhurst
Rodney Champness, VK3UG
Mike Sheriff, B.Sc, VK2YFK
Stan Swan
SILICON CHIP is published 12 times
a year by Silicon Chip Publications
Pty Ltd. ACN 003 205 490. ABN 49
003 205 490 All material copyright
©. No part of this publication may
be reproduced without the written
consent of the publisher.
Printing: Hannanprint, Noble Park,
Victoria.
Distribution: Network Distribution
Company.
Subscription rates: $89.50 per year
in Australia. For overseas rates, see
the subscription page in this issue.
Editorial office:
Unit 1, 234 Harbord Rd,
Brookvale, NSW 2100.
Postal address: PO Box 139,
Collaroy Beach, NSW 2097.
Phone (02) 9939 3295.
Fax (02) 9939 2648.
E-mail: silicon<at>siliconchip.com.au
ISSN 1030-2662
* Recommended and maximum price only.
2 Silicon Chip
Publisher’s Letter
Electrical wiring in older
houses can be dangerous
As might be expected, our recent articles on
do-it-yourself wiring have generated quite a deal
of comment, some of it very useful. For example,
following our story on Light Switches in the July
2008 issue, a reader rang to point out that if anyone
is changing a light bulb or doing anything else with
a light fitting, they should be aware that the light
socket can easily have power on it, even when the
light switch is turned off.
This is true and is particularly the case if the “loop” terminal has been
used to terminate an Active wire. People should also be aware that some
Edison sockets are inherently unsafe if they expose any of the metalwork
which is connected to the lamp itself. This is because the outer screw thread
of the lamp is part of the lamp circuit. In fact, in my opinion, 240VAC Edison
lamps and fittings should never have been approved for use in Australia. So
if you want to safely work on a light fitting or change an Edison screw light
bulb, perhaps you should kill the power at the switchboard.
So we do acknowledge that DIY wiring is not without its hazards. But
provided people use common sense and the information available on the
relevant New Zealand government websites, it can be done safely and
correctly.
However, Australian electrical supply authorities continue to the push the
line that DIY wiring is “rooly rooly” dangerous. I am indebted to a reader
who sent me a 4-page liftout inserted by Energex into the Brisbane Sunday
Mail on June 8, 2008. In it they provide some perfectly innocuous information about using electricity safely, not using appliances with frayed power
cords or overloading power points and so on. No problems there.
But they go on to warn about the dangers of do-it-yourself wiring and state
that “Hundreds of Queenslanders have been killed as a result of unauthorised
or unsafe electrical work being carried out around the home”. Well, really?
Over what period? Since Federation? This statement is patently untrue. Sure,
hundreds of people may have been killed over a period of many years due to
electrocution but the vast majority of those were nothing to do with wiring
in the home, unauthorised or not. Our article in the June 2008 issue quoted
from ABS figures and these show that there are typically three electrical
fatalities in Queensland in a year. Only three? Yes.
So why does Energex and other Australian electrical supply authorities
continue to spend huge amounts of money advertising the evils of DIY wiring? We can only surmise that it is to stay on the good side of the electrical
trades unions. Even then we cannot understand it, because most electricians
would admit that they have more work than they can handle.
In fact, it could be argued that if the electrical supply authorities really
want to promote electrical safety, they should be highlighting the dangers
of decrepit wiring in older homes, particularly those with cotton-covered
or vulcanised rubber insulation. As fire departments and insurance companies can attest, this old wiring is a real fire hazard. In fact, if your home
is 50 years old or more, the wiring is almost certain to be unsafe or in need
of upgrading.
Furthermore, if the supply authorities have so much money to spare,
perhaps they should use it as subsidies for those people on lower incomes
who cannot afford the cost of a full rewiring job.
Leo Simpson
siliconchip.com.au
“I need an affordable power supply
that won’t risk my DUTs.”
Done. And we added memory, too.
Introducing the Agilent U8000 Series single-output, non-programmable power supply. It comes
packed with more features than you’d normally expect in an affordable power supply. Fully
integrated overvoltage and overcurrent protection keep your DUTs safe while you work. A keypad
lock and physical lock provide added security. And, the capability to save and recall up to three
memory states shortens set-up time and reduces mistakes.
What’s more, it’s an evolution of the best-selling Agilent E3600 Series and backed by 40 years of
experience in power supplies, so you know it
• Power Range - 90 W to 150 W
has reliability you can count on.
• Voltage/Current Range - up to 30 V/5 A
For more on the U8000 Series, www.agilent.com/find/lowcostpower
Call Agilent 1800 629 485
Agilent Authorised Distributors
www.measurement.net.au
Western Australia,
Northern Territory
(08) 9437 2550
www.rftest.co.nz
New Zealand
(64) 4 570 2480
www.triosmartcal.com.au
Australia
ACT, NSW, QLD, SA, TAS, VIC
(1) 300 853 407
© Agilent Technologies, Inc. 2008
siliconchip.com.au
August 2008 3
MAILBAG
Letters and emails should contain complete name, address and daytime phone number. Letters to
the Editor are submitted on the condition that Silicon Chip Publications Pty Ltd may edit and has the
right to reproduce in electronic form and communicate these letters. This also applies to submissions
to “Ask SILICON CHIP” and “Circuit Notebook”.
Brushless DC is the
correct motor description
The article on the Vectrix motorcycle has a point in asking whether
the motor should properly be called a
“brushless DC motor”. In fact, the motor proper is either an AC synchronous
motor or an induction motor. Either
type can be fed from an inverter, in
principle.
But then nearly all DC motors
have an armature which is that of a
synchronous motor. The commutator
and brush gear ensure the armature
is always “in sync”, including at zero
speed.
The only true DC motor is rarely
seen and is called the homopolar or
acyclic configuration. The rotor is the
armature and is just a very large flat
copper disc with a brush at the axis
and another at the rim. The field is a
horseshoe magnet mounted so that the
magnetic field is normal to the radial
line between the two brushes.
Wrong capacitor in
frequency indicator
I built the “Frequency Indicator
For Generating Equipment” from
Circuit Notebook (SC May 2008).
I had trouble getting the oscillator
going at 500Hz. I think the 150nF
capacitor should have been 15nF.
However, even using this value
I couldn’t get the required range
of frequencies. Instead, I ended up
using a 1.2MW resistor in series
with the 100kW trimpot and a 10nF
(0.01mF) capacitor. I also think that
The acyclic motor is thus very simple; the drawback is that the armature
current required is enormous, up to
one million amps, depending on the
application.
Therefore, “brushless DC motor” is
arguably an appropriate term as the
inverter does exactly the same job
as the commutator and brush gear. I
prefer to separate the two functions
into “inverter” and “AC motor”, the
latter being either synchronous or
asynchronous (induction). My reason
is the combination is much more capable, albeit more expensive, than the
conventional DC motor.
John Waller, Plainfield,
Connecticut, 06374-1429, USA.
Don’t change settings
while power is applied
I read the article on the Low Voltage
Adjustable Regulator (SILICON CHIP,
May 2008) with some interest because
the design is nearly the same as one I
calibration can be made by plugging the plugpack into the 240VAC
mains which is really close to the
50Hz required for calibration. This
will avoid the need for accurate
frequency meter.
Jim Graham,
Moonah, Tas.
Comment: it does appear as though
the 150nF capacitor is out by a
factor of 10, as you suggest. Using
50Hz mains to calibrate the unit is
an obvious approach – why didn’t
we think of that?
built for myself nearly a decade ago.
In my design, I used a 6-position wafer switch to change the value of the
resistor between the regulator’s adjust
terminal and ground. However, the
switch was a break-before-make type
and that led to the demise of a perfectly
good Walkman cassette player.
I realised after I’d plugged the Walkman into the regulator that I had set
the voltage selector switch to 3V instead of 6V. Without thinking of the
consequences, I changed the voltage
output setting with the switch, without
disconnecting the Walkman. For the
brief period while the adjust terminal is disconnected from ground via
a resistor, the output of the regulator
rises to almost the input voltage, in
my case 24V. Ouch!
The result was one dead Walkman. I
think it would be a good idea to issue a
warning in the next edition of SILICON
CHIP that removing the jumper shunt
with a load connected is asking for
trouble. Otherwise it’s a great project
that will be very useful for many of
your readers.
Peter van Schaik,
Tenterfield, NSW.
Website for info on
connectors and pinouts
Your readers may be interested
to review the AllPinouts’ website at
http://www.allpinouts.org
AllPinouts, a community-built
reference archive for connectors and
cable pinouts, is currently the world’s
largest pinouts archive, listing more
than 1400 technical pages. This is a
www.furzy.com
We Create Electronic Controllers
4 Silicon Chip
siliconchip.com.au
EVs & solar power
are viable together
I feel the need to put pen to paper and wade into the argument
for EVs, especially relating to Dave
Waplington’s letter in the February
2008 issue.
Dave has a system that recharges
his EV from a solar array and he tells
us that after a few hours his batteries
are full and he is ready to do his day’s
driving. Presumably, the vehicle in
question has adequate range for his
day-to-day driving needs and he,
like most of us, has another car that
runs on some sort of liquid fuel for
any longer trips.
Peter Seligman replied that the
solar array produces X amount of
power on average and electricity
costs Y amount so that the array will
take Z (where Z is a big number)
years to pay off but that’s not correct is it? In fact, Dave’s solar array
displaces petrol and if he would
have used, say, $50 per week, then
his array will only take around 6.5
years to pay off.
But Dave no longer has to pay
for maintenance for the engine or
drive-train that he doesn’t have –
things like filters, cam belts, radiator
coolant, etc. Most especially, he will
free content project that collects information about hardware interfaces
of modern and obsolete hardware,
including pinouts of ports, expansion
slots, and other connectors of computers and different electronic devices
such has cellular phones, GPS, PDA
and game consoles.
Created with the same MediaWiki
software that was developed for the
Wikipedia project, AllPinouts allows
registered users to contribute and improve the website. All text is available
under the GNU Free Documentation
License (GFDL) and may be distributed
or linked accordingly.
Nicola Asuni,
Cagliari, Italy.
When an electrical engineer
cannot do electrical work
I have a Degree in Electrical Engineering which I received as a cadet
with Pacific Power, formerly known as
The Electricity Commission of NSW.
siliconchip.com.au
not have to pour five litres of highly
refined oil into his engine every six
months.
So let’s plug in some hypothetical
numbers: Dave sells his electricity to
the grid during the day when it’s 10c
per kilowatt-hour. Let say he makes
10kWh so he gets 100c credit.
During the night, he charges his
car from off-peak electricity that he
purchases for 5c/kWh and it costs
him around 40c (since it only takes
around 8kWh to charge the car).
That means he ends up with 60c
worth of credit to offset against his
daily consumption; not a fortune to
be sure, but still pleasing to behold.
As far as I’m concerned, that really puts things into the realm of the
financially possible – especially if an
EV was competitive in price to that
new car that you now covet. It helps
out the country’s energy situation
too. The system produces power
when it’s really needed and perhaps
keeps the power companies from
having to fire up their huge turbines
to meet the demand peaks during
the day. And then it puts some load
onto the spinning reserve at night.
Nice one Dave!
Ned Stojadinovic,
Gunning, NSW.
I majored in Telecommunications but
my electives were all Power Engineering-related. I also have a Certificate III
in Telecommunications Cabling and
an Advanced Amateur Radio License.
Within the Ham Radio world, I am the
only non-North American board member of TAPR, who pioneered Packet
Radio Technologies.
In my professional life I was employed by Pacific Power/Electricity
Commission of NSW for 13 years,
from 1990 until 2002. My first five
and a half years with them were as
an undergraduate attending UTS and
working at various sites.
While at University, my first Industrial Semester of about nine months
was at the Homebush Apprentice
Training School, where I learned electrical trades with first year apprentices.
I then spent some time working in
an office situation with Controls and
Instrumentation, with regular power
station trips. This was followed by a
Atmel’s AVR, from
JED in Australia
JED has designed a range of
single board computers and
modules as a way of using the
AVR without SMT board design
The AVR570 module (above) is a way of
using an ATmega128 CPU on a user base
board without having to lay out the intricate,
surface-mounted surrounds of the CPU, and
then having to manufacture your board on
an SMT robot line. Instead you simply layout
a square for four 0.1” spaced socket strips
and plug in our pre-tested module. The
module has the crystal, resetter, AVR-ISP
programming header (and an optional JTAG
ICE pad), as well as programming signal
switching. For a little extra, we load a DS1305
RTC, crystal and Li battery underneath,
which uses SPI and port G.
See JED’s www site for a datasheet.
AVR573 Single Board Computer
This board uses the AVR570 module and
adds 20 An./Dig. inputs, 12 FET outputs, LCD/
Kbd, 2xRS232, 1xRS485, 1-Wire, power reg.
etc. See www.jedmicro.com.au/avr.htm
$330 PC-PROM Programmer
This programmer plugs into a PC printer
port and reads, writes and edits any 28 or
32-pin PROM. Comes with plug-pack, cable
and software.
Also available is a multi-PROM UV eraser
with timer, and a 32/32 PLCC converter.
JED Microprocessors Pty Ltd
173 Boronia Rd, Boronia, Victoria, 3155
Ph. 03 9762 3588, Fax 03 9762 5499
www.jedmicro.com.au
August 2008 5
More on the
Enersonic Power Saver
With reference to your article on
the Enersonic “Power Saver” in the
May 2008 issue, I acknowledge that
this device is a fraud. However, I feel
when it came to the power factor
correction, Leo expressed surprise
when he plugged the Power Saver
in with a fridge and got a greater
power reading. As electronic gurus
I assume we know about Apparent,
Reactive and Real powers right?
What Leo forgot is that the Apparent
power of his fridge remained essentially the same with or without the
“Power Saver”; what changed was
the power factor.
A quick calculation proved that by
changing the power factor, the power
increased from 220W to 240W, and
the Reactive Power decreased from
3-month placement with the Environmental Section at Wallerawang Power
Station.
Following graduation, I was appointed to Bayswater Power Station’s
Electrical Branch where I was a plant
owner for DC Systems, Switchboards
and Motors. I obtained my High
Voltage certification, and performed
240V/415V work at various times
without supervision. AS3000 exempted supply authorities, meaning
that I was permitted to operate in this
6 Silicon Chip
101VAr to 31VAr. Leo thus neglected
to mention that “because of this”, it
uses more power, as our homes are
measured in Watts. It could only
work if Apparent power is measured
and power factors are an issue (as
pointed out in the article).
“You haven’t told us anything
new!” Yes, I have. In the article it
was stated several times that it uses
power in its internal circuitry and
that negates any savings the power
factor correction does. What I’m
telling you now is, that by correcting the power factor, it’ll make the
home meter tick over more power, so
it doesn’t save anything there either,
ie, the fridge, with 220W compared
to the 240W, you will be paying for
20W more with the “Power Saver”.
Matthew Thompson,
Gawler, SA.
manner. I was one of two engineers
in the branch and my boss held an
Electrician’s License as well as being
an Electrical Engineer.
After spending about nine months
at Bayswater, the organisation was
split up and I spent my remaining
time assisting with the management
of Engineering Information such as
drawings. When I left, my employer
paid for me to complete my Certificate
III in Telecommunications Cabling as
part of a redundancy.
With all this experience you would
think that it would be easy for me
to obtain an Electrical License. It is
actually basically impossible for me.
You see, I need to have two years of
electrical wiring experience in order
to get my license. This is a special requirement because I have an Electrical
Engineering Degree. Any other type of
Engineering Degree would make me
ineligible. But the experience must all
be post-graduation so the structured
experience I have from the Apprentice
Training School does not apply.
If I did manage to get the experience
I would still need to do a TAFE course
to prove that I have the expertise. In
my professional life, I have needed to
install alligator clips onto the end of a
3-phase 415V lead in order to test the
protection on an 11kV motor at a safe
voltage. I have worked on a 240VDC
800A Battery Charger live in order to
repair a faulty card.
The organisation I was working for
trusted me to do these things in order
for me to do my job. But I have also
seen a tradesman injured when he
came in contact with live wires on
a switchboard when a cover was not
replaced. And I have seen electrical
apprentices make extension cords
with plugs on both ends.
I am qualified and competent to design the electrical system for a house
or factory. I can legally install any of
the communications infrastructures. I
siliconchip.com.au
Banning live mains work
will save lives
In your Publisher’s Letter in the
June 2008 issue of SILICON CHIP
you have hit the nail right on the
head – electrical safety legislation
in Australia is a joke. The New Zealanders have it right and they have
the statistics to prove it.
Banning live mains work? That’s
a joke! What about intermittent
mains power problems that can’t be
fixed other than by live work? Most
people in this industry understand
such problems from personal experience.
I am not suggesting that workplace
safety programs are a waste of time.
Quite the opposite – so long as they
get results and reduce injuries and
deaths, I’m all for it.
“Nanny state”? You’re so right
again. There are so many examples,
can design a control system down to
board level. But I am not permitted in
this country to install any of it.
I do not begrudge the need to ensure
that people are competent but there
must be some middle ground. At the
moment there is no middle ground.
Darryl Smith, VK2TDS
Ingleburn, NSW.
Comment: your situation is identical to
that of many highly-qualified electrical
and electronics engineers throughout
it would take forever. Most obvious
is the near exponential increase in
the number of regulations that an
ordinary citizen must now comply
with. You need to be a bush lawyer
just to get a driver’s licence or build
a dunny these days. Oh, sorry, you
can’t install a toilet without being a
licensed plumber.
I believe that excessive regulation is a blight and is ultimately
self-defeating. Even law-abiding
citizens ignore lots of petty rules in
a desperate attempt to simplify their
already overloaded lives.
Colin Beeforth,
Doveton, Vic.
Comment: we think there is considerable merit to banning live mains
work. After all, if the majority of
electrocutions occur among electricians and electrical contractors,
such a ban is in their interest.
FRONT PANELS
& ENCLOSURES
Customized front panels can
be easily designed with
our free software
Front Panel Designer
• Cost-effective prototypes
and production runs
• Wide range of materials or
customization of provided
material
• Automatic price calculation
• Fabrication in 1, 3 or 7 days
Sample price:
USD 43.78 plus S&H
Australia. This is just another example of how over-regulation produces
ridiculous results.
Another engineer’s viewpoint
on electrical wiring
www.frontpanelexpress.com
When SILICON CHIP last raised the
issue of DIY electrical work I was fully
in support of what you were trying
to achieve. I believed that I should
have the “right” to do electrical work
since I have a degree in electrical
engineering, I grew up in a family
business which involved some types
of electrical work and I held other jobs
and interests which were related to
electrical work.
Several years ago I began an electri-
Australia’s Lowest Priced DSO!
Now you’ve got no excuse ... update your old analogue scopes!
Whether you’re a hobbyist, TAFE college or university workshop,
the GW GDS-1022 has the price and performance for you.
GW GDS-1022 25MHz
25MHz Bandwidth, 2 Ch
250MS/s Real Time Sampling
4k Memory Per Channel
TFT Colour Display
19 Auto Measurements
Built-in USB & SD Card Slot
GW Brand - 28 years in Australia
Sydney
Melbourne
Tel 02 9519 3933
Tel 03 9889 0427
Fax 02 9550 1378
Fax 03 9889 0715
email testinst<at>emona.com.au
siliconchip.com.au
Brisbane
Tel 07 3275 2183
Fax 07 3275 2196
Adelaide
Tel 08 8363 5733
Fax 08 83635799
Perth
ONLY $
Tel 08 9361 4200
Fax 08 9361 4300
web www.emona.com.au
499
inc GST
SAVE $
50
EMONA
August 2008 7
Mailbag: continued
Helping to put you in Control
PLC’s
We have a selection of programmable logic controllers and HMI displays
XC3 High Performance PLC
features a large
number of functions, large memory, small size and
fast scan times. Functions include
PWM and 2 axis Stepper and Servo
Motor control. Prices from
$215+GST. Programming available starts at $99+GST
XC5 High Performance PLC
A more powerful
and larger I/O
version of the
XC3. Includes
PWM and 4 axis Stepper and Servo
Motor controls
Prices from… $525+GST
XMP3 PLC and
HMI The XMP3 is
a PLC and HMI
display all
wrapped up in 1
unit. Can do 2
axis stepper and servo motor control
$425+GST
OP320A Operator Panel
4 x 24 Character
LCD, 20 Programmable keys supports popular PLC
protocols. Can be connected to our
XC3 and XC5 PLCs $249.00+GST
TP562-T Touch
Screen Display
5.6 inch 256 color
TFT 320*240 pixels
4MB FlashROM 4KB
SRAM. Support for
various popular PLC's $799+GST
TPA61-T Touch
Screen Display
10.4in, 256 color TFT
800 x 600 pixels
8MB FlashROM 4KB
SRAM. Support for
various popular PLC's $1699+GST
Contact Ocean Controls
Ph: 03 9782 5882
www.oceancontrols.com.au
8 Silicon Chip
cal apprenticeship and I realised that
what the electrical industry claims is
in fact true – there’s a lot more to electrical work than just the perceived ability to connect a few wires. A home’s
wiring is an intelligently planned
and carefully built system which
is designed to reduce or eliminate
many dangers with using electricity.
Any one defect can bring that whole
system down.
I learnt that despite my previous
skills and qualifications even my own
knowledge was limited. No amount of
study or other experience can compensate for real experience while working
under a fully licensed electrician.
The wiring rules, AS3000, are over
450 pages and it takes years to learn it
thoroughly. You’d be amazed at how
many rules are applicable for something even as “simple” as renewing
a power point – rules and techniques
which you’d never know unless you
do an apprenticeship. Personally, I
don’t care if I come across unlicensed
work as long as it complies with the
rules. But I can easily identify it if it
is done wrongly and I have to fix it.
Make no mistake that a false sense of
confidence in electrical work will lead
to more dodgy work.
Now with respect to the June 2008
article, so you remove your switch
or power point and one of the wires
breaks off. How do you fix it? What’s
the difference in technique between
solid or stranded cable? Are all the
wires the same size? What if the insulation is degraded? What if there is
no earth? Or bare earth? Or a flexible
cable connected? Or a red and black
wire connected together?
You can’t just shove it back in the
wall and pretend it’s not there – it must
be made compliant or disconnected.
Only an electrician has the knowledge
to rectify ANY problem arising.
How many handymen do you think
will pay $100 for AS3000? Then how
many would learn and understand it
thoroughly? Yet this is the bible for
electricians, a code to which all work
must comply. Except for a few people
such as yourselves at SILICON CHIP,
most won’t even want to know about
these wiring rules because “it’s only
a few power points anyway.”
A good test for all who demand the
right to do electrical work is to take
a sample Licensed Electrical Theory
(LET) exam: http://www.electroskills.
com.au/downloads/LET Sample
Exam.pdf
The pass mark is 75% and the time
limit is two hours. The two practical
exams are similar and are the culmination of four years of training. Are you
handymen capable of passing these?
I surmise another reason for this
debate is that electricians are perceived by some to be of low skill and
education. Well, I can tell you that
the schooling and final exams were
no walk in the park. Combined with
the practical aptitude required, it
makes electrical work into a skilled
profession and that’s the reason why
government authorities treat it as such.
Robert Hatvani, B.E
(Electrical) RMIT; Cert. III in
Electrotechnology (Systems
Electrician) Box Hill TAFE.
Digital LC Meter
calibration procedure
With regard to the Digital LC Meter described in the May 2008 issue,
maybe there’s something omitted from
the explanation of how the “calibration mode” works but it seems to me
that equation (3) calculates C1 from C2.
The problem is that it doesn’t know
the value of C2. If it assumes C2 is
precisely 1nF but is off by 1% it cannot “measure” the value of C1 to any
better than 1%. This is a bit useless
if we already know the value of C1 to
within 1%. Can you please explain
how “calibration mode” really works?
Mike Hudson,
Chester Hill, NSW.
Comment: you are correct in deducing
that the calibration of the LC Meter is
essentially based on the accuracy of
C2. However, if this is only known within 1%, the calibration modes allow the
instrument itself to be ‘fine calibrated’
against an external capacitor if you
have one whose value is known more
accurately than 1%.
The important thing to remember is
that once the meter is calibrated, its
accuracy is the same for inductance
siliconchip.com.au
Comment on
electric cars
I have been an enthusiastic reader
of SILICON CHIP since 1999. Its wellbalanced content has always been
able to retain my full attention over
all these years.
In contrast to a recent reader’s letter, I am always waiting for the next
publication of a PICAXE-related article. Since the advent of the PICAXE
VSM simulator (SILICON CHIP, January & February 2008), it all became
even more exciting.
I also would like to congratulate
you on your regular “Publisher’s Letter” and the very personal stand you
take on socio-economic issues that
will influence all our futures. You
recent articles on electric cars and
the Vectrix were very interesting. I
think, it is important to push ahead
in this field regardless of the present
shortfalls of the current technologies and products available. They
all are essential “path cutters” to
better solutions in the future. What
would have become of aviation if
people had given up at the stage of
the Tiger Moth?
Now back to the electric car:
Your article in the April 2008 issue
stimulated me to build a simple
spreadsheet model regarding the
economy and the availability of
alternative power sources. What it
shows is that even if we could convert all cars to electric over a short
period of time, there would not be
enough power available. We would
have to roughly triple the output of
our power stations!
as well as capacitance. And even 1%
accuracy is adequate for measuring
inductors.
Home Electrical Safety License
should be available
Your article on DIY wiring in the
June 2008 issue was a good read and
challenged the convention in Australia. It would seem that entrenched
thinking and powerful lobbies keep
us from being credited with a small
amount of intelligence and ability to
learn.
I do have a suggestion. Might it be
possible to introduce a “Home Electrisiliconchip.com.au
A couple of years ago, I was involved in projects with fuel cells
and hydrogen for temporary storage
of electric energy in remote areas.
Although there are merits for these
special applications, I think fuel
cells will not be a satisfactory and
available solution for individual
transport, for the simple reason
that the generation (or availability)
of hydrogen is too inefficient and
expensive.
In a little fuel-cell model system
we used an electrolyser to generate
hydrogen from electric energy (solar
panel or mains supply). The hydrogen was then stored in metal hydride
cylinders and released to the fuel
cell on demand, which converted
it back into electric power driving
some load.
The loss of energy (very rough
estimate) from electric to hydrogen
was 50% and from hydrogen back
to electric another 50%. This means
that from 100W injected into the
system, only 25% was retrieved.
Any battery or super-capacitor can
do much better.
Bio-fuel, already in competition
with the production of food, seems
to be no alternative either. What remains suggests being a drastic cut in
overall energy consumption, which
would mean using public transport
for the majority of our needs, supported by small low-energy vehicles
to get from home to the next bus or
train stop. Cars as status symbols
have become a joke.
Klaus D. Fahrner
Munster, WA.
cal Safety License” that would allow
Australians to work on their homes in
a similar manner to New Zealanders
after a suitable training course? This
concept of a suitable short training
course aimed at specific required
knowledge is not new and is already
embodied in such areas as the “Skippers Ticket” here in WA, obtaining the
Marine Radio Operators Certificate of
Proficiency or even the Foundation
Amateur Radio License.
It seems to me that the essentials
of electrical safety around the home
could be covered in a short course
followed by a practical and theory
ew
See revi’08
e
n
u
in J
HIP
SILICON C
ALTITUDE
3500-SS
Valve Stereo
HiFi Amplifier
32W/Channel, 4 or 8Ω
“This particular
valve amplifier
performs very well”
Leo Simpson
SILICON CHIP June 2008
A blend of quality components and modern
design
Beautifully finished in 7mm brushed
aluminium
Four stereo analog inputs
Gold plated connectors and selectors
Extended bandwidth of 10Hz to 90kHz
Carefully chosen design layout and wiring
location
Direct input coupling improves transient
response
Specialised wide-bandwidth audio output
transformers
Class A/B pentode output using genuine
Russian-made Electro-Harmonix EL34 valves
Matched pairs, factory bias adjusted
Stainless steel heat shields improve overall
efficiency
High quality capacitors
Beautiful in looks, design and listening
The A3500-SS is an exclusive and
advanced version developed by Stones
Sound Studio. Retail price is just
$1899, available now from
ELECTRONIC SERVICES AUSTRALIA
138 Liverpool Rd, Ashfield NSW
(Locked Bag 30, Ashfield NSW 2131)
Ph: (02) 9798 9233 Fax: (02) 9798 0017
Web: www.wagner.net.au
August 2008 9
Save Up To 60% On
Electronic Components
Great New ET-AVR Stamp
Only $23.88
* Includes ATMega128 Microcontroller
* Up to 53 I/O Points
* 8-Channel 10-bit A/D
* Direct In-Circuit Programming
* Ideal as a Removable Controller
Exciting New ET-ARM Stamp
* Includes LPC2119 Microcontroller
* High-Speed Operation
* Heaps of I/O plus CAN, UART, I2C
* In-Circuit Programming
* Supporting Board Also Available
Only $33.48
New Solar Regulator
Compact, inexpensive,
easy-to-use solar regulator
in 5A, 10A and 30A sizes.
Only $31.08
We are your one-stop shop for Microcontroller Boards,
PCB Manufacture and Electronic Components.
www.futurlec.com.au
examination to establish the candidate has understood
the course content. A license could then be issued to the
successful candidate to work on his own home.
It seems simple and there would be organisations out
there willing to run such courses if it meant they could
charge and make money from it. The electrical lobby
groups could even do it and perhaps through the course
might encourage people to take up an electrical apprenticeship or am I dreaming?
Nigel Dudley,
Oakford, WA.
Comment: that’s a great idea.
Old inverters need not
cause interference
In response to Bruce Bowman’s letter in the May 2008
issue, I am surprised about the interference he experienced
10 Silicon Chip
Mailbag: continued
Old TV sets
need good homes
Having had a keen interest in TV over the years, I
have a number of old non-working colour TVs (late
1970s to mid 1980s) that I am going to trash if I am
unable to give them away. I am willing to deliver them
in the Brisbane, Logan & Redlands areas if required.
I should have schematic diagrams for most of them.
The list of sets is:
Brand Name Model/Chassis Circuit Available
Commander CHT 9102
Yes
Goldstar CB2 6105
Yes
JVC 7465 AU
Yes
Kriesler 59-1
Yes
Kriesler 37-104
Yes
Philips KT2A
Yes
Pye Series85 48 LRIN-T
No
Rank Arena C 2252
No
Sharp C 206X
No
Sony KV-A29115
No
Thorn 9014
Yes
Please contact me via email at llwinter<at>bigpond.
com.au, with “Old TV’s” in the subject line. I really
do not wish to see them go to the tip.
Lawrie Winter,
Logan, Qld.
from the Ferris vibrator inverter described in the February
2008 issue. I have several of these in my collection and as
I run a small 12V wind and solar-powered lighting plant,
one of them often runs all day, powering a 1948 Breville
mains/battery portable valve radio.
I live 80km west of the Sydney AM stations and receive
them without any problems, and that’s with the internal
loop aerial alone. However, I should point out that there
was some interference until I earthed the negative of the
12V supply. I wonder if lack of earthing was the cause of
Mr Bowman’s problem.
I am also surprised at the claim that these inverters
were not meant for powering radios. Not only does the
label on the front panel indicate their suitability for this
but this model of inverter was specifically meant as a
companion to the Ferris 106 mains/battery portable, for
in-car operation.
siliconchip.com.au
Incidentally, running the radio off a 100Hz square wave
will be more efficient as far as power supply filtering
goes. Not only will the filter choke and capacitors be
more effective but the square wave means there’s a lot
less “dead” time in the supply waveform that the filter
has to compensate for. Any interference problems are
therefore likely to be RF-related.
Just to clear up any possible misconceptions that vibrator power supplies are inefficient, I fail to see how this
is so when there is virtually no voltage drop across the
contacts when closed (as opposed to the saturation voltage of a bipolar power transistor). Apart from transformer
losses, the only power required to run such an inverter
is the 200-odd milliamps to drive the vibrator reed. The
fact that a 100W transistor inverter needs heatsinking and
the vibrator equivalent doesn’t says something.
The other advantage is that the vibrator inverter isn’t
damaged by momentary overloads and happily works irrespective of input polarity. Modern inverters with their
H-bridge of power Mosfets switching 340VDC are rather
fragile by comparison. It only takes microseconds to end
up with an array of blown (an expensive) Mosfets.
I have quite a collection of homemade and commercially made vibrator inverters, as well as vibrator-powered
valve radios. From current measurements, it seems that
efficiency is very good; 80% is not impossible to obtain.
I’ve built a few inverters with toroidal transformers and
these work even better, with greater efficiency and less
RFI suppression required.
Neither has reliability been an issue with the MSP
(AWA) or other vibrators with series-driven reeds. The
Ferrocart (Astor) units, on the other hand, sometimes
need some TLC but there is an MSP plug-in replacement (type V0410) which completely eliminates that
problem.
Having said that, I have come across some bad examples of vibrator power supplies with poorly chosen
buffer capacitors or poor transformer design. To horrify
people even more, apart from running valve radios and
vibrator inverters off my solar/wind supply, there’s also
a multitude of incandescent light bulbs!
Finally, in response to the claim by Rodney Champness in his Vintage Radio column in the May 2008 issue,
that there were no 12V or 32V TV receivers made locally,
there were, in fact, some Ferris models, such as the C21F.
These had an external power supply in a stand-alone box
and allowed for mains or battery operation. The valve
heaters were wired in series/parallel for 12V or 32V.
The mains supply was conventional except for the 12V
or 32V heater winding and the battery supply had two
separate vibrator supplies in the one box with their DC
outputs paralleled.
A later set, the 32V model B23, used a transistor supply
to provide the high tension. There was also the AEI-Ekco
TX276 9-inch portable with 12/240V operation. The 12V
supply was internal and simply consisted of an extra
power transformer winding and vibrator which were
brought into operation for 12V DC operation.
John Hunter,
SC
Hazelbrook, NSW.
siliconchip.com.au
Small Colour TFT LCDs
Door Camera
5.6‛‛ Small TFT LCD
√
√
√
√
√
4.0‛‛ Small TFT LCD
Full Color TFT LCD
NTSC&PAL Compatible
With Picture Quality Control
DV 12V Operation
Simple Wire Harness Connection
Digital Video Recorder Modules
DVR8100 Video & Still Image
Recording On Motion Detect
√
√
√
√
√
√
√
2 Video Ch Input
NTSC&PAL
Alarm output
Trigger input
SD card
On Board Flash
JPG&AVI file format
√
√
√
√
√
√
√
Real time clock
Date & time stamp
PIP, OSD
With keyboard
RCA connections
DC input (9V to 12V)
Kit available
DVR623 DSC/DV Module
√ Mega pixel image sensor
√ Real time Video output
√ Storage to SD card
√ OSD
DV:
√ VGA or QVGA
√ Frame rate 1, 10, 30fps
√ Recording from 1-99 sec
√ Preset capture schedule
√ Trigger input
DSC:
√ 3M, 1.3M & VGA
√ Picture-in-picture
√ Preset capture schedule
√ External trigger input
√ Keyboard snap shot
TM
www.tenrod.com.au
sales<at>tenrod.com.au
NSW: tel: (02) 9748 0655 fax: (02) 9748 0258
VIC: tel: (03) 9886 7800 fax: (03) 9886 7799
QLD: tel: (07) 3879 2133 fax: (07) 3879 2188
NZ : tel: (09) 298 4346 fax: (09) 353 1317
Unit 1, 24 Vore Street Silverwater NSW 2128
August 2008 11
By Ross Tester
Printing in the
Third Dimension
Imagine a colour printer that outputs images not just in the
two dimensions we’re all familiar with – width and depth –
but adds the third dimension, height, so that the “printed”
images can be physically held, picked up, turned, inverted
. . . just like any other 3D object.
12 Silicon Chip
siliconchip.com.au
A
few months ago, a company called SOS Components
placed a flyer in SILICON CHIP advertising their rapid
prototyping bureau.
It looked fascinating but, not being involved with anyone
who needed or used such a service, I’d all but forgotten
about it . . . until I came across the company’s stand at this
year’s national manufacturing week exhibition.
Centrepiece of the stand was a magnificent model boat.
It would have been well over a metre long, 250mm wide
and perhaps 350mm deep. I was informed that this boat
was an exact scale model of a boat currently being built in
Queensland for a (very!) well-heeled individual.
Now prototypes or models are not exactly new – a lot of
models, for all sorts of “products” are built before production begins. The client might want to make structural or
cosmetic changes once they see how the “thing” actually
looks. And it’s normally a lot cheaper to do it earlier than
later.
A lot of companies also make accurate models of proposed new products for evaluation, testing, checking and
so on.
But this was no ordinary model boat. It wasn’t carved
from a block of balsa or modelling plastic by a skilled
modelmaker, labouring away for perhaps several weeks.
In fact, it wasn’t carved at all.
It was printed, in the true sense of the word, layer after
layer after layer – and in colour! Due to size limitations of
the printer, (maximum build size is 250 x 350 x 200mm),
it was “printed” in four sections which were then glued
together. Because each section was extremely accurate,
there were virtually no join edges – just some very minor
retouching was all that was needed to hide the seams.
That’s a photo of it at left, with the man who “printed”
it, Jeff Condren, from SOS Components in Brisbane.
To say it was impressive is at best an understatement.
However, it wasn’t all that SOS were displaying. Across
the back of the stand was a large (>2m x 2m) model of a
proposed Brisbane motorway intersection. Note the word
You better believe it: it’s a model of a Tupperware bowl,
complete with removable lid moulded in “Superflex” –
developed in Australia by SOS Components.
“model”. It wasn’t just your usual flat “map” with a few
cars and trucks added to make it look more realistic; this
one had all the terrain in accurate scale, the cuts for the
motorway lanes where required, the hills and landscaping
alongside – it was just like looking down on the scene from
a few hundred metres up.
Then there were quite a number of “model” buildings,
engineering samples, appliances, components, even soft
plastic bottles (more on this innovation shortly) – all in accurate scale, most in colour. Because the layers are printed,
any “internal” parts are formed exactly as they would be
in the real thing – even movable parts.
For designers and engineers creating a new product,
this aspect is so valuable. They can actually see how the
components fit into one another, how they react, if the
clearances are correct and so on.
But it takes a little bit to get your head around the fact
that every one of these is printed, not carved, cast, stamped
or any other, shall we say “conventional” method of producing models or miniatures.
A sense of déjà vu?
Regular SILICON CHIP readers may recall a story we
published back in the September 1996 issue on a process
Take a set of architect’s drawings, convert them to 3D . . . and print them! Just imagine how much more likely the sale
would be when a potential buyer can see a real model of what they are being offered!
siliconchip.com.au
August 2008 13
for producing prototypes. At first glance, it might appear
that the processes are the same. While they are, to some
degree, similar, that’s like saying Minis and Maseratis
are similar. Things have changed significantly in the last
decade or so.
For a start, the process we looked at in 1996 used a laser
beam to “sinter” a layer of fine powder together. (Sintering is
the amalgamation of material by heat, without melting). The
article also discussed a process where a layer of adhesivebacked paper was laser-cut and stuck to a previous layer,
building up one layer at a time.
The process we are looking at here is true printing – in
fact, four-colour (CMYK – cyan, magenta, yellow and black)
printing, as used in this magazine. There aren’t many colours that CMYK printing can’t replicate reasonably well –
fluoro colours and bright orange/bright green are the main
exceptions. However, by combining various percentages
of inks, the vast gamut of colours can be produced very
successfully and is one of the reasons the CMYK process
is used so extensively.
However, unlike the offset (roller) printing used for most
CMYK jobs, the 3D printer works in much the same way
as an inkjet printer. First it deposits a very fine layer of
tiny beads of powder, then sprays microscopic droplets
of ink onto the powder in the required pattern as the head
passes over.
As the powder is “wet” by the ink, it effectively turns it
into a glue which bonds to the layer immediately underneath. As the ink dries, the powder/glue hardens. Then
the process is repeated – over and over – and every time
the printer head makes a pass over a layer and it is completed, the whole thing drops down about 0.1mm, ready
for the next layer.
Thus the image is built up, layer by layer, until the 3D
image is produced. Only the areas of powder hit by ink
droplets are affected, so all of the other powder remains in
its original condition and is available for re-use – in fact,
it is collected for that very purpose.
If the original had printing, colouring, texture mapping
or labelling, so will the 3D-printed “image”
Complexity is no problem – it takes exactly the same
time to print a highly detailed, intricate image such as
those shown on these pages as it does to print a brick the
same size!
Where does it get the image to print?
Like any “conventional” printer, the 3D printer requires
“driving instructions” to tell it where to deposit which ink
The medical applications, particularly in a learning
environment, are enormous: above is a human heart,
printed from an MRI Scan. This heart, though, comes apart
as seen top right so that all the chambers and valves can
be seen exactly as they should appear. For good measure,
lower right is a “slice” or cross-section of a human kidney,
complete with colour-coding to show how it works.
14 Silicon Chip
siliconchip.com.au
and in which quantities to reproduce the colours required
in the places required.
Most printers simply need X and Y co-ordinates but the
3D printer also needs Z – the depth.
The image might come from a 3D laser scan, an architect’s
or engineer’s drawing in a CAD program or even, as we saw
earlier, scaled down plans of a ship, a building, a spacecraft . . . in fact, just about anything that can be plotted in
all three dimensions can be used to print the solid object.
Where did the process come from?
The 3D printing process was invented by Dr Jim Bredt
and Tim Anderson, students at the Massachusets Institute
of Technology during the early 1990s.
Part of Dr Bredt’s PhD thesis involved the use of low-cost
printer technology to produce 3D images.
They formed ZCorporation which, with a licence from
MIT for the 3D printing process, has now grown to an
organisation with distribution and service in 61 countries
and over 160 employees.
SOS Components are the Australian distributors of
ZCorporation products. The can produce elastometric
parts, direct casting moulds, investment cast patterns and
snap-fit parts directly off the printer with no machining
required. These take hours instead of the traditional prototype days – and in fact are generally much more accurate
than a hand-made (machined) prototype.
Superflex
However, SOS has taken the ZCoporation idea another
step further with Superflex. By using a compound they
developed themselves, SOS can produce flexible parts in
a 24-bit colour process.
Complexity is no problem, as this highly-detailed model of
a machine demonstrates. This would have taken exactly
the same time to print as a brick of the same size!
(Right): Complete with obligatory “Save $XXXX” show
stickers, one of the ZCorporation 3D printers – in this case
the Spectrum Z510 – on display at the Manufacturing Week
exhibition. Below is a close-up of the business end of the
printer. On the extreme right is the movable print head
which sprays microscopic ink droplets onto the powder in
the well at left. As each pass is made, the bin containing the
powder drops down a miniscule amount and a fresh layer of
powder is laid down, ready for the next ink spray. The size
limitation of this particular printer can be seen; hence the
need for the model boat at left to be printed in four sections
and then glued together. Because the printing process is so
precise, the complete model appears virtually seamless.
siliconchip.com.au
August 2008 15
Want to know how a turbine works? The students can see
“inside” the turbine with this exploded view of a turbine.
Printed with all components already in place (and again
colour-coded to aid understanding) this model would take
hours to produce instead of weeks in a model-making
shop.
A “plastic” bottle printed with Superflex. As you can see, it
behaves just like a “real” plastic bottle would behave.
This enables the customer (and therefore evaluation
and market research groups) to not only touch and feel a
prototype product, they can squeeze it and flex it – just
like the real thing would behave.
Prototype squeeze bottles or extrusions that can be
squeezed or flexed make a world of difference when it
comes to product evaluation.
Because they are printed and the (non-hardened) inside
sections removed, empty bottles can be just that. If the
design has movable internal parts , the model will have
movable internal parts. And parts in the design that move
with respect to other parts can move with respect to other
parts in the model – and be checked that they do move!
Who uses this service?
Just about anyone who needs a highly accurate model of
just about anything – for just about any purpose!
The obvious users are in product design and development, advertising agencies, architects, real estate developers, colleges and universities . . . and then there are the
not-so-obvious such as demonstrated by the model boat
photograph.
16 Silicon Chip
As a sales aid, it is without peer. You can just imagine
how much more impressive is a scale model of a multimillion dollar bridge or freeway than even the best aerial
photos. It’s more than likely that the 3D printing process
has used those same aerial photographs, added data from
topographic maps and voila! – a 3D “map” where everyone
can see heights and relativities.
Similarly, product prototypes: Proctor and Gamble’s
Tim Smith said “We’ve handed people pictures, we’ve
even handed them 3D glasses to watch a screen. But I
never saw jaws hit the floor until I handed them a part
in full colour!”
Motorola’s V70 phone was extensively designed using
the ZCorp 3D printing process. Many different models were
made to be market-tested as well as in-house evaluation,
with the final design achieving the design goals simply
because it was so close to the “real thing”.
Then there are all the people who use the process to produce extremely accurate moulds with no costly machining
to worry about. It’s suitable for a wide range of moulding
processes including direct casting moulds in metal or polyurethane and investment cast pattern moulds, sand casting,
RTV moulding and thermoforming, among others. In fact,
the system is now being used by most of the big names in
the industry, simply because it cuts so much time out of
the production equation.
Investment casting, by the way, means a (usually) metal
part produced from a mould that was created by surrounding an expendable pattern with a ceramic slurry.
It offers a very smooth surface finish with intricate design and detail possible. The dimensional accuracy is very
high – in the order of ±.002cm/cm.
More information?
SOS Components offer a free CD which contains an
extensive library of 3D models as well as explanation on
how the processes work. They are located at 30 Paradise
St, Banyo, Qld (on Brisbane’s northside, not far from
Brisbane airport). Phone no is (07) 3267 8104. Website is
www.3dprinting.com.au
SC
siliconchip.com.au
SILICON
CHIP
Order
Form/Tax Invoice
Silicon Chip Publications Pty Ltd
ABN 49 003 205 490
www.siliconchip.com.au
PRICE GUIDE: SUBSCRIPTIONS
YOUR DETAILS
(Note: all subscription prices include P&P).
(Aust. prices include GST)
Your Name________________________________________________________
(PLEASE PRINT)
Organisation (if applicable)___________________________________________
Please state month to start.
Australia: 1 yr ...................... $A89.50
1 yr + binder ....................... $A105
NZ (air): 1 yr ....................... $A96
Overseas (air): 1 yr ............. $A135
2 yrs ...................... $A172
2 yrs + 2 binders .... $A203
2 yrs ...................... $A190
2 yrs ...................... $A260
Address__________________________________________________________
PRICE GUIDE: OTHER PRODUCTS
_________________________________________________________________
Postcode_____________ Daytime Phone No. (
)_____________________
Email address (if applicable) ___________________________________________
(all prices include GST on Aust. orders)
*SILICON CHIP BACK ISSUES in stock: 10% discount for
10 or more issues or photocopies. Australia: $A9.50 ea
(including p&p). Overseas: $A13 each (including p&p by air).
Method of Payment:
*ELECTRONICS AUSTRALIA: project photocopies. Australia:
$A9.50 each (including p&p). Overseas: $A13 each (including
p&p by air).
o Cheque/Money Order o Visa Card o Master Card
*BINDERS: BUY 5 or more and get them postage free.
(Available in Aust. only): $A13.95 each plus $7 p&p per order.
*ELECTRONICS PROJECTS FOR CARS, VOL.2: Aust.
$A14.95; Overseas $A18.00. (Prices include p&p & GST
where applicable).
Card No.
*PERFORMANCE ELECTRONICS FOR CARS: Aust.
$A22.50; Overseas $A26.00. (Prices include p&p & GST
where applicable).
Card expiry date:
Signature_____________________________
SUBSCRIBERS QUALIFY FOR 10% DISCOUNT ON ALL SILICON CHIP PRODUCTS*
* except subscriptions/renewals
Qty
Item
Price
Item Description
Subscribe to SILICON CHIP on-line at: www.siliconchip.com.au
Both printed and on-line versions available
Total
TO PLACE
YOUR
ORDER
siliconchip.com.au
P&P if
extra
Total
Price
BUY
MOR 10 OR
ISSU E BACK
ES
A 1 0 & G ET
DISC %
OUN
T
$A
Phone (02) 9939 3295
9am-5pm Mon-Fri
Please have your credit
card details ready
OR
Fax this form to
(02) 9939 2648
with your credit card details
24 hours 7 days a week
OR
Mail this form, with your
cheque/money order, to:
Silicon Chip Publications Pty Ltd,
PO Box 139, Collaroy, NSW,
August
Australia
20972008 17
08/08
TekTronix DPO3034
Digital Phosphor
Oscilloscope
Review by
Mauro Grassi
The 300MHz DPO3034, with its
wide “digital phosphor” LCD
screen, is a serious oscilloscope
with an impressive list of features
and an excellent user interface.
T
he TekTronix DPO3034 is an
impressive oscilloscope with
the latest version of Tek’s “digital phosphor” screen and advanced
features like extended MATHs functions and waveform replay, zoom and
search.
Its bandwidth is 300MHz and the
sampling rate is 2.5Gs/s for each individual channel.
With some 4-channel oscilloscopes,
the sampling rate is shared among the
channels or pair of channels. This
means that the effective sampling rate
is frequently half that of the quoted
specification, when all channels are
in use.
However, this oscilloscope achieves
2.5GS/s on each channel at all times.
The vertical resolution of the digitising system is 8 bits and the sensitivity is better than most comparable
oscilloscopes, ranging from 1mV/div
to 10V/div.
Phosphor display
This scope has the latest version
of Tek’s so-called “digital phosphor”
display. The colour screen is a 228mm
(9-inch) (diagonal) WVGA (wide VGA:
18 Silicon Chip
Specifications at
a glance:
Input channels:.....
... 4
Analog Bandwidth:
.... DC to 300MHz
Sampling Rate:.....
... 2.5GS/s at all tim
es for each channe
Memory Depth:.....
l
... 5Mpts
Vertical Sensitivit
y:... 1mV/div to 10
V/div
Vertical Resolutio
n:.. 8 bits
LCD Screen:........
... WVGA (800x480
pixels)
Screen size:........
.... 22.8mm (9-inch
) diag
Weight:..............
... 4.2kg
800 x 480 pixels) LCD that looks bright
and shows good contrast.
The display refresh rate is fast at
50kHz.
The screen emulates the desirable
features of the phosphors used in
analog oscilloscopes employing CRTs
(Cathode Ray Tubes).
The intensity of the traces can be
varied over a wide range while the
persistence time can be selected from
periods ranging from 10 seconds down
to milliseconds. This is useful when
you have fast glitches or you are using
single step triggering.
Interestingly, the display has a wide
screen aspect ratio and is 198mm wide
by 120mm high (1.65:1). This allows
you to see more time domain data and
effectively gives you the advantage of
an even larger screen.
Replay and review waveforms
One of the best features of this
oscilloscope is its ability to capture
and replay waveforms. This feature
is part of the so-called Wave Inspector module.
It has a zoom and pan control knob
that allows you to search and mark the
waveform data by comparing it to a
preset trigger pattern. Its deep memory
of 5Mpts (million points) means that
at a reasonable resolution acquisition
rate of say 100Kpts you can capture
almost a minute of waveform data.
Wave Inspector then allows you
to mark and search waveforms. You
may be interested in a small portion
of a waveform, one that may occur
relatively infrequently yet occurs very
quickly.
While having a deep memory is essential, it is also essential to be able
to search that large memory.
The search feature functions much
like a trigger except that it is applied to
an already acquired waveform rather
than a real time waveform. There is
the added advantage that once the
data has been captured you can try
different searches. You may then mark
the relevant points where the search
found the trigger and go back to it or
scroll back and forth between saved
markers.
A screen grab showing the Wave
Inspector is shown in Fig.1.
You can also pan and zoom in on
parts of the captured waveform to insiliconchip.com.au
spect it in closer detail. These features
make the DPO3034 a very powerful
debugging tool.
Advanced triggering
As is usual in current oscilloscopes,
the trigger can be AC or DC-coupled
or low or high pass filtered to reduce
spurious noise.
The standard triggering modes of
the DPO3034 include the usual edge
and pulse triggering modes as well
as standard video triggering (NTSC,
PAL, SECAM). For the newer HD (high
definition) TV formats however, the
DPO3034 must be upgraded with an
optional module.
The DPO3034 also has some advanced triggering modes, one of which
is sequential triggering. This mode allows you to select a primary trigger and
a secondary trigger. The triggering will
occur only if the primary trigger occurs
followed by the secondary trigger.
Normally the two triggers would take
their input from different channels.
Optional modules
Application modules are available
to enhance the DPO3034. These are
siliconchip.com.au
unlocked by purchasing an additional
licence.
For example, there are modules
to decode serial protocols like I2C,
RS232/485, LIN, CAN and SPI as well
as for the HD TV formats, as mentioned
previously.
The serial protocol modules are especially useful if you are debugging an
embedded application. It is common
to find a few different serial busses
operating concurrently even if all you
are using is a small microcontroller.
In Fig.2 we show the result of decoding an RS232 stream using the optional
module.
The DPO3034 also includes, for the
serial protocols, an event table, shown
in Fig.3. This is a log of the relevant
decoded data in chronological order.
These modules are implemented
as small “cards” that plug into one
of four ports on the front of the oscilloscope.
The automotive serial protocols
CAN/LIN are separate to the data protocols, so you will need two different
modules if you want all of these.
Considering that many cars use both
CAN and I2C this could have been
better offered as a single module, especially since the number of upgrade
ports is limited to four.
Unfortunately, you cannot trigger on
these serial events or on the optional
video formats unless the module is
installed. Some oscilloscopes allow
you to trigger on serial protocols and
only the decoding is optional.
For the DPO3034 you need the module for both triggering and decoding.
For modules not installed in your
oscilloscope, there is a 30-day free
trial activated when you first use your
oscilloscope.
Probes
The DPO3034 and other oscilloscopes in this range are supplied
with one 500MHz passive probe per
channel. Each of the four BNC inputs
has auto-sensing and can also provide
power for active probes.
In fact, the DPO3034 can provide up
to 20W of power for active probes.
August 2008 19
Fig.1: this shows the Wave Inspector enabled. Having captured
an audio stream, we can zoom in and “play” it back. The
small white triangles visible at the top of the bottom window
indicate the edge trigger events (the triggering was set to a
falling edge at 0.0V and the audio stream is AC coupled). You
can then pan across from one marked event (trigger) to the
next inspecting the captured waveform data.
Apart from the usual passive probes,
you can optionally use current sensing
and differential probes.
The input impedance of each channel can be selected from 1MW, 75W or
50W. The 50W input impedance is useful for RF circuit analysis, while 75W
is used for TV or video work.
The DPO3034 incorporates in-built
75W terminators that will be appreciated
by video technicians, as this is not commonly found in oscilloscopes.
Each channel can be AC or DC
coupled and bandwidth limited to
150MHz or 20MHz. In general you
should use the lowest bandwidth
which will still give optimum resolu-
tion. Any higher bandwidth will just
add noise to the signal.
MATHs features
The MATHs features of this oscilloscope are exceptionally good. You can
do real-time FFT analysis on a signal
but you can also define a general mathematical expression and display it as a
trace on the screen in real time.
In Fig.4 we show the result of using
the MATHs function to compute, in
real time, the gain-bandwidth product
of an op amp.
Maths waveforms can be created
from real time channel data or from
previously stored reference wave-
Fig.5: a Triac controlling a mains light using phase control. We
have used a 100:1 probe to monitor the A1 output of the Triac
(green trace) and the vertical scale stands at 200V/div. The
cycle RMS measurement for this channel shows 218V and the
duty stands at 72%. Also shown is the gate pulse used to turn
on the Triac through an optocoupler (pink trace). The positive
pulse width of the gate turn on is measured to be 140.4us.
20 Silicon Chip
Fig.2: a decoded RS232 stream from a microcontroller as the
B1 trace (purple). The data format is set to 8 bits, no parity
and one stop bit, while the baud rate is set at 9.6Kbps. The
decoded data is shown as a hexadecimal byte (0xE2) and the
triggering occurs on the start bit. Custom baud rates are also
allowed for non-standard systems. The input to the decoder
is shown as the yellow trace, which is channel 1.
forms. You can also inspect the maths
waveforms like any other waveform.
You can use a maths waveform to
estimate the power consumption of a
circuit or integrate a waveform to estimate the brightness of a light source
driven in switchmode.
Fig.5 shows the result of measuring
the output of a Triac in switchmode.
Making measurements
All the usual measurements of a
waveform can be made: RMS, frequency and peak-to-peak voltage etc.
You can also capture a “snapshot” of
a waveform. In this case, all measurements will be taken simultaneously.
Fig.6: the OpenChoice PC software supplied free-of-charge
with the oscilloscopes in this series. It allows you to record
your work with the oscilloscope and store important settings.
Interface with the oscilloscope is via the USB port (connecting
cable supplied). Other software is also supplied.
siliconchip.com.au
Fig.3: the event table associated with the serial stream shown
in Fig.2. The single byte of data is shown in the table and the
time relative to the trigger point (155.6us) chronicles the activity
on the channel. The event table can be exported to a computer
for storage or further analysis either by saving to the on board
non-volatile memory and transferring later to a PC or by saving
to a USB flash disk connected to the host port on the front.
You can also customise an automatic measurement. For example,
gating is the name given to restricting
measurements on a waveform to a
specific portion. With gating enabled,
you can restrict the chosen measurement to within the visible screen area
or to within the area designated by
cursors.
Measurement indicators can be
turned on and switched off. This allows you to see on the display the
actual part of the waveform that the
displayed measurement corresponds
to. It can be considered a kind of automatically set cursor.
Cursors can also be used for manual
measurements on stored or real time
waveforms, including the output of
the MATHs function.
Connections & software
The DPO3034 has all the connections you would expect as standard: a
built in ethernet port, USB 2.0 device
and host ports and video output for
connecting an external monitor.
A variety of PC software is supplied
with the scope. OpenChoice software
shown in Fig.6 allows you to save
screen grabs and settings. The settings
can then be recalled at a later time.
There is also data logging software
supplied, NI LabView SignalExpress
which allows you to remotely control
the oscilloscope using an ethernet,
USB or GPIB port. You can, for example, obtain a live waveform display
from the oscilloscope through your
network, and by extension, through a
siliconchip.com.au
Fig.4: the MATHs function (red trace at top of screen) used
to compute the gain-bandwidth product of an amplifier. The
input is a sinewave at around 3kHz and 1.5V RMS (yellow
trace). The gain is computed by dividing the amplitude of
the output (cyan trace) by the input. We then multiply this
by the real time measurement of the input frequency. The
measured mean of the result is around 38,900.
range of inter-networks.
NI LabView SignalExpress software
can also produce statistical reports
including histograms and can be used
for limit testing.
Limit testing refers to the procedure
for measuring the limit-cases (ie,
the maximum and minimum levels)
and is useful for rating a design and
ascertaining the best and worst cases
for operation. For example, what’s the
absolute maximum current drawn and
power dissipated by a circuit?
Conclusion
The DPO3034 is a serious oscilloscope with an impressive list of features and an excellent user interface.
We have very few negative things to
say about this oscilloscope. The user
interface sometimes is slow to respond
to changes in settings. However, this
only occurs at certain points in the
menus and does not affect the waveform display when running.
The Auto Set feature can take up to
five seconds which is slow compared
to other oscilloscopes. However, it
is still much shorter than if you had
to change all the relevant settings
manually.
On the other hand, the user interface
of the DPO3034 and what you can do
with it is among the best we have seen
in comparably priced oscilloscopes.
The general MATHs features are
powerful. The ability to make automatic and custom measurements and
to search, zoom in on and play back
waveforms makes this oscilloscope a
desirable debugging tool. It has an attractive screen and many connection
options as standard.
The DPO3034 is supplied with four
500MHz passive probes, manuals
and NI LabView SignalExpress and
Open Choice PC software. The price
of this particular model is $9832.00
(ex GST).
Other oscilloscopes in this Tektronix range are priced from $5680 (2
channels, 100MHz) to $13960.00 (4
channels, 500MHz).
The optional modules are priced at
$1265.00 (I2C/SPI decoding and triggering), $1265.00 (CAN/LIN decoding
and triggering), $1265.00 (RS232C/
RS422/485 decoding and triggering)
and $799.00 (HD TV decoding and
triggering).
It can be purchased from Tekmark
Australia, Suite 302, 18 Orion Rd Lane
Cove, NSW 2066. Phone: (02) 9911
3888 or visit www.tekmark.net.au SC
A NOTE TO
SILICON
CHIP
SUBSCRIBERS
Your magazine address sheet shows when
your current subscription expires.
Check it out to see how many you still have.
If your magazine has not turned up by the
first week of the month, contact us at
silchip<at>siliconchip.com.au
August 2008 21
SILICON
CHIP
If you are seeing a blank page here, it is
more than likely that it contained advertising
which is now out of date and the advertiser
has requested that the page be removed to
prevent misunderstandings.
Please feel free to visit the advertiser’s website:
dicksmith.com.au
SILICON
CHIP
If you are seeing a blank page here, it is
more than likely that it contained advertising
which is now out of date and the advertiser
has requested that the page be removed to
prevent misunderstandings.
Please feel free to visit the advertiser’s website:
dicksmith.com.au
Ultra-LD Mk.2 200W
Power Amplifier
A new class-AB
design with
ThermalTrak
Power Transistors
This new amplifier module supersedes both the Plastic Power
module described in the April 1996 issue and the Ultra-LD module
presented in the March 2000 issue. It produces high power at
very low distortion. In fact, as far as we are aware, it is the lowest
distortion class-AB amplifier that has ever been published.
Pt.1: By LEO SIMPSON & JOHN CLARKE
24 Silicon Chip
siliconchip.com.au
Specifications & Performance
Output Power: 200 watts RMS into 4W; 135 watts RMS into 8W
Frequency Response at 1W: -3dB at 4Hz, -1dB at 50kHz (see Fig.4)
Input Sensitivity: 1.26V RMS for 135W into 8W
Input Impedance: ~12kW
Rated Harmonic Distortion: < .008% from 20Hz to 20kHz for 8W operation;
typically < .001% (see Figs.5-8)
Signal-to-Noise Ratio: 122dB unweighted with respect to 135W into 8W
(22Hz to 22kHz)
Damping Factor: <170 with respect to 8W at 100Hz; <50 at 10kHz
Stability: Unconditional
T
HE ULTRA-LD MK.2 AMPLIFIER
Module uses the new On Semiconductor ThermalTrak power transistors
in a circuit which is largely based on
our high-performance Class-A amplifier which was featured in SILICON CHIP
during 2007. The ThermalTrak transistors are a new version of the premium
MJL3281A & MJL1302A and have an
integral diode for bias compensation.
As a result, the circuit has no need
for a quiescent current adjustment or
a “Vbe multiplier” transistor.
This is also our first amplifier module to use a double-sided PC board.
Ostensibly, there is no reason to
use a double-sided board for a
relatively simple circuit such
as this, especially as our previous single-sided amplifier
boards have had few links.
In fact, we have used the doublesided design to refine and simplify
the external wiring to the PC board
which has been arranged to largely
cancel the magnetic fields produced
by the asymmetric currents drawn by
each half of the class-B output stage.
We provide more detail on this aspect
later in this article.
Power output of the new module
is on a par with the above-mentioned
Plastic Power module and significantly more than the original Ultra-LD
module. As well, it uses a considerably
simpler power supply than the UltraLD module.
Power output is 135 watts RMS into
an 8-ohm load and 200 watts into a
4-ohm load for a typical harmonic
distortion of less than .001%. The
new module also has slightly higher
gain than the Ultra-LD module but
siliconchip.com.au
Design Features
•
•
•
•
Very Low Distortion
No adjustment for quiescent
current required
Double-sided PC board
simplifies wiring
PC board topology cancels
class-B induced magnetic
fields
still manages to produce an improved
signal-to-noise ratio of -122dB (unweighted) with respect to 135W into
8W. This is extremely quiet.
A look at the accompanying performance panel and the performance
graphs will show that this is a truly
exceptional amplifier, bettered only
by the Class-A amplifier described
during 2007. In fact, some of the distortion figures we have obtained are so
low, around .0007% for operation into
8-ohm loads, that we were amazed. We
had expected this Class-AB amplifier
to be better than anything we had
published before – but not this good!
Circuit description
Fig.1 shows the full circuit of the
new amplifier. As already mentioned,
the front end of the circuit (ie, all except the output stages) is based on the
Class-A amplifier published in May
2007 and subsequent issues. While the
general configuration was designed to
optimise performance of the Class-A
design, it provides similar benefits
to Class-AB operation, such as low
residual noise and excellent power
supply rejection ratio (PSRR).
We have already mentioned that
there is no need for a “Vbe amplifier”
stage and no quiescent current adjustment. Also the complementary-feedback pair (CFP) power output stage of
the original Ultra-LD module has been
discarded in favour of a more conventional complementary-symmetry
Darlington emitter follower stage.
So let’s go through the circuit in
detail. The input signal is coupled via
a 47mF non-polarised (NP) electrolytic
capacitor and 100W resistor to the base
of transistor Q1. This is one of the
input differential pair (ie, Q1 & Q2)
using Toshiba 2SA970 PNP low-noise
transistors which are responsible for
the very low residual noise of the
amplifier. The 100W input resistor and
820pF capacitor constitute a low-pass
filter with a -6dB/octave rolloff above
1.9MHz.
This is a much lower impedance
network than our previous designs, in
order to provide the lowest impedance
for the signal source.
Both the bias resistor for Q1 and the
series feedback resistor to the base of
Q2 are set at 12kW (instead of 18kW
in the original Ultra-LD and Plastic
Power designs), again to minimise
source impedance and thereby, Johnson noise.
The gain of the amplifier is set by the
ratio of the 12kW and 510W feedback
resistors to a value of 24.5, while the
low-frequency rolloff (-3dB) of the
gain is set by the 220mF capacitor to
1.4Hz.
Feedback capacitors
Some readers may wonder why we
used such large electrolytic capacitors
in the input and feedback networks.
The answer is that we are acting to
eliminate any effects of capacitor
distortion in the audio pass-band
and as noted above, to minimise the
source impedance “seen” by the input
transistors.
To explain this point, consider that
the typical source impedance of a DVD
or CD player is only a few hundred
ohms. If we use a much smaller input
capacitor, say 2.2mF, its impedance
will be 1447W at 50Hz. This will only
have a small effect on the frequency
response but represents a very large
increase in the source impedance
“seen” by the input stage. By contrast,
the 47mF input capacitor will have an
impedance of only 67W.
August 2008 25
26 Silicon Chip
siliconchip.com.au
210mV
Q3
BC546
A
K
E
C
820pF
D1, D2: 1N4148
12k
B
B
E
C
100nF
B
Q1, Q2:
2SA970
68
C
E
E
C
A
K
68
A
D1
470 F
63V
210mV
Q4
BC546
D2
B
100
47 F
35V
2.2k
K
B
2.2k
B
12k
B
B
Q8
BC639
E
C
E
K
K
A
A
K
K
A
A
Q7
BF470
Q9
BF469
C
C
E
47
2SA970, BC639
E
C
22k
100nF
2.2k
54.3V
220 F
16V
510
6.2k
6.2k
B
100pF
100V
C
E
ULTRA-LD MK.2 200W AMPLIFIER MODULE
10
1M
100
6.8k
1W
B
47 F
35V
2.2V
B
C
B
C
B
7-10
mV
Q14
NJL1302D
0.1 7-10
5W mV
E
B
Q13
NJL3281D
FUSE1
5A
C
E
B
C
FUSE2
5A
Q15
NJL1302D
B
0.1 7-10
5W mV
E
C
BF469, BF470
Q11
MJE15031
C
E
100
7-10
mV
B
Q12
NJL3281D
100
E
C
10 1W
B
B
Q10
MJE15030
BC546, BC556
54V
100
DQ15
DQ14
DQ13
DQ12
E
54V
100
100nF
100nF
E
1000 F
63V
C
B
E
390
1W
–55V
(NOM.)
0V
SPEAKER
OUT
PHONES
OUT
CA
K
NJL3281D, NJL1302D
1000 F
63V
150nF
400V
6.8 1W
L1 6.8 H
MJE15030,
MJE15031
100nF
0.1
5W
0.1
5W
C
E
E
C
+55V
(NOM.)
Fig.1: the circuit employs the new ThermalTrak power transistors from On Semiconductor. These have an integral diode which is used to control the quiescent
in the Class-B output stage. The four diodes are shown separately on this circuit (ie, DQ12, DQ13, DQ14 & DQ15) for clarity but are actually integral with the
output transistors which have five connecting leads instead of three. Note that the various voltages marked on the circuit will vary according to the supply rails.
2008
SC
COM
SIGNAL
IN
47 F NP
C
100
43V
Q5
BC556
E
100
Q6
BC556
Parts List
1 double-sided PC board, code
01108081, 135 x 115mm
1 heatsink, 200L x 75mmH x
46Dmm
4 M205 PC-mount fuse clips
(F1,F2)
2 5A M205 fast-blow fuses
1 6.8mH air-cored inductor (L1) (or
1 20mm OD x 10mm ID x 8mm
bobbin and 1.5m length of 1mm
enamelled copper wire)
2 3-way PC-mount screw terminals,
5.08mm spacing (Altronics P
2033A) (CON2, CON3)
1 2-way PC-mount screw
terminals with 5.08mm
spacing (Altronics P 2032A)
(CON1-CON3)
2 TO-220 mini heatsinks, 19 x 19
x 9.5mm
2 TO-220 silicone insulating
washers
4 TO-264 ThermalTrak silicone
insulating washers
2 transistor insulating bushes
4 M3 tapped x 9mm standoffs
6 M3 x 20mm screws
2 M3 x 10mm screws
Readers might also wonder why we
have not used a non-polarised (NP)
electrolytic for the 220mF capacitor in
the feedback network since this is normally preferable where the capacitor’s
operating voltage is extremely low.
The answer is that an NP electrolytic
could have been used except for its
greater bulk and we wanted to minimise any extraneous signal pickup
which could happen with a physically
larger capacitor.
Extraneous signal pickup is one of
the unwanted side-effects of a much
wider frequency response – the amplifier is more prone to EMI and in
the extreme case, to supersonic oscillation, if the wiring details are not
duplicated exactly.
Diodes D1 & D2 are included across
the 220mF feedback capacitor as insurance against possible damage if
the amplifier suffers a fault which
pegs the output to the -55V rail. In
this circumstance, the loudspeakers
would be protected against damage
by a loudspeaker protection module
(such as that published in the July
2007 issue of SILICON CHIP) but the
siliconchip.com.au
8 M3 x 6mm screws
8-M3 nuts
Semiconductors
2 2SA970 PNP transistors (Q1,
Q2)
2 BC546 NPN transistors (Q3,Q4)
2 BC556 PNP transistors (Q5,Q6)
1 BC639 NPN transistor (Q8)
1 BF470 PNP transistor (Q7)
1 BF469 NPN transistor (Q9)
1 MJE15030 NPN transistor
(Q10)
1 MJE15031 PNP transistor
(Q11)
2 NJL3281D NPN ThermalTrak
transistors (Q12,Q13)
2 NJL13020D PNP ThermalTrak
transistors (Q14,Q15)
2 1N4148 switching diodes
(D1,D2)
Capacitors
2 1000mF 63V PC electrolytic
1 470mF 63V PC electrolytic
1 220mF 16V PC electrolytic
2 47mF 35V PC electrolytic
1 47mF NP electrolytic
220mF capacitor would be left to suffer
reverse current.
Note that we have used two diodes
here instead of one, to ensure that there
is no distortion due to the non-linear
effects of a single diode junction at
the maximum feedback signal level
of about 1V peak.
Voltage amplifier stage
Most of the voltage gain of the amplifier is provided by Q9 which is fed via
emitter follower Q8 from the collector
of Q1. The emitter follower transistor
is a BC639 which has higher ratings
than the BC546 used for this function
in the Class-A amplifier. It is used to
buffer the collector of Q1, to minimise
non-linearity.
Q9 is operated without an emitter resistor to maximise gain and its
output voltage swing. We need to
maximise voltage swing from the voltage amplifier stage in order to obtain
the maximum power output from the
output stages.
The collector loads for Q1 & Q2 are
provided by current mirror transistors
Q3 & Q4. Similarly, the collector load
1 150nF 400V MKT polyester
5 100nF 63V MKT polyester
1 820pF ceramic
1 100pF 100V ceramic (eg,
Altronics R 2882)
Resistors (0.25W, 1%)
1 1MW
8 100W
2 12kW
2 68W
1 22kW
1 47W
1 6.8kW 1W
1 6.8W 1W
2 6.2kW
1 10W
3 2.2kW
1 10W 1W
1 510W
4 0.1W 5W
1 390W 1W
2 0W
2 68W 5W (for testing)
Transistor Quality
To ensure published performance,
the 2SA970 low-noise transistors
(Q1 & Q2) must be from Toshiba.
Be wary of counterfeit parts, as
reported by us in the past.
All other transistors should be from
reputable manufacturers, such as
Philips (NXP Semiconductors), On
Semiconductor and ST Microelectronics. This applies particularly to
the MJE15030 & MJE15031 output
driver transistors.
for Q9 is provided by a constant current load comprising transistors Q6 &
Q7. Interestingly, the base bias voltage
for constant current source Q5 is also
set by Q6. Q5 is the constant current
“tail” for the input differential pair and
it sets the collector current through
these transistors.
The reason for the rather complicated bias network for Q5, Q6 and Q7
is to produce a major improvement
in the power supply rejection ratio
(PSRR) of the amplifier. Similarly,
the PSRR is improved by the bypass
filter network consisting of the 10W
1W resistor and 470mF 63V capacitor
in the negative supply rail.
Why is PSRR so important? Because
this amplifier runs in class-B, it pulls
large asymmetric currents which can
be 9A peak or more, from the positive
and negative supply rails.
Let’s explain this. When the positive
half of the output stage (Q12 & Q13)
conducts, the DC current drawn is effectively the positive half-wave of the
signal waveform, ie, rectification takes
place. Similarly, when the negative
half of the output stage (Q14 & Q15)
August 2008 27
+Vcc
CURRENT
SOURCE
Q10
Q13
Q12
DQ12
DQ13
0.1
0.1
0.1
0.1
2.2V
DQ14
DQ15
Q14
Q9
Q15
Q11
–Vcc
Fig.2: this schematic demonstrates how the four integrated diodes of the
output transistors set the quiescent operating conditions of the Darlington
emitter follower output stage. Note that the voltage drop across each diode
is quite low at round 0.55V.
conducts, the DC current is the negative half wave of the signal.
So we have half-wave rectification
ripple of the signal superimposed on
the supply rails, as well as the 100Hz
ripple from the power supply itself.
And while the PSRR of an amplifier
can be very high at low frequencies, it
is always poorer at the high frequencies. So what happens is that these
nasty ripple voltages inevitably get
into the earlier stages of the amplifier
and cause distortion. Which is why
we need to keep these ripple voltages
to a minimum.
That is why we employed separate
regulated high-voltage supply rails
for the original Ultra-LD amplifier.
However, the extra filtering we employed in the Class-A amplifier (using
techniques suggested by Douglas Self)
now performs much the same function in this new Class-AB amplifier
module so that we can dispense with
the regulated supplies.
The scope grab on page 30 in this
article gives a graphic demonstration
of the signal rectification phenomenon
we have just described. The centre
(yellow) trace shows a 1kHz sinewave
output signal from the amplifier at
100W into an 8-ohm load. The top
(red) trace shows the ripple on the
positive supply.
28 Silicon Chip
Note the large 100Hz sawtooth
component which is ripple from the
power supply. Superimposed on this
is the half-wave rectified signal frequency at 1kHz. The bottom (blue)
trace shows the same process on the
negative supply rail.
The 100pF capacitor between the
collector of Q9 and the base of Q8
sets the open-loop bandwidth of the
amplifier. Since it is subject to the full
output voltage swing of the voltage
amplifier stage, it must have a rating
of 100V or more.
Output stage
The output signal from the voltage
amplifier stage Q9 is coupled to driver
transistors Q10 and Q11 via 100W
resistors. These protect Q7 and Q9
in the event of a short circuit to the
WARNING!
High DC voltages (ie, ±55V) are present on this amplifier module when
power is applied. In particular, note
that there is 110V DC between
the two supply rails. Do not touch
the supply wiring (including the
fuseholders) when the amplifier is
operating, otherwise you could get
a lethal shock.
amplifier output which could possibly
blow these transistors before the fuses
blow. The 100W resistors also have a
secondary function in acting as “stopper” resistors to help prevent parasitic
oscillation in the output stage.
As already mentioned, the output
stage uses complementary Darlington
transistor pairs rather than the complementary feedback pairs (CFP) used
in the previous Ultra-LD module and
the Class-A modules. There are two
reasons for this approach. First, we are
using the highly linear ThermalTrak
output transistors with their integral
bias compensation diodes. To take
advantage of these diodes we need to
employ Darlington emitter followers,
as will be explained in a moment.
Second, a CFP output stage does not
give good current sharing between the
paralleled output transistors and we
wanted this in order to make this new
Ultra-LD Mk.2 suitable for delivering
full power into 4-ohm loads.
Bias compensation
With four Thermaltrak power transistors used in the output stage, we
have four integrated diodes available
for bias compensation. As shown on
the circuit, the four diodes are connected in series between the collector
of Q7 and the collector of Q9. Some
readers may be aware that this arrangement, together with an adjustable series resistor, was a common method for
setting the output quiescent current,
before the “Vbe multiplier” became
the standard method over 30 years ago.
Now for a given bias setting in any
Class-B amplifier, the base-emitter
voltage in the output transistors will
drop with a rising temperature. So as
the output transistors heat up, they
draw more current which makes them
hotter and soon you have “thermal
runaway” and eventual transistor
destruction.
Since the bias setting for the output
stage transistors is set by the voltage
drop across the four integrated diodes,
there is little chance of thermal runaway. Not only are the diodes matched
to the base-emitter junctions of the
transistors, they are also on the same
die (chip) so the tracking between the
two is very close.
This is a great advantage over a Vbe
multiplier transistor mounted on the
heatsink because the latter arrangement inevitably has a considerable
thermal lag which can be as much as
siliconchip.com.au
MJE15030 MJE15031
BF470
L1
6.8 1W
10 1W
100pF
100V
12k
6.8 H
390 1W
BF469
Q9
6.2k
NJL1302D
18080110 FUSE 2 (5A)
reifilpmA 2.KM DL-artlU
0.1 5W
100
100nF
Q7
2.2k
1000 F 63V
Q5,Q6: BC556
2.2k
Q5 Q6
100nF
100nF
6.8k 1W
100
100
100
47 F
35V
47 F
47
0.1 5W
0.1 5W
FUSE 1 (5A)
6.2k
100nF
Q15
NJL1302D
Q11
Q10
1000 F 63V
Q14
0.1 5W
NJL3281D
100
Q13
NJL3281D
2.2k
Q12
2 x 2SA970
0
510
0
12k
1M
47 F
NP
820pF 220 F
10
D1
4148
4148
D2
Q8
Q3 Q4
CON2
BC639
2 x BC546
470 F 63V
100nF
150nF 400V
100
68
100
Q1 Q2
68
100
CON3
SPEAKER +
SPEAKER –
PHONES OUT
22k
CON1
SIG COM
+55V 0V –55V
Fig.3: the PC board parts layout of the new amplifier module. The double-sided design allows
much better cancellation of magnetic fields due to the asymmetric currents in the output stage.
30 minutes (depending on the size of
the heatsink).
With the Thermaltrak transistors, we
don’t have to worry about thermal lag
or runaway. The quiescent current settles quickly at switch-on. Thereafter, it
can drift about, depending on the supply voltage and signal conditions but
it will always come back to the initial
“no-signal” value. On Semiconductor
also claim that the harmonic distortion
of the amplifier is lower than it would
be with a Vbe multiplier stage.
Fig.2 shows the method of setting
the output quiescent current. As depicted here, the four integrated diodes
compensate for the four base-emitter
junctions which control the quiescent
current in the output stage. These are
the two base-emitter junctions in the
driver stages (Q10 & Q11) and the two
paralleled base-emitter junctions of
the four output transistors (Q12, Q13
& Q14, Q15).
The quiescent current is set by the
difference in voltage drops between
the aforementioned base-emitter juncsiliconchip.com.au
tions and the four diodes and this
voltage difference appears across the
0.1W emitter resistors of the output.
Typically, the voltage across the emitter resistors will be around 7-10mV,
giving a quiescent current of around
70-100mA for each transistor; somewhat higher than we would have set
with a Vbe multiplier.
Output RLC filter
The remaining circuit feature to be
discussed is the output RLC filter, comprising a 6.8mH air-cored choke, a 6.8W
resistor and a 150nF capacitor. This
output filter was originally produced
by Neville Thiele and is still the most
effective output filter for isolating the
amplifier from any large capacitive reactances in the load, thereby ensuring
unconditional stability. It also helps
attenuate any RF signals picked up by
the loudspeaker leads and stops them
being fed back to the early stages of the
amplifier where they could cause RF
breakthrough.
Note that if the amplifier is intended
for an application that requires continuous high-power output at frequencies of 10kHz or more, then the 6.8W
resistor will need to be a 5W or 10W
wirewound resistor.
Fuse protection
The output stages are fed via 5A fuses
from the ±55V rails. These provide the
only protection to the amplifier against
short-circuits or other failures which
could cause high current drain. Note that
we recommend the use of a loudspeaker
protector such as the one described in
the July 2007 issue of SILICON CHIP.
Double-sided PC board
As already noted, a double-sided PC
board is used to simplify the power
supply wiring. The general layout of
the PC board is very similar to that
used in the SC480 amplifier featured
in the January & February 2003 issues
which was itself a refinement of the
layout used in the original Ultra-LD
module. As such, the PC board has
two important features.
August 2008 29
Audio Precision
Frequency Response 8 Ohm (1W) 07/04/08 08:03:15
Fig.4: frequency response at 1W into 8 ohms. While the
minimum frequency shown here is 10Hz, the response
extends well below that to around -3dB at 4Hz.
First, it has “star earthing” whereby
all earth (0V) currents come back to
a central point on the board, thereby
avoiding the possibility of output, supply and filter bypass currents flowing
in the sensitive signal earth return
conductors.
More importantly, the placement of
Audio Precision THD vs Power 8 Ohm
Fig.5: total harmonic distortion versus power at 1kHz into
to an 8-ohm resistive load. Maximum power at the point of
clipping is 135W.
heavy copper supply and earth tracks
on the board is arranged to cancel
the magnetic fields produced by the
asymmetric currents drawn by each
half of the output stage. In the aforementioned amplifiers, we arranged
this cancellation by having the main
supply leads to the module lie closely
This scope grab gives a graphic demonstration of the signal rectification
phenomenon in the Class-B output stage. The centre (yellow) trace shows a
1kHz sinewave output signal from the amplifier at 100W into an 8-ohm load.
The top (red) trace shows the ripple on the positive supply. Note the large 100Hz
sawtooth component which is ripple from the power supply. Superimposed on
this is the half-wave rectified signal frequency at 1kHz. The bottom (blue) trace
shows the same process on the negative supply rail.
30 Silicon Chip
07/04/08 10:48:58
underneath the respective tracks on
the PC board. While this arrangement
works well, if it is to be effective it
depends on the constructor following
the wiring diagram very closely.
The PC board layout is shown in
Fig.3.
To visualise how the field cancellation occurs, consider how the positive
rail fuse (Fuse1) is placed close and
parallel to the emitter resistors for Q12
& Q13. So the magnetic field produced
by the half-wave currents in Fuse1 are
more or less cancelled by the same current flowing back through the emitter
resistors. The same mechanism applies
with Fuse2 in the negative rail and the
emitter resistors for Q14 & Q15.
Now consider the two heavy tracks
which carry the positive and negative
supply rails from the connector CON2
up the centre of the PC board and then
diverge at rightangles to the two fuses,
Fuse1 & Fuse2. Directly under the
diverging supply tracks are the tracks
which connect the pairs of emitter
resistors together to connect them to
the output via the RLC filter. Almost
complete magnetic field cancellation
takes place because of this track arrangement.
Finally, the main earth (0V) return
track to CON2, underneath the board,
cancels the magnetic field produced by
the main supply tracks running on the
top centre of the board.
By the way, merely twisting the positive and negative supply wires of a classB amplifier together gives no magnetic
siliconchip.com.au
Audio Precision THD vs Power 4 Ohm
07/04/08 08:54:09
Fig.6: total harmonic distortion versus power at 1kHz into
a 4-ohm resistive load. Maximum power at the point of
clipping is 200W.
field cancellation at all in the absence of the return earth.
Why? Simply because the positive half-wave currents do not
occur at the same time as the negative half-wave currents.
To sum up, the Class-B magnetic field cancellation technique employed is important because it greatly reduces
the overall harmonic distortion of the amplifier. In the
SC480 module, it produced good results from ordinary
power transistors. In this design, with a double-sided PC
board complementing the new very linear ThermalTrak
power transistors and special filtering of the supply rails,
the results are very much better.
Finally, we need to clear up a few points. At various
times we have referred to this amplifier as operating in
class-B and in class-AB. Strictly speaking, the amplifier
operates in class-AB, ie, a mixture of class-A which means
that a constant current flows in the output stage and class-B
which refers to the separate operation of the positive and
negative sections of the output stage.
Audio Precision THD+N vs FREQ 8 Ohm (100W)
07/04/08 08:24:27
Fig.7: total harmonic distortion versus frequency into an
8-ohm resistive load. This is measured with a bandwidth
of 10Hz to 80kHz.
Audio Precision THD+N vs FREQ 4 Ohm (100W)
07/04/08 08:40:33
Coming next month
Next month, we will describe the assembly of the module
and give the test procedure. We’ll also describe a suitable
SC
power supply.
Fig.8: total harmonic distortion versus frequency at 100W
into to a 4-ohm resistive load, measured with a bandwidth
of 10Hz to 80kHz.
into MOTORS/CONTROL?
Electric Motors and
Drives – by Austin Hughes
Fills the gap between textbooks and
handbooks. Intended for nonspecialist users; explores all of the
widely-used motor types.
$
60
Practical Variable
Speed Drives
– by Malcolm Barnes
An essential reference for engineers
and anyone who wishes to
or use variable
$
105 design
speed drives.
AC Machines – by Jim Lowe
Applicable to Australian trade-level
courses including NE10, NE12 and
parts of NE30. Covers all types of
AC motors.
$
66
DVD Players and
Drives – by KF Ibrahim
DVD technology and applications with
emphasis on design, maintenance
and repair. Iideal for engineers, technicians, students, instal$
95 lation and sales staff.
There’s something to suit every
microcontroller
motor/control master
maestroininthe
the
SILICON CHIP reference bookshop:
see the bookshop pages in this issue
Performance Electronics
for Cars – from SILICON CHIP
16 specialised projects to make your
car really perform, including engine
modifiers and controllers,
$
80 instruments and timers.
19
Switching Power
Supplies – by Sanjaya Maniktala
Theoretical and practical aspects of
controlling EMI in switching power
supplies. Includes bonus CD$
ROM.
115
! Audio ! RF ! Digital ! Analog ! TV ! Video ! Power Control ! Motors ! Robots ! Drives ! Op Amps ! Satellite
siliconchip.com.au
August 2008 31
By JIM ROWE
A low-cost, easy-to-build
Planet Jupiter Receiver
How would you like to try some basic radio astronomy – listening
to the bursts of noise originating from the planet Jupiter, or from
the Sun? You don’t need a lot of fancy equipment to do this,
just the simple shortwave receiver described here. It’s hooked
up to a basic dipole antenna (which we describe as well) and
to the sound card in your PC, so that you can print out “chart
recordings” of the noise signals.
M
ENTION THE TERM “radio astronomy” to most people, and
they’ll either look completely blank
or visualise huge arrays of steerable
dish antennas – like the one at Narrabri in NSW. Of course, a lot of radio
astronomy is done nowadays using
these big arrays or huge ‘valley sized’
32 Silicon Chip
antennas like the one at Aricebo in
Puerto Rico. But it’s still possible to do
interesting observations using much
simpler antennas and equipment, at
“decametric” frequencies (8-30MHz)
in the HF radio band.
In fact, a NASA-sponsored project
called “Radio Jove” has been promot-
ing this type of radio astronomy for the
last 10 years as a science project for
high-school students and interested
hobbyists. Over 1000 simple receiver
kits have been sold, for 20.1MHz reception of noise bursts from the planet
Jupiter, the Sun and other objects in
the Milky Way galaxy.
siliconchip.com.au
There’s only one problem with the
US-designed Radio Jove receiver as far
as Australian students and hobbyists
have been concerned: the receiver kits
cost US$155 each plus shipping from
the USA, so it will set you back about
A$200 to have one sent over here. This
has discouraged more than a handful
of people in Australia from getting into
radio astronomy.
To encourage more Australian
students and hobbyists to have a go,
SILICON CHIP has developed its own
low-cost receiver project. And that’s
the background to the new receiver
described in this article. You’ll find
its basic specifications summarised
in the “Main Features” panel but the
bottom line is that it’s quite suitable
for basic radio astronomy at decametric frequencies around 21MHz. This
makes it fine for receiving noise bursts
from Jupiter, the Sun or other sources
in the Milky Way.
We estimate that it will cost you
around $75 for the basic receiver
module, plus $7.30 if you decide to
house it in an ABS instrument box. In
other words, less than half the cost of
the Radio Jove receiver. We also think
it is a much better design, by the way.
How it works
The complete circuit for the receiver
is shown in Fig.1. The heart of the
circuit is IC1, an SA605D single-chip
receiver IC which includes a local
oscillator, an RF mixer, a high-gain
IF amplifier and an IF limiting amplifier, plus a quadrature detector for FM
signal demodulation.
We are not using the last of these
sections here, because we’re using the
SA605 in a slightly unusual way – for
AM signal demodulation. We do this
by taking advantage of the chip’s RSSI
(received signal strength indicator)
output from pin 7.
This works because associated with
the high-gain IF amplifier and limiter
stages inside the SA605 are a number
of signal level detectors, whose outputs are combined to provide a DC output current from pin 7. This DC output
current is logarithmically proportional
to the incoming signal strength, so it
is essentially an AM detector output.
We convert it into a voltage signal by
passing the current through a 91kW
load resistor, shunted by a 470pF capacitor for low-pass filtering.
The centre intermediate frequency
(IF) of the receiver is set at 5.5MHz
siliconchip.com.au
The parts for the Jupiter Receiver are all mounted on a double-sided PC
board. The top groundplane pattern is necessary to ensure stability.
using ceramic filters CF1 and CF2.
These require no alignment. The local
oscillator circuit inside IC1 is brought
out to pins 3 & 4, to which we connect
frequency determining components
L3 and VC3, together with 22pF
and 39pF capacitors. Together, these
components allow the local oscillator
to be tuned manually over the range
from 25.75-28.0MHz, which is 5.5MHz
above the input signal range of interest
(20.25-22.5MHz).
The use of a 5.5MHz IF means that
the receiver’s image frequency will be
11MHz above the wanted frequency
– giving a good image rejection ratio.
The input of IC1’s mixer stage is
tuned to the centre of the wanted
frequency band (ie, about 21MHz) by
means of inductor L2 and trimmer
Main Features
The receiver is a single-conversion superhet design tuning from about 20.2522.5MHz, with a sensitivity of approximately 1mV for a 10dB signal-to-noise
ratio. Only three controls are provided: RF gain, tuning and audio gain.
All components are mounted directly on a small PC board measuring only
117 x 102mm, which can either be used “naked” or housed in a standard
low-profile ABS instrument case (140 x 110 x 35mm).
The receiver can be powered from either a 12V battery or a mains plugpack
supply delivering between 15-18V DC. The current drain is typically between
55-75mA.
There are two audio outputs from the receiver: (1) a line output suitable for
connection to the line-level input of a PC sound card and (2) a low-impedance
output capable of driving external headphones or a small 8W speaker. Both
outputs can be used at the same time.
August 2008 33
Parts List
1 PC board, code 06108081, 117
x 102mm (double sided, with
plated-through holes)
1 plastic case, 140 x 110 x 35mm
(optional)
2 Murata 5.5MHz ceramic filters
(CF1, CF2)
3 mini RF coil formers (Jaycar LF1227) for L1-L3
1 300m length of 0.25mm
enamelled copper wire
1 47mH RF choke (RFC1)
1 68mH RF choke (RFC2)
2 trimmer capacitors, 6.3-30pF
(green) (VC1, VC2)
1 miniature tuning capacitor with
edgewise knob (VC3) (Jaycar
RV-5728)
1 50kW 16mm PC-mount linear
pot (VR1)
1 50kW PC-mount 16mm log pot
(VR2)
2 16mm-diameter control knobs
1 8-pin DIL socket (for IC2)
2 PC-mount RCA sockets (CON1,
CON2)
1 PC-mount 3.5mm stereo jack
(CON3)
1 PC-mount 2.5mm concentric
DC socket (CON4)
1 TO-220/6093B heatsink
4 M3 x 10mm tapped spacers
5 M3 x 6mm machine screws
5 M3 nuts (two used as spacers
for VC1)
2 M2.5 x 5mm machine screws
(for VC1)
1 15 x 7mm copper sheet or
tinplate (for IC1 shield)
1 14 x 10mm copper sheet or
tinplate (for Q1 shield)
1 3.5mm mono jack plug to
3.5mm mono jack plug audio
cable
Semiconductors
1 SA605D single-chip receiver IC
(IC1)
capacitor VC2. The ‘Q’ of this circuit
is fairly low, so that the receiver’s sensitivity is reasonably constant over the
2MHz wide tuning band. As a result
tuning is achieved purely by adjusting
the local oscillator frequency.
Although the SA605 IC does provide
a great deal of gain in the IF amplifier
and limiter sections, we have included
34 Silicon Chip
1 LM358 dual op amp (IC2)
1 LM386 audio amplifier (IC3)
1 7812 +12V 3-terminal regulator
(REG1)
1 78L05 +5V 3-terminal regulator
(REG2)
1 BF998 dual-gate Mosfet (Q1)
1 PN100 NPN transistor (Q2)
1 3mm green LED (LED1)
1 3mm red LED (LED2)
1 1N4004 diode (D1)
1 16V 1W zener diode (optional)
Capacitors
1 2200mF 16V RB electrolytic
1 470mF 25V RB electrolytic
1 330mF 16V RB electrolytic
1 22mF 16V tag tantalum
4 10mF 16V RB electrolytic
1 470nF MKT metallised polyester
8 100nF monolithic ceramic
1 47nF MKT metallised polyester
6 10nF monolithic ceramic
7 2.2nF disc ceramic
1 470pF disc ceramic
2 39pF NPO disc ceramic
1 22pF NPO disc ceramic
2 18pF NPO disc ceramic
Resistors (0.25W 1%)
2 220kW
2 1.5kW
1 150kW
5 1kW
1 110kW
1 820W
1 100kW
1 360W
1 91kW
1 300W
2 47kW
1 220W
1 22kW
1 100W
1 10kW
1 47W
1 2.2kW
2 10W
1 1.8kW
Antenna Parts
1 UB5 plastic box, 83 x 54 x
31mm
1 35 x 21 x 13mm ferrite toroid
(Jaycar LO-1238)
50-ohm coaxial cable plus RCA
plug for downlead
an RF amplifier stage ahead of the IC to
ensure that the receiver has adequate
sensitivity. As you can see, this RF
stage uses a BF998 dual-gate MOSFET
(Q1), with the second gate (G2) voltage
adjusted via VR1 to allow easy control
of RF gain.
The RF input signal from the antenna enters the receiver via CON1,
and is fed into the input tuned circuit
(L1/VC1) via an impedance matching
tap on inductor L1. As before, the ‘Q’
of this circuit is kept relatively low, so
once it’s tuned to about 21MHz it does
not need to be changed.
From the RSSI output of IC1,
the demodulated audio signals are
passed through op amp IC2a (half of
an LM358) which is connected as a
voltage follower for buffering. They
then pass through a simple low-pass
RC filter (the 1kW resistor and 10nF
capacitor) before being fed to IC2b.
This is the other half of the LM358
and is configured as an audio amplifier with a gain of 5.7 times, as set by
the 47kW and 10kW feedback resistors.
From IC2b, the signals pass through
a 470nF coupling capacitor to VR2,
the volume/audio gain control. They
are then fed through IC3, an LM386N
audio amplifier configured here to
provide a gain of about 40 times. The
amplified audio signals are then coupled via a 330mF output capacitor to
speaker output jack CON3 and also
to line output socket CON2 via a 1kW
isolating resistor.
Notice that the buffered RSSI signal
from the output of IC2a is also fed to
transistor Q2, which is used to drive
LED2, the RSSI/overload indicator.
Because Q2 does not conduct until
the output voltage from IC2a reaches
a level of around +2.65V, this means
that LED1 really only lights when a
very strong signal is being received, ie,
when the receiver is tuned to a shortwave radio transmission or some other
strong terrestrial signal source. So the
main purpose of LED2 is to help you
tune AWAY from such signals, rather
than to them.
Power supply
The receiver’s power supply arrangements are very straightforward.
Most of the circuitry operates from
+12V, which can come directly from
a battery if you wish. In this case
regulator REG1 is not used but instead
replaced by a 10W resistor. The 2200mF
capacitor is also replaced by a 16V
1W zener diode, to protect the circuit
from damage in case of higher-voltage
transients (when the battery is being
charged, for example).
On the other hand, if you wish to
operate the receiver from a 15-18V
DC source such as a mains plugpack
supply (Americans call them ‘wall
warts’), this is very easy to do. In this
siliconchip.com.au
siliconchip.com.au
August 2008 35
S(1)
VC1
6-30pF
2.2nF
150k
D(2)
G1
G2
2x
2.2nF
A
K
470 F
25V
IN
GND
2200 F*
16V
OUT
REG1 7812
A
K
ZD1*
16V
1W
+12V
K
A
B
LED2
RSSI
100k
IN
GND
OUT
REG2 78L05
220
LED1
POWER
2.2k
K
A
E
C
39pF
39pF
91k
220k
10nF
100nF
100nF
8
47k
IC2b
10 F
10k
6
5
8
10
11
470pF
12
100nF
220k
7
RSSI
* ZD1 FITTED IN PLACE OF 2200 F
CAPACITOR WHEN REG1 IS NOT
USED (12V BATTERY OPERATION)
47
100nF
+6V
RFC2
68 H
1k
Vcc
6
+6V
IC1 SA605D
13
100nF
10nF
1k
14
LIM
IN
CF2
5.5MHz
820
17 16
15
IFA
OUT
22 F
TANT
300
5
MUTE
18
IFA
IN
100nF
100nF
19
10nF
1k
10nF
1k
RF
IN2 LCL OSC
B
E
4
3
10nF
2
20
1 RF MXR
IN1 OUT
10nF
L3
1.2 H
Q2
PN100
22pF
2.2nF
VC2
6-30pF
L2
1.8 H
10 F
21MHZ 'PLANET JUPITER' RECEIVER
–
+
D1
1N4004
FIT 10 RESISTOR
WHEN REG1 NOT USED
(12V BATTERY OPERATION)
+12V
TUNING
VC3
10-120pF
360
18pF
2.2nF
100
RFC1
47 H
1.5k
2
3
7
1
C
B
E
PN100
AUDIO
GAIN
VR2
50k
LOG
470nF
100nF
IC2: LM358
4
IC2a
1
6
1
10 F
16V
4
A
K
OUT
LEDS
GND
IN
7812
7
8
5
10 F
16V
1.5k
K
A
K
1N4004
A
ZD1
47nF
16V
10
330 F
1k
8
SPEAKER
OUT
CON3
AUDIO
OUT
TO PC
CON2
CERAMIC FILTERS CF1 AND CF2
ARE MURATA SFSRA5M50BF00-B0
OR SIMILAR
10
CHAMFER
SIDE
OUT
IC3
2 LM386N
3
+12V
NOTCH
20
SA605D
IN
COM
78L05
Fig.1: the circuit is based on an SA605D single-chip receiver IC (IC1) which includes a local oscillator, an RF mixer, a high-gain IF amplifier and an IF limiting
amplifier, plus a quadrature detector for FM signal demodulation. The latter feature is not used here. Instead, the SA605 is used in a slightly unusual way to
obtain AM signal demodulation.
SC
2008
15-18V (OR 12V)
DC INPUT
CON4
S
D
2.2nF
1.8k
Q1
BF998
47k
RF GAIN
2.2nF
110k
VR1
50k
LIN
22k
COIL DETAILS:
L1, L2 & L3 all on Jaycar LF-1227 3mm diameter
mini coil formers using 0.25mm enamelled copper
wire, close wound at bottom of former.
L1: 20 turns with tap at 4 turns from earth end
L2: 20 turns
L3: 15 turns
NOTE: Ferrite slugs and shield cans are NOT used.
18pF
L1
50 1.8 H
RF
INPUT
CON1
G1(4)
G2(3)
BF998
+12V
CF1
5.5MHz
ANTENNA
INPUT
CON4
CON1
LINE OUT
TO PC
SPEAKER
15-18V DC
OR 12V DC
CON2
S
T
R
IC1
SA605D
39pF
2.2nF
VR1
A
LED2
LED1
TUNING
Table 1: Capacitor Codes
36 Silicon Chip
Q2
PN100
VC3
22k
IEC Code
470n
100n
47n
10n
2n2
470p
39p
22p
18p
1k
10nF
RSSI
case, REG1 is fitted to regulate the
supply down to +12V, while a 2200mF
capacitor is also fitted to provide the
necessary filtering.
The only part of the receiver which
does not operate directly from the
+12V line is IC1, which needs a supply
of +6V. This is provided by REG2, a
low-power 5V regulator arranged here
to provide an output of +6V by means
of the 300W/47W resistive divider
across its output.
LED1 is connected to the +12V sup-
mF Code
0.47mF
0.1mF
.047mF
.01mF
.0022mF
NA
NA
NA
NA
470nF
1
1.2 H
RF GAIN
Value
470nF
100nF
47nF
10nF
2.2nF
470pF
39pF
22pF
18pF
10 F
220k
IC2
LM358
L3
50k LIN
1
47
470pF
100nF
10nF
22pF
2.2nF
39pF
6-30pF
1.5k
100nF
+
1
VC2
68 H
RFC2
5.5MHz
100nF 10nF
10nF
+
+
220
2.2k
18pF
CF2
2x100nF
10k
47k
220k
100k
10nF
L2
CF1
100nF
10nF
1k
1.8 H
100nF
C02008
8
02 C
06108081T
B18080160
100nF
820
1.5k
1k
5.5MHz
2.2nF
91k
2.2nF
300
78L05
100
22 F
D
S
10 F
REG2
1k
Q1
1.8k
2.2nF
BF998
47nF
+
10
2200 F
470 F
K
+
47 H
RFC1
G2
G1
D1
10 F
110k
150k
360
2.2nF
47k
1k
330 F
4004
6-30pF
2.2nF
VC1
18pF
A
CON3
A
10 F
Tap
L1
IC3
LM386
1.8 H
A
REG1
7812
EIA Code
474
104
473
103
222
470
39
22
18
POWER
VR2
50k LOG
AUDIO GAIN
ply via a 2.2kW series resistor to provide power indication, while diode D1
is in series with the DC input to protect
against reverse-polarity damage.
Construction
As you can see from the photos, all
of the receiver’s parts are mounted
on a small double-sided PC board
measuring 117 x 102mm and coded
06108081. The board has platedthrough holes incidentally, to ensure
good connections between the copper
on each side – especially in the area
of IC1, where a sound earth plane is
essential for stability.
All the input-output connectors are
mounted along the rear edge of the
board, while the controls and two indicator LEDs are mounted along the front
edge. Note that tuning capacitor VC3
(a standard “mini” tuning gang with
only one section used) is mounted
upside down on the top of the board,
with its edgewise tuning knob fitted
under the board.
Two 3mm nuts are used as standoffs
between the capacitor body and the
Fig.2: install the parts on the
PC board as shown on this
overlay diagram and the
accompanying photo. Make
sure that all polarised parts
are correctly orientated.
top of the board, to bring the knob up
closer to the board. This is important
if you want to fit the receiver into a
low profile instrument case, because
the knob will otherwise interfere with
the bottom of the case.
All the components mount on the
top of the board, including IC1 and Q1
which are both surface-mount devices
or “SMDs”.
Although you need to be especially careful when fitting IC1 and Q1,
building the receiver should be quite
straightforward if you work carefully
and use the board overlay diagram
(Fig.2) and the photos as a guide. Here
is the suggested order of assembly:
(1) Fit connectors CON1-CON4 along
the rear of the board.
(2) Fit all of the resistors, taking
care to fit the correct values in each
position.
(3) Fit the 8-pin socket for IC2, orientating it as shown to guide you in plugging in the IC later. Note that a socket
is not used for IC3, as the LM386N is
more stable when soldered directly
into the board.
siliconchip.com.au
What Is Radio Jove?
Radio Jove is a radio astronomy education project sponsored by NASA – the US
Government’s National Aeronautics and Space Administration. Other organisations
involved in the project are the University of Florida’s Department of Astrophysics,
the University of Hawaii, Kochi National College of Technology, the INSPIRE Project and companies such as Raytheon, RF Associates and Radio-Sky Publishing.
The goal of Radio Jove is to promote science education by observing and analysing radio signals emanating from the planet Jupiter, the Sun and our Milky Way
galaxy. The project is directed primarily at high-school science classes, both
in the USA and internationally, but interested hobbyists and radio amateurs are
welcome to participate.
The Radio Jove project has an office at NASA’s Goddard Space Flight Center and
also has its own website at http://radiojove.gsfc.nasa.gov/
On this site there are a wide range of resources and reference
materials, including observing guides and links to useful secondary sites.
Radio Jove also sells kits for a simple radio receiver suitable
for reception of “decametric” noise signals from Jupiter or the
Sun, around 20.1MHz (14.915m). The kits cost US$155.00
each plus shipping (from Greenbelt in Maryland). An assembly manual for the receiver can be downloaded from
the Radio Jove website, for those interested.
(4) Now fit IC1 and Q1 to the board,
taking the usual precautions with
these SMDs. Use an earthed soldering iron with a fine chisel-shaped tip
(very clean) and hold each device in
position with a wooden toothpick or
similar while you apply a tiny drop
of solder (tack solder) to the diagonal
end pins of the device, to hold it in
position while you solder all of the
remaining pins.
The idea is to make each joint quickly and carefully, using a bare minimum
of solder so you don’t accidentally
bridge between adjoining pins. Also
make sure you orientate Q1 correctly;
this 4-pin device is very tiny but its
source (S) pin is wider than the other
three. Orientate the device so that this
pin is at lower left, and tack-solder
this pin first if possible.
(5) Next fit trimmer capacitors VC1
and VC2, making sure their flat sides
face the centre of the board.
(6) After these, fit all the smaller fixed
capacitors. These are not polarised
Table 2: Resistor Colour Codes
o
o
o
o
o
o
o
o
o
o
o
o
o
o
o
o
o
o
o
o
siliconchip.com.au
No.
2
1
1
1
1
2
1
1
1
1
2
5
1
1
1
1
1
1
1
Value
220kW
150kW
110kW
100kW
91kW
47kW
22kW
10kW
2.2kW
1.8kW
1.5kW
1kW
820W
360W
300W
220W
100W
47W
10W
4-Band Code (1%)
red red yellow brown
brown green yellow brown
brown brown yellow brown
brown black yellow brown
white brown orange brown
yellow violet orange brown
red red orange brown
brown black orange brown
red red red brown
brown grey red brown
brown green red brown
brown black red brown
grey red brown brown
orange blue brown brown
orange black brown brown
red red brown brown
brown black brown brown
yellow violet black brown
brown black black brown
5-Band Code (1%)
red red black orange brown
brown green black orange brown
brown brown black orange brown
brown black black orange brown
white brown black red brown
yellow violet black red brown
red red black red brown
brown black black red brown
red red black brown brown
brown grey black brown brown
brown green black brown brown
brown black black brown brown
grey red black black brown
orange blue black black brown
orange black black black brown
red red black black brown
brown black black black brown
yellow violet black gold brown
brown black black gold brown
August 2008 37
L1
16T
L2
20T
TAP
4T
L3
A
B
15T
A
B
A
B
1. BEFORE WINDING EACH COIL, REMOVE
ENAMEL FROM END OF WIRE (5mm).
THEN TIN AND WRAP IT AROUND
TOP OF ONE PIN (A) ON UNDERSIDE
OF FORMER. THEN SOLDER.
2. THEN WIND WIRE TIGHTLY AROUND
FORMER FROM BOTTOM, WITH
TURNS CLOSELY WOUND.
3. WITH L1, WIND 4 TURNS THEN
LOOP OUT AND TWIST AS
SHOWN TO MAKE 'TAP'. THEN
WIND REMAINING TURNS.
4. WHEN ALL TURNS HAVE BEEN
WOUND, CUT WIRE ABOUT 13mm
FROM END OF LAST TURN. THEN
REMOVE ENAMEL FROM LAST 5mm
OF WIRE, TIN AND BRING DOWN
TO WRAP AROUND TOP OF
SECOND PIN (B) ON UNDERSIDE
OF FORMER. THEN SOLDER.
5. REMOVE ENAMEL FROM OUTER
END OF L1'S TWISTED LOOP 'TAP',
THEN TIN SO IT CAN BE SOLDERED
TO PAD ON PC BOARD WHEN
COIL IS FITTED TO BOARD.
Fig.3: follow these instructions to
wind coils L1-L3.
15 x 7mm RECTANGLE
OF COPPER FOIL OR
TINPLATE ON
TOP OF IC1
WIRES SOLDERED
IN EARTH VIAS
NEAR PIN 1 END
OF IC1
1
SHIELDING PLATE FOR IC1
14 x 10mm RECTANGLE
OF COPPER FOIL OR
TINPLATE OVER CENTRE
LINE OF Q1
S
WIRES SOLDERED TO VIAS
IN Q1 SOURCE COPPER,
AT EACH END OF Q1
VERTICAL SHIELDING PLATE FOR Q1
Fig.4: here’s how to make and fit
the shield plates for IC1 and Q1.
apart from the 22mF tantalum capacitor
which fits between the 1kW and 91kW
resistors, just to the right of IC1. This
capacitor is polarised, so make sure
its positive lead is towards the front
of the board.
(7) Now fit the remaining electrolytic
capacitors, which are again all polarised. The correct orientation of each
electrolytic capacitor is shown clearly
in the overlay diagram.
38 Silicon Chip
These two photos show the shield
plates for IC1 (above) and transistor
Q1 (right). You can make the shield
plates from either copper or tinplate.
(8) Next fit RF chokes RFC1 and RFC2,
which should both be about 2mm
above the PC board.
(9) Now fit the two ceramic filters CF1
and CF2, which are not polarised.
(10) Follow these with transistor Q2,
diode D1, REG2 and LED1 & LED2.
Note that the green LED is used for
LED1 and the red LED for LED2.
LED1 is fitted first, with its leads bent
down by 90° about 8mm from the body.
It’s mounted with its body 6mm above
the board surface. LED2 is then fitted
with its leads bent down about 14mm
from the body and so that it sits about
14mm above the PC board.
(11) Fit REG1, if you are using it, noting
that it is mounted on a small 6093B
type heatsink. The regulator leads are
bent down at 90° 6mm away from the
device itself, so they can pass down
through the matching board holes.
Then the device and its heatsink are
fastened to the board using an M3 x
6mm screw and nut, after which the
leads are soldered to the pads under
the board.
(12) Fit IC3 directly on the board, orientating it carefully as shown in the
overlay diagram.
(13) Next, fit tuning capacitor VC3.
As noted earlier, this fits upside down
on the top of the board at centre front,
with M3 nuts used as standoffs. The
capacitor’s tuning knob must be removed from the spindle before it is
mounted and only refitted once the
capacitor’s leads have been soldered
under the board.
(14) Fit VR1 and VR2 (the RF and audio gain control pots). These first have
their spindles cut to 10mm long and
any burrs removed with a small file.
Then each pot is fitted to the board,
making sure that you fit the linear
(B50k) pot in the VR1 position, and
the log (A50k) pot in the VR2 position. Pass their pins carefully through
the board holes as far as they’ll go
comfortably (ie, without undue strain)
and then solder them to the pads underneath. Then you can fit the control
knobs to the pot spindles.
(15) Wind the three tuning coils L1L3. As you can see from the data box
in Fig.1, all three coils are wound on
3mm diameter mini coil formers (Jaycar LF-1227), using 0.25mm enamelled
copper wire. In each case, the coils
are close-wound at the bottom of the
former, as shown in the small diagram
of Fig.3.
Oscillator coil L3 has 15 turns, while
the other two have 20 turns each. The
difference between L1 and L2 is that L1
has a “tap” four turns from the bottom.
This tap is formed from a loop of the
winding wire, twisted and tinned at
the end so that it can be soldered to the
appropriate pad on the PC board (just
below CON1) when the coil is fitted.
It’s a good idea to apply a small amount
of clear nail varnish to the upper part
of each coil, to hold it in place.
(16) When the three coils are completed, they can be fitted to the board.
When doing so, make sure you orientate each coil so that its “A” pin (connected to the bottom of the coil) mates
with the earthy or “colder” pad on the
board. The board overlay diagram has
a small “A” next to each coil, to guide
you in this regard.
(17) Next, you need to make a couple
of copper shield plates for IC1 and
transistor Q1 to ensure stability. Fig.4
and the photos show how these plates
are made and fitted (note: if you are
unable to obtain copper foil, you can
use tinplate or blank PC board).
Both shields are attached using short
pieces of tinned copper wire which go
into adjacent holes in the PC board.
(18) Finally, plug IC2 (LM358) into its
socket, with its notched end nearer
IC1.
siliconchip.com.au
The PC board fits inside
a standard plastic case
measuring 140 x 110 x
35mm. Note how the two
LEDs are bent forwards, to
go through their holes in
the front panel.
Your Jupiter Receiver board should
now be complete and ready for switchon and set-up.
Set-up
Before applying DC power to the
board via CON4, turn both VR1 and
VR2 to their fully anticlockwise position. Then plug a small loudspeaker
(8W) or a pair of stereo headphones
into CON3, so you’ll be able to monitor the receiver’s operation audibly.
When you then apply power, very little should happen initially apart from
LED1 beginning to glow.
If LED1 doesn’t light, odds are that
you’ve connected the DC supply to
the board with the polarity reversed.
Now try turning VR2 clockwise
slowly. You should begin to hear a
gentle hissing sound in the speaker or
one of the ’phones. If you have a DMM
(digital multimeter), measure the voltage at pin 8 of IC2. It should measure
very close to +12V if you’re using
REG1, or +11.4V if you are powering
the receiver from a 12V battery. Now
measure the voltage at the rear end of
RFC2 (ie, the end nearer REG2) which
should be very close to +6V.
siliconchip.com.au
Finally, measure the voltage at pin 1
of IC2; this should be quite low – a few
tens of millivolts. If you then turn VR1
clockwise, this voltage should steadily
rise due to noise being amplified by
Q1, as its gain is increased. The hissing
sound in the speaker or ’phone should
increase at the same time.
If all is well so far, your receiver is
very likely to be working as it should
and you’ll be ready for setting it up.
This mainly involves adjusting trimmer capacitors VC1 and VC2 so that
the input and output circuits of the
RF stage are tuned to around 21MHz.
The easiest way to do this is if you
have access to an RF oscillator or signal
generator, able to deliver an amplitude
modulated RF signal of 21MHz to the
receiver’s input. The generator’s output is set to a level of about 100mV at
first. Then you should turn up both
VR1 and VR2 to about the centre of
their ranges (‘12 o’clock’), after which
you can slowly turn the knob of tuning capacitor VC3 up from its lowest
setting, until you hear a 400Hz or
1kHz tone (the generator’s modulation signal).
Now fine-tune VC3 carefully back
and forth with your thumb, to achieve
the loudest signal. If the sound becomes too loud or LED2 (the RSSI
indicator) begins glowing, turn down
VR2 and/or VR1 to reduce the gain.
And if the signal is still too loud, try
reducing the output level from the RF
generator.
Once you are sure that the oscillator is correctly tuned for reception at
21MHz, the next step is to carefully
adjust trimmer VC2 with a small alignment tool, to again find the correct
position for maximum signal. You may
again need to reduce the generator’s
output level, to prevent overload when
you do achieve a peak.
Once the correct tuning position for
VC2 has been found, the last step is
to adjust VC1 in the same way. In this
case, you will almost certainly have
to reduce the output level from the
generator to prevent overload.
In fact, by the time the tuning
procedure is finished, the generator’s
output should be wound down to a
mere 1mV or so.
No RF generator
If you don’t have access to an RF
August 2008 39
The antenna should be suspended as high as possible above
the ground with a north-south orientation. This can be done by
taping it to Nylon clothesline rope and running this between
two high fixing points (eg, between a house gable and a mast).
The balun and its connections are made waterproof by housing
it in a UB5 jiffy box – see inset.
generator, you’ll have to delay this tuning operation until you have built the
receiver’s antenna, erected it outside
in a suitable position and connected
it to the receiver’s input so that it can
provide you with some sort of signal
– either a short-wave broadcasting station somewhere in the 20.25-22.5MHz
range or just some atmospheric noise.
More about this shortly, after we’ve
talked about antennas.
Antennas for 21MHz
For reception of noise burst signals
from Jupiter or the Sun in the northern
hemisphere, the Radio Jove people
recommend the use of a twin-dipole
antenna array in which two halfwave dipoles are each aligned in an
east-west direction and spaced about
one half-wave apart, with them both
suspended at least 3.6m above ground.
The outputs of the two dipoles are
combined using a phasing cable arrangement, to tilt the antenna’s main
receiving lobe towards the south –
because currently, Jupiter’s orbit is inclined somewhat south of the equator.
In fact, the “declination” of its highest point (“transit”) in moving over
the sky is about -20° in the Northern
sky (ie, quite low towards the south).
6960mm
35mm OD x 13mm
thick L15 toroid
ONE END OF SECONDARY
CONNECTED TO CENTRE
CONDUCTOR OF COAX,
OTHER END TO SHIELD BRAID
(COAXIAL DOWNLEAD
TO RECEIVER)
CENTRE OF ANTENNA WIRE LOOPED THROUGH TOROID 6 TIMES, TO FORM PRIMARY OF BALUN.
SIX LOOPS OF SAME WIRE PASSED THROUGH TOROID TO FORM SECONDARY WINDING.
FOR BEST RESULTS SUSPEND ANTENNA AS HIGH AS POSSIBLE (>3.6m ABOVE GROUND),
AWAY FROM METAL OBJECTS AND WITH A ROUGHLY NORTH-SOUTH ORIENTATION.
Fig.5: this simple single-dipole antenna can be used with the Jupiter
Receiver to receive Jupiter’s noise bursts. The dipole is cut to a length of
6960mm to make it resonant at close to 21MHz and is coupled to a coaxial
downlead using a simple 1:1 balun made from a ferrite toroid.
40 Silicon Chip
In the southern hemisphere, Jupiter’s orbit is currently much higher
in the sky. In Sydney at the time of
writing, the declination of its transit
point is only slightly north of directly
overhead and it’s predicted to take a
couple of years before it swings significantly north. That’s because the
cyclic period of Jupiter’s declination
is almost 12 years and its southerly
peak was earlier this year.
All this means that for the next
couple of years, in Australia and New
Zealand it should be quite feasible to
use a basic single-dipole antenna for
reception of Jupiter’s noise bursts.
Accordingly, we have produced and
tested the very simple antenna design shown in Fig.5. It consists of a
single length of multi-strand copper
wire (we used one side of a length of
figure-8 speaker cable), cut to a length
of 6960mm (6.96 metres) to make it
resonant at very close to 21MHz.
This antenna should be suspended
at least 3.6m above the ground and
aligned as closely as possible to a
north-south direction. I did this by
taping it to a 6m length of Nylon
clothesline rope, which was then run
between a high point on the gable of
my house and the top of a 3m mast,
attached to the side of a workshop in
the backyard.
To couple signals from the antenna
siliconchip.com.au
to a cable running back to the receiver’s
input, I made up a 1:1 balun (balanced
to unbalanced transformer) using a
small ferrite toroid as shown. This
toroid uses L15 material and is 35mm
in outside diameter, with a thickness
of 13mm (Jaycar LO-1238 or similar).
The centre of the antenna wire itself
is looped through the toroid six times
to form the primary winding of the
balun, while a short length of the same
type of wire is also looped through the
toroid six times to form the secondary
winding.
To make the balun weatherproof and
secure, I housed it in a little UB5 jiffy
box (83 x 54 x 31mm), with the two
ends of the antenna wire brought out
through a 3mm hole on each side near
the top. A BNC socket was then fitted
to the lower end of the box, with the
ends of the balun secondary winding
connected to the socket inside. The
downlead cable was connected to the
socket on the outside, after the box lid
had been screwed on.
The whole thing was then hauled
up on the Nylon rope, as it’s very light
in weight. I used short strips of gaffer
tape to attach the antenna wire and
balun to the rope but Nylon cable ties
would also be suitable.
No-generator tune-up
As mentioned earlier, if you don’t
have access to an RF oscillator or signal generator it’s still possible to tune
up the receiver reasonably well once
you have an antenna to provide it with
some signals in the vicinity of 21MHz.
The way to do this is to connect the
antenna, apply power to the receiver
and set both VR1 and VR2 to their midrange (12 o’clock) positions, so you
can hear a reasonable level of noise.
Now try adjusting tuning control
VC3 very slowly, to see if you can
find a shortwave broadcasting station.
I found a Chinese station at about
21.68MHz, for example – about twothirds of the way up the tuning range.
If you do find a station, leave VC3
set to the position for clearest reception and then try adjusting trimmer
VC2 very slowly and carefully with a
small alignment tool. You should find
a position which gives a peak in the
signal’s reception but you may need to
turn down gain controls VR2 and/or
VR1 to lower the volume and prevent
overload, so you can accurately find
this peak.
Once you are confident that VC2
siliconchip.com.au
Decametric Radio Astronomy
B
ACK IN 1955, US radio astronomers Bernard Burke and Kenneth Franklin
discovered that the planet Jupiter was a strong source of “noise burst”
radio signals in the frequency range between about 8MHz and 40MHz – where
the radio wavelength is in the tens of metres (hence the term “decametric”).
They were using a “Mills Cross” antenna array, by the way, the design of which
had been pioneered by Australian radio astronomer Bernard Mills of CSIRO’s
Division of Radiophysics. The first Mills Cross had been built at Fleurs (about
40km west-south-west of Sydney) the previous year.
It was soon discovered that the Sun itself is also a source of noise bursts during periods of sunspot activity and “coronal mass ejections” (CMEs). These
solar noise bursts extend from the decametric range up to around 80MHz.
The relative ease of receiving noise bursts from Jupiter and the Sun in the
decametric frequency range using low-cost equipment seems to be why the
Radio Jove project selected this range (rather than in the UHF or microwave
regions). It should be noted though that because the signals are broadband
in nature, the specific frequency used to receive the signals is not critical. The
main requirement is to avoid frequencies occupied by international broadcasters and other terrestrial sources of radio signals.
Useful websites
A great deal of useful information on Jovian and Solar decametric radio
astronomy – both theory and practice – can be found on the following
websites:
http://radiojove.gsfc.nasa.gov/
http://ufro1.astro.ufl.edu/dec-contents.htm
http://www.jupiterradio.com/
http://www.radiosky.com/
The last of these sites is the source of the Radio-Skypipe software, which runs
on a Windows PC and allows you to record noise data from a Radio Jove or
similar receiver and print out “chart recordings” of them. There is a freeware
version of the software which can be downloaded from this site.
A useful source of skycharts and information on the rising and setting times
for Jupiter (as well as many other astronomical bodies) in any specific location is: http://www.heavens-above.com/
An Australian site with useful information on solar storms and their effect on
terrestrial radio conditions, etc is: http://www.ips.gov.au/
has been set correctly, leave both VC2
and VC3 with their current settings
and turn your attention to VC1, the
input circuit trimmer. Again it’s a matter of adjusting this very slowly and
carefully until you achieve a signal
peak, turning down VR2 and VR1 if
necessary to prevent overload and
distortion.
What if you can’t find a shortwave
station to help in this tuning-up procedure? That needn’t be a complete
disaster, because if you have a DMM
it’s possible to use a similar procedure
using just the decametric “cosmic
noise” being picked up by the antenna.
To do the tuning up this way, set
your DMM to a low DC voltage range
(say 0-2V) and connect it to the re-
ceiver to monitor the voltage at pin 1
of IC2. Then set tuning capacitor VC3
to the centre of its range and gain pots
VR1 & VR2 to the centre of their ranges
as well. When you apply power to the
receiver, you should get a reading of
100-200mV or so on the DMM, as well
as hearing the received noise in the
speaker or ’phone.
Now try adjusting VC2 slowly, first
in one direction and then the other, to
see if you can increase the DMM reading. Keep turning slowly in that direction, until the meter reading reaches
a peak and then begins to drop again.
Then return to the position where the
reading peaks and leave VC2 in that
position.
If the DMM reading rises above about
August 2008 41
There are just three controls on the front panel: an RF gain control, a tuning thumbwheel and an audio gain
control. The RSSI (received signal strength indicator) LED lights when there is a signal overload (see text).
800mV, lower the RF gain by turning
potentiometer VR1 anticlockwise, to
bring the reading down again to
200mV. This will make it easier to see
the peak reading on the DMM as you
adjust variable capacitor VC2.
After VC2 has been set to produce a
peak in this way, leave it as before and
follow the same procedure with VC1.
Again turn down VR1 if necessary to
prevent the DMM reading from rising
above about 800mV.
Once VC2 and VC1 have been set,
your Radio Jupiter receiver should be
tuned up about as well as possible
without access to a generator.
Fitting it to a case
The PC board is designed to fit inside
a low-profile plastic instrument case
measuring 140 x 110 x 35mm. First, you
will have to drill holes in the front and
rear panels. Figs.9 & 10 show the front
and rear panel artworks and these can be
downloaded from our website, printed
out and used as drilling templates.
The board is secured to the two
corner pillars at the back of the case
using self-tapping screws, while the
front of the board is secured to the
front panel via the pot shafts and their
nuts. Note that the board sits slightly
proud of the front pillars in the case.
Don’t attempt to screw the board down
to these pillars (otherwise the board
could crack).
Testing with Radio-Skypipe
To try out the new receiver and the
Chart Started 11 June 08 by Jim Rowe in Sydney, Australia
Fig.6: this recording chart covers almost the full period (about 11 hours) of Jupiter’s pass on the night of June 11,
2008 but shows very little evidence of signal bursts from Jupiter. Things were quiet around Jupiter that night!
42 Silicon Chip
siliconchip.com.au
siliconchip.com.au
www.siliconchip.com.au
15-18V DC
(OR 12V DC)
ANTENNA
SILICON
CHIP
LINE OUT
TO PC
SPEAKER
TUNING
POWER
POWER
RSSI
RF GAIN
also able to print it out as a pseudostrip chart recording – see Fig.6.
As you can see, the recording covers
almost the full period of Jupiter’s pass
that night (June 11, 2008), because it
rose at about 7pm, reached full transit
at 2:07am and set again at around 9am
the next morning. But the sky was very
overcast that night, so perhaps that’s
why there’s very little evidence of any
bursts of signal from Jupiter. Either
that, or things were pretty quiet around
Jupiter that night.
Looking around for some more
information, I discovered that there
are two different kinds of decametric
noise burst from Jupiter: “L” or long
bursts and “S” or short bursts. Both
seem to be controlled by various factors, including which side of Jupiter is
facing our way at the time and also the
orbital position of Jupiter’s principal
moon, Io.
Sunspot and storm activity on the
Sun also seem to play a role. They affect the way the Sun sends out streams
of charged particles which can spiral
RADIO
JUPITER
basic home-brew dipole antenna described above, I decided to download a
copy of the “Radio-Skypipe” software
which is recommended by the Radio
Jove people. This is a data-logging application which runs under Windows
95/98/NT/2000/XP and can be configured to log data signals via either the
ADC (analog-to-digital converter) in a
standard 16-bit PC sound card or an
external ADC.
There’s a free-download version for
non-commercial and non-government
users and a Pro Edition with extra bells
and whistles available for US$39.95,
for commercial and serious users.
I had no trouble installing the RadioSkypipe software on my old Win98
workshop PC and I was soon using it to
take samples of the Jupiter Receiver’s
audio signal twice every second. I then
left it running so that it would log a
complete pass of Jupiter over the following night.
When I stopped the logging at
7.00am the next morning, I then saved
the log file to the hard disk and was
SILICON
CHIP
Fig.8 (left): the RadioSkypipe software has
lots of logging options,
including start and
logging duration times.
AUDIO GAIN
Fig.7 (above): this
screen grab from the
Radio-Skypipe software
shows a recording chart
of the 21MHz signal for
a 10-minute period.
Fig.9: these artworks can be used as
drilling templates for the case panels.
around in Jupiter’s magnetic field.
So it seems that there probably
wasn’t much happening around Jupiter the night of my first logging run.
The only way to find out is to keep
trying, I guess. How about giving it a
SC
go yourself?
August 2008 43
SERVICEMAN'S LOG
She was just what I’d always fancied
Occasionally, when I am allowed out by
myself, I wander off to the auctions for the
day. I always enjoy the experience but I have
learnt that what you might gain is at the
expense of a day’s lost wages and if you do
buy something, it’s often a pig in a poke with
no guarantees.
I’ve got to admit that I buy a lot of
stuff at auctions. But you can never
have enough stuff and so there I was
recently at another auction, recklessly
bidding for all sorts of ex-government/
ex-university electronic gizmos I
didn’t really need. And that was when
I spied her. She was gorgeous and just
what I had always fancied.
Now before you all get too excited,
“she” was in fact a Gould Classic
6000 4-Channel 200MHz True Trace
Digital Storage Oscilloscope with an
LCD readout. It looked in good order
apart from two gouges on the edges
of the front escutcheon where it may
have been dropped and I was advised
it didn’t work.
That didn’t worry me too much as it
would reflect in the price which it indeed did and I was a very happy bidder
when I walked out with my prize for
only $100! Subsequently, I found out
that these units were made in Ilford,
Essex in the UK about 12 years ago (my
old stomping ground) and at the time
sold for about $5000 plus.
When I got it back to the workshop,
I found that the 2A mains fuse had
blown and a replacement also did the
same immediately. Oh well, she was
never going to be that easy!
Opening the case revealed what
looked like a full-blown computer and
a large complicated power supply unit
which I removed. Obviously, I didn’t
have a circuit diagram but I figured
that this must be similar to an ordinary
computer power supply.
I carefully measured all the components in the primary circuit but
44 Silicon Chip
couldn’t initially find much wrong.
There were no obvious short circuits
and the only components I could possibly find a slight problem with were
TR1 & TR5 (MJE13009), C10 & C11
(100mF 63V), R4 & R5 (22kW 1W) and
the MOV1 & MOV2 varistors across
the two main electrolytic capacitors
(C1 & C2, 680mF 200V). These VDRs
were marked 20N241KJVRXHT and
are not easy to source. I also noted a
3300mF 10V electrolytic capacitor in
the secondary with a domed top, so
this too would require replacement.
I tried tracing out the circuit diagram
of this part of the power supply but
it required removing a lot of components in order to trace the tracks of
the double-sided PC board. Anyway,
I replaced all the above suspect parts
with the best equivalents I could find
but found that the main electros (C1 &
C2) were now getting hot and the fuse
kept blowing.
After further investigation, I removed T3’s FL black lead that was
stretched tightly across transformer
T4. And when I did so, T4 fell out,
severing its remaining leads to the
PC board.
I now realised what had happened.
The oscilloscope had indeed been
dropped and transformer T4 (Part
No. JK9501-01) had broken one of its
primary winding legs.
Well, now that I knew what was
wrong I thought it would be a piece
of cake to get the parts. Initially, I
tried all the usual wholesalers like
WES Components, Farnell and RS
Components, etc without success, so I
Items Covered This Month
•
•
•
•
•
•
•
Gould Classic 6000 4-channel 200MHz True Trace Digital
Storage Oscilloscope
Sony STRDA50ES 120W
tuner-amplifier
Hitachi PMA-300 plasma TV
PanaSound A51 5-channel
amplifier
NEC FS-68V81F TV set
JVC VMZ50DX4 127cm
plasma TV
Holden Vectra
went to the Internet and tried to track
down the English manufacturer. I then
discovered that Gould was now part of
a number of EU conglomerates (Gould
Nicolet, Nicolet and LDS Groups)
around the world. I emailed all of them
but did not get a single reply.
While I was trying to work out what
to do next, I accidently found a label on
the opposite end of the power supply
which said that it was made by a third
party, Ferrus Power of Peterborough
UK, and that the model number of
the power supply was FP250-510/1.
This English company is also part
of another group of companies but
their website advises that they do not
sell spare parts, nor do they provide
circuits. I emailed them and although
they can service the power supply, it
would cost me more than $400 by the
time freight was factored in.
I will now devote my energies to
converting a Chinese-built computer
power supply. If you can’t scrounge
one, these are available new at almost
give-away prices. This oscilloscope
only requires ±5.2V <at> 6A, ±12V <at>
3A and 22V at 2A. Hardly a big deal.
Sony tuner-amplifier
A 1998 Sony STRDA50ES 120W
tuner amplifier was brought in DOA
(dead on arrival). First, I removed
siliconchip.com.au
the covers and checked at least five
cartridge fuses but all were intact. I
then applied power but there were no
lights and no clicking relays – in fact,
absolutely no signs of life.
Looking in on the top righthand
side, there is a small power board
with a relay on it which then feeds
another larger power supply board
(PS) beneath it. The problem looked
to be on the lower board but the access
wasn’t straightforward.
First, I had to remove the upper
board, some covers and loosen the
back panel before I could access the
six screws that hold this PS board. I
then had to unplug all the leads that
go into it before lifting it up towards
the front and pulling it out vertically.
It was so tight that the board had to be
flexed quite bit, so much so that a small
piece broke off at the back.
When I examined the board, I
found that it was cracked in a number of places, possibly due to it being
flexed during removal. As a result,
I resoldered all the copper tracks as
necessary and repaired any cracks in
the fibreglass using superglue. Apart
from that, I could find no other problems with it.
Having completed these repairs, I
reinstalled it very carefully and reconnected all the plugs and sockets. I then
checked it over carefully and reapplied
power and it burst into life.
So fixing the cracks repaired the
fault which meant I wasn’t responsible
for the cracks (at least not for all of
them). But how did this come about?
Well, my theory is that either someone else removed the board before me
siliconchip.com.au
(and damaged it) or the set had been
dropped. But if it had been dropped,
why did this board crack while all the
other boards were undamaged?
The only clue I have is that the top
lid on the lefthand side has a dent in
it. Perhaps the PS board is held in so
tightly by its six screws that a heavy
drop can cause the metalwork
to temporarily distort and
crack the board.
Digital tuners
Recently, we have been
having fun and games with
digital tuners. One was in a
Toshiba TV set whose picture was pixellating on UHF
Channels 9 and 90. By contrast,
analog reception on this set was
perfect on all channels.
The problem was due to the
automatic scan that picked up
and stored four Channel 9s – UHF
Ch9, UHF Ch90, VHF Ch9 and VHF
Ch90. However, it puts in the UHF
stations first (ie, ahead of the VHF
stations) and it was the UHF channels
that were pixellating.
You can fix this by selecting the best
stations and making them favourites
but it is a nuisance. One way is to
disconnect the aerial for the first half
of the scan (ie, while it scans the UHF
channels) and then replace it for the
second part (ie, for the VHF channel
scan). The set will then only tune in
the VHF stations and skip the UHF
channels.
There has also been a tuning problem with JVC digital tuners which,
fortunately, is easily fixed. Actually,
the problem isn’t just confined to JVC
but to several other brands manufactured by the same factory in China
as well.
To tune in, you select the Quick
Search Menu and then the location (eg,
NSW). The tuner then starts scanning
August 2008 45
Serviceman’s Log – continued
a design fault or one that happened
with normal wear and tear. Either the
unit had been struck by lightning or
more likely, the client had plugged
something pretty dangerous into a line
input to cause such a major failure.
Unfortunately, due to lack of evidence, the manufacturer had to wear
the cost of this gross neglect. The
dealer was annoyed too because he
had to swap the unit over when the
part had to be ordered, so as not to
inconvenience the idiot customer.
Talking of idiots
for stations but may come back with
the message “Cannot Find Stations”.
We changed the Digital Tuner Board
(DTU) which sometimes fixed the
problem temporarily but it wasn’t until
we got five returns from Victoria that
we worked out what was happening.
Initially, we traced the problem to
the EEPROM but it wasn’t until we
reset it every time before searching
for stations that we realised there was
no automatic overwriting facility for
stored channels. So if the unit had
been tuned into Victorian channels, for
example, there was insufficient space
left to tune in NSW stations.
Hopefully, the manufacturers will
fix this soon. In the meantime, you
have to do a full factory reset from the
menu each time before rescanning.
Hitachi PMA-300 plasma
An Hitachi PMA-300 plasma set
came in with a vertical green venetian
blind affect on the lefthand half of the
screen. Initially, we thought it was the
control panel but in fact, it was the
y-drive upper and lower boards that
were short circuit on the output (pins
7-14).These measured 0.4W instead
of 1.8MW.
These boards are cheaper to buy
from LG, who actually make them.
46 Silicon Chip
In the course of all this, the picture
decided to fail and a “y-sus” kit consisting of three boards from LG had to
be installed as well.
ParraSound 5-ch amplifier
We had a ParraSound 5-channel
Amplifier A51 come in under warranty from a dealer. The set would not
turn on but it wasn’t the on/off switch
that was at fault, as some people think
when a set won’t start.
This set has a complex protection
circuit involving no less than five
relays. The unit is packed with electronic circuitry and the main power
supply unit is mounted underneath
which make access difficult.
After a lot of intemperate language,
I found that a +15V rail was missing
due to a burnt out 15V IC regulator on
this bottom board. This was replaced
and the board reinstalled but when the
unit was switched on, it immediately
started to cook again.
Obviously, there was a short somewhere on the +15V rail and this turned
out to be on the input preamp board.
In fact, there were dead shorts on the
three control ICs mounted on it. A new
board was ordered and fitted, which
fixed the fault.
It was fairly obvious this was not
Talking of idiots, I was called out
to a supposedly dead NEC FS-68V81F
TV set.
When I arrived, I could see that the
set was in standby with the red LED
on. I asked for the set’s remote control
and was first passed the video’s remote
followed by the Foxtel remote.
While he was looking for the original TV remote control he swore blind
he never used, I pushed the front
control buttons on the front of the
set. One of them switched the set on,
much to my client’s disbelief and my
annoyance. He had been using the
master on/off switch only and was
then using the remotes to select the
source of entertainment he wanted.
A power cut or surge had meant
that the set had switched to Standby
and so using the master switch only
made no difference. Like most modern
TVs, this set uses an on/off system that
remembers how it was last switched
off. So if it is switched off in Standby
mode, it will come back on in Standby.
Similarly, if it is switched off when
fully on, it will switch back on fully
on. This sequence had been broken
at one stage – it was just a matter of
switching it on again.
It’s all in the instruction book and
is dead simple if you have the remote.
And yes, I had asked him about all this
over the phone before I called.
The PC & the plasma TV
I was recently called out to a bowling club that wanted to connect a
computer to their plasma TV. Apparently, they had connected it correctly
but were getting nothing.
I arrived to find that the TV was a
Panasonic TH50 PX600A Viera plasma
set which had been connected via 15pin VGA socket to an Acer notebook.
I found that the notebook PC had to
be told to use an external display by
siliconchip.com.au
pressing the Function plus F5 keys,
so that both the internal and external
displays could be used together. This
then gave a distorted image on the
plasma set but after going into the
TV PC Setup menu and setting it for
WXGA and Horizontal and Vertical
Sync, I got a perfect picture.
Back at the computer I messed with
the resolution and set it to 1024 x 768
resolution and 32-bit colour. I was a bit
confused with the choice of multiple
monitors but an Intel 830M Graphics
was the driver chosen. This gave an
excellent picture so I chose to leave
well alone (if you set the resolution too
high, you can often lose the picture).
JVC VMZ50DX4 plasma TV
We had a JVC VMZ50DX4 127cm
plasma (also made by LG) come into
the workshop with its accompanying
Multi Media Box. This set would start
to turn on but then turn off again.
A few quick voltage checks showed
that neither the 65V rail nor the 180V
rail were coming out of the power
supply unit to feed the y-sus board.
Disconnecting this board restored
these supply rails but the real cause of
the problem turned out to be a short on
the z-sus board which plugs directly
into the y-sus board.
The z-sus board is actually quite
a bit cheaper from LG ($233 + GST)
than it is from JVC but we could not
match the exact part number. The z-sus
board in the JVC was 6871QZH043B
and the nearest LG part numbers were
6871QZH041B, 042B or 043B. However close examination of these boards
showed the only difference to be one
of the main electrolytic capacitors (C5)
which wasn’t fitted. Instead, the other
three in parallel are increased in value
from 330mF to 680mF.
In the end, we ordered the LG board
and simply added the extra electrolytic
capacitor from the faulty board, just in
case! The set worked well after that.
The faulty Vectra
This story is about an electrical
problem in a Holden Vectra and
was sent in by D. S. from Howard in
Queensland. Here’s how he tells it:
I read the story about the Falcon
XE electrical problems in the service-
man’s section of the March
2008 issue with more then
a little joviality. It reminded
me of my days on the tools
as an automotive electrician
and one of the many tales of
woe which arose from those
everyday jobs which pay the
bills.
The vehicle was a 2001
Holden Vectra with pretty
much every conceivable
labour-saving device fitted.
When turned on, the dashboard display has a small monitor-type display
which informs of low fluid levels or
inactive globes, etc and the instrument
cluster also lights up with all the relevant warning lights. It’s quite a dazzling sight until the self-test routine is
complete, at which point the displays
dissolve into darkness and the everpresent economy readings.
The initial fault was that the “SRS
Airbag” warning light had illuminated
and the SRS system had disabled. This
is usually an easy fault to fix. Most
problems are caused either by one of
the accelerometers becoming detached
(or damaged) or by the clock spring
mechanism in the steering column.
Plugging in the mandatory system
scanner revealed a mixed hash of
fault codes, none of which bore any
direct relationship to the SRS systems!
Maybe the SRS control module had
suffered damage or had a logic fault?
Subsequent testing revealed that this
was not the case.
As this stage, I then began getting
other fault reports, like a brake-lamp
globe not working. The traction control
WE USE INNOVATIVE METHODS THAT ENABLE OUR CLIENTS TO
ACCELERATE THE PRODUCTION OF PROTOTYPES AND UNIQUE PRODUCTS
•
•
•
•
Rapid Prototyping
3D Cad Design
Toolmaking
Fused Deposition Modelling (FDM)
30 Paradise St, Banyo Queensland 4014
sales<at>3dprinting.com.au
Ph: + 61 7 3267 8104
Fax: + 61 7 3267 8971
www.3dprinting.com.au
siliconchip.com.au
•
•
•
•
24 Bit Colour 3 Dimensional Printing
Direct Casting Moulds
Investment Casting Patterns
Flexible Elastomeric Printed Parts
•
•
•
•
Snap Fit Parts
Urethane Moulding
Vacuum Metallising
Superex
REDUCE DEVELOPMENT COSTS
AND
ACCELERATE SPEED TO MARKET
Australian Agent ZCorp 3D Printers
The World’s Fastest AND Most Cost Effective
Rapid Prototyping System
August 2008 47
Serviceman’s Log – continued
An auto-electrician’s lot – there’s lots of wiring in modern cars and tracking
down a fault in this wiring can be a real nightmare.
warning lamp also came on, although
the traction control was not actually
outputting any actual fault codes.
Furthermore, a quick check of the
brake lamps showed that they were
working OK.
The next fault to show was an ABS
(anti-lock braking) fault. Now the ABS
system is tied into both the SRS and
traction control systems, so maybe we
were now getting somewhere. Again,
the control modules were tested and
again no fault was found. The modules
were all functioning perfectly.
Next, I removed and tested each
individual component and again, I
found no faults. The wheel sensors
were perfect and the accelerometers
were correct and in calibration. The
rear globes were even removed and
their individual resistances checked!
It was time to get tough.
My next step was to start checking
the wiring harness. Unfortunately
though, this isn’t an easy job as the
harness mostly sits inside the interior
trim in it’s own recess and is secured
using cable ties. The interior trim is
also like a big jigsaw puzzle and you
have to remove it in the correct order
to prevent damage.
For example, to remove the centre
console, you first have to remove the
trim around the radio, then unplug
the wiring harness to the switches
mounted in this trim, then unscrew
48 Silicon Chip
and remove the radio. This then allows
you to detach and remove the lower
section of the radio console, giving
access to the screws which hold the
gear lever cover in place.
Once you remove the gear lever covers, you can then remove the remaining screws and trim from the centre
console, detach the wiring harness to
the window switches and then remove
the console!
Once all this had all been done,
it gave me access to one of the SRS
modules and allowed me to check the
wiring. However, on testing, I found
that I had several conductors which
were outputting my trace tones! This
was promising and it was looking
like there were shorted conductors.
Another test on the harness behind the
glove box gave the same symptoms.
Locating the shorts
Now all I had to do was locate the
shorted cables in an enclosed wiring
harness, with an average of 60 conductors in each harness section, Easy!
Eventually, I did locate the damage
to the wiring harness although it took
a little time. However, getting the
harness to a point were it could be
repaired took a lot longer.
The damage was located above the
steering column, between the column
cradle and the firewall. Getting at it
required the removal of the entire
dashboard, dashpad and instrument
cluster, along with the steering column, etc. The accompanying photo
shows the amount of disassembly
required to gain access to this harness.
The damage was caused by the loss
of the protective wrapping between the
harness and the metal of the column
cradle and the firewall. The metal had
rubbed through the cable insulation
and caused shorts between various
conductors and to ground (ie, to the
vehicle’s body).
Many of the wiring circuits must
be protected by current limiting in
the modules, as a short to ground
on a supply circuit usually results
in blown fuses and fireworks! Many
damaged conductors did show signs
of heat damage and carbonisation due
to arcing and part of the harness which
connected the dashboard diagnostic
display to the body control module
was badly burnt. However, the modules showed no signs of damage!
A replacement harness would not
have been any easier and would have
been expensive, so I decided to repair
the existing harness. That repair was
completed in a couple of hours and the
vehicle was reassembled and passed
all its functional tests with flying colours! Luckily, none of the fibre-optic
cables had suffered damage and neither had any of the shielded cables.
When it comes to automotive electronics, we are always quick to blame
the computers for any faults and issues. However, they are really very
reliable and in this case, it was the
cables that were at fault.
Modern on-board diagnostics are
also reliable but can cause confusion
if not interpreted correctly. After all,
diagnostic outputs are only accurate
when the input signals are accurate
and if those same signals become corrupted or mixed, so do the electronic
control module diagnostics.
The vehicle has now been performing flawlessly for several months
without problems. However, this job
serves as a reminder that not all faults
are simple ones or are located in the
electronic modules and that finding the problem and gaining access
to it can sometimes take a lot more
time then the actual repair. Some are
caused by simple components like the
wiring, which we all take for granted.
Others are caused by even simpler
components, like the owner or driver
SC
but that’s another story!
siliconchip.com.au
August 2008
NEW HEAVY DUTY TV
WALL BRACKETS
Capable of taking up to 80kg, these heavy-duty
LCD or plasma TV brackets will save valuable floor
space and keep your investment out of reach of
mischievous fingers.
Two types are available:
• CW-2822 has a 30° range
of tilt movement only
• CW-2824 is able to tilt 30°
& swivel left & right through 80°
and extend up to 30cm away from the wall.
Note: TV not included
$
89 95
$
Cat: CW-2822
149 95
Cat: CW-2824
LABORATORY
MAGNIFIER LAMP
This desktop magnifier
lamp features a 100mm
glass lens that will
provide you with
3x magnification.The lamp
has a solid base and a bright 12W energysaving fluorescent lamp.
The lamp also
features a swivel
$
joint enabling you to
95
position the lens to
Cat:
QM-3529
suit your needs.
FAST BATTERY
CHARGER
Recharge up to four AA or AAA Ni-Cd or
Ni-MH batteries with this handy charger
that utilises Delta V voltage detection to
ensure maximum battery life. Integrated
LCD status display. Charge on the go
with the included car cigarette lighter
cord or with the included mains
plugpack.
$
95
• Charge time varies
to battery's capacity.
Cat: MB-3549
CW-2824
$
CW-2822
99 95
Cat: XC-0338
PURE SINE WAVE
INVERTERS
HIGH CURRENT MOTOR
SPEED CONTROLLER KIT
Ref: Silicon Chip Magazine March 2008
This kit will control a 12 or 24VDC motor at up to 40A
continuous and features automatic soft-start,
fast switch-off and a 4-digit display to
show settings.
From
$199
180 WATT MI-5160 • Power surge 300W
• Weighs 1kg • 240(L) x 119(W) x 60(D)mm $199.00
380 WATT MI-5162 • Power surge 650W
• Weighs 1.1kg • 240(L)x119(W) x 60(D)mm $229.00
600 WATT MI-5164 • Power surge 1000W
• Weighs 1.4kgs • 300(L) x 119(W) x 60(D)mm $349.00
Speed regulation is maintained even under heavy loads
and the system includes an overload warning buzzer
and a low battery alarm.
• Kit contains PCB and all
$
95
specified electronic components.
79
Cat: KC-5465
STEREO VALVE AMPLIFIER
2 X 25WRMS
39
40W SOLDERING
STATION
STOCK
Keep track of important weather parameters like wind
speed and rainfall. It also has a calendar and a clock
with alarm function. In addition, it measures indoor and
outdoor temperature and humidity.
• Wind speed in km/h or mph
• Max min and rainfall history
in mm or inches
• Temperature in Celsius or Fahrenheit
• Requires 2 x AA & 2 x AAA batteries
• Display: 180(H) x 104(W) x 24(D)mm
*Parts shown not to scale
These inverters provide clean
230VAC power to run sensitive
electronic equipment
such as clocks, TVs,
electronic scales, etc.
from your car's battery.
We have models
suitable for running your
laptop in the bush to powering a small
microwave in a motor home. They
have fan assisted cooling and
electrical isolation for safety.
39
This temperature
controlled station
comes with a
lightweight iron with
anti-slip grip and tip
cleaning sponge,
with temperature
adjustment up to
450°C. It also has
a 4mm banana
socket connected
to mains earth for
soldering
static-sensitive
components.
NOW IN
WIRELESS DIGITAL RAIN GAUGE
WITH ANEMOMETER
Most valve amps have ridiculously low power
output, no tone controls, hum like a substation and cost ludicrous amounts of
money. Not this one: it has 25WRMS per
channel, tone controls, very low hum and
distortion, sounds pretty damn
good and costs no more than an
equivalent solid state amp.
• Valves: 2 x 6N1, 2 x 6P15
• Power output: 25WRMS per channel
• Input sensitivity: 300mV
• S/N ratio: >80dB • THD: <0.5%
• 270(W) x 290(D) x 140()mm
$
NEW STORE
NOW OPEN IN
LIVERPOOL, NSW.
299
Cat: AA-0474
6-IN-1 COMPACT
$
49 95
Cat: TS-1620
SCREWDRIVER
This innovative screwdriver has
six of the most useful blades. They
are made of a vanadium and
molybdenum alloy and store neatly in the
handle. This may become one of the handiest
tools in your kit. Supplied with the following
$
95
blades. • 128mm long • Slotted: 4, 5, 6mm
• Phillips: #1, #2, #3
Cat: TD-2028
15
Free Call: 1800 022 888 for orders! www.jaycar.com.au
3/381 Macquarie St, 2170.
Ph: (02) 9821 3100
Fax: (02) 9821 3188
1
AUTOMOTIVE
PREVENT DRIVEWAY ACCIDENTS
Advanced Car Alarm
with Pin Code Function
2.4GHz Wireless
Reversing Camera
A full featured car alarm at a bargain price. It features code
hopping remotes, a 2 stage shock sensor, microwave, door and
boot trigger and a 125dB
battery backup siren
and much much more!
It also has a valet
parking or car wash
feature that enables
the system to remain
disarmed, but the door and boot
release will work normally.
Simply splice the monitor
and camera power lines into
the car's reversing light
cable and it will
automatically switch on when
you select reverse gear.
Once activated the camera
and monitor deliver a clear
view of the area behind your
car.
• 2.4" wireless
colour LCD screen
• Colour CMOS camera
• 110° Camera viewing
angle
$
Car Speakers
This new improved range of full range car speakers feature
injection moulded woofer cones and silk dome tweeters for
smooth high-end response. The 3-way models have piezo
mid-range drivers and all have grilles and crossovers
included at a price that won't break the bank.
See in-store or website for speaker measurements.
4" 2 Way
• Power handling 55WRMS
• Freq resp 100Hz - 20kHz
Cat. CS-2385 $29.95 pr
Response UnderSeat Active
Subwoofer
Has a wired remote
control unit with mute
and volume controls.
Line level (RCA) inputs or
speaker signal inputs.
• 130mm polycone woofer
• Power: 90W RMS
• Frequency response: 80 - 200Hz
• 288(L) x 200(W) x 69(H)mm
• While Stocks Last - No Rainchecks
Was $129.95
$5
6 x 9" 4 Way
• Power handling 100WRMS
• Freq resp 45Hz -20kHz
Cat. CS-2388 $59.95 pr
$
109
95
Cat: CS-2273
$
34 95
Cat: CS-2277
• See our Website for full specifications
$
2
Cat: BI-8207
Low Profile Subwoofer
Their huge power handling and cone excursion make these
the ideal subs for people who really want massive SPL in a
compact package. Two models available.
Nominal impedance 4 ohms
10" 250WRMS
Cat. CS-2356 $79.95 ea
12" 350WRMS
Cat. CS-2358 $99.95 ea
From
$
79
95
This kit has all the electrical wire,
speaker cables, connectors,
screws and lugs
required to install
most systems and will
support up to 100W.
See in-store or website
for list of
included parts.
Was $44.95
$10
$
29 95
Cat: QP-2251
Car Noise Filters
Car noise filters or hot line
filters are used to reduce
noise and interference
entering your car stereo
through the power lead.
The car alternator is one of
the most common sources
of problems, and these
essential devices can help
to reduce this. Three sizes
available depending on the
power rating of the affected
amplifier / radio etc.
From
$
AA-3072
AA-3076
AA-3081
13
AA-3072 For basic car stereos
• 63 x 31mm • 5 Amp
$13.00
AA-3076 For medium car stereos
• 78 x 60 x 46mm • 20 Amp $22.50
AA-3081 Effective against 'engine hum' & 'ticking
• 75 x 40 mm • 40 Amp
$29.95
Audio Wiring Kit
Installing A Sound
System In Your Car
149
Cat: LA-9008
This handy test unit makes it so
easy to measure current on
individual circuits. Simply
plugs into any standard blade
type fuseholder and provides an
easy-to-read LCD of the
circuit's performance.
• Measures up to 20A.
$20
Literaly feel the bass! Works like a speaker,
but instead of a cone it has a steel
mass that transmits a jolt of energy
to give an interactive feel to your
home cinema or sound system.
Use single or multiple units to give
bass a
new meaning.
Was $39.95
6" 3 Way
• Power handling 85WRMS
• Freq resp 65Hz - 20kHz
Cat. CS-2387 $49.95 pr
$
Auto Current Tester
Bass Shaker 4 Ohm 25WRMS
5" 2 Way
• Power handling 70WRMS
• Freq resp 80Hz -20kHz
Cat. CS-2386 $39.95 pr
2
269
Cat: QC-3721
CAR AUDIO
This essential book thoroughly
covers all areas of installation
including , but not limited to,
amplifier configurations, speaker
placement, second batteries, DC
cable selection, cable resistance
and speaker box venting.
• A4 8 pages
BONUS SPARE 9
REMOTE LA-900
VALUE $34.95
In-Dash Multimedia Player
$
34 95
Cat: AA-0440
3 Channel Video Distribution
Amplifier for Cars
This one-to-three video amplifier is ideal for automotive use
and will let you share the video signal from your in-car video
or DVD system with back seat passengers or other screens
in the car.
• Composite video input
and output
• One input to three outputs
• Works with all in-car
video screens
• 12 volt powered
• Female RCA I/O connectors
• Dimensions: 63(L) x 32(W) x 30(H)mm
Cat: QC-3436
• Lead length: 200mm
$
29 95
This excellent unit will play DVDs, VCDs, MP3s, CDs, and
AM/FM radio. The built-in 3" TFT screen doubles as a
control panel when listening to MP3s etc. It also has an
auxiliary audio input for external MP3 or tape player etc.
The player fits a standard DIN slot and has a detachable
face and can be operated by the included remote.
Mounting hardware included.
• Resolution 500TV lines
• 2 x video inputs
• 1 x camera input
• 45W RMS per channel
• Frequency response:
20Hz - 20kHz
$
349
Cat: QM-3787
Great Audio
Deals In-store!
Free Call: 1800 022 888 for orders! www.jaycar.com.au
COMPUTER PRODUCTS
External 3.5" HDD Cases
for IDE or SATA Drives
Add gigabytes of storage to your
PC or move large files from
work station to work
station with ease.
This HDD case is
made from strong
aluminium and will
accommodate a 3.5" hard drive. It
has a USB 2.0 interface, fan cooling and an independent
power switch. Supplied with pullback, software and USB
interface lead. • Size: 117(W) x 183(D) x 50(H)mm
Two types available:
For IDE drives From
• Silver Cat. XC-4664 $49.95
$
95
For SATA drives
• Black Cat. XC-4666 $59.95
49
1000 Mbps PCI Network Card
Upgrade your home or work computers to
blazingly fast gigabit speeds.
Transferring large amounts of
data can bring
the common
100 Mbps
network to a
$
crawl. This 1000 Mpbs Ethernet
card will you give you the bandwidth
you need to quickly move large files.
Cat: YN-8063
Combined Keyboard, Mouse
and Monitor lead to provide a
neat connection between your
computer and PS/2 Switchbox
or KVM.
$
19 95
Cat: WC-7570
USB Wireless Rechargeable
Optical Mouse
The pack contains a retractable
USB charger to keep your
mouse batteries topped up and
the optical mouse has 400dpi
resolution.
Cat: YN-8066
Common specifications:
• IEEE 802.11g wireless
network compatible.
Interoperation with
IEEE 802.11b 11Mbps networks.
• 64 / 128 Bit WEP encryption.
• 54Mbps high speed transfer rate.
• 40 - 100m indoor range.
• 100 - 300m outdoor range.
• Low power consumption. • Plug & Play
• Compatible with Win98SE/2000/ME/XP
PCMCIA Wireless Network Adaptor
Cat. YN-8068
PCI Wireless
Network Adaptor
Cat. YN-8066
$
WHILE STOCKS
LAST NO
RAINCHECKS
$
Cat: XM-5132
USB Roll Up Keyboard
$
19
95
Cat: XC-5148
$20
$
79
Cat: XC-4668
Cat: YN-8068
34 95
Lightning Protector
The video splitter takes the
computer's video signal and
sends it to two analogue
monitors. The same image is
displayed on both monitors.
The splitter provides fast,
flexible solutions for test bench facilities,
data centres or video broadcasting such as remote
monitoring, presentations, education and stock quotes etc.
Supports VGA, SVGA, XVGA and Multi-Sync.
Includes mains power adaptor.
• Input DB15HD Male
• Outputs DB15HD Female
• 350 MHz video bandwidth
• Max. resolution 2048 x 1536
<at> 60Hz
• 72(W) x 43(H) x 121(L)mm
Cat: YN-8098
$
79 95
KVM switches allow you to
use one keyboard,
mouse and monitor
to control several
computers. These
switches are designed to
allow IT administrators to control
servers, which don't require their
own monitor or keyboard etc but are
just as suited to the power user who has more than one
computer on their desk.
$
• Integrated cables on the PC side
• Max Resolution: 2048 x 1536 pixels
Cat: YN-8095
• Video Bandwidth: 400MHz
59
COMPUTER SECURITY
Hard Drive Enclosure with
Fingerprint Security
29 95
Cat: YN-8067
2 Port Automatic KVM Switch
29 95
Portable hard drives allow easy
mobile data storage but can
make confidential
information vulnerable to
embarrassing disclosure.
This drive case prevents this by
using onboard fingerprint recognition &
encryption software to secure the
data on the drive. 125mm long. USB
powered. Hard drive not included.
Was $99
34 95
Two Port Video Splitter
95
Keyboard, Mouse, Monitor Lead
for PS/2 Switchbox or KVM
This QWERTY keyboard rolls up for easy
transportation or storage
and is waterproof. You
can spill coffee on it.
Perfect for workshops,
garages, food preparation
areas, and travellers.
• Compatible with Windows
98/2000/Me/XP
$
A range of wireless networking
cards to suit all computers
and provisions.
USB 2.0 Wireless
Network Adaptor
Cat. YN-8067
24
$
WIRELESS NETWORKING
802.11g PCI Wireless
Network Adaptors
PCMCIA Fingerprint ID for Laptops
It slides into the PCMCIA slot in your laptop and
utilises biometric technology to identify authorised
users of the computer.
Mainly intended for laptops,
it can be used on any
computer with a
PCMCIA slot.
• Software included.
• 90(L) x 54(W) x
$
4.8(H)mm
Was $129
$30
99
Designed for 2.4GHz systems. Mount
where the cable enters the building so
if lightning does strike near the
antenna, high voltages will
not be passed through to
your equipment.
Was $69.95
$20
$
WHILE STOCKS
LAST NO
RAINCHECKS
49 95
Cat: AR-3278
Wireless Network Access Point
with 4 Port Router
This router allows
communication with up to four
wireless network computers. It
includes support for WAN, web
based & remote management,
auto detection & configuration
of ISP, built in firewall, and more!
• IEEE 802.11g & IEEE 802.11b
compatible
• Up to 54Mbps data rate
• Static and dynamic routing
• VPN pass through
Was $69.95
$10
$
59 95
Cat: YN-8086
Wireless Networking
Starter Kit (2nd Edition)
This book covers both the MAC and
PC environments and will help you set
up your wireless network like the Pros.
It includes hints on network security
and how to prevent outside attack.
• Soft cover 560 pages
$
49 95
Cat: BP-7100
2.4GHz Parabolic Antenna 24dB Gain
Designed for long term
outdoor use in fixed
locations and is suitable
for all 2.4GHz wireless
networks, both data and
voice transmissions. Also
excellent for 2.4GHz
security surveillance
transmissions.
• Note: Picture may vary
from stocked product.
Cat: XC-4843
Free Call: 1800 022 888 for orders! www.jaycar.com.au
$
149 95
Cat: AR-3276
3
SIGHT & SOUND
LOOKING FOR A PARTY DEAL?
15" Party Speakers
• The big daddy of party sound!
• 15" bass driver
• 120 Watts RMS Power
• Size 740 x 505 x 350mm
Cat. CS-2515 Normally $179.00 each
Buy
2 x CS-2515
& 1 x AA-0478
for only $499
Rack Mount Amplifier
2 x 160WRMS
Features two 1/4" & two line level RCA inputs.
• Separate level controls for each channel
• Clipping & overload protection indicator LEDs
• 3U rack mount
• Power output: 2 x 118WRMS <at> 8 ohms
• 2 x 158WRMS <at> 4ohms
• 480(W) x 135(H) x 247(D)mm
Cat. AA-0478 Normally $249.00
Save $108
Mini Stereo
Resonator Speaker
$
99 95
Cat: AR-1870
This uber-cool gadget turns any flat
surface into a speaker, creating
high quality 360 degree sound.
Great for travellers.
Mains plugpack included.
• Measures: 47(Dia) x 44(H)mm
• Requires 8 x AA batteries for
portable use
*Laptop/mobile phone not included
1950s Styled Music Players
With their 50s styling these music
centres are sure to liven up any
room and keep the party pumpin!
Black and Chrome Cabinet
• CD player with remote control
• AM/FM analogue radio
• 310(W) x 295(D) x 145(H)mm
Was $89.95
Red Cabinet
• Automatic turntable 33 & 45 RPM
• CD player with remote control
• MP3, CD-R & CD-RW compatible
• AM/FM analogue radio
• 315(W) x 290(D) x 165(H)mm
Was $149.95
$
$30
$
59
Cat: GE-4066
$20
129 95
Green Laser Display System
Create a dazzling
atmosphere at
your next
party with
the green
laser
show. The
unit comes fitted
with a microphone that changes the pattern
of the lasers to the beat of the music.
• Mains 240VAC lead
• Inbuilt microphone
• 230(L) x 155 (W) X 60(D)mm
Cat: SL-2935
4
This two
channel system
supports two
separate
microphones.
Each channel
has a separate balanced XLR
output. A single unbalanced (mixed)
line output is also available. The
system includes 2 microphones
and batteries, receiver unit and
plugpack.
$
89 95
Cat: GE-4059
Smart and stylish design that will suit the home or office. It
features a CD player, AM/FM radio, alarm clock, USB port,
full function remote control and an iPod® docking station.
What more could you ask for?
• Recharges iPod® batteries
• Measures 340(L) x 270(D) x 172(H)mm
See website for full details
iPod® not included
199
PARTY LIGHTING & EFFECTS
4 Colour Light Chaser
Simple but effective! When music is playing they
swtich in time with it.
• Uses 240V 60W ES
reflector lamps
• Supplied with a red,
Cat: SL-2942
yellow, green & blue globe
$
Cat: AM-4078
Pro-Swivel Headphones
These great looking pro-style
headphones are ideal for DJs and
other professionals. They feature an
in-line volume control and a unique
ear cup swivel action.
• 32 ohm impedance
• 40mm driver diameter
$
95
• Full range response
• 100 dB sensitivity
Cat: AA-2053
69 95
A great pair of headphones at
a fantastic price! Setup is quick
and easy and the sound clarity
is excellent. The ultra-light
design allows them to
comfortably sit on your head
and you’ll hardly know they're
there.
• Operation distance: up to
15m
• Requires 2 x AA batteries
$
49 95
Cat: AA-2049
18 Watt RMS Stereo PA Amplifier
This simple, low cost 18W per
channel transistor amp is
surprisingly loud! It is
protected from
accidental speaker
wiring shorts and, if
abused will simply
shut down and reset
after it has cooled off. It has
a front panel microphone input,
bass and treble controls as well
as a master volume control.
See our website or catalogue for
full specifications.
$
39 95
Cat: AA-0472
Coloured Theatre Spotlight
This sophisticated LED spotlight uses DMX protocols to
enable remote control of colour and brightness via the
theatrical three pin DMX control interface.
Manual control also available. Made from
lightweight ABS plastic and 240VAC
mains powered. 137mm dia.
$
129 95
Cat: SL-2914
Rave Fog Machine
1 Litre Fog Juice available
separately AF-1212 $11.95
199
Infrared Wireless
Stereo Headphones
Retro CD Player
with iPod® Docking Station
Produces clouds of white fog on
demand by using the wired remote
control. Use with laser light shows,
mirror balls & other party lighting.
• Mains powered
• 70 cubic metres/min fog output
• 800ml fog juice capacity
• 330(L) x 160(W) x 140(H)mm
$
29
Cat: GE-4067
• GE-4069 Spare Stylus
available separately $19.95
299
This handy turntable
is perfect for the
occasional bout of
nostalgia and allows
you to play those old
vinyl records or make
back-up copies in a
convenient digital
format. The turntable
plays singles, EPs,
albums and even your
old 78s.
• 33/45/78 rpm
• 240 volt powered
• Magnetic cartridge
• NAB centre adaptor
• Analogue or digital audio output
$
Cat: GE-4068
$
95
USB
Turntable
Wireless Microphone
UHF Dual Channel
Bubble Machine
$
79 95
Cat: AF-1214
Create instant, continuous bubbles
with this affordable portable bubble
machine! Great special effect for kids
parties, weddings or anything.
• Mains adaptor included.
For best results use Bubble Mania
Liquid (946ml) AB-1222 $6.95
$
29 95
Cat: AB-1220
Free Call: 1800 022 888 for orders! www.jaycar.com.au
SIGHT & SOUND
8 Way Speaker Selector with
Impedance Matching
Tweeters
Perfect to use for general PA
applications where long throw is
required. Has built-in protection
to allow them to handle
400WRMS. At high power levels,
a PTC opens, allowing the
tweeter to continue to play at a
compressed power level.
See our Website for full measurements
$
From
$
Cat
Description
RSN1141 Piezo
CT-1932
RSN1142 Piezo CD Horn CT-1934
14 95
RRP
$14.95
$24.95
HOME THEATRE
High-End
Speakers
Equipped with light
and rigid
Kevlar/Paper
composite yellow cone,
fatigue resistant rubber
surround, a strong CNC
machined magnesium aluminium basket, oversized
Neodymium magnet and high temperature Kapton voice
coil, they have extremely high power handling and long
cone excursion. Also features vented pole piece design for
effective heat transfer and 8 ohm nominal impedance.
• 4" high end speaker
• Power handling: 25WRMS
• Recommended enclosure
ea
volume 5 litres ported
Cat: CW-2151
See our Website for full measurements
Also available:
Cat
RRP
Rec. Enclosure
Size Power
Volume
5" 60WRMS CW-2152 $74.95 8 litres ported
6.5" 60WRMS CW-2154 $89.95 15 litres ported
8" 150WRMS CW-2156 $139.95 25 litres ported
10" 150WRMS CW-2158 $159.95 75 litres ported
$
39
95
Glass Base Speaker Stand
Good stands are essential for
isolating your speakers from
the floor and for optimal
positioning from walls and
furniture. These stands have glass
bases for maximum isolation
and machined heightadjustable carpet spikes for
maximum stability. Gloss black.
Dimensions:
• Base:
pr
278(W) x 300(D) x 12(H)mm
• Speaker base:
Cat: CW-2843
140(W) x 140(D) x 9.5(H)mm
• Column: 280(H) x 78(Dia)mm
Pedestal Speaker Stands also available
Cat. CW-2846 400mm High.
Black in colour.
Sold in pairs for $99
$
69 95
Mini Universal
Speaker Brackets
5.8GHz AV Sender
249
A perfect match for a
multi-room sound system!
Turn on up to 8 pairs of speakers
Cat: AC-1682
without worrying about your amplifier
blowing up. Housed in a rugged metal case, speakers are
easily connected via the strong spring terminals mounted on
the rear, and then quickly turned on and off via the front
mounted push buttons.
• Up to two amplifiers can be connected and selected.
• Max power: 100WRMS.
50 Watt RMS Faders
Control extention speaker volume without
miss-matching the amplifier output.
A great solution
for speakers near
the BBQ or pool,
etc.
Cat: AC-1672
$
19 95
$
Remote Controlled Two Input
HDMI Switcher
$
24.75
Cat: CW-2804
$30
NOW WORKS
WITH DIGITAL PAY
TV REMOTES
169
Cat: AR-1840
HDMI
Audio Video Switcher
$20
69
A simple device for switching
$
95
between two high definition
Cat: AC-1692
multimedia (HDMI) sources.
Supplied with an I/R receiver fitted
to a 2m cable.
• Size 80(L) x 55(W) x
17(H)mm
Was $89.95
Remote Controlled 4 Channel
HDTV Input Selector
$
149
This four input HDMI selector
routes HD
Cat: AC-1694
video and
$50
audio signals
from the
selected
input to the
HDMI output.
The switcher also supports optical and coaxial audio inputs
which are switched in unison with the HDMI channels.
• Includes remote control and mains adaptor
• Fully HDMI and HDCP compliant
• 165MHz bandwidth Was $199
HDMI In-Line
Repeater/Extender
Extend the range of any HDMI
device such as a monitor or TV,
set-top box, DVD player, PC or
gaming system up to 60 metres
(powered). It will work with DVI
components with an adaptor.
Plugpack included.
• Size: 62 x 22 x 20mm Was $79.95
$20
$
59 95
Cat: AC-1698
5.1 Home Theatre Receiver
Well designed, made of super
strong ABS plastic, this attractive
two- piece swivel bracket is easy
to install and adjust (Phillips head
screwdriver required). Primarily
designed for mounting small /
medium sized speakers for surround
sound setups, or could easily be used for mounting security
lights, CCD cameras....etc.
• Wall mount section dimensions:
46(W) x 93(H) x 61(D)mm
• Speaker mount dimensions:
41(W) x 83(H) x 61(D)mm
New and
improved.
Transmit clear
video and sound
from sources
such as your
set-top box, TV,
DVD, pay TV,
camcorders and
security cameras
to anywhere in your
home, office or building.
Avoid the congestion and
interference on the crowded
2.4GHz band & enjoy reliability
and assured picture quality with
this 5.8GHz AV sender.
• Range of up to 50 metres
(line of sight)
• Built-in IR remote functionality
• No messy wires Was $199
Not much you
can't do
with this
receiver
- home
theatre,
stereo, or dock
your iPod® and use it for karaoke. The remote control
operates all the functions of the amp, receiver and a docked
iPod®
• Analogue audio inputs
• 2 microphone inputs with digital echo
• Variable channel modes: 2 ch,
Cat: AA-0471
sim 2.1, 3.1 & 5.1
• 435mm wide •iPod® not included
$
299
Watch one video source and record another simultaneously
with this slimline selector. This 6 input unit supports
component and composite video, S-video, digital audio
with automatic or manual selection with the included
remote control.
$
• Unit dimensions:
280(W) x 130(D) x 60(H)mm
119
Cat: AC-1686
Dual Output Video
Distribution Amplifier
With two outputs, this amplifier is ideal
for video distribution
applications.
Features automatic
gain adjustment
plus twin on-board
brightness and
contrast controls for
optimum picture quality on each output .The unit is
housed in a compact ABS plastic case with an integral
mounting flange.
• Requires 12VDC power
• Size 140(W) x 28(H) x 65(D)mm
$
79 95
Cat: QC-3438
Economy Antenna
Perfect for Caravans
or space-conscious
metropolitan areas
Designed to enable
positions in all
horizontal, vertical or
horiz/vert. polarities
and is suitable for all
transmitters across
Australia.
• Heavy duty construction
• Stainless steel connection screws
• Black UV resistant plastics
• Boom length: 720mm
• Max. width: 880mm
• Check our website, catologue or
in-store for full antennae range
Free Call: 1800 022 888 for orders! www.jaycar.com.au
$
69 95
Cat: LT-3172
5
Ref Silicon Chip
Aug. & Sept. 08
This ultra low distortion
amplifier module uses
the new ThermalTrak power
transistors and is largely based on the
high-performance Class-A amplifier which
was featured in SILICON CHIP during 2007. This improved
circuit has no need for a quiescent current adjustment or a
Vbe multiplier transistor and has an exceptionally low
distortion figure. Kit supplied with PCB and all electronic
components. Heatsink and power supply not included.
• Output Power: 135WRMS into 8 ohms and
200WRMS into 4 ohms
$
95
• Freq Resp. at 1W: 4Hz to 50kHz
• Harmonic Distortion:
Cat: KC-5470
<.008% from 20Hz to 20kHz
Not available until part 2 in Sept. 08.
89
UHF Remote Controlled Mains Switch
Ref Silicon Chip February ‘08
This UHF system will operate up
to 200m and is perfect for
remote power control systems
etc. The switch can be activated
using the included hand held
controller or our KC-5461 water
tank level sensor base station. Kit supplied
with case, screen printed PCB, RF modules
and all electronic components.
$
99 95
Cat: KC-5462
Temperature
Controlled
Soldering
Station
The soldering station
features a high quality
ceramic heating element
for accurate temperature
control, which is adjustable
between 200 and 480°C. The
soldering pencil is
light weight,
making it comfortable for
use for extended periods.
See in-store or our website
for full features.
NEW KITS FOR ‘08
Emergency 12V Lighting
Controller Kit
Ultra Low Distortion
135WRMS Amplifier
Module
Refer Silicon Chip Magazine February ‘08
• Automatically supplies power
for 12V emergency
lighting during a blackout.
The system has its own
7.5Ah SLA battery which
is maintained via an external
smart charger. Includes
manual override and overdischarge protection for the
battery. Kit supplied with all
electronic components, screen
printed PCB, front panel and case.
Charger and SLA battery available
Cat: KC-5456
separately.
$
69 95
Cat: TS-1560
Duratech 240V 25 Watt Soldering Iron
Ideal for the hobbyist and handy person. Has a stainless
steel barrel and orange cool grip, impact resistant handle.
29
12
95
$
Robot Arm Kit with Controller
Anti-Static Wrist
Strap
4.8 Volt Cordless
Screwdriver
$
11.25
Cat: TH-1780
All metal construction
with two internal
collars. The head
rotates freely making it ideal for drilling
delicate PCBs or plastic cases.
$
$
Every DIY Dad should own this
little beauty that is comfortable
and easy to use.
• Bright LED torch
• Magnetic bit
holder
• LED battery
level indicator
• 4 bitset included
• Mains charger included
11.25
59 95
TOOLS
$
19 95
Cat: TD-2498
Cat: TH-1772
Tapered Reamer
Ideal for enlarging and shaping holes in plastic,
thin metals and wood. Tapers from 3 to 12mm
$
14.50
Laser Level with Tape Measure
Use this tool to hang pictures, paintings or mirrors in your
home, install shelving, lay tiles etc. The laser line projects
up to 6m with a spread beam to create guide lines along
walls etc. It also includes a handy 2.5m tape measure and
a ruler on the side with inches on one side and millimetres
on the other.
$
Digital Vernier Calipers
Cat: TS-1465
24 95
This arm is a must for budding robot enthusiasts and
operates just like the real thing. It is capable
of 5 separate movements and can
easily perform complex tasks.
Individual control is available for
opening and closing the gripper
plus control of wrist, shoulder,
elbow and base rotation. The arm
is supplied as a kit of parts and makes an
excellent project for anyone
interested in robotic construction
and basic electrical connections.
100g lift capacity.
Cat: KJ-8916
• Suitable for ages 8+
95
Cat: TD-2130
$
Lets you run a stereo
amplifier in 'Bridged Mode' to
effectively double the power
available to drive a single speaker. There are no mods
required on the amplifier and the signal
processing is done by the kit before the signals
are fed to the stereo amp. Ideal for say, using a
stereo amp as an occasional PA amp for social
functions or using an old amplifier to drive a sub-woofer in a
home theatre. Kit supplied with silk
screened PCB and all specified
components. Requires balanced
(+/-) power supply.
Ref: Silicon Chip Magazine June ‘08
Here's a new and
Cat: KC-5464
completely updated
version of the very
popular low cost
12VDC electronic
timer. It is link
programmed for either a single
ON, or continuous ON/OFF cycling for up
to 48 on/off time periods. Selectable periods are
from 1 to 80 seconds, minutes, or hours and it can be
restarted at any time. Kit includes PCB and all specified
electronic components.
$
Pin Vice
99
Refer Silicon Chip July ‘08
Cat: KC-5469
Low Cost Programmable
Interval Timer
It has an adjustable
wrist strap, coiled lead, and
banana plug/alligator clip.
• Expanded lead length
approx. 1.8m.
$
Bridge Mode Adaptor for
Stereo Amplifiers
14 95
Cat: ST-3113
Spare tips Cat. TS-1466 $3.20
Adjustable Holesaw
An excellent cutter designed to cut plaster board and
ceiling tiles. Features calibrated hole size adjustment.
Two sizes available:
• 62 to 177mm hole
size Cat. TD-2520
• 158 to 264mm hole
size Cat. TD-2522
WHILE STOCKS
LAST NO
RAINCHECKS
NOT AVAILABLE
AT ALL STORES
6
$
49 95
Both Models (ea)
Simple and easy to use
with digital readout
• Accurate to 0.01mm
• Metric or imperial measurment
Storage Box
Help Dad keep his garage neat
and tidy with this niffty 24
compartment storage box.
Measures: 370 x 65 x 285mm.
$
10 95
Cat: HB-6314
$
39 95
Cat: TD-2082
Low Cost DMM
19 Ranges
• 3.5 Digit
• Transistor Test
• Diode Test
• 10A DC Current
• Ideal First Meter
• Compact Size
$
7 95
Cat: QM-1500
Free Call: 1800 022 888 for orders! www.jaycar.com.au
POWER
Mains Power Meter
150W 12VDC to 230VAC Isolated Can Inverter
Designed to fit into your car's drink holder, this can-sized inverter
alleviates the need for permanent mounting. Featuring a 150W output,
this inverter is deceptively small but still
has the grunt to power everything from
$
95
battery chargers right through to your
Cat: MI-5121
laptop computer.
000’S
SOLD
The meter can tell you how much an
appliance is costing to run and tracks the
actual power being used. It can also
display the instantaneous voltage or
current being drawn as well as peak
levels etc. 10A max rating.
Was $39.95
$
49
29 95
12V 7Ah SLA Battery
Cat: MS-6115
$10
Universal 90W Laptop
Power Supply
This laptop power supply has adaptors
to fit the major manufacturers' power
sockets. It also displays the output voltage and
automatically adjusts the output for the
adaptor used.
• 138(L) x 58(W) x 37(H)mm
• Will charge newer Dell
model laptops!
Cat: MP-3474
$
59
95
Home Theatre Powerboard
29
Full range of SLA Batteries in-store!
Surge protection and filtering is provided to
all your home theatre equipment connected
to this powerboard as well as current
protection via the in-built circuit breaker.
• Provides protection to telephone, data via
a network connection, satellite/cable TV
and TV aerials
$
59 95
Alkaline batteries for every occasion.
Cat
RRP
Pack Size
24
AAA SB-2331
$12.95
24
AA
SB-2330
$12.95
40
AA
SB-2332
$19.95
4
C
SB-2320
$6.95
4
D
SB-2321
$8.25
6
9V
SB-2417
$13.95
6 95
(0.8A / 3.8A, IP65 rated)
A truly versatile
charger
suitable
for wet
cell, gel and
AGM SLA
batteries from
1.25Ah to
120Ah. Computer controlled for optimum
performance and rain proof as well.
• Short circuit and reverse polarity protection
• Anti-spark protection
$
95
• 1.8m charging cable,
with interchangeable
Cat: MB-3604
fly leads
• Dimensions: 175(L) x 60() x 45(H)mm
79
Modified Sine Wave Inverters
Eclipse Batteries Buy in Bulk & Save
From
12V 5-Stage Car & Motorbike
Maintenance Charger
MAINS POWER ON THE GO
Cat: MS-4024
$
Use as an
emergency
power
source for
security
alarms or
as a
portable power
source for VCRs
or with solar
$
95
panels for
remote power.
Cat: SB-2486
• Leak proof
• High discharge capacity
• See catalogue, in-store or website
for discharge characteristics
Mains Power from your vehicle's battery
anytime. Take your creature comforts with you
when you go bush or on any road trip as these
inverters will produce mains power from your
vehicle's battery. A 150W inverter will run some
laptops, lights, small TVs and recharge
batteries. Inverters 300W and above will also run
power tools, fluorescents and larger style TVs.
Cat.
Power
Voltage
Price
MI-5102
MI-5104
MI-5106
MI-5108
150W
300W
400W
600W
12VDC to 230VAC
12VDC to 230VAC
12VDC to 230VAC
12VDC to 230VAC
$48.95
$79.95
$139.95
$229.00
LIGHTING
Rite Lights
Simple one touch operation and super bright LEDs make these
the most versatile, easy to install lights you'll ever purchase.
No need for cords or plugs. • 3 styles available separately
• Each requires 3 x AAA batteries
Powertech Rechargeable Batteries
• Packs of 4 Ni- MH rechargeable batteries.
SB-1735 2400mAh AA
$15.95
SB-1737 2000mAh AA
$13.95
SB-1738 2500mAh AA
$19.50
SB-1739 900mAh AAA $11.95
$
ST-3165 - Round Puck
• 5 LEDs • 2 lighting modes
• Measures 90mm Dia.
$
11 95
ST-3167 - Rectangle
FOUR PACK
SAVINGS
In-Car Battery Charger
14
$
14 95
Cat: ST-3166
$
• 6 LEDs • Rotatable light tube
• Measures 220(L) x 56(W) x 30(H)mm
14 95
Cat: ST-3167
Emergency Road Flasher
Power Point and
Leakage Tester
Test your power points using this versatile
tester. It checks most types of power points
within 110V to 240V for correct
wiring and earth leakage circuit
breaker trip levels.
Recharges 2 x AA or 2 x AAA Ni-Cd
or Ni-MH batteries.
• Delta V voltage detection ensures
the batteries are charged to their
optimal levels for long life.
• Keep a spare set of batteries
topped up and
ready to go,
$
95
wherever you
are.
Cat: MB-3552
9 95
Cat: ST-3165
ST-3166 - Square
• 6 LEDs • 2 adjustable angled light blocks
• Measures 100mm x 100mm
From
Models
up to
2,000 watt
available
$
19
95
Cat: QP-2000
Switch them on and place them on the ground to warn
other motorists and guide them around a problem.
• 3 high intensity LEDs
$ 95
• Requires 2 x AAA batteries
• 90(Dia.) x 25(H)mm
Cat: ST-3185
9
Solar Powered Keyring Torch
Features twin hibrightness LEDs and
in-built solar cell. Just
a few minutes
exposure per day will
keep the torch fully
charged and
ready for immediate use.
• Approx 70mm long
$
14 95
Cat: ST-3385
Free Call: 1800 022 888 for orders! www.jaycar.com.au
Keyring Torch
Cool car-shaped keyring fob with
three detachable key rings for
valet parking and a
built in superbright LED
torch.
Batteries incl.
Measures
$ 95
48mm long.
9
Cat: ST-3196
7
GREAT FATHERS DAY IDEAS - SUNDAY SEPTEMBER 7TH
Miniature Golf Buggy
with LCD Alarm Clock
$5 OFF ALL THESE GOLF DESK ACCESSORIES
This miniature 1:18 scale golf buggy with
clock will make a cherished
gift for any golf
enthusiast. The
windshield is a LCD
screen which has full
clock functions with a
calendar and
temperature setting.
Batteries included.
• 2 Sets of
miniature golf clubs
• Measures
$
95
140(L) x 75(W) x
100(H)mm Was $24.95
Cat: GH-1880
Golf Cart Pen Holder
This miniature golf caddy
pen holder includes
three pens
in red,
blue and
black
which
are
cleverly
shaped as real
golf clubs.
$
Was $19.95
19
14
Golf Course
Smokers Set
95
39 95
$
Dynamo Wind Up LED Torch
39
8
6021
9699
9709
9678
9369
9905
4620
4365
9439
9476
9821
4965
4721
8832
9267
6788
4699
2822
9669
3899
4130
7155
3433
4799
6221
3100
3799
8337
3121
1614
39 95
Cat: GT-3515
$
14 95
Play against the computer or a
real opponent. The game can
also suggest moves and hints
if you need a bit of help.
Software included.
• 3 skill levels
• Board 260mm square
$
44 95
Cat: GE-4094
GIVE DAD A JAYCAR GIFT VOUCHER
Wireless Weather Station
with Outdoor Sensor
NEW SOUTH WALES
Albury
Ph (02)
Alexandria
Ph (02)
Bankstown
Ph (02)
Blacktown
Ph (02)
Bondi Junction Ph (02)
Brookvale
Ph (02)
Campbelltown Ph (02)
Erina
Ph (02)
Gore Hill
Ph (02)
Hornsby
Ph (02)
Liverpool
Ph (02)
Newcastle
Ph (02)
Penrith
Ph (02)
Rydalmere
Ph (02)
Sydney City
Ph (02)
$
USB Roll-up
Chess Game
Cat: ST-3337
Cat: SL-2811
YOUR LOCAL JAYCAR STORE
Play Chess, Draughts, Reversi
(Othello), 4-in-a-Row,
Grasshopper or Nim against
an opponent, the computer or
recreate one of 320 famous Chess
Masters games. It also has a
teaching mode, different skill levels
and an LCD to keep track of moves.
• Requires 4 x AA batteries
(Use SB- 2425)
29 95
Perfect for the Dad who loves travelling or
camping. Just one minute of
winding will give you 30
minutes of light.
• 3 super-bright LED lights
• Water-resistant
• Internal rechargeable
battery
• While stock lasts - no rainchecks
Cat: GH-1882
6-in-1 Electronic
Games Board
Cat: GH-1063
This will be the handiest light in the
house. It clips on to any surface up
to 25mm thick and the lamp
can be removed and used as a
separate torch.
• Charger included.
• Strong gooseneck
• 18 superbright LEDs
• 180mm high
$
(approx)
95
14 95
GADGETS
This mirror won't ever steam up. It also
has a water resistant compartment where
you can connect and play your iPod ® or
MP3 player through the unit's speakers.
• Twin LEDs
• Stereo speakers
• AM/FM radio
• 245mm high
• Requires 4 x AA batteries
(Use SB-2425)
Cat: SL-2715
Clip-on Rechargeable LED Lamp
This attractive home weather
station not only displays current
weather data, it also forecasts
the weather for
the next 12 hours
and shows the
moon phase as
well as the current
time and
sunrise/sunset times. A very informative system
that is well designed & easy to use.
• Measures indoor and outdoor
temperature & humidity, & air pressure
• Up to 30m transmission range
• Indoor display 225mm wide
This AM/FM radio not only has a
stainess steel
front but also a
real golf ball
and tee. The
driver's shaft
controls the volume and
channel selection.
• Measures 245(L) x
$
125(W) x 113(H) mm
• Requires 3 x AA batteries
(Use SB-2425)
Was $19.95
Anti-Fog Shaving Mirror
Solar Powered Garage LED Light
Australia Freecall Orders: Ph 1800 022 888
The bunker with
rake is the ashtray,
the tee flips open
at the push of a
button to reveal
your hidden cigarettes and
the golf buggy becomes a
$
95
lighter at the push of the
rear wheel. No-one will guess
Cat: GH-1886
what little wonders this course
contains.
• 260(L) x 205(W)mm Was $24.95
19
Cat: GH-1884
Ideal for garages, gazebos and greenhouses,
the 360° adjustable solar
panel will allow for custom
positioning. It's waterproof,
features a cord-switch to
operate, and is simple to
install.
• Solar panel and mounting
bracket included
• 2.4m cable and
$
rechargeable enclosed
Ni-Cd battery included
Golf Driver AM/FM Radio
$
Can’t make up your mind?
Too hard to choose?
Give Dad a Jaycar
Electronics Gift Voucher
so he can have all the fun
of choosing for himself
from our range of over
6,500 products.
69 95
Cat: XC-0339
Taren Point
Tweed Heads
Wollongong
VICTORIA
Coburg
Frankston
Geelong
Melbourne
Ringwood
Springvale
Sunshine
Thomastown
QUEENSLAND
Aspley
Cairns
Ipswich
Maroochydore
Mermaid Beach
Ph (02) 9531 7033
Ph (07) 5524 6566
Ph (02) 4226 7089
Ph
Ph
Ph
Ph
Ph
Ph
Ph
Ph
(03)
(03)
(03)
(03)
(03)
(03)
(03)
(03)
9384
9781
5221
9663
9870
9547
9310
9465
1811
4100
5800
2030
9053
1022
8066
3333
Ph
Ph
Ph
Ph
Ph
(07)
(07)
(07)
(07)
(07)
3863
4041
3282
5479
5526
0099
6747
5800
3511
6722
Townsville
Ph (07) 4772 5022
Underwood
Ph (07) 3841 4888
Woolloongabba Ph (07) 3393 0777
AUSTRALIAN CAPITAL TERRITORY
Belconnen
Ph (02) 6253 5700
Fyshwick
Ph (02) 6239 1801
TASMANIA
Hobart
Ph (03) 6272 9955
SOUTH AUSTRALIA
Adelaide
Ph (08) 8231 7355
Clovelly Park Ph (08) 8276 6901
Gepps Cross
Ph (08) 8262 3200
WESTERN AUSTRALIA
Maddington
Ph (08) 9493 4300
Midland
Ph (08) 9250 8200
Northbridge
Ph (08) 9328 8252
NORTHERN TERRITORY
Darwin
Ph (08) 8948 4043
NEW ZEALAND
Christchurch Ph
Dunedin
Ph
Glenfield
Ph
Hamilton
Ph
Manukau
Ph
Newmarket
Ph
Palmerston Nth Ph
Wellington
Ph
Freecall Orders Ph
(03) 379 1662
(03) 471 7934
(09) 444 4628
(07) 846 0177
(09) 263 6241
(09) 377 6421
(06) 353 8246
(04) 801 9005
0800 452 9227
Free Call: 1800 022 888 for orders! www.jaycar.com.au
CIRCUIT NOTEBOOK
Interesting circuit ideas which we have checked but not built and tested. Contributions from
readers are welcome and will be paid for at standard rates.
Q1 IRF9540
+
S
D
K
ZD4
16V
0.5W
G
1k
A
22
A
TP1*
2.2k
1k
FROM
CHARGER
K
A
100 F
25V
ZD1
16V
1W
ZD2
3.3V
0.4W
ZD3
3.9V
0.4W
–
K
+7.2V
VR1
5k
K
3
IC1
LM311
1
A K
100
8
2
CHARGING
LED1
47k
7
4
2.2k
A
* SET VR1 FOR 7.2V AT TP1
WHEN BATTERY VOLTAGE
IS 13.8V
IRF9540
D
LED
ZD1–ZD4
A
K
K
A
G
D
S
Charging controller for 12V lead-acid batteries
Many low-cost chargers for 12V
lead-acid batteries are little more
than a step-down transformer and
bridge rectifier. As a result they
tend to overcharge a battery if left
connected to it for an extended
period.
This simple charging regulator
circuit is connected between the
charger and the battery and is easily
adjusted to prevent the battery being
overcharged beyond the optimum
level between 13.8V and 14.0V.
P-channel power Mosfet Q1 is
connected as a switch in the positive
battery lead, controlled by LM311
comparator IC1. IC1 monitors the
battery terminal voltage and compares a portion of the battery volt-
age from trimpot VR1 with a fixed
+7.2V at the inverting (-) input. This
reference voltage is derived from the
battery voltage via a shunt regulator circuit using zener diodes ZD2
and ZD3.
When the battery voltage is below
13.8V, the voltage at TP1 will be
lower than 7.2V. Therefore the output of IC1 will switch low, drawing
current through LED1 and its series
100W and 1kW resistors and thus
providing forward bias for Q1. Q1
switches on, allowing charging current to flow into the battery.
As soon as the battery terminal
voltage rises to 13.8V (or the preset voltage), TP1 rises above 7.2V
and this causes the output of IC1
to switch high. The current
through LED1 falls to zero and
+
Q1 is switched off, preventing
any further charging. The 47kW
resistor between pins 2 & 7 of
IC1 provides about 0.5V of
hysteresis so that the battery
voltage will need to drop by
500mV or so, before the circuit
can turn back on to provide
TO 12V
more charge.
BATTERY
Zener diodes ZD1 and ZD4
together with the 22W resistor
are added to prevent overvoltage damage to either IC1
or Q1.
Note that although Q1 is
being used here as an on-off
switch, it has an on-resistance
–
of about 0.2W and therefore
needs to be provided with a
good heatsink because of the
heat dissipation during charging.
We suggest a finned extrusion heatsink like the
Jaycar HH-8566, which has
a thermal resistance of 2.2°C/W.
You’ll need to provide electrical
insulation between the device tab
and the heatsink though, because
the Mosfet tab will be at positive
battery potential.
Setting up the regulator is easy,
because LED1 provides direct indication of when Q1 is switched on to
allow charging. All you need to do
is connect the output terminals to
either a battery or a DC power supply, with a voltage of between 13.8V
and 14.0V. Then adjust trimpot VR1
until the voltage at TP1 is very close
to 7.2V and LED1 is clearly at its
switching point.
Jim Rowe,
SILICON CHIP.
Issues Getting Dog-Eared?
Keep your copies safe with these handy binders.
REAL
VALUE
AT
$13.95
PLUS P
&
P
Available Aust, only. Price: $A13.95 plus $7 p&p per order (includes GST). Just fill in
and mail the handy order form in this issue; or fax (02) 9939 2648; or call (02) 9939 3295
and quote your credit card number.
siliconchip.com.au
August 2008 57
Circuit Notebook – Continued
–
–
FROM TRAIN
CONTROLLER
+
TO
TRACK
D1
K
A
12-18V
AC IN
+
REG1 7812
IN
+12V
OUT
K
GND
1000 F
35V
100nF
100k
5
6
14
4
A
A
LED1
K
C
B
Q1
BC338
A
6
1
2
IC1: 4093B
IC2: 4013B
3
3
D
S
1.2M
470k
14
Vdd 1
Q
IC2a
CLK
Q
R
C
Q2
BC338
E
1k
1k
IC1a
LED2
K B
E
7
5
RELAY2
FWD/REV
D6
A
IC1b
10nF
K
RELAY1
RUN/STOP
D5
8
9
2
11
4
D
S
Q
IC2b
CLK
Q
Vss
R
10 7
13
LEDS
12
K
A
D2
A
22 F
TANT
K
8
9
IC1c
12
10
13
100k
270k
D3
K
IC1d
33k
A
100nF
7812
11
100k
B
D4
K
GND
BC338
A
100nF
E
IN
C
D1,D5–6: 1N4004
A
K
GND
OUT
D2–4: 1N4148
A
K
Random direction control for
a model railway layout
This simple circuit connects between a model train controller and
the train track. It automatically starts
and stops the loco at random; sometimes it runs forward, sometimes in
reverse and sometimes it just stops
for a while.
Two 12V relays are used to start or
stop the loco and to run it in forward
or reverse. Using relays avoids any
problems with back-EMF sensing
controllers. In the unpowered state,
the two relays connect the train
controller directly to the track, so
the train runs according to the train
controller setting.
When Relay1 is energised, the
train always stops. When Relay2
is energised, the train will run in
reverse as long as Relay1 is deenergised. LED1 and LED2 indicate
the on state of the relays (ie, they
light when the relays are on).
Here’s how it works: NAND gate
58 Silicon Chip
IC1a is configured as an oscillator
with a 20-second period and a high
duty cycle. The output at pin 3 is
only low for a few seconds every
20 seconds due to diode D2 and its
series 470kW resistor.
Two D-type flipflops, IC2a &
IC2b, drive the two relays. Their D
inputs are connected to two separate
low-duty cycle oscillators based on
gates IC1c & IC1d. They latch the D
inputs on the low-to-high transition
of IC1a.
As a result, the state of IC1c and
IC1d is clocked into the flipflops
every 20 seconds. This results in a
random state for the relays since all
three oscillators run independently.
However, the low duty cycle of both
IC1c and IC1d (due to the parallel
diode-resistor combinations) means
the relays will be off more often than
on, so the loco will run forwards
most of the time.
When IC1a goes from high to low
it triggers a monostable based on
IC1b which is connected to the SET
input (pin 6) of flipflop IC2a. This
turns on Relay1 and means the loco
always stops for a few seconds every
20 seconds.
This feature was included to avoid
the possibility of the loco going
instantly from forward to reverse
or vice versa, with the danger of
derailing.
The circuit requires 10-12V DC to
operate the 12V relays correctly and
can be powered from the auxiliary
AC terminals that are usually provided on train transformers.
Geoff Nicholls,
Hamburg, Germany. ($60)
Editor’s note: a project providing a
similar function, together with optoelectronic sensing of locomotive
position, was featured in the July
1995 issue of SILICON CHIP.
siliconchip.com.au
S1
being the antenna under test. The
antenna is connected to the circuit
and the 100kW pot VR1 adjusted for
a suitable reading on the meter, to
indicate that the unit is operating.
The frequency can then be determined by tuning for the signal with a
shortwave receiver or by connecting
a frequency counter to the termi-
nal provided. The effect of nearby
objects, long-term degradation in
performance, losses and corrosion
can be monitored by the setting
required on the unit to achieve the
same meter reading over a period
of time. With experience, this can
indicate a problem before a failure
occurs.
Transistor Q2 is connected as a
grounded-base oscillator with FET
Q1 providing buffering and the
required phase change. FET Q3 is
also a buffer to prevent any serious
loading from the frequency counter,
if used. Simply tuning to the signal
with another radio is the easier
method. The unit will test any antenna, with the proviso that there is
a DC path through the system under
test. Long wire or Beverage antennas,
etc, will require a balun.
If VR1 is fitted with a calibrated
scale, it will allow documenting results as compared to the meter reading. The meter in the prototype was
a VU meter salvaged from a defunct
cassette recorder.
Dayle Edwards,
Taylorville, NZ. ($40)
as determined by the components
connected to pins 1, 2 & 3. This
square-wave output drives complementary transistors Q1 & Q2 which
act as buffers to drive the diode
pump comprising D1, D2 and the
470mF capacitors.
The resultant output of about -10V
is then regulated to -5V by REG2, a
7905 regulator. The circuit provides
50mA at -5V but if higher currents
are required, BD681 and BD682 Darlington transistors can be substituted
for Q1 & Q2.
L. Kerr,
Ashby, NSW. ($45)
METER
–
+
33k
D
D1 OA90
K
A
56k
B
VR1
100k
100nF
G
Q1
MPF102
100nF
S
E
9V
BATTERY
A
LED1
Q2
BC557
K
47pF
C
100nF
1k
10k
10pF
22k
ANTENNA
UNDER
TEST
Q3
MPF102
D
G
10nF
TO
FREQUENCY
COUNTER
S
1k
1M
LED
OA90
A
MPF102
K
K
A
Antenna resonance
indicator
This circuit provides a quick and
easy way to find the resonant frequency of antennas for HF marine
installations. The circuit is a simple
2-terminal RF oscillator with its
frequency-determining component
BC547
B
S
G
D
E
C
Balanced supply rails
from a 12V battery
This circuit derives +5V and -5V
regulated supply rails from a 12V
battery. The +5V rail is derived
directly via a standard 7805 3-pin
regulator while the -5V rail is derived from an oscillator and a simple
diode pump.
A 4047 astable multivibrator provides an asymmetrical square-wave
output at pin 10 of approximately
12V peak-to peak at about 580Hz,
siliconchip.com.au
August 2008 59
Circuit Notebook – Continued
+5V
330
4.7k
12
IR Rx
MODULE
13
IC1: 4093B
3
1
1
39k
2
2
4.7 F
1
3
A
K
3
IC1a
5
10k*
6
D1
K
2
A
4
10nF
8
9
IC1b
14
11
IC1d
'CLOCK'
6
'START'
4
1
Vdd
P0
P1
P3
IC2
5
PICAXE P2
-08
P4
SER 2
IN
IC1c
10
7
3
'DATA'
Vss
D2
1
22k
PROG
SKT
2
8
3
10k
82k
100nF
OUTPUT
7
100nF
0V
D1, D2: 1N4148
A
Universal IR remote
control repeater
This project came about during
the development of a PICAXEbased home-theatre controller. The
PICAXE has built-in infrared (IR)
signal decoding capabilities but this
is limited to the Sony Infrared Code
(SIRC) 12-bit code. Since the hometheatre controller was to be used in
conjunction with a Sony LCD TV,
another solution was required.
A check of the other IR remote
controls that I had accumulated
showed they all used a 32-bit data
code based on the NEC IR format.
This uses infrared pulses modulated
K
* VALUE MAY REQUIRE ADJUSTMENT IN THE RANGE 8.2k – 12k,
DEPENDING ON COMPONENT TOLERANCES
on a carrier of around 38kHz. IR
receiver modules (available from Altronics and Jaycar) do the demodulation and provide a TTL-compatible
output signal.
While the PICAXE is an easily programmed PIC controller, the
overhead of its internal interpreter
makes it too slow to reliably process
a 32-bit IR signal on its own. The
main IR signal from an IR remote
consists of an extended header pulse
of between 4ms and 8ms carrier, followed by an “off” period of 2-8ms.
These periods are constant for a
particular manufacturer’s device but
will differ between manufacturers/
devices/models etc. The “data” that
follows is a series of 32 binary bits.
The transmitter “on” period for
each bit is constant at around 500ms
with the following “off” period determining whether the bit is a 0 or
1. A “0” is transmitted as a ~500ms
pulse followed by a break of a similar
length. On the other hand, a “1” is a
~500ms pulse followed by a break of
around 2000ms (2ms). A final “on”
period, called a “lead out”, of ~500ms
indicates the end of the data.
Most IR remotes also transmit
other pulse sequences but this receiver ignores these for simplicity.
The circuit uses an IR receiver
module, a CD4093 quad Schmitt
trigger and a PICAXE-08M or larger.
Looking for real performance?
PERFORMANCE ELECTRONICS
FOR CARS
160 PAGES
23 CHAPTE
RS
• Learn how engine management systems work
• Build projects to control nitrous, fuel injection and turbo boost systems
• Switch devices on and off on the basis of signal frequency, temperature
and voltage
• Build test instruments to check fuel injector duty cycle, fuel mixture and
brake and coolant temperatures
• Speedo Corrector, Turbo Timer & Digital Thermometer Projects
Fro m the
pub lish ers
of
Intelligen
t
turbo timer
I SBN 0958
5229
9 7809
5
8 5229
4
$19.80 (inc GST)
4-4
TURBO B
OOST
& nitro
us fuel cont
rollers
6
NZ $22.00 (inc
GST)
How eng
in
manageme e
nt works
Mail order prices: Aust. $A22.50 (incl. GST & P&P); Overseas: $A26.00 via airmail.
Order by phoning (02) 9939 3295 & quoting your credit card number; or fax the details to (02) 9939 2648; or mail your
order with cheque or credit card details to Silicon Chip Publications, PO Box 139, Collaroy, NSW 2097.
60 Silicon Chip
siliconchip.com.au
The output of the IR receiver module is connected to a 4.7kW pull-up
resistor. This output is normally
high (+5V) and is pulled low when
a 38kHz carrier is present.
IC1a, configured as an integrator,
detects the header pulse. Its output
goes high about 3.5ms after the leading edge of the header pulse. Diode
D1 causes the output to restore
quickly after the pulse stops.
The rising edge or end of each carrier pulse is used as a clock signal to
indicate to the PICAXE that a bit can
be read. IC1b is used to detect the
longer “off” periods of the “1” bits.
When data is present, the output of
IC1b is pulled high by the presence
of signal and stays high until the
carrier is off for more than 1.5ms.
This coincides with the longer “off”
periods of the “1” bits.
IC1c is wired as a monostable
multivibrator. Its input is configured
as a differentiator, triggered by the
rising edge of the previous gate. This
effectively creates a delayed pulse
whenever a “1” bit is received. By
the time the PICAXE has responded
to the clock signal, the output of this
monostable will indicate the inverse
of the received bit.
The PICAXE program is critical
to the operation of the IR receiver.
The PICAXE must be run at 8MHz
or higher in order to decode and
store the IR data. The program code
structure has been optimised for
speed and to save program space.
This is necessary so that the smaller
08M or 14M chips can be used. The
PICAXE chip must run faster than
the incoming data so that overhead
tasks, like saving data bytes and
clearing the accumulator, can be
completed before the next incoming
bit needs to be read.
As mentioned previously, the
IR code consists of 32 bits or four
bytes. The first two bytes indicate
the device ID and the second pair
indicates the device’s command.
Dealing with the command pair first,
the first byte indicates the command
value (0-255) and the second byte is
the 1’s complement or “inverse” of
the first. This provides a level of error checking of the received signal. If
the sum of the two command bytes is
255, then the data is treated as valid.
The device ID pair of bytes can be
interpreted in two ways, depending on the protocol adopted by the
manufacturer. Most manufacturers
use the 1’s complement algorithm
described previously for checking
the device ID code. However, some
manufacturers use the full 16 bits
(0-65,535) with no error checking
as the device ID. Since the decoder
must match the received device ID
code with a lookup value, an error
will cause the sequence to be ignored
anyway.
In addition to the device ID, the
loop count for the header pulse “on”
and “off” periods can be recorded in
byte variables and can offer another
Peter
is this m Gee
on
winner th’s
Peak At of a
las
Instrum Test
ent
level of device discrimination, where
required.
When used in proximity with other IR code
controlled devices, the
receiver program must discriminate
between its own and foreign IR signals. This includes codes that are
shorter than the 32-bit one used by
this receiver.
As an example, if Sony’s 12-bit
code is detected, its sequence will
be complete before the code receiver’s reception routine is halfway
through, resulting in it “hanging”,
waiting for further clock pulses. This
will result in the next IR sequence
completing the clocking of the
32-bits required, almost certainly
causing the received code to be
discarded after error checking. The
receiver will thus ignore one button
press but should synchronise to the
following one.
The RC values used with the integrators and differentiators are all
±5% and have proven to give reliable results. However, there may be
circumstances where some adjustment is required, particularly with
the data integrator time constant.
Finally, the software for the PIC
AXE-08 microcontroller can be
downloaded from the SILICON CHIP
website. The software filename is:
“InfraDecoder-08M-V1.0.bas”.
Peter Gee,
Inglewood, WA.
Contribute And Choose Your Prize
As you can see, we
pay good money for
each of the “Circuit
Notebook” items published in SILICON CHIP.
But now there are four
more reasons to
send in your circuit
idea. Each month,
the best contribution published will
entitle the author to
choose the prize: an LCR40 LCR meter,
a DCA55 Semiconductor Component
Analyser, an ESR60 Equivalent Series
Resistance Analyser or an SCR100
siliconchip.com.au
Thyristor & Triac Analyser, with the
compliments of Peak Electronic Design
Ltd www.peakelec.co.uk
So now you have even more reasons
to send that brilliant circuit in. Send it
to SILICON CHIP and you could be a
winner.
You can either email your idea to
silicon<at>siliconchip.com.au or post it
to PO Box 139, Collaroy, NSW 2097.
August 2008 61
Pt.1: By JOHN CLARKE
LED Strobe &
Tachometer
This versatile LED Strobe & Tachometer can be used to observe
and measure the RPM of rotating machinery. It offers three
different measurement methods and the readout is via a 2-line
LCD module.
I
T’S EASY TO MEASURE the speed
of rotating machinery with this
versatile project. It uses three different “contactless” sensing methods,
making it ideal for checking the RPM
of objects such as rotating shafts, fans
and model aircraft propellers.
In addition, the strobe feature allows
62 Silicon Chip
rotating machinery to be effectively
“frozen” for close visual inspection.
The strobe is based on a high-brightness white LED and can also be used
to provide basic stroboscopic speed
measurement. Alternatively, speed
measurements can be made using
either an infrared reflective optical
pickup or a slotted disk/photo-interruptor pickup.
Strobing
Many people consider strobes as just
a party effect, for use in discos and
other venues. A typical disco strobe
flashes at about four times a second
siliconchip.com.au
Warning!
1000 RPM
TACHOMETER
STROBE
LIGHT
MACHINE
BASIC STROBOSCOPIC MEASUREMENT
Fig.1: using a strobe light to measure rotational speed. The
strobe flash rate is manually adjusted until the machine
appears to stop (see text) and the result read from the LCD.
Flashing lights, particularly in the
lower frequency range from about
5Hz (300 RPM) and upward can induce seizures in people subject to
photosensitive epilepsy. Flashing
lights can also trigger a migraine
attack. It is recommended that
people prone to these effects avoid
stroboscopic lights.
SLOTTED DISK
1000 RPM
TACHOMETER
MACHINE
PHOTO
INTERRUPTOR
STROBE LIGHT
(OPTIONAL)
TRIGGERED MEASUREMENT VIA SLOTTED DISK
Fig.2: this technique uses a photo-interruptor assembly to
send a series of trigger pulses to the tachometer. The tacho
counts these pulses and shows the result on the LCD. In
this case, the strobe light is optional – it is triggered by the
photo-interruptor and used to observe the machine.
REFLECTIVE STRIP
ON SHAFT
1000 RPM
TACHOMETER
STROBE LIGHT
(OPTIONAL)
REFLECTIVE MACHINE
OPTICAL PICKUP
TRIGGERED MEASUREMENT BY REFLECTION
Fig.3: this triggered measurement technique uses the tacho
to count the pulses from a reflective optical pickup.
and the strobing effect makes people
appear to move in a jerky manner.
That’s because, at night, you only see
each person’s position when the strobe
flashes. The intermediate positions
between flashes are not seen.
Strobing rotating machinery gives
much the same effect, depending on
the strobe frequency and the RPM of
the rotating part. If the strobe is set to
flash at a rate of once per rev, then the
rotation will appear to stop. The reason
for this is simple – the machine will
be in the same position each time the
strobe flashes.
In fact, the effect is so convincing
that it can be dangerous. You must
be alert to the fact that the machine
must not be touched, since it is still
actually moving and could cause serious injury.
siliconchip.com.au
Other strobe effects also become
apparent as the strobe frequency
drifts out of step with the rotational
frequency. For example, if the strobe
flashes slightly faster than the rotational speed of the machine, then the
machine will appear to rotate slowly
backwards. Conversely, if the strobe
flashes at a slightly slower rate than
the rotational speed of the machine,
the machine will appear to rotate
slowly forward.
One area where this is often apparent is in western movies, where the
wheels of a stage coach initially appear to slowly rotate backwards and
then stop while the stage coach is still
moving. That happens because movies
are shot at a rate of 24 frames/s and
this has the same effect on the wheels
spokes as a strobe.
Initially, the wheel spokes are travelling too slowly to keep up with the
strobing effect of the frame rate. Then,
as the speed increases, the wheels appear to stop before finally appearing
to rotate forwards.
If we know the number of spokes
in the wheel, we can even calculate
its rotational speed when it appears
to be stopped. For example, if the
wheel has eight spokes, then its speed
is equal to 1440 (ie, the number of
frames per minute) divided by eight,
or 180 RPM.
Similarly, the rotational speed of
any machine can be measured by setting the strobe rate so that the motion
appears to stop. Note, however, that
you have to set it to the highest speed
at which the machine appears to stop,
since the same effect will also occur
if strobing takes place at 1/2-speed or
1/3-speed, or 1/4-speed, etc.
You also have to take into consideration the number of blades on a fan or
propeller, or the number of marks on
a shaft. For example, if there are two
blades on a prop, then the prop will
also appear to stop if strobed at twice
the rotational speed. The solution to
this problem is to place a single mark
on the shaft or a propellor, etc.
Fig.1 shows how the unit is used
with a strobe to measure machine rotation. Note that if the strobe is set at
twice the speed of the machine, there
will appear to be two reference positions, each 180° apart. However, if the
strobe is set at half rotational speed,
there will be one reference position
but it will appear dimmer than when
the strobe is set at the correct speed.
Photo-interruptor
Fig.2 shows another way to measure
rotational speed. In this case, a trigger
signal is sent to a tachometer from a
sensor attached to the machine. This
August 2008 63
5MHz
OSCILLATOR
COUNTER
LCD READOUT
CALCULATE
COMPARE
VALUE FOR
DISPLAYED
RPM
COMPARE
1000 RPM
RPM
FINE
ADJUST
STROBE
RPM 'SET'
SWITCHES
GENERATOR MODE OF OPERATION
Fig.4(a): this is the block diagram for the generator operating mode. The
Up & Down “RPM Set” switches and a fine adjust pot on the tachometer
set the stroboscope’s flash rate, while the LCD shows the corresponding
reading in RPM,
TRIGGER
INPUT
5MHz
OSCILLATOR
COUNTER
EDGE
DETECTOR
& DIVIDER
CAPTURE
CLEAR
CALCULATE
RPM
1000 RPM
LCD READOUT
STROBE
TRIGGERED MODE OF OPERATION
Fig.4(b): the triggered mode of operation. In this mode, the counter counts
the number of pulses from a 5MHz oscillator between each successive
external trigger signal. This value is used to calculate the RPM which is
then displayed on the LCD.
sensor could be either an optical trigger or Hall effect trigger that is interrupted by a rotating vane or magnet.
As the shaft rotates, it sends a series of pulses to the tachometer. The
tacho
meter measures the frequency
of these trigger signals and calculates
the RPM for display on the LCD. As
Main Features
•
•
•
•
•
•
•
•
•
•
RPM and frequency readout on
LCD panel
Generator or triggered strobe
Can be triggered via slotted
disk or reflective light
Adjustable flash period
Fine frequency adjustment in
generator mode
Wide frequency range
1 RPM resolution
Divider options when triggering
Triggering indicator
Readout averaging
64 Silicon Chip
an option, the strobe can also be fired
in synchronisation with the sensor.
The more rotating vanes used on
the trigger, the greater the number of
pulses generated for each rotation of
the shaft. As a result, the unit can be
set to a division ratio from 1-8, so that
the displayed reading is correct.
For example, if there are eight
pulses per rotation, the division
ratio is set to eight to get the correct
reading.
A 0.5 divider has also been included. This can be used if the sensor
is being triggered by a shaft that runs
at half the speed of the shaft we want
to measure.
For divisions from 2-8, you also
have the option of firing the strobe
on any one of the trigger signals. For
example, if there are eight pulses per
rotation, you can have the strobe fire
either on the first pulse, the second
pulse, the third pulse or on any other
pulse up to the eighth pulse.
In addition, the pulse edge can be
selected so that the strobe fires when
the pulse signal goes high or when
it goes low. Each of these triggering
points will provide a different view of
the machine – ie, the strobed position
of the machine will vary.
Reflected IR
A third method of measuring the
RPM of a rotating machine is shown
in Fig.3. This is a purely a non-contact
method and relies on light reflection
from the machine.
In some cases, a reflecting strip will
have to be attached to the machine in
order to get sufficient variation in the
light reflection as the machine rotates.
However, for rotating parts such as
propeller or fan blades, the brightness
variation should be sufficient without
adding any reflective material.
In this measuring mode, an infrared
(IR) light source is shone onto the machine and the resulting reflected light
variations detected using an infrared
photodiode. Using infrared prevents
other light sources such as fluorescent
lights from affecting the reading.
Strobe duration
When using a strobe, the duration
of the flash determines just how much
of the machine’s rotation can be seen.
Ideally, the flash should be as short
as possible to prevent blurring of the
strobed image (ie, we don’t want the
machine to move too much during the
flash period).
Traditional strobes use Xenon tubes
and these produce short, bright flashes
that are ideal for strobing rotating
machinery. However, this circuit uses
a high-brightness white LED and its
output is much lower than that from
an Xenon tube.
As a result, the flash period needs
to be a compromise between brightness and the amount of movement
that can be tolerated during the flash.
And in case you’re wondering, most
white LEDs can be driven with very
short pulse widths for use in strobe
applications. If you are not convinced,
read the “Busting a Myth” panel in Pt.2
next month.
For our LED strobe, the flash period
can be set anywhere between 32ms
and 6.5ms. A longer flash period
gives a brighter light but in practice,
the period needs to be set to suit the
application. The faster the machine
spins, the lower we need to set the
flash duration to prevent “blurring”
of the strobed machine.
For example, if the machine is rotatsiliconchip.com.au
ing at around 5200 RPM, then we need
to set the flash duration to just 32ms to
limit the movement during this period
to 1°. However, at just 166 RPM, the
flash duration can be increased to 1ms
for 1° of movement.
As an alternative to a fixed flash period, there is an automatic mode which
sets the flash period as a percentage of
the measured RPM. This percentage
can also be manually adjusted from
1-10% in 1% steps.
Note, however, that these percentage settings are not obtainable at very
high or very low RPM values, due to
the limited flash duration range (32ms
to 6.5ms).
Operating modes
In order to carry out the different
measurement techniques depicted in
Figs.1-3, the unit has two different
operating modes: (1) generator and
(2) triggered. Block diagram Fig.4(a)
shows the generator mode of operation, while Fig.4(b) shows the triggered
mode.
The generator mode is used for basic
stroboscopic measurements and when
this mode is selected, the unit directly
drives the strobe light. In operation,
the tachometer is initially adjusted
using Up & Down pushbuttons and
this sets the strobe rate and adjusts
the corresponding RPM reading on
the LCD.
Each pushbutton alters the RPM
setting in 100 RPM steps, while an
adjacent knob provides for fine adjustment to 1 RPM resolution. The resulting LCD readout shows both the RPM
(1 RPM resolution) and the frequency
in Hz (.01Hz resolution).
The alternative triggered mode
is used to make the measurements
depicted in Figs.2 & 3. In this mode,
the tachometer is triggered by the
pick-up sensor and the LCD shows the
RPM and the frequency of the incoming trigger signal. The strobe light is
optional and is also triggered by the
pick-up sensor.
As discussed above, the sensor can
be either a slotted disk and photointerruptor assembly or an optical
pick-up relying on reflected IR light.
Note that, in this mode, the RPM reading cannot be adjusted manually and
the tachometer reads the rotational
speed according to the trigger pulses
from the sensor.
If there is more than one trigger
pulse per revolution, the strobe can
siliconchip.com.au
The strobe technique is used for measuring the speed of fan blades and for
“freezing” the motion while the machine is running. Alternatively, the infrared
optical pickup method can be used for measuring the RPM of fans and model
aircraft propellers, since the blades usually give good reflection variations.
The infrared optical pickup method is
also ideal for measuring the rotational
speed of shafts. A reflective strip
attached to the shaft provides the
required variations in the amount of
reflected light as the shaft rotates.
be set to fire on any one of these by
pressing either the Up or Down switch,
to shift to the next trigger edge. In addition, the division ratio must be set
to get the correct reading.
How the tacho works
The way in which the tachometer
works to measure the incoming RPM
pulses is rather unconventional.
The traditional method of measuring frequency is to count the number
of incoming pulses over a set period,
usually one second. This is quite an acceptable method when the frequency
is high and a lot of counts are obtained
during the 1s period.
However, for RPM readings, the incoming frequency is usually relatively
low and in most cases there just aren’t
enough counts over a 1s period to ensure sufficient accuracy. For example,
at 1000 RPM, the incoming frequency
would be just 16.66Hz (assuming one
pulse per rev) and so we would read
either 16Hz or 17Hz on a counter. After
multiplying by 60 to convert to RPM,
the display would show either 960
RPM or 1020 RPM.
In other words, there would be a 60
RPM uncertainty in the reading.
Of course, we could count the signal
over 10s or even 100s to get 6 RPM or
0.6 RPM resolution. However, 10s is a
long time to wait for a reading update
and a machine can vary its RPM value
quite significantly during that time. As
for waiting 100s, forget it.
So how do we measure RPM with
high resolution and a fast update time?
Fig.4 shows how it’s done.
For the triggered mode of operation, the tachometer utilises a 5MHz
oscillator and a counter. The counter
is configured to count the number
of pulses from the 5MHz oscillator
between each trigger signal.
For example, if the trigger signal
August 2008 65
REG1 7805
+5V
100 F
16V
27pF
X1
20MHz
27pF
16
15
FINE
FREQUENCY
ADJUST
(RPM)
OUT
1k
100nF
4
14
Vdd MCLR
K
100 F
16V
A
OSC2
S4
ZD1
16V
1W
RB4
10
11
39 5W
220
C
B
IC1
PIC16F88-I/P
10k
4
13
6
18
RA1
1
RA2
17
RA0
2
RA3
TO
TRIGGER
CIRCUIT
6
CON3
Vdd
RS
CONTRAST
EN
D7 D6 D5 D4 D3 D2 D1 D0 GND
2
14 13 12 11 10 9 8 7
3
LCD
CONTRAST
VR2
10k
10 F
R/W
5
7
RB1
9
RB3
8
RB2
RB0
7805
GND
BC337
1nF
S1
Vss
5
S2
B
S3
E
MODE
SC
–
Q1
BC337
1
12
16 x 2 LCD MODULE
2008
S5
TO 1W
WHITE
LED
AN4
RB7
3.5mm JACK
SOCKET
CON1
CON2
+
220
12V DC
INPUT
–
470 F
16V LL
LED
ON/OFF
RB6
1k
A +
K
E
3
100nF
2.2
D1 1N4004
OSC1
RB5
VR1
10k
IN
GND
100 F
16V
POWER
10
DOWN
C
IN
GND
OUT
UP
LED STROBE & TACHOMETER
ZD1
A
D1
K
A
K
Fig.5: the circuit is based on a PIC16F88-I/P microcontroller (IC1) and an 16 x 2 LCD module. External trigger signals
are applied to RB0 of IC1 via CON1, while RB4 & RB5 drive the white-LED strobe via transistor Q1. Power comes
from an external 12V DC plugpack, with regulator REG1 providing a +5V supply rail for IC1 and the LCD.
has positive going edges that are
60ms apart, the counter will count to
300,000 between each pulse. The value
of the count is then stored in a capture
register and the counter cleared so that
it is ready for the next count.
Next, a calculation is made to derive the RPM. This simply involves
dividing 300,000,000 (ie, the number
of pulses from a 5MHz counter in one
minute) by the register value. So if
the register value is 300,000, we get
1000 RPM.
Another calculation is made to derive the trigger frequency (50,000,000
divided by the register value).
This 1000 RPM calculation is made
in just 60ms and has a resolution of 1
in 300,000, thus giving a display resolution of 1 RPM. This is significantly
better than the method first described,
which involved counting the 16.66Hz
signal over a 1s period.
66 Silicon Chip
For the Generator mode, the operation is slightly different. The counter
still counts the 5MHz signal but in
this case, a calculation is made to
determine the value that the counter
must reach to provide the required
RPM value and strobe flash rate.
In this case, this calculation is
300,000,000 divided by the RPM setting. The calculated value is placed
in the compare register and when the
counter reaches this value, the strobe
is fired. The counter is then reset and
counts again to fire the strobe at the
set RPM rate.
Circuit details
Fig.5 shows the full circuit details
for the LED Strobe & Tachometer. It
consists of a PIC16F88-I/P microcontroller (IC1), a 16x2 LCD module and
not much else.
So in spite of the seemingly complex
operation, the circuit itself is really
very simple.
Most of the “smarts” are hidden
inside the micro, which is really the
heart of the circuit. It runs at 20MHz
using crystal X1 as its timebase and
this signal is also divided by four to
derive the 5MHz oscillator that’s used
for the RPM calculations.
In operation, IC1 monitors the external trigger signal (if one is present)
at its RB0 input, while RB1, RB3 &
RB2 monitor the Up, Down & Mode
switches respectively. In addition,
IC1’s AN4 analog port monitors the
position of potentiometer VR1 which
is used for fine RPM adjustments.
Note that RB1-RB3 have internal
pull-up resistors, so these inputs are
normally pulled high to +5V. When a
switch is closed, the associated input
is pulled to 0V and so IC1 can detect
this button press.
siliconchip.com.au
IC1 also directly drives the LCD
module. RA0-RA3 are the data outputs, while RB6 and RB7 drive the
register select and enable lines respectively. Trimpot VR2 sets the display
contrast voltage.
When IC1 is operating in trigger
mode, the signal applied to the RB0
input is used as the trigger for RPM
measurements. This input is protected
from excessive current using a 1kW
series resistor, while a 1nF capacitor
filters out any transient voltages to
prevent false counts.
The external trigger circuit is connected via a 3.5mm jack socket and
is fed with a +5V rail via the socket’s
ring terminal and a 2.2W resistor. The
tip carries the external trigger signal
and in the absence of signal, is pulled
high via a 10kW pull-up resistor to the
+5V rail.
Potentiometer VR1 is connected
across the 5V supply and the wiper can
deliver any voltage from 0-5V to the
AN4 analog input of IC1. IC1 converts
this input voltage to a digital value to
set the fine frequency adjustment over
a 100 RPM range (but only when IC1
is operating in the generator mode).
Note that the operational range of
VR1 has been deliberately restricted
to 0.54-4.46V. This has been done
because potentiometers often have
abrupt resistance changes towards the
ends of their travel. Using a 0.54-4.46V
range ensures that the more linear
section of the potentiometer is used.
Driving the strobe
IC1’s RB4 and RB5 outputs provide
R
Fig.6: the photointerruptor trigger
circuit uses a
slotted LED and
phototransistor
package, plus
a rotating vane
assembly attached
to the machine.
T
S
150
A
LED
3.5mm PLUG
(TO TRIGGER
INPUT CON1)
C
PHOTO
TRANSISTOR
A
K
E
K
PHOTO INTERRUPTOR TRIGGER CIRCUIT
the strobe LED drive. Each output
can source about 20mA into the base
of transistor Q1 which turns fully on
each time a positive going pulse is
applied.
Each time Q1 turns on, it also turns
on a 1W high-brightness white LED
which is connected via CON3 (provided S5 is closed). Power for this LED
is derived from the +12V supply rail
via reverse polarity protection diode
D1. A 39W 5W series resistor limits
the peak LED current to about 220mA.
This resistor value was chosen so that
even if the supply is 15V, the current
will still be below the 350mA maximum for a 1W Luxeon LED.
Switch S5 allows the strobe LED to
be manually switched on or off.
Power supply
Power for the circuit is derived from
an external 12V DC plugpack and this
is fed in via DC input socket CON2
and power switch S4. A 470mF 16V
capacitor decouples the +12V supply
which is then fed to regulator REG1
and the strobe, while a 10W resistor
and a 100mF capacitor provide additional decoupling for the supply to
REG1. Zener diode ZD1 clamps the
input to REG1 to 16V.
REG1’s +5V output is used to supply both IC1 and the LCD. This rail
is decoupled using a 100mF capacitor
directly at the regulator’s output, while
an additional 100mF capacitor and a
100nF capacitor bypass the supply
close to pin 14 of IC1. A 10mF capacitor provides additional bypassing for
the supply at the LCD module.
Photo-interruptor circuit
Fig.6 shows the circuit for the photointerruptor. It’s very simple and is
based on a slotted LED and phototransistor package, plus a vane assembly
that rotates in the slot.
Power for the circuit comes from
the +5V rail of the main circuit and is
applied via the ring (R) terminal of a
3.5mm jack. A 150W resistor limits the
150
R
T
A
IR
LED1
3.5mm PLUG
(TO TRIGGER
INPUT CON1)
100k
IC2: LM358
10 F
2
3
IC2a
5
1
6
100k
4
IR
SENS 1
A
S
100 F
10k
K
K
E
C
1k
8
IC2b
7
150
ACTIVE
AREA
470k
IR LED
IR SENSOR
1k
100 F
A
K
K
A
IR REFLECTOR AMPLIFIER CIRCUIT
Fig.7: the IR reflector amplifier uses an IR LED and an infrared photodiode (IR SENS1) to pick up the reflected light
pulses. The resulting current variations through IR SENS1 are then fed to current-to-voltage converter stage IC2a
which in turn drives amplifier stage IC2b. IC2b’s output then drives the trigger input of the main tachometer unit.
siliconchip.com.au
August 2008 67
Table 1: Capacitor Codes
LCD MODULE
X1 20MHz
100nF
IC1 PIC16F88-I/P
10 F
100nF
4-WAY
SOCKET
STRIP
1k
1nF
1k
100 F 100 F
CON2
+
10
ZD1
VR2
10k
470F 16V
27pF
REG1
7805
100 F
CON1
Value mF Code IEC Code EIA Code
100nF 0.1mF
100n
104
1nF
.001mF
1n0
102
27pF
NA
27p
27
D1
22 1
13
11
9
7
5
3
1
220
220
10k
2.2
14
14 13
27pF
18070140
CON3
3-WAY SOCKET STRIP
VR1
39 5W
Q1
E B ORTS DEL
MAIN BOARD
S4
3-PIN SIL
HEADER
(UNDER
BOARD)
S1
04107082
SWITCH BOARD
S2
LED STROBE SWITCH
S3
4-PIN SIL
HEADER
(UNDER
BOARD)
S5
Fig.8: follow this layout diagram to install the parts on the main board and to
assemble the small switch board. Take care with the orientation of the switches
– they must all be installed with their flat sides to the left.
Below: this view shows the completed
main board assembly prior to mounting
the LCD module and switch board.
LED current to around 20mA.
With no vane in the slot, the photo
transistor is illuminated by the LED.
As a result, the phototransistor turns
on and its collector pulls pin 6 of microcontroller IC1 low via the tip connection of the jack socket. Conversely,
when a vane passes through the slot,
68 Silicon Chip
the phototransistor turns off and its
collector is pulled to +5V via the 10kW
pull-up resistor on the main circuit
IR reflector amplifier
The optical pick-up circuit is a bit
more complicated – see Fig.7. It’s
based on an infrared LED (IRLED1),
an infrared photodiode (IR SENS1)
and an LM358 dual op amp (IC2).
The infrared LED is powered via a
150W resistor from the +5V 3.5mm
jack connector ring terminal and operates continually while ever power
is applied.
As mentioned previously, the
photodiode is aimed at the rotating
machine and the light is reflected
back to the photodiode via a blade or
a reflective strip attached to a shaft.
The infrared photodiode is connected to pin 2 of IC2a. This op amp
is wired as an inverting amplifier
and operates as a current-to-voltage
converter. As shown, its non-inverting
(pin 3) input is biased to about 0.5V by
a voltage divider consisting of series
10kW and 1kW resistors connected
across the 5V supply.
In operation, the current through the
photodiode varies with the reflected
light and these current variations are
converted to voltage variations at
IC2a’s pin 1 output. This signal is
then AC-coupled to pin 5 of IC2b
via a 10mF capacitor.
IC2b is connected as a noninverting amplifier with a gain
of 471, as set by the 470kW
feedback resistor and the 1kW
resistor at the inverting input.
As with IC2a, IC2b is also biased
to about 0.5V by the series 10kW
and 1kW resistors across the 5V
supply. The 100kW resistor between
pin 5 and this 0.5V supply ensures
that, in the absence of signal from IC2a,
IC2b’s output normally sits at 0.5V.
Each time sufficient light is reflected
onto the infrared photodiode, IC2b
amplifies the signal from IC2a and
its output swings to about 4.5V. This
signal is then fed to the tip of a 3.5mm
jack plug via a 150W isolating resistor
and applied to pin 6 of IC1.
Construction
The main LED Strobe and Tacho
meter circuit is built on two PC boards:
a main PC board coded 04108081 (115
x 65mm) and a switch PC board coded
siliconchip.com.au
The 14-way DIL header is installed
from the underside of the LCD module
and soldered to the pads on the top of
the module’s PC board.
04108082 (52 x 15mm). This switch
board plugs into the main board and
the assembly is housed in a bulkhead
style case with a clear lid.
Another two boards are used for the
photo-interruptor and IR reflector amplifier circuits. The photo-interruptor
board is coded 04108083 and measures
50 x 25mm, while the IR reflector amplifier board is coded 04108084 and
measures 53 x 32mm.
Fig.8 shows the main board assembly details. Begin by first checking the
board for any defects. Check also that
the hole sizes for the connectors and
potentiometer VR2 are correct by test
fitting these parts. Enlarge these holes
so that the parts do fit, if necessary.
In addition, the holes for the four
corner mounting screws, the LCD
mounts and for REG1 must be 3mm in
diameter. Check also that the PC board
is cut and shaped (note the corner cutouts) so that it fits into the box.
Once these checks have been completed, install the two wire links then
solder the resistors in position. Table
2 shows the resistor colour codes but
you should also check each value using a digital multimeter (DMM) before
soldering it to the board.
Follow these parts with the 10 PC
stakes. Seven PC stakes are used for
Once the header has been attached, the LCD module is plugged into matching
socket strips on the main board and secured to four M3 x 9mm Nylon spacers.
The main PC board
assembly is completed
by plugging the switch
board into its matching
header strips.
Table 2: Resistor Colour Codes
o
o
o
o
o
o
o
o
o
siliconchip.com.au
No.
1
2
2
4
2
2
1
1
Value
470kW
100kW
10kW
1kW
220W
150W
10W
2.2W
4-Band Code (1%)
yellow violet yellow brown
brown black yellow brown
brown black orange brown
brown black red brown
red red brown brown
brown green brown brown
brown black black brown
red red gold brown
5-Band Code (1%)
yellow violet black orange brown
brown black black orange brown
brown black black red brown
brown black black brown brown
red red black black brown
brown green black black brown
brown black black gold brown
red red black silver brown
August 2008 69
The main PC board assembly
is secured to integral pillars
inside the case using four
self-tapping screws. Be sure
to fit heatshrink tubing over
the lead connections to the
switches and the PC stakes,
to prevent the leads from
breaking after they have been
soldered.
potentiometer VR1, three for its terminals and four more to support its
body. The remaining three PC stakes
are used to terminate the wiring from
switches S4 & S5.
Next, install diode D1, zener diode
ZD1 and a socket for IC1, taking care
with their orientation. That done,
install the 3-way and 4-way single inline (SIL) socket strips that are used to
mount the switch board. These socket
strips made by cutting down an 8-pin
IC socket using a hobby knife or side
cutters. Clean up the edges of these
socket strips with a small file before
soldering them in position.
Similarly, the LCD module is conVR1
LCD MODULE
BOX
39 5W
MAIN BOARD MOUNTED ON INTEGRAL
STANDOFFS USING SMALL SELF TAPPERS
nected via a 14-pin DIL socket strip.
This is made by cutting a 14-DIL IC
socket to produce two 7-way strips
which can then be installed adjacent
to each other on the board.
The capacitors can go in next. Note
that the electrolytic types are polarised
and must be oriented as shown. Note
also that the 470mF capacitor goes
under the LCD module and must be
mounted horizontally (ie, with its
body flat against the PC board). The
100mF capacitor to the left of IC1 must
also lie horizontally – see photos.
Next on the list is regulator REG1.
As shown, this device also mounts
horizontally on the PC board, with its
PC BOARD
LCD MODULE ON 9mm LONG
M3 TAPPED SPACERS
6mm LONG
M3 SCREWS
Fig.9: this diagram shows how the main board assembly is secured to the case
pillars and how the LCD module is secured to the M3 x 9mm Nylon spacers.
70 Silicon Chip
leads bent down by 90° to go through
the relevant holes.
To do this, first bend the two outer
leads down about 9mm away from
its body and the middle lead down
about 6mm away. The device is then
fastened into position using an M3 x
6mm screw, nut and washer and its
leads soldered.
Don’t solder REG1’s leads before
bolting its tab down. You could crack
the PC tracks or lift the solder pads as
the nut is tightened down if you do.
The DC sockets, the 3.5mm PCmount jack socket and trimpot VR2
can now be installed, followed by
potentiometer VR1. Before mounting
VR1 though, it will be necessary to
cut its shaft to a length of about 14mm
(from the end of its threaded boss), to
suit the knob used.
As shown in the photos, the pot is
mounted upright on the PC board, with
its body soldered to four PC stakes.
Note that you will have to scrape
away some of the coating on the pot
body at each solder point, in order to
get the solder to “take”. Once it’s in
position, solder its three terminals to
their adjacent PC stakes.
The LCD module is connected via
siliconchip.com.au
Parts List
Main Unit
1 PC board, code 04108081,
115 x 65mm
1 PC board, code 04108082,
52 x 15mm
1 bulkhead case with clear front,
120 x 70 x 30mm (Jaycar HB6082 or equivalent)
1 12VDC 350mA plugpack
1 1W Luxeon white LED or Cree
XR-C white LED with collimator lens
1 small torch to house LED and
optics
1 2.5mm DC line plug
1 LCD module with backlight
(Jaycar QP-5516 or equivalent)
1 16mm 10kW linear potentiometer (VR1)
1 10kW horizontal trimpot (code
103) (VR2)
1 knob to suit potentiometer
1 20MHz parallel resonant crystal (X1)
2 PC-mount 2.5mm DC sockets
1 PC-mount stereo 3.5mm jack
socket
3 click-action PC-mount switches
(S1-S3)
2 sub-miniature SPDT toggle
switches (S4,S5)
1 14-pin DIL header (2.54mm
pin spacing)
1 4-way SIL header (2.54mm
pin spacing)
1 3-way SIL header (2.54mm
pin spacing)
1 14-pin DIL IC socket (cut to
suit the 14-pin DIL header)
a 14-way pin header strip at one end
and is supported on four M3 x 9mm
at its corner positions. We’ll describe
how the header strip is fitted to the
LCD module shortly. For the time being, just fit the four Nylon spacers to
the PC board and secure them using
M3 x 6mm machine screws.
Switch board
There are just three switches and
two header strips on the switch board
– see Fig.8. Install the three switches
first, taking care to ensure that the
flat side of each switch is oriented
correctly. The 3-pin and 4-pin header
strips can then be installed.
siliconchip.com.au
1 8-pin DIL IC socket (cut to
make a 4-way SIL socket and
a 3-way SIL socket)
1 18-pin DIL IC socket
4 9mm M3 tapped Nylon spacers
8 M3 x 6mm screws
1 M3 x 10mm screw
1 M3 nut
4 No.4 x 6mm self-tapping screws
1 80mm length of 0.7mm tinned
copper wire
1 500mm length of medium-duty
hookup wire
1 30mm length of 1.5mm heatshrink tubing
10 PC stakes
Photo Interrupter Detector
1 PC board, code 04108083,
50 x 25mm
1 photo-interruptor (Jaycar ZD1901 or equivalent)
1 150W 0.25W resistor
1 3.5mm stereo jack plug
2 M3 x 6mm screws
2 M3 nuts
3 PC stakes
1 1m length of 2-core shielded
cable
IR Reflector Amplifier
Capacitors
1 470mF 16V low-ESR electrolytic
3 100mF 16V PC electrolytic
1 10mF 16V PC electrolytic
5 100nF MKT polyester
1 1nF MKT polyester
2 27pF ceramic
1 PC board, coded 04108084,
53 x 32mm
1 plastic utility box, 82 x 53 x
31mm
4 M3 tapped 6mm Nylon spacers
4 M3 x 12mm countersunk
screws
4 M3 nuts
1 LM358 dual op amp (IC2)
1 infrared photodiode (IR SENS1)
1 infrared LED (IR LED1)
2 100mF 16V PC electrolytic
capacitors
1 10mF 16V PC electrolytic
capacitor
1 1m length of twin-core shielded cable
1 cable gland to suit 3mm cable
1 3.5mm stereo PC-mount jack
socket
3 PC stakes
Resistors (0.25W, 1%)
1 10kW
1 39W 5W
2 1kW
1 10W
2 220W
1 2.2W
Resistors (0.25W, 1%)
1 470kW
2 1kW
2 100kW
2 150W
1 10kW
Semiconductors
1 PIC16F88-I/P microcontroller
programmed with 0410808A.
hex(IC1)
1 7805 5V 3-terminal regulator
(REG1)
1 BC337 NPN transistor (Q1)
1 1N4004 1A diode (D1)
1 16V 1W zener diode (ZD1)
Both headers are mounted on the
copper side of the board. In each case,
the longer pins of the header are first
pushed into their mounting holes so
that they sit about 1mm above the top
of the board. That done, solder the
pins to the board pads, then slide the
plastic spacer along the pins towards
the PC board, so that it rests against
the soldered joints – see photo.
Once the assembly is finished,
the assembled switch board can be
plugged into the main board.
Fitting the LCD header
The next step in the assembly is to
fit a 14-pin DIL header to the lefthand
end of the LCD module. As before, this
header is installed from the underside
of the module.
Before soldering the header pins,
you first have to adjust the plastic
spacer so that the pins will protrude
exactly 8mm below the module’s PC
board. This is done by simply placing
the pins on a flat surface and then sliding the spacer along them in one direction or the other so that the pin length
below the spacer is about 5.5mm (the
spacer thickness is 2.5mm).
Once this adjustment has been
made, the header can be installed from
the underside and the pins soldered
to the pads on the top of the module.
August 2008 71
Specifications
Generator Mode
RPM Range: 1 RPM (0.0166Hz) to 65,535 RPM or 1092Hz
Accuracy: within 1 RPM at 17,000 RPM, 1.33 RPM at 20,000 RPM
Adjustment: 100 RPM coarse steps with separate 1 RPM fine adjustment
over a 100 RPM range
Display: both RPM and Hz
Display Resolution: 1 RPM and 0.01Hz
Flash Period: adjustable from 32ms to 6.50ms in 25.4ms steps or adjustable
from 1-10% of period
Display Update Period: 200ms
Triggered Mode
A larger-than-life size view of the 1W
white LED. It is wired using a 1.5m
length of shielded 2-core cable. Solder
the red wire to the positive terminal
and the white wire to the negative
terminal and cut the shield wire off
short.
RPM Range: 1 RPM (0.0166Hz) to 65,535 RPM (1029Hz) recommended
maximum
Don’t plug the LCD module in at this
stage though.
Accuracy: within 1 RPM at 17,000 RPM, 1.33 RPM at 20,000 RPM
Voltage checks
Display: both RPM and Hz
Display Resolution: 1 RPM and 0.01Hz
Flash period: adjustable from 32ms to 6.50ms in 25.4ms steps, or adjustable
from 1-10% of period
Display Update Period: 200ms but can be slower for measurements below
300 RPM (5Hz) and with averaging.
Division Ratios: 0.5, 1, 2, 3, 4, 5, 6, 7 & 8
Flash Position: can be shifted to any pulse edge or edge number when the
division ratio is 2 or more
Averaging: from 1-10 measurements for measurements over 300 RPM,
reducing in number at lower RPM
Trigger Edge: rising or falling (user selectable)
Flash Period: setting can be either fixed or automatic
Before applying power, check that
IC1 is out of its socket and that the
LCD module is unplugged. That done,
temporarily wire in power switch
S4, apply power and check for 5V
between pins 14 & 5 of IC1’s socket.
If this is correct, switch off, remove
the switch and install both IC1 and
the LCD module.
Note that there is a tab beneath the
LCD module (bottom, centre) that
needs to be bent flat against the module’s PC board, so that it clears IC1.
Secure the LCD module in place using
four M3 x 6mm screws.
Flash Delay From Triggered Edge To Flash: 8.75ms
Preparing the case
Reflective Trigger Range: 65mm for off-white plastic, 95mm for white paper
If you are buying a complete kit,
the case will probably be supplied
pre-drilled and with screen-printed
lettering. If not, then you will have to
drill the holes yourself.
The first step is to drill two 6mm
holes in the side of the case to provide
access to DC sockets CON2 & CON3.
These holes should be located 9mm
down from the top of the base and
17mm and 27mm in from the outside
front edge.
Next, drill another 6mm hole in the
other end of the case for CON1. This
hole must be positioned 13mm down
from the top and 29mm in from the
outside top-front edge of the case. The
PC board can then be fitted in place
and secured on the integral standoffs
using No.4 self-tapping screws.
Now for the lid. Fig.10 shows the
full-size artwork for the lid and this
can be attached to the inside of the lid
SILICON
CHIP
POWER
ON
STROBE
ON
LED STROBE & TACHOMETER
TRIGGER
IN
DC IN
FREQUENCY
(FINE ADJ)
STROBE
OUT
MODE
DOWN
UP
Fig.10: this full-size artwork can be used as a drilling template for the front panel.
72 Silicon Chip
siliconchip.com.au
The connecting cable is secured to the
back of the 1W white LED assembly
using silicone sealant.
Silicone sealant is also used to secure
the collimator lens inside the front
assembly of the torch.
and used as a drilling template. You
can either photocopy the artwork in
the magazine or you can download and
print out the artwork from the SILICON
CHIP website.
All holes in the lid should initially
be drilled using a small pilot drill,
then carefully enlarged to size using
a tapered reamer. Switches S1-S3
require 10mm holes, S4 & S5 require
5mm holes and VR1’s shaft requires
a 7mm hole.
Once the holes have been drilled,
fit switches S4 & S5 and wire them
to the PC board. It’s a good idea to fit
heatshrink tubing over these connections, to prevent the wires from breaking (hint: push the heatshrink tubing
over the switch wires before soldering
the connections, then slide the tubing
into place and shrink it down).
The assembly of the main unit is
now complete. Now let’s build the
strobe unit.
Testing
Strobe construction
The first step here is to apply power
and adjust VR2 for best contrast on
the LCD. The display should show
a reading of between 1000 RPM and
1100 RPM on the top line and 16.66Hz
on the bottom line. The Mode should
be GEN.
If this checks out, attach the lid and
mounting brackets to the case using
the four screws supplied.
Now check that the RPM value can
be adjusted over a 100 RPM range using
potentiometer VR1. Similarly, the UP
and DOWN switches should change
the reading in 100 RPM steps.
The default flash period is set to automatic at 5% in generator mode. In the
triggered mode, the defaults are: edge
is rising, division is 1, flash period is
automatic at 5% and averaging takes
place over two measurements.
As shown in the photo above, the
1W white LED for the strobe is housed
in a small plastic torch housing. The
original reflector inside the torch was
removed and the LED and its associated collimator lens placed just behind
the front torch lens.
Depending on the torch, the reflector may be easy to remove or it may be
integrated with the screw thread that
secures the front assembly to the torch
body. In the latter case, the reflector
can be removed by cutting around its
perimeter using a hobby knife.
The 1W white LED is wired using a
1.5m-length of shielded 2-core cable.
Connect the red wire to the positive
LED terminal, the white wire to the
negative terminal and cut the shield
wire off short. Once it’s wired, secure
this lead to the back of the LED as-
siliconchip.com.au
The 1W white LED is then clipped
into the collimator lens and secured
using additional silicone sealant.
This is the completed strobe assembly.
A knot tied in the cable (or a cable
tie) will prevent the cable from being
pulled out through the end cap.
sembly using silicone sealant.
Silicone sealant is also used to secure the collimator lens to the front
lens assembly of the torch. Once it’s in
place, leave it to cure for several hours,
then clip the LED assembly to the back
of the collimator lens and secure it using additional silicone sealant. Leave
this assembly to cure overnight.
Once the silicone has cured, feed
the lead from the LED through a hole
drilled the rear end-cap of the torch.
Use a cable tie or tie a knot in the wire
to prevent the wire being pulled out of
the end of the torch when the end-cap
is refitted.
The far end of the cable is fitted
with a 2.5mm DC plug. Connect the
red (positive) lead to the centre pin of
the plug and the white (negative) lead
to the earth terminal.
That’s all we have space for this
month. Next month, we’ll show you
how to build the IR Reflector Amplifier and Photo-Interruptor boards and
SC
describe how the unit is used.
August 2008 73
SILICON
CHIP
If you are seeing a blank page here, it is
more than likely that it contained advertising
which is now out of date and the advertiser
has requested that the page be removed to
prevent misunderstandings.
Please feel free to visit the advertiser’s website:
www.altronics.com.au/
SILICON
CHIP
If you are seeing a blank page here, it is
more than likely that it contained advertising
which is now out of date and the advertiser
has requested that the page be removed to
prevent misunderstandings.
Please feel free to visit the advertiser’s website:
www.altronics.com.au/
SILICON
CHIP
If you are seeing a blank page here, it is
more than likely that it contained advertising
which is now out of date and the advertiser
has requested that the page be removed to
prevent misunderstandings.
Please feel free to visit the advertiser’s website:
www.altronics.com.au/
SILICON
CHIP
If you are seeing a blank page here, it is
more than likely that it contained advertising
which is now out of date and the advertiser
has requested that the page be removed to
prevent misunderstandings.
Please feel free to visit the advertiser’s website:
www.altronics.com.au/
DSP Musicolour:
calibrating and
operating
PT.3: By
MAURO GRASSI
In last month’s article, we detailed the construction of the DSP
Musicolour. In this month’s article, we guide you through the final
testing of the DSP Musicolour and give troubleshooting tips. We
also explain the operation of the firmware in more detail as well as
discussing possible accessories.
W
hile the circuit of the DSP Musicolour (published in
June) may at first seem complicated, it is relatively
simple when you consider all the features that we
have been able to pack into this powerhouse. Check out the
list opposite. We think you’ll agree!
We assume that you have read the first and second parts
of the article in the previous two issues of SILICON CHIP.
If you have followed the construction in last month’s issue,
you should have a fully assembled DSP Musicolour in its
case and you should have tested the supply rails at test
points TP0 and TP1. These should have measured close to
their correct values of +5V and +10V respectively.
If they do not measure close to these values, you should
refer to the troubleshooting section below for further hints,
although we mentioned some extra checks to perform in that
case in last month’s issue, to which you should refer first.
In last month’s article, we mentioned that LK4 is optional
78 Silicon Chip
and is normally omitted. When LK4 is omitted, the DSP
Musicolour has three independent audio inputs which can
be used to modulate the output channels. These are the
Microphone input, the Left Audio channel and the Right
Audio Channel.
The Left and Right Audio channels from the speaker
terminals on the back panel are attenuated by the LEFT and
RIGHT potentiometers on the front panel. The Microphone
line input is a mix of the on-board electret microphone signal and any external microphone connected to the 6.5mm
jack on the back panel.
When LK4 is installed, however, the Left and Right Audio
channels from the back panel are mixed in hardware before
being digitised by the microcontroller. In this case, either
the LEFT or RIGHT potentiometer can be used to attenuate
the input signal before it is digitised (and you should not
install both potentiometers).
siliconchip.com.au
POTENTIOMETERS
FFT
AMPLITUDES
&
EQUALISATION
OP
AMP
AUDIO
CHANNEL
INPUTS
OP
AMP
MIC
INPUT
DIGITISING
AND
SOFTWARE
MIXING
LOGICAL
OUTPUT
CHANNEL
LEVELS
SET
PHYSICAL
OUTPUT
CHANNEL
LEVELS
SET
OP
AMP
Fig.1: block diagram of the DSP Musicolour. Use
this in conjunction with the text to understand
operation, programming and calibration.
In other words, when LK4 is installed you lose one
independent audio channel but you need only one potentiometer on the front panel. LK4 therefore controls
whether the DSP Musicolour Left and Right audio channels are mixed in hardware or software (Dual mono or
joint stereo). The most common option is to omit LK4 and
to disable hardware mixing.
With regards to the jumper links LK5 and LK6, we mentioned in the first part of the article that the default is to
have LK5 installed and LK6 omitted. In fact, the firmware
will ignore the state of links LK5 and LK6 – it does not
matter if they are installed or not.
Power up
First, make sure that the plastic case has been screwed
shut. When you first apply power, you should see the start
up screen scroll past on the dot matrix LED display. The
DSP Musicolour will go through a number of tests and then
go to its default state. If you do not, you should switch off
mains power immediately and go to the Troubleshooting
section below.
Boot-Up sequence
When the DSP Musicolour first boots up, it goes through
a number of internal checks before commencing operation.
The following occurs on boot up (in chronological order):
1. The firmware displays the start up screen and its version
number (this can be disabled for a quicker boot by changing
the start up settings in the SYSTEM>Startup sub-menu).
2. The firmware measures the frequency of the mains supply. If the measured value is within tolerance, the firmware
accepts the measured value and assigns its internal settings
for either 50Hz or 60Hz operation (the firmware chooses
the value closest to the measured frequency).
If the measured value is not within tolerance, the firmware will display a warning indicating that no mains was
detected and will default to 60Hz operation. In normal
mains powered operation, this warning should never be
seen. If it is, it indicates a problem with the Musicolour’s
zero crossing detection system.
The fallback value of 60Hz was chosen because it is the
safer value for the purpose of controlling the Triacs in the
output stages.
siliconchip.com.au
TRIGGER
OUTPUT LEVELS
FROM FFT SYSTEM
CHASER
PROGRAM
VIRTUAL
MACHINE
OUTPUT LEVELS
FROM CHASER
PROGRAM
DSP MUSICOLOUR FEATURES
1. Selectable 8-band equaliser
2. Auto detection of mains frequenc
y (50Hz or 60Hz)
3. Selectable phase-controlled or zero
voltage-switched
output channels (8-bit resolution)
4. For each logical output channel:
(a) Selectable gain
(b) Selectable audio passband
: arbitrary minimum
and maximum frequencies
(c) Selectable acquisition mod
e: peak or average
(d) Selectable quiescent level
(filament preheat)
(e) Selectable zero voltage mod
e, strobe mode,
direct mode or continuous
mode
5. Selectable logical channel for each
physical output channel
6. Chaser modes implemented as a
virtual machine
7. Trigger channel with:
(a) Selectable audio passband
(b) Selectable trigger threshol
d
8. Firmware support for RC5 remote
control (requires
additional PC board; to be described
next month)
9. Firmware support for high speed
UART (requires
additional PC board)
10. Selectable balance
11. Selectable display frequency, brig
htness and screen
saver time-out period
12. Selectable sampling frequency from
16kHz to 50kHz
simultaneous on all channels
13. Real time 7-bit FFT using double
buffering
14. Persistent software settings and
multiple non-volatile
user memories
15. Self calibration and Diagnostics
16. Automatic and manual tuning of
the internal fast
RC oscillator for increased accuracy
17. Adaptive potentiometer controls
18. Silence detection and triggering
19. Input op amp stage clipping dete
ction
August 2008 79
3. If you are running from a 50Hz supply and somehow the
frequency is not properly detected and defaults to 60Hz, the
shorter mains period will at worst mean that less power is
delivered to the output loads. Therefore even if your mains
supply is 50Hz and the detection fails, at least the outputs
will not flicker. Flickering can occur when the Triacs are
switched on beyond the next zero crossing of the mains
waveform and should not occur in normal operation.
Another fail-safe feature is that in the rare event that no
good mains frequency is detected, the firmware will disable
all output channels (the rest of the firmware will function
normally, however);
4. The firmware will load any persistent settings from
the last active session and initialise all internal peripherals,
including enabling all interrupts in the correct sequence;
5. The firmware will detect and enable any connected
accessories. It is possible to add a small infrared remote
control PC board to the main board to allow the DSP Musicolour to be operated by a standard RC5 remote control.
Also, the firmware implements a RTSP (Run Time Self
Programming) server in a secure part of program memory
(it also switches the interrupt vectors to an alternative location), which can be used with a UART. The DSP Musicolour
is highly customisable but for most applications you will
not need to change any settings, as the preloaded defaults
should be adequate.
6. The firmware will jump to the main loop (described
below).
Automatic Calibration
Although the DSP Musicolour will adjust its settings according to the detected mains frequency, all its calculations
assume a fixed system clock.
The system clock is derived from the microcontroller’s
(dsPIC30F4011) internal fast RC oscillator (nominally
7.37MHz) and a 16xPLL multiplication stage is used to
achieve around 30MIPs operation (4 clocks per instruction).
Since this oscillator’s frequency tolerance can be relatively high due to internal manufacturing variations, it may
be necessary, if you are experiencing unusual effects like
flickering lights on the output channels, to calibrate the
frequency as close to 7.37MHz as possible. This is a good
thing to do just in case.
The dsPIC30F4011 has an internal non-volatile calibration setting to achieve this, meaning the internal fast RC
oscillator can be tuned to bring it as close as possible to its
intended frequency. The firmware assumes that the mains
line frequency is very close to its theoretical value of either
50Hz (if you are in Australia, Europe and most other parts
of the world) or 60Hz (if you are in America, Japan and a
few other places).
Since the mains frequency can be measured by the
firmware against the system clock, the firmware can then
calculate the error in the internal fast RC oscillator and
automatically adjust it to minimise the error.
This is what the firmware does in its automatic calibration. It will run once when you first power up but if you
need to, you can also do it manually.
To do this, go to the ADVANCED>Calibration sub-menu.
If you wish to see how far from the ideal the microcontroller
is operating, go to the INFORMATION>Error menu and the
current percentage error in the measure mains frequency
will be displayed.
The Main Loop
After boot up, the firmware spends most of its time in the
main loop, whereby the Musicolour is either in Automatic
mode (AUTO LED is lit) or User Mode (USER LED is lit).
Either way, the AUTO LED or the USER LED will flash if
there is no input signal detected. The SET LED will also
flash if there is clipping (overload) in the op-amp stages of
either the Left or Right audio input channels.
While clipping is very undesirable in an audio amplifier,
greatly affecting the sound quality, its effect may actually
help in getting a good display from the DSP Musicolour.
So the detection of clipping is merely an indication that
you may want to turn down the LEFT and RIGHT potentiometers.
While in the main loop, you may enter the menu system by pressing the SET button. The display is refreshed
according to the currently selected display. The selected
display can be scrolled to the next available display using
the AUTO button when already in Automatic Mode and
the USER button when already in User Mode.
Some of the implemented main loop displays are shown
in Table 1. Note that they do not affect the internal operation
of the DSP Musicolour; they only affect what the display
shows.
In the main loop in Automatic Mode, the CH1-CH4 LEDs
will light according to the logical output channel levels.
The main difference between Automatic mode and User
Mode is that in Automatic mode the Musicolour uses its
current settings for all functions, whereas in User Mode, one
of four previously stored settings profiles is used instead.
Thus User Mode can be used to quickly run the Musicolour in a previously set configuration. In User Mode, the
CH1-CH4 LEDs will indicate one of the four preset profiles
currently active. You may press the CH1-CH4 buttons to
Table 1: The display modes in the main loop
Spectrum Fine:
The spectrum is displayed on the display from lowest to highest frequency (left to right).
Spectrum Centered:
The spectrum is displayed in centred mode.
Logical Channel Displayed Single:
The output levels of each channel are displayed. The top horizontal bar indicates the first logical
channel’s level. The third horizontal bar from the top indicates the second logical channel’s level.
Similarly, the fifth and seventh horizontal bars from the top indicate the third and fourth logical
channels’ levels respectively.
Logical Channel Display Averaging:
Same as above except every horizontal bar in between the output channel bars is the average
of the previous and next bars.
RMS display:
Displays the RMS level of the input signal as an analog meter.
80 Silicon Chip
siliconchip.com.au
change the preset on the fly while in User Mode.
The main loop running in Automatic or User Mode consists of the following sequence, which is diagrammatically
represented in Fig.1.
Logical and physical channels
We should first mention that the firmware supports four
logical output channels and four physical output channels.
The physical output channels correspond to the outputs on
the back panel. Each of these can be associated to a logical
channel. In normal operation, the physical channel N is
associated to the logical channel N.
However, added effects can be achieved by changing
the mapping from output channels to logical channels.
For example, you can have all four physical channels on
the back panel controlled by one logical output channel.
We now explain the operation of the main loop. As
can be seen in Fig.1, the three inputs consisting of the
Left and Right audio inputs and the Microphone inputs
are digitised and mixed according to the balance settings
under AUDIO>Balance. Any combination of these three
channels can be used as the input signal. The result of
this software mixing is passed to the FFT (Fast Fourier
Transform) system.
The output of the FFT resolves the captured slice of the
input audio waveform into 128 (27) frequency amplitudes.
These are equally spaced from 0Hz up to the sampling frequency. The smallest frequency that the FFT can resolve
is F/128, where F is the sampling frequency. For example,
when F is 48kHz we can resolve down to 375Hz or ±137Hz.
If you are not very interested in the audio sub-band above,
say, 10kHz, then you can lower the sampling frequency
to 20kHz and the FFT will be able to resolve frequency
components down to 156Hz or ±78Hz.
The audible spectrum for humans is nominally from
about 20Hz to 20kHz. Although the sampling frequency
of the ADC system can be set anywhere from 16kHz up to
50kHz, keep in mind that according to the Nyquist sampling
theorem the highest frequency that can be resolved using a
sampling frequency F is F/2.
This means that aliasing will occur at least somewhere
in the audible spectrum if the ADC system’s sampling
frequency is set below about 44kHz. Aliasing is usually an
unwanted characteristic of a digitising system. However,
since most music has very little high harmonic content, in
fact little content above 4kHz, it may be desirable to lower
the sampling frequency in order to increase the resolution
of the FFT.
The FFT system computes logical output channel
levels in two acquisition modes. These can be set in the
CHANNELS>Mode sub-menu.
The two acquisition modes are PEAK and AVERAGE.
In AVERAGE mode, the average of the relevant frequency
components falling within the channel’s passband (set by
the minimum and maximum frequencies for the channel)
will be the output level requested in the output stage. In
PEAK mode, however, only the maximum level within the
channel’s passband will be the output level requested in
the output stage.
There is an optional Equaliser module which can be enabled or disabled. The levels of the equaliser can be changed,
however, by going to the AUDIO>Equaliser sub-menu.
The equaliser has eight bands set to affect preset portions
siliconchip.com.au
Warning!
The DSP Musicolour operates
from the 230/240V AC
mains and many internal compon
ents and sections of the
PC board tracks are also at mains
potential. Contact with
any of these could be FATAL.
DO NOT TOUCH any of these parts
unless the power cord
is unplugged from the mains supp
ly. DO NOT CONNECT
this device to the mains unless
it is fully enclosed in the
specified case.
This project is not for the inexperi
enced. Do not build
it unless you know exactly wha
t you are doing and are
completely familiar with mains
wiring practices and construction techniques.
of the audible spectrum. The current equaliser bands can
be seen under the INFORMATION>Equaliser sub-menu
and cannot be changed by the user (it can be changed by
reprogramming the device however).
Note that the equaliser affects the output of the FFT, not
the input. After any equalisation is performed, the levels
of the logical output channels are set by the FFT system,
if the chaser mode is set to OFF (see the CHASER>Mode
sub-menu below).
If the chaser mode is not set to OFF then the level data produced by the FFT system is ignored and the data produced
by the current chaser program (see the CHASER>Program
sub-menu below) is used to set the logical output channel
levels instead. If the chaser mode is set to TRIGGERED, then
the trigger pulse (produced by the FFT system) is used to
step through the chaser program.
Triggering
Triggering can either occur directly from the Trigger
channel or from the Silence detection. Silence detection
triggers when there is a relative silence in the input Left
or Right audio signals (the MIC input is not used for the
silence detection).
The trigger can be considered a separate logical channel.
It has its own selectable passband and threshold. When the
threshold is reached the trigger occurs. The trigger is used
by the chaser system to trigger the current chaser program
in TRIGGERED mode.
Tips: If, for example, you want bass response triggering a pre-set chaser program, you would set the TRIGGER
minimum frequency to 0Hz and the maximum frequency
to around 300Hz. Then adjust the threshold level to get an
acceptable level of triggering.
Light Chaser
The chaser program is either executed at the rate set in
OUTPUT>Output Rate or each step in the program is triggered. Both the Chaser system and the FFT system produce
a set of output levels for the logical output channels. Depending on the chaser mode being used, the chaser levels
or the FFT levels will be used to change the levels of the
logical output channels. These will then affect the physical
output channels.
Channel Modes and Settings
Each of the four logical output channels can operate in
one of four primary modes: DIRECT mode, CONTINUOUS
August 2008 81
Mode, ZV Mode or STROBE mode.
In the DIRECT and CONTINUOUS modes, the brightness
of the logical output channel is varied in 256 levels (8 bit
resolution). The output brightness is approximately linear
as the firmware uses an internal dimming curve to correct
the non-linearity inherent in phase control. The difference
between DIRECT and CONTINUOUS mode is how the
output level is set by the output system.
The main difference between the DIRECT and CONTINUOUS modes is that while in DIRECT mode the brightness
is set directly, in CONTINUOUS mode, the brightness is
“continuously” modified from the current brightness level.
In other words, in CONTINUOUS mode, if the requested
level is higher than the current level, the current level is
increased by the ATTACK setting for the channel, while
if the requested level is lower than the current level, the
current level is decreased by the DECAY setting for the
channel. Setting different ATTACK and DECAY levels for
the channel can affect the level of the output logical channels in CONTINUOUS mode.
In ZV Mode, the output channel responds as in DIRECT
and CONTINUOUS modes, except that the output is not a
brightness level but a digital output. The output is either
fully on or fully off. This mode approximates a zero voltage
switching mode and can be used to reduce RF interference
or achieve a digital effect.
In STROBE Mode, the output level sets the frequency
of the logical output channel rather than the brightness
level. The strobe frequency will be set from the maximum
(equal to the mains supply frequency, either 50Hz or
60Hz, down to 1/256th of the mains supply frequency,
ie. around 0.2Hz).
Quiescent Level or Filament Preheat
In all channel modes except STROBE, each logical output channel has a settable quiescent level, which is used
to reduce the stress on the filaments in your incandescent
lamps and to reduce surge currents through the Triacs at
switch on.
The quiescent level can be set by going to OUTPUT>
Fig.2: one of the physical output channels being switched
without software correction for asymmetrical phases.
The yellow trace is the output of the Triac while the green
trace is the trigger pulse applied to the gate through
the optocouplers.
82 Silicon Chip
Quiescent Level and is settable from 0 to 25% of the full
brightness level. Note that if the channel mode is ZV (zero
voltage switching) and the Quiescent Level is not 0% the
channel may seem to be continuously on, depending on
the ZV threshold. In this case, you should set the Quiescent
Level to 0% or disable ZV mode or change the ZV threshold
by going to OUTPUT>ZV Threshold.
A closer look at the operation of the Musicolour
The Triacs are controlled through the optocouplers using
the four output compare channels of IC1 (dsPIC30F4011).
In order to maintain a constant brightness of the output
lights, it is necessary for the switch-on pulses to the Triacs
to be synchronised to the frequency of the mains supply.
To achieve this, the microcontroller uses the INT0 external interrupt pin which is supplied by one side of the
transformer’s secondary winding. An interrupt can be triggered on a rising or falling edge of INT0. Now a low level
on INT0 is any voltage lower than about 1.5V while a high
level is considered to be anything above 3.5V.
We have a 5V supply but a 7.5V secondary winding.
This means that the triggers to INT0 (which is the microcontroller’s zero detection interrupt) are asymmetrical. The
measured duty cycle is about 42% rather than the expected
50%. The firmware corrects this asymmetry, adjusting the
value of a phase counter to take account of this.
Compare Fig.2. (Without software correction) and Fig.3
(with software correction). In the scope screen grab of Fig.3,
the yellow trace is the output of the Triac and the green
trace is the trigger pulse.
You can see that the trigger pulse period is only 8.5ms
whereas for symmetrical triggering it should be close to
10ms (this is the 100Hz rate which is twice the mains
frequency in Australia) as shown in Fig.3.
User Operation of the DSP Musicolour
The Musicolour has many settings which can be changed
by the user. As mentioned, the preloaded default values
should be adequate for most applications. You can go to
Fig. 3: the same set up as in Fig.2 but with software
correction. The period is now much closer to the correct
value of 10ms. The firmware automatically corrects this
asymmetry when driving the Triacs. It does so in real time
at a frequency twice the mains line frequency.
siliconchip.com.au
the SILICON CHIP website and download more complete
user instructions for the DSP Musicolour that were too
long to include here.
Front Panel
There are seven push buttons on the front panel which
are used to navigate through the menus and change internal settings. Some buttons have multiple functions,
according to context. The SELECT potentiometer is also
context-sensitive and is used to change settings. The
incorporated LEDs in each of the buttons will light depending on the context. Usually, a lit or flashing button
will mean that the button has an active function in the
current menu. When the firmware is executing the main
loop, the LEDs will indicate the state of the output channels and the current operating mode.
Adaptive Potentiometer Controls
The DSP Musicolour firmware implements adaptive
potentiometer controls. This means that if a setting is to
be modified using the SELECT potentiometer, the setting
will begin to change only when the potentiometer position first matches the current value of the setting. This
gives the potentiometer a kind of memory and is used
to seamlessly change internal settings depending on the
current menu.
Menu System
The settings of the DSP Musicolour are changed through
a hierarchical menu system. When the DSP Musicolour
is in the main loop, pressing the SET button allows you
to enter MENU mode.
Keep in mind that some of the behaviour of the Musicolour is dependent on its current settings. For example,
the display will be blank if the screen saver has been set
to NONE and there is no key activity for the period of the
screen saver timeout.
Using the Chaser Modes
Go to the CHASER>Mode sub-menu. Here you can
choose Normal or Triggered modes. In NORMAL mode,
the currently selected Chaser program is executed. In
TRIGGERED mode, the currently selected Chaser program
is executed but the stepping through the program depends
on the trigger (affected by the music). If you are using
TRIGGERED mode, you should know that the triggering
will depend on the current settings for the trigger channel. Go to the TRIGGER sub-menu. There you should set
the pass-band and threshold. Set the mode to OFF to run
the output channels from the FFT.
Once you have set the Chaser mode, you then select
the Chaser Program that you wish to run by going to
CHASER>Program.
Conclusion
As you can see, the DSP Musicolour offers an amazing repertoire of features – far too many to allow us to
describe in detail here.
Next month, we plan to have more information on
driving the DSP Musicolour, as well as an optional PC
board which gives you complete remote control. What?
A lightshow with remote control? You betcha!
siliconchip.com.au
Quick Setup Checklist
Here’s how to set up the DSP Musicolour quickly and the relevant
settings that will affect its operation:
1. Set the ADC system’s sampling Frequency:
go to AUDIO>Sampling Frequency.
2. Set the mixing settings for the input signal:
go to AUDIO>Balance.
3. Set the minimum and maximum frequencies for each logical output channel: go to CHANNELS>Min Freq and CHANNELS>Max
Freq. Alternatively go to CHANNELS>Freq to set a non-overlapping frequency mask.
4. Set the gain for each logical output channel:
go to CHANNELS>Gain.
5. Set the mode for each logical output channel:
go to CHANNELS>Mode.
6. Set the output connections of the logical channels:
go to OUTPUT>Logical Channels.
7. Set the CHASER>Mode and CHASER>Program
8. Exit the menu system.
Tip: Every submenu has a Default option to reset all values in that
submenu to default values.
Simple Setup Guide
Assuming you have a music source connected to an audio amplifier,
connect the output terminals of your amplifier to the speaker terminals
on the back panel of the DSP Musicolour.
Next, adjust the sensitivity of the Left and Right channels using the
LEFT and RIGHT potentiometers on the front panel.
Load default values by going to the menu. Press SET while in the
main loop to be directed to the menu. Scroll down to the DEFAULTS
sub-menu using the UP and DOWN buttons on the front panel.
Press SET to enter the DEFAULTS sub-menu. Scroll down to “Load
Defaults” and press SET. This will restore all default values. Exit the
menu system by pressing CH 4/D (the back button while in menu
mode) and the DSP Musicolour should start running the main loop
in Automatic mode. The output channels will respond to the music.
Remember that the DSP Musicolour has many user options. As
a summary you should know that:
(a) Each of the four physical output channels must be connected
to a logical channel. Two physical channels can be connected to
the same logical channel. Go to OUTPUTS>Logical Channels to
set these.
(b) The input signal source is an arbitrary mix of the Microphone,
Left and Right audio inputs. You set this in the AUDIO>Balance
sub-menu.
(c) The inputs are sampled at the set Sampling Frequency.
Go to AUDIO>Sampling Frequency to set this.
(d) For each logical channel, you should select its pass-band (the
minimum and maximum frequencies). Only frequencies in the
input signal that fall in this pass-band will affect that logical
channel.
(e) For each logical channel, you can select the gain. The higher
the gain the more sensitive the channel will be to pass-band
frequencies in the input signal.
(f) For each logical channel, you should select its mode. This affects how the channel responds to level requests. Choose from
PEAK or AVERAGE acquisition modes. These determine how the
FFT data affects the level of the logical output channel. This level
is interpreted differently according to the whether the channel is
in DIRECT, CONTINUOUS, ZV or STROBE mode. So you should
choose one of these 4 modes as well.
August 2008 83
User Operating Instructions: Menu System
The Musicolour uses a hierarchichal menu system. From the main loop press the SET button to enter the menu system. You will be directed to the main
menu, where you may scroll up or down between sub-menus by using the UP and DOWN buttons. Use the SET button to enter a sub-menu. In any
submenu, you may use the CH4/D button to go back to the previous menu (if you are in the main menu, you will be directed back to the main loop).
Sub-menus available in the main menu:
1. CHANNELS: this sub-menu allows you
to change any settings related to the four
logical channels;
2. TRIGGER: this sub-menu allows you to
change the trigger passband and the trigger threshold;
3. CONSOLE: this sub-menu contains user
applications, allowing the Musicolour to
function as a light dimmer or communications terminal;
4. OUTPUT: this sub-menu is used to set
the chaser mode, the chaser program, the
output rate, the quiescent level of each
physical channel and to define the logical
to physical channel translation;
5. AUDIO: this sub-menu is used to change
the equaliser settings, the software mixing/
balance of the input signal and the sampling
frequency;
6. DEFAULTS: this sub-menu is used to save
and recall settings and to load default
values;
7. ADVANCED: this sub-menu is used to access advanced features, including calibration, software upgrade and tuning;
8. INFORMATION: this sub-menu displays
information about the Musicolour’s operation like the mains frequency, the frequency
of the ADC system and the screen refresh
frequency. The error in the overall accuracy
of the timing system can also be seen;
9. DISPLAY: this sub-menu is used to change
the display’s settings, including the screen
refresh frequency, the screen brightness
and the screen saver time out period;
10. SYSTEM: this sub-menu can be used
to change system settings, the firmware
version is displayed, the baud rate of the
UART can be changed, the remote control
system can be enabled and other system
settings changed;
Here are the major sub-menus used at this
stage:
CHANNEL submenus:
CHANNELS>Min Freq: Press the channel
buttons CH1-CH4 to display the current
minimum frequency for that logical channel;
Use the SELECT potentiometer to change
84 Silicon Chip
the minimum frequency;
CHANNELS>Max Freq: Press the channel buttons CH1-CH4 to display the current maximum
frequency for that logical channel; Use the
SELECT potentiometer to change the maximum frequency;
CHANNELS>Freq: this is similar to the
CHANNELS>Mi n Freq menu, except that
after exiting, the minimum and maximum
frequencies for the four channels are set in
non-overlapped fashion.
CHANNELS>Gain: Press the channel buttons
CH1-CH4 to display the current gain for that
logical channel; Use the SELECT potentiometer to change the gain.
CHANNELS>Mode: Press the channel buttons
CH1-CH4 to display the current mode for
that logical channel; Use the UP and DOWN
buttons to scroll through the available modes;
CHANNELS>Attack: Press the channel buttons
CH1-CH4 to display the current attack rate
for that logical channel; This is only relevant
when the channel is operating in CONTINUOUS mode. Use the SELECT potentiometer to
change the attack rate.
CHANNELS>Decay: Press the channel buttons
CH1-CH4 to display the current decay rate
for that logical channel; This is only relevant
when the channel is operating in CONTINUOUS mode. Use the SELECT potentiometer to
change the decay rate.
CHANNELS>Test Channel: Press the channel
buttons CH1-CH4 to test the relevant logical
channel with a range of output level requests
from 0 to full level; This can be used to test
the current settings for the channel.
CHANNELS>Defaults: Press SET to restore
default CHANNEL sub-menu values;
TRIGGER sub-menus
TRIGGER>Min Freq: Press the UP and DOWN
buttons to set the minimum frequency defining the trigger pass-band. Exit using the SET
button.
TRIGGER>Max Freq: Press the UP and DOWN
buttons to set the maximum frequency defining the trigger pass-band. Exit using the
SET button.
TRIGGER>Threshold: Use the SELECT potentiometer to change the threshold level for the
trigger. Triggering will occur when the input
signal has an amplitude component within
the trigger pass-band that is greater than the
trigger threshold. The level is indicated as
a horizontal bar. Exit using the SET button.
TRIGGER>Defaults: Press SET to restore default
TRIGGER sub-menu values.
CONSOLE sub-menus:
CONSOLE>Dimmer: Press the channel buttons
CH1-CH4 to select the relevant logical output
channel. Use the SELECT potentiometer to
change the output level of this channel. Here
the Musicolour functions as a four channel
light dimmer.
CONSOLE>Com: The Musicolour enters an echo
terminal mode. Received data from the UART
is displayed on the display. The UART can be
enabled using additional hardware.
OUTPUT sub-menus:
OUTPUT>Chaser Mode: the current chaser mode
is displayed. Press the SET button to scroll to
the next available mode.
OUTPUT>Chaser Program: the current chaser
program is displayed. Press the UP and
DOWN buttons to set the program. Press
SET to exit.
OUTPUT>Output Rate: the current output rate is
displayed. Use the SELECT potentiometer to
change the rate; Press SET to exit.
OUTPUT>Quiescent Level: Press the channel buttons CH1-CH4 to select the relevant
logical output channel. Use the SELECT
potentiometer to change the quiescent level
of this channel.
OUTPUT>Logical Channels: Press the channel buttons CH1-CH4 to select the relevant
physical output channel (on the back panel).
Use the UP and DOWN buttons to change
the logical output channel associated to that
physical channel. In Normal operation, you set
CH1=1, CH2=2, CH3=3, CH4=4; if for example,
you wish to have logical channel CH1 control
two physical outputs on the back panel you
could set CH1=1 CH2=1 CH3=3 CH4=4; If you
would like to permute the channels you can
also do that here.
OUTPUT>Defaults: Press SET to restore default
OUTPUT sub-menu values.
AUDIO sub-menus:
siliconchip.com.au
AUDIO>Equalizer: The current equalizer settings
are shown as vertical bars. Use the UP and
DOWN buttons to scroll to the next setting,
and use the SELECT potentiometer to vary the
current equalizer setting.
AUDIO>Balance: the current percentages of each
the three audio channels contributing to the
input signal are shown. Press SET to change
these. The levels are then displayed as bars.
The first bar from the left is the MIC line level.
The next two bars indicate the LEFT and RIGHT
levels respectively. Use the SELECT potentiometer to change the LEFT/RIGHT balance. Use
the UP and DOWN buttons to change the MIC
contribution to the input signal.
AUDIO>Sampling Frequency: the current sampling frequency in kHz is displayed. Press
SET and use the SELECT potentiometer to
vary this value.
AUDIO>Defaults: Press SET to restore default
AUDIO sub-menu values.
DEFAULTS sub-menus:
DEFAULTS>Load Defaults: Press SET to restore
all settings to default values;
DEFAULTS>Save Settings: Press UP and DOWN
buttons to change the memory number to save
to. Press SET to save all current settings to
non volatile memory.
DEFAULTS>Recall Settings: Press UP and DOWN
buttons to change the memory number to load
values from. Press SET to load all settings with
previously stored values.
ADVANCED sub-menus
ADVANCED>Calibration: Press SET to automatically calibrate the Musicolour’s internal fast
RC oscillator against the mains frequency.
ADVANCED>Software Upgrade: Press SET to
upgrade the firmware. This mode requires a
functioning UART connecti on, which needs
additional hardware.
ADVANCED>Tune Oscillator: Press UP and
DOWN to change the internal calibrating value
for the system clock. This value is updated
by the automatic calibration above. You can
manually adjust the value here.
INFORMATION sub-menus
There are no settings to change here. Only
the values of certain system parameters are
displayed. This is for operating information
like the mains frequency, the screen refresh
rate, the sampling frequency, the system
clock, the error in the system timing from
the ideal, etc.
DISPLAY sub-menus:
DISPLAY>Brightness: Press SET to change, us-
siliconchip.com.au
ing the SELECT potentiometer, the brightness
of the display.
SYSTEM>Reset: Press SET to reset the
Musicolour.
DISPLAY>Frequency: Press SET to change,
using the SELECT potentiometer, the screen
refresh frequency. Note that strange display
effects can occur at low screen refresh
frequencies. If this is the case, increase the
frequency. Usually a level around 65Hz or
higher is adequate.
SYSTEM>System Defaults: Press SET to load
SYSTEM submenu defaults.
DISPLAY>Timeout: Press SET and use the UP
and DOWN buttons to select the timeout
period for the screen saver.
DISPLAY>Screen Saver: Press SET and use the
UP and DOWN buttons to select the current
screen saver.
DISPLAY>Display Defaults: Press SET to restore
all DISPLAY submenu defaults;
SYSTEM sub-menus:
SYSTEM>Version: displays the current firmware
version.
SYSTEM>Uart: Press UP and DOWN to change
the baud rate for the UART. This requires additional hardware.
SYSTEM>Remote Control: Press SET to enable
or disable the remote control decoding. This
requires additional hardware and can be
used to control the Musicolour using an RC5
compatible remote control.
SYSTEM>IrDA: Press SET to enable or disable
the IrDA decoding. This requires additional
hardware and can be used to add a wireless
infrared serial port. This can be used to send
and receive data from a PC.
SYSTEM>Test: Press SET to run a test on the
display, the output channels and the LEDs.
Can be used to check that all these are working correctly.
SYSTEM>Detected Mains: this shows the detected mains frequency and is either 50Hz
or 60Hz. It should match your area’s mains
supply frequency.
SYSTEM>Startup: Press SET to scroll through
the start up modes for the Musicolour. The
initial startup can be made quicker by disabling
the normal boot-up messages.
SYSTEM>RF6: Press UP and DOWN to change
the RF6 pin mode. This is an advanced feature
that can be useful to debug any problems
with the Musicolour. The RF6 output of the
microcontroller is a digital output and is available at pin 9 of CON3 on the main board. The
system clock frequency can be measured at
this pin, as well many other internal operating
frequencies like the screen refresh frequency
and the ADC system frequency. You will not
need to normally use this menu.
In Depth Explanation of the Main Loop
In more detail the main loop is as follows:
1. The firmware waits until the internal ADC
system signals that the buffer has been filled
with digitized and software mixed audio
data (while waiting all interrupts are active,
including all timers, key press detection and
display refresh interrupts);
2. Once a full buffer of data has been acquired,
the Fourier Transform is computed;
3. For each logical output channel, a level
corresponding to the channel is computed.
This may involve adjusting the output of the
FFT with equalization, it will depend, for each
channel on its selected acquisition mode;
4. A request is made, for each logical output
channel to set its output level to the previously computed level. The implementation
of this step is dependent on the channel’s
current setting. If a channel should be accepting data from an active chaser program,
the level requested in this step is ignored;
5. If a Chaser program is active, it is serviced
by the virtual machine; This may involve the
triggering channel if the program is in trigger mode; Any output level requests made
by the chaser program are set. Again, the
implementation of this step is dependent
on the channel’s current settings;
6. The display is refreshed according to the
currently selected display:
1. Spectrum Fine: the spectrum is displayed
on the display;
2. Spectrum Centered: the spectrum is display
in centered mode;
3. Logical Channel Displayed Single: the output
levels of each channel are displayed. The
top horizontal bar indicates the first logical
channel. The third horizontal bar from the
top indicates the second logical channel.
Similarly, the fifth and seventh horizontal
bars from the top indicate the third and
fourth logical channels respectively.
4. Logical Channel Display Averaging: same
as 3. above except every horizontal bar
in between the output channel bars is the
average of the previous and next bars.
5. RMS display: displays the RMS level of the
input signal as an analog meter.
6. The firmware updates any LEDs on the front
panel and returns to step 1. It also responds
to key presses.
August 2008 85
FRO NT
SEC ON DARY
100 nF
E NIL N OITAL OSI
ISO LATION
220 Ω
220 Ω
220 Ω
PIN
3:
4.7k
0V
100 nF
10k
100 k
+
5.6nF
10k
10k
10k
CON 2
1k
47 µF
IC2 LM3 24
4148
PIN 5:
+5V DC
220 Ω
270 Ω 1W
+
1k
470 Ω
100 nF
dsPIC 30F4 011
IC1
+
Problem:
You apply power and there is a sudden short of the mains
supply (consequently the fuse blows or the circuit breakers/
fuse in your home open). There seems to be a short of the
mains supply.
Possible Cause:
This could be caused by incorrect link settings for LK1, LK2
and LK3 underneath the mains transformer.
first” mode
If all goes to plan, you’ll bui
ld the DSP Musicolour, turn
it on . . . and1kit will work per
TRANSFO RM ER
fectly, first time.
But what if it doesn’t?
4148
D8
100 Ω
+
We’ve warned a number of
TP0
470 times tha
t the Musicolour
must not be run with the lid µF
off and the ma
TPI ins connected.
It is simply too dangerous. D11
So how can you work on an
unpowered circuit?
D12
LED8
T1
Obviously, you can’t. But D13
fortunately, all of the log
30V
D14
icA 7.5 V
and processing circuitry (inc
luding the dsPIC) can be
run from a 5V DC supply (ra
ted at 500mA or so) so you
can troubleshoot with safety 4700µF
.
If you need to poke around 16V
the Musicolour, CON3 can
LK5 LK6
be used to supply pow
er to the100
circ
Ω uit. Simply
+5V to pin 5 and 0V to pin
100con
Ω nect
3 of CON3 and all of
100the
Ω lowvoltage circuitry will be pow
1 µF
ered, up to and including the
D10
fou
r opto-couplers. DON’T plu
g in D9
the mains lead!
1k
Problem:
You apply power and there seems to be no activity, there is
no display.
Possible Cause:
Is the fuse blown? Have you installed a fuse?
8 0 0 2/ 4 0 G M
RU OL O CISU M
Troubleshooting in “safety
YRAD N O CES
Some common problems that may help you troubleshoot
the DSP Musicolour.
1 8 0 7 0 1 0 1 CS
REG 1
LM3 17T
CON 1
4148
Troubleshooting Tips:
TNORF
+
33k
33k
3.3k
OPTION AL
Problem:
9
1
Section +
270 Ω 1W
10
2
One or both voltages at test points TP0 and TP1 are not at LINK
47 µF
of full MIC
normal levels around +5V and +10V respectively.
270 Ω 1W
overlay
Possible Cause:
from the
CON 3
68nF
68nF 68nF
One possible cause is that links LK1, LK2, LK3 are impropJuly 2008 68nF
erly set or omitted. Remember these have to be installed
SILICON CHIP
according to the mains supply voltage. Install LK2 and omit
LK1 and LK3 if you are using a 220-240V mains supply;
install LK1 and LK3 and omit LK2 if you are using a 110-120V mains supply. These links are
found under the mains transformer, so you may have to unsolder the transformer to change them. If you have erroneously configured these links for 110-120V operation while you are actually in a 220-240V region of the world, you will
get double the intended voltage at test-point TP1. This can very easily destroy REG1 and cause further damage to the
main PC board. Disconnect power immediately if the voltages at TP0 or TP1 are much higher than their intended values.
Problem:
The main board seems to be operating correctly, except nothing is shown on the dot matrix LED display.
Possible Cause:
The most common cause of this problem is that the 26-way ribbon cable connecting the main board and the display
board is either faulty, not all connections are good, or it is incorrectly oriented. If you can verify that the ribbon cable’s
26 connectors are good, it may indicate a fault with incorrectly oriented parts. Check the transistors and ICs are correctly oriented on the display PC board. Check also that the dot matrix LED modules are in their sockets the right
way around.
Problem:
At least one key does not respond to key presses or its LED does not light up.
Possible Cause:
This is most likely caused by the tactile switch being incorrectly oriented, improperly soldered, or its accompanying
diode being incorrectly oriented.
Problem
When in a menu, moving the SELECT potentiometer does not affect the setting, or does so after much turning.
Possible Cause:
This is most likely not a problem but a feature. It is called adaptive control. See the text for an explanation.
Tips and Tweaks
Notice that if the display frequency is set too low you may see strange effects on the display. Increase the screen refresh
frequency if this occurs. Also, if the sampling frequency is lower than twice the highest frequency of the input audio,
aliasing will occur.
86 Silicon Chip
siliconchip.com.au
OPTO 1
MOC 30
What About the Musicolour
Display – ie, the Lights!
The DSP Musicolour is capable of driving up to 2400W of lights over its four
channels, with a maximum of 800W in
any one channel.
That’s an awful lot of coloured light
– far more than you’d normally find at a
party, which tend to be on the dark side
anyway.
Let’s look at the type of lights you can
use (and shouldn’t use).
First of all, steer clear of halogen (QI)
lights. Their problem is the time the filament takes to cool and the light to go “out”.
They also get very hot and this can be a
problem with coloured films – depending
on the type, they scorch with high temperatures and can even catch fire. That’s
about the last thing you want.
By far the most popular display/party
lights are the coloured ES (Edison screw)
PAR38 or R80 bulbs. The coloured PAR38s
are usually rated at 120W (their plain white
cousins are usually 150W, some 120W).
Incidentally, just in case you wanted to
know, PAR38 means Parabolic Aluminised
Reflector, 38 eights of an inch (or 4.75
inches) in diameter. R80 means an 80mm
diameter reflector light globe. So there!
The biggest problem with coloured
light globes is the price – they are rather
significantly more expensive (like about
four times or more!) than white. But I have
a sneaky solution here: paint white globes
and save heaps!
You can’t use ordinary paint, of course
– it is opaque. But you can buy translucent
glass paint at better craft stores in a wide
variety of colours. The most usual colours
for light displays are also the easiest to
get – red, yellow, blue and green.
This paint is intended for making (fake!)
“stained glass” windows but I’ve found it to
be quite tolerant of high temperatures so
can be painted directly onto white globes.
The brand I use is Vitrail, from France. But
I’ve also seen other brands of this type of
paint advertised on eBay (just make sure
it is translucent/transparent when dry!).
I’ve used it for years instead of buying
coloured globes and it works very well.
You simply paint it on so that the glass
has an even covering; usually only one
coat is required.
Allow it to dry before turning on the
light – even then, you’re likely to get some
coloured vapours given off and it does tend
siliconchip.com.au
to stink a little! If I’m in a real hurry, I might
apply a little heat from the light globe – say
ten seconds on, a minute off – to impart a
little forced drying.
OK, so that’s the coloured globe side
covered. Now, how about their mounting?
Simple, I thought: just go and buy some
ES batten lampholders, mount them on a
length of flat timber and wire them up. Yeah,
simple all right: have you seen the price of
ES battens recently?
You can get standard BC (Bayonet Cap)
batten lampholder for about $3-$5 just about
anywhere. The same things in ES (Edison
Screw), which are required for the PAR38
and many R80 bulbs, tend to start at around
$13-$14 and go up from there. (Why?!!)
But I cheated here, too. In our local Bunnings Hardware store, I spotted a PIR movement detector security light, complete with
two ES lampholders and two 150W PAR38
bulbs, all for just $15.95. So I bought two
of these, giving me four ES lampholders and
four PAR38 bulbs for just over thirty bucks!
I discarded the two PIR sensors (anyone
know what to do with two brand new PIR
sensors?) and mounted the two sets of two
ES lampholders on the length of flat timber
and wired them (individually) to short 240V
mains leads.
Even here I was able to save, by using
old 240V leads. Call it the scrounger in me if
you will but every time I discard any electric
appliance, if the mains lead is OK I cut it off
and save it – just in case. Well, here’s the case
and phhhhttt to all those who have criticised
me for hoarding rubbish saving and recycling
perfectly good stuff!
In fact, I used two such salvaged mains
leads and two old IEC mains leads, which had
also been saved from the scrapheap (actually
By Ross Tester
rescued from the last council clean-up).
The IEC plugs themselves were not needed
(not now, at least!) so I cut them off with
maybe 250mm of mains lead attached (just
in case!) and put them back in my “spare
mains lead” box. You never know. . .
That gave me four mains leads, complete with three-pin plugs, about 1.5m
long. Perfect!
I’ve shown a photo of my el-cheapo
Lamp Display Unit above. While this is
very obviously only one approach, it gives
you an idea of what you can do to make
a very reasonable lightshow for a very
reasonable price.
The ES bases even have some very
handy terminal blocks inside so wiring
them up is delightfully easy. Each light
operates completely independently to any
other so all are wired separately.
Remove the wires from the PIR unit
and discard it. Connect the active (red or
brown wire) in one of your mains leads
to the white wire going to the lampholder,
the neutral (black or blue) to the blue wire
and the earth (green/green yellow) to the
green/yellow wire in the terminal block.
Repeat for the second mains lead and
ES base, then fasten the mains leads
under the anchor strip provided (there
is just room). Screw the assembly onto
a suitable piece of timber. Put the top on,
screw it all up and put your two PAR38
bulbs into their holders. Connect both
mains plugs to a suitable outlet to ensure
both lights work.
Repeat all this for the other ES base
assembly, check it – and you’re ready to
plug it into your DSP Musicolour and light
up your life. Oh, you did remember you
SC
had to build the Musicolour first?
August 2008 87
Vintage Radio
By RODNEY CHAMPNESS, VK3UG
The incredible 1925 RCA 26
portable superhet receiver
portables was not particularly difficult
at the time. By contrast, designing a
workable superheterodyne receiver
wasn’t particularly easy in 1925, as
the valves that were then available
were not very suitable for the task
of frequency conversion. In fact, the
design could be quite critical if the set
was to operate at all.
That situation improved in the early
1930s with the development of the
2A7 and similar converter type valves.
These new valves proved to be quite
tolerant of circuit design inadequacies,
making the design and manufacture of
superhet receivers much easier.
The RCA 26 portable superhet receiver
with its front open, ready for use.
Prior to the 1930s, virtually all domestic
broadcast receivers used TRF circuits.
One exception was the 1925 RCA 26
portable which was one of the very first
domestic superhets. It used some truly
innovative technology for the era.
U
NTIL RECENTLY, I’d always
thought that “portable” radios
(if you could call them that) were an
innovation of the mid to late 1930s.
However, at the HRSA’s 25th Anniversary celebrations last year, I was
amazed when I saw Mike Osborne’s
1925 RCA 26 portable. Not only is it a
fully-working concern but it also uses
a superheterodyne circuit.
88 Silicon Chip
Why was this so remarkable? Well,
superheterodyne receivers didn’t become common in Australia until the
mid-1930s. This means that, at the
time, this set was a truly innovative
design that was at the leading edge of
technology.
The RCA 26 was also one of the
earliest, commercially-made portable radios, although manufacturing
Superhet principles
Before the 1930s, most sets employed TRF (tuned radio frequency)
circuits. However, these had their
shortcomings and superhet designs
quickly took over when suitable valves
became available.
The superhet (or superheterodyne)
principle was developed during World
War 1 by Major Edwin Armstrong of
the US Army. Armstrong was a prolific
radio inventor who also developed
other radio techniques, including
regeneration, super regeneration and
frequency modulation (FM).
Basically, the superhet was developed because during WW1, the allies
needed direction finding (DF) receivers that could receive the extremely
weak spark transmissions used by the
Germans in Europe. Apparently, tuned
radio frequency (TRF) receivers could
not be made sensitive enough or stable
enough for this task, so an alternative
technique had to be found.
In operation, a TRF receiver tunes
siliconchip.com.au
and amplifies the incoming RF
(radio frequency) signal at the
frequency of interest and then
presents the amplified signal to
the detector. This then feeds an
audio amplifier stage which boosts
the audio signal to headphone or
speaker levels.
Although this had the benefit of
simplicity, there were a few problems with TRF sets which limited
their usefulness. The first was that
they had to be capable of accurately
tuning the incoming RF signal across
a wide range of frequencies. In the
early days, this was achieved by
adjusting several tuning capacitors
or variometers to obtain the best
reception, as ganged capacitors were
not available. In some sets, this could
involve up to four or even five adjustments.
In addition, some detectors require
a certain minimum level of signal for
them to work effectively. This meant
that, in some cases, additional RF gain
was needed. Unfortunately, this is difficult to achieve with a TRF set due to
problems with feedback between the
various stages.
During the early 1920s, triodes were
almost exclusively used to amplify
both RF and audio signals. However,
at RF, triodes must be “neutralised”
in order to achieve reasonable gain
and stability. This “neutralisation”
involves adding an extra capacitor to
cancel out the grid-to-plate capacitance inherent in each triode RF stage,
to prevent it from oscillating.
In addition, triodes were not good at
amplifying frequencies above 500kHz,
again due to inter-electrode capacitance and also due to lead inductance.
Even in those very early days of radio,
the TRF failed to meet the “state of
the art” needs of the military during
WW1.
By contrast, in a superheterodyne
receiver, the RF stage (or stages) provides only moderate amplification,
which allows easier tuning and greater
stability. This also means that there
is less need for significant shielding
between stages.
The amplified RF signal is then applied to a converter (or mixer) stage
where is mixed with a signal from a
local oscillator stage. In an AM broadcast receiver, this local oscillator stage
typically operates at a frequency that’s
455kHz (or thereabouts) higher than
the tuned RF signal.
siliconchip.com.au
Another view of the 26 receiver, this time with the access covers removed
for the valves (top) and the reflexed horn speaker. The loop antenna was
housed in the hinged section attached to the front cover.
As a result, the output from the
mixer stage consists of four separate
frequencies: (1) the original tuned signal frequency; (2) the signal frequency
plus the local oscillator frequency; (3)
the local oscillator minus the signal
frequency; and (4) the local oscillator frequency. Lets’s take a look at an
example to illustrate this;
If the tuned frequency is (say)
1000kHz (1MHz), then the local oscillator will run at 1455kHz (ie, 455kHz
higher). As a result, the mixing frequencies will be 1000kHz + 1455kHz
= 2455kHz and 1455kHz - 1000kHz
= 455kHz.
This means that the following frequencies will appear at the plate of
the converter valve: 455kHz, 1000kHz,
1455kHz & 2455kHz. These signals are
all fed to the following intermediate
frequency (IF) stage but since this stage
is tuned to 455kHz, only this frequency
is passed on for amplification. It does,
however, contain all the audio information that was included with the
original signal frequency.
Because the IF amplifiers and the
RF amplifiers are on different frequencies, they do not inter-react with one
another. Because of this, significant
gain can be achieved in the IF amplifier and so the overall gain can be quite
high. In addition, the IF stages amplify
only a narrow band of frequencies and
because these are usually lower than
the signal frequencies, amplification
is easier to achieve.
Initially, in the 1920s, an IF of
100kHz was used, then a very low
IF centring on 25kHz was used followed a little later by 55kHz. In fact,
this latter IF is used in the RCA 26
portable. At such low frequencies,
most triodes didn’t need any neutralisation. In addition, the gain of
the UV99 RF valve used in the RCA
receiver is only 6.6 under optimum
conditions, so the IF stages in the 26
were not neutralised.
Following the IF stages, the signal
was fed to the detector and the IF
component removed. The resulting
audio signal was then fed to the audio
amplifier.
Audio amplifier stages are generally
easier to design than RF amplifiers.
Most of the triodes of the 1910s and
early 1920s were quite stable at audio
frequencies but the gain of individual
UV99 triodes was quite low (6.6).
As a result, to achieve a higher
gain per stage, inter-stage audio transformers were used. These generally
had step-up turns ratios somewhere
between 3:1 and 5:1, which could
boost the gain of a UV99 stage up to a
maximum of 30 times. However, these
audio transformers had a very limited
frequency response, as well as having
peaks and troughs in the response.
On the other hand, a 6AV6 with simAugust 2008 89
would be just 10kHz on either side
of 100kHz. In fact, it was the low “Q”
factor of early tuned circuits and the
meagre amplification of signals above
500kHz by the triodes of the era that
dictated the use of low intermediate
frequencies in early superhets.
Overcoming the problems
The view shows the chassis after it has been removed from the cabinet. The
valves are easily accessible so that they can be replaced while most the rest of
the circuitry is sealed in the “catacomb box” (or sealed container) at the right, to
prevent users fiddling with the adjustments.
ple resistance/capacitance coupling will
easily exceed this figure, with amplification of up to 70 times per stage. It will
also have a much improved bandwidth
and no nasty peaks and troughs across
the frequency band.
Early superhet problems
Unfortunately, despite their clear
advantages, early superhets also had
their problems. However, these were
quickly overcome by Edwin Armstrong and other designers of the era.
One early problem involved the
large 60-100cm tuned-loop antennas
that were commonly fitted to receivers from the 1920s to the early 1930s.
Initially, the superhets had a converter
stage connected to the loop antenna
and a separate local oscillator was
coupled into the loop. The following
IF section then had up to five stages
of amplification.
However, with this arrangement, it
was found that the local oscillator radiated signals via the loop antenna and
this was picked up as interference (in
the form of whistles) by nearby receivers. In addition, the action of tuning
90 Silicon Chip
the loop (or even someone walking
near it) caused the oscillator to change
frequency, so much so sometimes that
the wanted signal was shifted out of
the pass-band of the IF amplifier.
This effect was particularly evident
as the loop and the oscillator were
tuned to frequencies quite close to
one another.
Another problem with early super
hets was that one tuned circuit could
lock onto the frequency of another
stage with a higher “Q” factor. “Q” refers to a tuned circuit’s “quality factor”
and is a measure of the “sharpness” or
selectivity of the tuning response. A
circuit with a Q of 100 is much more
selective than one with a Q of 10.
As an example, let’s assume a
circuit with a resonant frequency of
1000kHz and a Q of 10. In this case,
the response at 950kHz and 1050kHz
will be half that at 1000kHz, ie, the
response will be 3dB down at the
+50kHz and -50kHz points. Or to put
it another way, the circuit has a -3dB
bandwidth of 100kHz.
However, at a tuned frequency of
100kHz, the -3dB bandwidth points
Oscillator radiation from the loop
antenna was overcome by adding
a neutralised triode RF amplifier
between the loop and the converter
stage. In addition, the RF stage and
the converter were coupled using
an untuned RF transformer and this
overcame much of the pulling of the
oscillator by the RF tuned circuits.
It was also found that running the
oscillator at half the received signal
frequency plus or minus the intermediate frequency, also substantially
reduced oscillator pulling. So how
did the circuit work if the oscillator
ran at half the required frequency. The
answer was quite simple – the second
harmonic of the oscillator was used to
heterodyne with the received signal to
give the IF.
Having solved most of the problems of producing a usable superhet
receiver, the designers found that no
less than eight valves were required to
build it. However, an 8-valve set, even
one using low-current valves, had a
higher current drain than was practical to expect dry batteries to supply.
In fact, the first superhet receivers
used 201 valves which draw 1A each
at 5V, thus giving a total current consumption of 8A. This meant that the
very early designs could not be used
as portables.
At that stage, a superhet receiver
used a neutralised triode RF stage (V1)
which was coupled to a triode mixer/
converter stage (V2). The signal was
then mixed with the heterodyning
signal from a separate local oscillator (V3).
The output from the converter then
fed two IF stages (V4, V5) and these in
turn were coupled to a grid leak detector (V6). This then fed two transformercoupled audio stages (V7, V8), with the
amplified audio signal then going to a
speaker or to headphones.
In order to produce a portable set,
it was necessary to find some way of
reducing the current drain. That meant
reducing the number of valves while
still maintaining good performance.
Two techniques were available to
siliconchip.com.au
RCA’s 26 portable receiver
RCA’s 26 portable receiver uses this
same 6-valve design technique. In fact,
this set is one of several variants built
by RCA at the time and their circuits
are almost identical – see Fig.1. However, some of the features shown on
the circuit are not included in the 26,
while some of the features of the 26 do
not appear on other variants.
For example SW1, SW2 and J1 are
not fitted to the 26. The 26 is switched
off by turning the battery rheostat (R3)
fully anti-clockwise, so SW1 was not
needed. In addition, the loudspeaker
is wired permanently to V6 so the use
of headphones is not an option.
The 26 uses UV99 valves in all six
valve sockets. This valve is designed
for a filament voltage of 3-3.3V and
a filament current of 60-63mA. As a
result, the receiver draws approxisiliconchip.com.au
Fig.1: the RCA 26 is an early superhet receiver employing a reflexed RF stage (V1) and an autodyne (or self-oscillating) mixer stage based on V2. In operation,
the reflexed RF stage functioned as both an RF stage and as the first IF stage. V3 is the second IF stage, V4 is the detector and V5 & V6 are the audio stages.
achieve this: (1) reflexing and (2) using
a self-oscillating mixer.
Last month, we looked at how reflexing was achieved in the Astor KM
receiver. However, in those early days
of superhet receivers, the technique
was applied in a slightly different way.
The RF amplifier stage amplified the
incoming signal, which then went to
the mixer. The resulting IF signal was
then fed back into the RF stage again
which now acted as the first IF stage.
Its output was then applied to the
second IF amplifier.
Basically, it was possible to use the
RF stage to handle both RF and IF
signals because the signals were at a
low level. In addition, the difference
between the IF frequency (25-55kHz)
and the signal frequency (520kHz or
more) meant that there was minimal
interaction between the two.
Initially, the mixer and local oscillator stages required two separate
valves. However, this was subsequently reduced to just one valve
when the designers came up with
the self-oscillating mixer. In other
words, one valve functioned as both
the mixer and the oscillator and this
stage became known as an “autodyne
mixer”. It was seldom used during the
later valve era but was commonly used
in transistorised receivers.
Thus, by using a reflexed RF stage
and an autodyne mixer stage, the designers were able to reduce the valve
count from eight to six. This not only
reduced the current drain but saved
on expensive valves as well.
August 2008 91
The large reflexed horn speaker sits behind a panel in the bottom of the cabinet.
of the photo). However, for home use, a
larger battery pack was normally used
to power the set.
The 26 receiver has the usual frame
(loop) antenna but provision was also
made to connect a larger loop antenna
and to connect long-wire antennas.
This tuned circuit feeds valve V1
which functions as a combined RF
and first IF amplifier stage. This stage
is neutralised using trimmer capacitor C6.
V1’s output is coupled via an aperiodic (untuned) RF transformer to
V2, the self-oscillating mixer. The
oscillator’s tuned circuit consists of
L9, L10 and C2. The resulting IF signal
is fed through L9, L2, L1b & L1a to the
grid of V1 where it is amplified and
fed via L3 the second IF transformer
(L5 & L6).
V3 is the second IF amplifier and its
output feeds grid detector stage V4 (via
L7, L8 & C8). The audio from this stage
is then applied via transformer T1 to
audio amplifier stage V5. Note that in
some sets (but not the 26), V5’s output
is either fed via switch SW2 to a set
of headphones or fed to audio output
stage V6 via transformer T2.
A reflexed horn speaker is fitted into
the bottom of the receiver case (see
photo) and this is driven by V6. The
efficiency of these speakers is quite
high, so the very low output from the
UV99 is perfectly adequate for normal
listening.
Tuning
This compartment at the rear of the set was used to house batteries for portable
use (the owner’s modern rechargeable battery pack is shown here). However, a
larger external battery was generally used to power the set for use at home.
mately 370mA from the three seriesconnected No.6 cells that are used in
the portable configuration.
Adjustable resistor R3 is used to
set the filament voltage applied to the
valves and this must not exceed 3.3V.
Note that if eight valves had been used,
the filament current drain would have
been 500mA.
In addition to the filament current,
valve data books indicate that a UV99
92 Silicon Chip
valve will draw 2.5mA with a bias of
-4.5V and a 90V plate supply. With all
valves drawing the maximum current,
the HT (high-tension) drain will be no
more than 15mA, which can easily
be handled by a relatively small HT
battery pack.
One of the accompanying photos
shows where the batteries sit for portable use (Mike’s modern, rechargeable
battery pack can be seen in the centre
The receiver is tuned using separate
local oscillator and RF controls on
the front panel. We rarely experience
“double-spotting” or image reception
in modern broadcast receivers but radios like the 26 allow the same station
to be heard on at least two other spots
on the broadcast band, this in addition
to the intended position. This is due to
the very low IF used (approximately
55kHz) and also due to the use of the
oscillator’s second harmonic to produce this IF.
As previously indicated, R3 is used
to adjust the filament voltage. It could
be adjusted so that the valves still
received around 3V even with almost
flat batteries.
R2 is the volume control and operates by varying the filament voltage
applied to valve V3. This rather crude
method of volume control was used
on many early radios. No form of AVC
(or AGC) is employed on this receiver
siliconchip.com.au
This plaque attached to the back of the set shows the patent
information relating to RCA’s Radiola 26.
and in fact, this feature didn’t become
common on radio receivers until the
1930s.
Access to the valves is obtained by
removing a metal cover near the top of
the set. The loop antenna is mounted
on the front lid of the receiver and
once the lid is opened, the loop can
be swivelled for best performance.
The antenna loop is terminated on a
4-terminal strip – see Fig.1.
Fig.1 also shows two sets of “A”
batteries, as used for the larger home
battery pack. In addition, the receiver
used four 22.5V B batteries to supply
90V of HT to all valves except the
grid-leak detector (V4).
The main workings of the receiver
are enclosed in a sealed box section
called the “catacomb”. This section
of the receiver is shown within the
dotted lines of Fig.1. The valve sockets
are mounted on the front face of the
catacomb and the valves are the only
components shown within the dottedline enclosure that are actually outside
the shielded box.
Apparently, early superhet receivers
This adjacent label gave advice on battery use. A lead
fitted with a jack plug selected the battery pack.
were difficult to service and the sealed
container was designed to stop people
from fiddling with the adjustments of
this rather critical circuit. Prior to the
introduction of superhets, experimenters and serviceman were only used
to TRF receivers and so might have
been tempted to experiment with the
adjustments in the absence of a cover.
As shown in Fig.1, there are a couple
of coils with the comment “dead end”
on them in the circuit. The purpose of
these coils is unclear, although they
may have been some form of neutralisation system for the IF stages.
No external antenna
Early superhet sets were popular
with people who did not want to take
out a radio listener’s licence, as no external antenna was necessary (which
meant they could avoid detection).
However, they were not used in Australia for many years, mainly because
they were so advanced for their time
that fault-finding proved difficult for
service people, who generally only understood TRF technology. In addition,
there were problems for non-technical
users such as double-spotting and
extraneous whistles.
AWA did make superhets from
1925-1927 but then stopped and made
nothing but TRF receivers until 1933.
It would appear that they found the
early superhets just too advanced for
the average serviceman to effectively
maintain.
The early AWA designs were very
similar to the RCA “catacomb” designs. However, there were a few variations such as the use of anode-bend
detectors and regeneration on the RF
stage (called an “intensifier”). Their
1927 models used L410 or P410 valves
in the audio output stage.
Summary
The RCA 26 was a remarkable
receiver for its time. Even today, it
performs remarkably well, with quite
good sensitivity, although doublespotting and other extraneous whistles
and noises are quite obvious. This
is a set well worthwhile having in a
SC
vintage radio collection.
into MICROS OR PICS?
There’s
There’s asomething
reference to
to suit
suit every
every
microcontroller maestro in the
SILICON CHIP reference bookshop:
see the bookshop pages in this issue
Microcontroller
Projects in C
– by Dogan Ibrahim
Graded projects introduce microelectronics, the 8051 and
$
8100 programming in C.
Programming 16-Bit
Microcontrollers in C –
by Luci Di Jasio
Learning to fly the PIC24. Includes a
CD ROM with source code in C,
Microchip C30 complier
$
8050 and MPLAB SIM.
Hands-On ZigBee
– by Fred Eady
An in-depth look at the clever little
2.4GHz wireless ZigBee chip that’s now
being found in a wide range
$
equipment from
9650 of
consumer to industrial.
PIC in Practice –
by DW Smith
Ideal introduction to PICs. Based on
popular short courses for the PIC for
professionals, techs, hobbyists,
$
60 students and teachers.
PIC Microcontroller –
know it all ( Newnes)
Newnes have put together the best of
subjects their authors have written on
over the past few years
$
7995 into this one handy volume!
The PIC Micro – personal
intro course – by John Morton
A very practical guide which assumes
no prior knowledge. So it is an
introduction to the widely$
52 ideal
used PIC micro.
! Audio ! RF ! Digital ! Analog ! TV ! Video ! Power Control ! Motors ! Robots ! Drives ! Op Amps ! Satellite
siliconchip.com.au
August 2008 93
ALL S ILICON C HIP SUBSCRIBERS – PRINT,
OR BOTH – AUTOMATICALLY QUALIFY FOR A
REFERENCE $ave 10%ONLINE
DISCOUNT ON ALL BOOK OR PARTSHOP PURCHASES.
CHIP BOOKSHOP 10% (Does not apply to subscriptions)
SILICON
For the latest titles and information, please refer to our website books page: www.siliconchip.com.au/Shop/Books
PIC MICROCONTROLLERS: know it all
SELF ON AUDIO
Multiple authors $85.00
The best of subjects Newnes authors have written over the past few years,
combined in a one-stop maxi reference. Covers introduction to PICs and their
programming in Assembly, PICBASIC, MBASIC & C. 900+ pages.
PROGRAMMING and CUSTOMIZING THE
PICAXE By David Lincoln (2nd Ed, 2011) $65.00*
A great aid when wrestling with applications for the PICAXE
See
series of microcontrollers, at beginner, intermediate and
Review
April
advanced levels. Every electronics class, school and library should have a
copy, along with anyone who works with PICAXEs. 300 pages in paperback. 2011
PIC IN PRACTICE
by D W Smith. 2nd Edition - published 2006 $60.00*
Based on popular short courses on the PIC, for professionals, students
and teachers. Can be used at a variety of levels. An ideal introduction to the
world of microcontrollers. 255 pages in paperback.
PIC MICROCONTROLLER – your personal introductory course By John Morton 3rd edition 2005. $60.00*
A unique and practical guide to getting up and running with the PIC. It assumes no knowledge of microcontrollers – ideal introduction for students,
teachers, technicians and electronics enthusiasts. Revised 3rd edition focuses entirely
on re-programmable flash PICs such as 16F54, 16F84 12F508 and 12F675. 226 pages
in paperback.
A collection of 35 classic magazine articles offering a dependable methodology for designing audio power amplifiers to improve performance at every
point without significantly increasing cost. Includes compressors/limiters,
hybrid bipolar/FET amps, electronic switching and more. 467 pages in paperback.
SMALL SIGNAL AUDIO DESIGN
By Douglas Self – First Edition 2010 $95.00*
The latest from the Guru of audio. Explains audio concepts in easy-to-understand language with plenty of examples and reasoning. Inspiration for audio
designers, superb background for audio enthusiasts and especially where it comes to
component peculiarities and limitations. Expensive? Yes. Value for money? YES! Highly
recommended. 558 pages in paperback.
AUDIO POWER AMPLIFIER DESIGN HANDBOOK
by Douglas Self – 5th Edition 2009 $85.00*
"The Bible" on audio power amplifiers. Many revisions and
updates to the previous edition and now has an extra three
chapters covering Class XD, Power Amp Input Systems and
Input Processing and Auxiliarly Subsystems. Not cheap and not a book
for the beginner but if you want the best reference on Audio Power Amps,
you want this one! 463 pages in paperback.
DVD PLAYERS AND DRIVES
by K.F. Ibrahim. Published 2003. $71.00*
OP AMPS FOR EVERYONE
By Bruce Carter – 4th Edition 2013 $83.00*
This is the bible for anyone designing op amp circuits and you don't
have to be an engineer to get the most out of it. It is written in simple language
but gives lots of in-depth info, bridging the gap between the theoretical and the
practical. 281 pages,
PROGRAMMING 32-bit MICROCONTROLLERS
IN C By Luci di Jasio (2008) $79.00*
Subtitled Exploring the PIC32, a Microchip insider tells all on this powerful
PIC! Focuses on examples and exercises that show how to solve common,
real-world design problems quickly. Includes handy checklists. FREE CD-ROM includes
source code in C, the Microchip C30 compiler, and MPLAB SIM. 400 pages paperback.
PRACTICAL GUIDE TO SATELLITE TV
By Garry Cratt – Latest (7th) Edition 2008 $49.00
Written in Australia, for Australian conditions by one of Australia's foremost
satellite TV experts. If there is anything you wanted to know about setting up
a satellite TV system, (including what you can't do!) it's sure to be covered
in this 176-page paperback book.
NEWNES GUIDE TO TV & VIDEO TECHNOLOGY
By KF Ibrahim 4th Edition (Published 2007) $49.00
It's back! Provides a full and comprehensive coverage of video and television technology including HDTV and DVD. Starts with fundamentals so is
ideal for students but covers in-depth technologies such as Blu-ray, DLP,
Digital TV, etc so is also perfect for engineers. 600+ pages in paperback.
RF CIRCUIT DESIGN
by Chris Bowick, Second Edition, 2008. $63.00*
The classic RF circuit design book. RF circuit design is now more important
that ever in the wireless world. In most of the wireless devices that we use
there is an RF component – this book tells how to design and integrate in a
very practical fashion. 244 pages in paperback.
A guide to DVD technology and applications, with particular focus
on design issues and pitfalls, maintenance and repair. Ideal for
engineers, technicians, students of consumer electronics and
sales and installation staff. 319 pages in paperback.
See
Review
March
2010
See
Review
Feb
2004
SWITCHING POWER SUPPLIES A-Z
by Sanjaya Maniktala, Published April 2012. $83.00
Thoroughly revised! The most comprehensive study available of theoretical and practical aspects of controlling and measuring
EMI in switching power supplies.
ELECTRIC MOTORS AND DRIVES
By Austin Hughes & Bill Drury - 4th edition 2013 $59.00*
This is a very easy to read book with very little mathematics or
formulas. It covers the basics of all the main motor types, DC
permanent magnet and wound field, AC induction and steppers and
gives a very good description of how speed control circuits work with these
motors. Soft covers, 444 pages.
AC MACHINES
By Jim Lowe Published 2006 $66.00*
Applicable to Australian trades-level courses including NE10 AC Machines,
NE12 Synchronous Machines and the AC part of NE30 Electric Motor
Control and Protection. Covering polyphase induction motors, singlephase motors, synchronous machines and polyphase motor starting. 160
pages in paperback.
PRACTICAL VARIABLE SPEED DRIVES &
POWER ELECTRONICS
Se
e
by Malcolm Barnes. 1st Ed, Feb 2003. $73.00* Review
An essential reference for engineers and anyone who wishes
to design or use variable speed drives for induction motors.
286 pages in soft cover.
Feb
2003
BUILD YOUR OWN ELECTRIC MOTORCYCLE
PRACTICAL RF HANDBOOK
by Ian Hickman. 4th edition 2007 $61.00*
by Douglas Self 2nd Edition 2006 $69.00*
by Carl Vogel. Published 2009. $40.00*
A guide to RF design for engineers, technicians, students and enthusiasts.
Covers key topics in RF: analog design principles, transmission lines,
couplers, transformers, amplifiers, oscillators, modulation, transmitters and
receivers, propagation and antennas. 279 pages in paperback.
Alternative fuel expert Carl Vogel gives you a hands-on guide with
the latest technical information and easy-to-follow instructions
for building a two-wheeled electric vehicle – from a streamlined
scooter to a full-sized motorcycle. 384 pages in soft cover.
*NOTE: ALL PRICES ARE PLUS P&P – AUSTRALIA ONLY: $10.00 per order; NZ – $AU12.00 PER BOOK; REST OF WORLD $AU18.00 PER BOOK
PAYPAL (24/7)
INTERNET (24/7)
MAIL (24/7)
PHONE – (9-5, Mon-Fri)
eMAIL (24/7)
FAX (24/7)
To
ilicon Chip Use your PayPal account
www.siliconchip.
Call (02) 9939 3295 with
silicon<at>siliconchip.com.au
Your order and card details to Your order to PO Box 139
Place94 S
com.au/Shop/Books silicon<at>siliconchip.com.au
Collaroy NSW 2097
with order & credit card details
with order & credit card details (02) 9939 2648 with all details
Your
You can also order and pay for books by cheque/money order (Mail Only). Make cheques payable to Silicon Chip Publications.
Order:
ALL TITLES SUBJECT TO AVAILABILITY. PRICES VALID FOR MONTH OF MAGAZINE ISSUE ONLY. ALL PRICES INCLUDE GST
ALL S ILICON C HIP SUBSCRIBERS – PRINT,
OR BOTH – AUTOMATICALLY QUALIFY FOR A
REFERENCE $ave 10%ONLINE
DISCOUNT ON ALL BOOK OR PARTSHOP PURCHASES.
CHIP BOOKSHOP 10% (Does not apply to subscriptions)
SILICON
For the latest titles and information, please refer to our website books page: www.siliconchip.com.au/Shop/Books
PIC MICROCONTROLLERS: know it all
SELF ON AUDIO
Multiple authors $85.00
The best of subjects Newnes authors have written over the past few years,
combined in a one-stop maxi reference. Covers introduction to PICs and their
programming in Assembly, PICBASIC, MBASIC & C. 900+ pages.
PROGRAMMING and CUSTOMIZING THE
PICAXE By David Lincoln (2nd Ed, 2011) $65.00*
A great aid when wrestling with applications for the PICAXE
See
series of microcontrollers, at beginner, intermediate and
Review
April
advanced levels. Every electronics class, school and library should have a
copy, along with anyone who works with PICAXEs. 300 pages in paperback. 2011
PIC IN PRACTICE
by D W Smith. 2nd Edition - published 2006 $60.00*
Based on popular short courses on the PIC, for professionals, students
and teachers. Can be used at a variety of levels. An ideal introduction to the
world of microcontrollers. 255 pages in paperback.
PIC MICROCONTROLLER – your personal introductory course By John Morton 3rd edition 2005. $60.00*
A unique and practical guide to getting up and running with the PIC. It assumes no knowledge of microcontrollers – ideal introduction for students,
teachers, technicians and electronics enthusiasts. Revised 3rd edition focuses entirely
on re-programmable flash PICs such as 16F54, 16F84 12F508 and 12F675. 226 pages
in paperback.
A collection of 35 classic magazine articles offering a dependable methodology for designing audio power amplifiers to improve performance at every
point without significantly increasing cost. Includes compressors/limiters,
hybrid bipolar/FET amps, electronic switching and more. 467 pages in paperback.
SMALL SIGNAL AUDIO DESIGN
By Douglas Self – First Edition 2010 $95.00*
The latest from the Guru of audio. Explains audio concepts in easy-to-understand language with plenty of examples and reasoning. Inspiration for audio
designers, superb background for audio enthusiasts and especially where it comes to
component peculiarities and limitations. Expensive? Yes. Value for money? YES! Highly
recommended. 558 pages in paperback.
AUDIO POWER AMPLIFIER DESIGN HANDBOOK
by Douglas Self – 5th Edition 2009 $85.00*
"The Bible" on audio power amplifiers. Many revisions and
updates to the previous edition and now has an extra three
chapters covering Class XD, Power Amp Input Systems and
Input Processing and Auxiliarly Subsystems. Not cheap and not a book
for the beginner but if you want the best reference on Audio Power Amps,
you want this one! 463 pages in paperback.
DVD PLAYERS AND DRIVES
by K.F. Ibrahim. Published 2003. $71.00*
OP AMPS FOR EVERYONE
By Bruce Carter – 4th Edition 2013 $83.00*
This is the bible for anyone designing op amp circuits and you don't
have to be an engineer to get the most out of it. It is written in simple language
but gives lots of in-depth info, bridging the gap between the theoretical and the
practical. 281 pages,
PROGRAMMING 32-bit MICROCONTROLLERS
IN C By Luci di Jasio (2008) $79.00*
Subtitled Exploring the PIC32, a Microchip insider tells all on this powerful
PIC! Focuses on examples and exercises that show how to solve common,
real-world design problems quickly. Includes handy checklists. FREE CD-ROM includes
source code in C, the Microchip C30 compiler, and MPLAB SIM. 400 pages paperback.
PRACTICAL GUIDE TO SATELLITE TV
By Garry Cratt – Latest (7th) Edition 2008 $49.00
Written in Australia, for Australian conditions by one of Australia's foremost
satellite TV experts. If there is anything you wanted to know about setting up
a satellite TV system, (including what you can't do!) it's sure to be covered
in this 176-page paperback book.
NEWNES GUIDE TO TV & VIDEO TECHNOLOGY
By KF Ibrahim 4th Edition (Published 2007) $49.00
It's back! Provides a full and comprehensive coverage of video and television technology including HDTV and DVD. Starts with fundamentals so is
ideal for students but covers in-depth technologies such as Blu-ray, DLP,
Digital TV, etc so is also perfect for engineers. 600+ pages in paperback.
RF CIRCUIT DESIGN
by Chris Bowick, Second Edition, 2008. $63.00*
The classic RF circuit design book. RF circuit design is now more important
that ever in the wireless world. In most of the wireless devices that we use
there is an RF component – this book tells how to design and integrate in a
very practical fashion. 244 pages in paperback.
A guide to DVD technology and applications, with particular focus
on design issues and pitfalls, maintenance and repair. Ideal for
engineers, technicians, students of consumer electronics and
sales and installation staff. 319 pages in paperback.
See
Review
March
2010
See
Review
Feb
2004
SWITCHING POWER SUPPLIES A-Z
by Sanjaya Maniktala, Published April 2012. $83.00
Thoroughly revised! The most comprehensive study available of theoretical and practical aspects of controlling and measuring
EMI in switching power supplies.
ELECTRIC MOTORS AND DRIVES
By Austin Hughes & Bill Drury - 4th edition 2013 $59.00*
This is a very easy to read book with very little mathematics or
formulas. It covers the basics of all the main motor types, DC
permanent magnet and wound field, AC induction and steppers and
gives a very good description of how speed control circuits work with these
motors. Soft covers, 444 pages.
AC MACHINES
By Jim Lowe Published 2006 $66.00*
Applicable to Australian trades-level courses including NE10 AC Machines,
NE12 Synchronous Machines and the AC part of NE30 Electric Motor
Control and Protection. Covering polyphase induction motors, singlephase motors, synchronous machines and polyphase motor starting. 160
pages in paperback.
PRACTICAL VARIABLE SPEED DRIVES &
POWER ELECTRONICS
Se
e
by Malcolm Barnes. 1st Ed, Feb 2003. $73.00* Review
An essential reference for engineers and anyone who wishes
to design or use variable speed drives for induction motors.
286 pages in soft cover.
Feb
2003
BUILD YOUR OWN ELECTRIC MOTORCYCLE
PRACTICAL RF HANDBOOK
by Ian Hickman. 4th edition 2007 $61.00*
by Douglas Self 2nd Edition 2006 $69.00*
by Carl Vogel. Published 2009. $40.00*
A guide to RF design for engineers, technicians, students and enthusiasts.
Covers key topics in RF: analog design principles, transmission lines,
couplers, transformers, amplifiers, oscillators, modulation, transmitters and
receivers, propagation and antennas. 279 pages in paperback.
Alternative fuel expert Carl Vogel gives you a hands-on guide with
the latest technical information and easy-to-follow instructions
for building a two-wheeled electric vehicle – from a streamlined
scooter to a full-sized motorcycle. 384 pages in soft cover.
*NOTE: ALL PRICES ARE PLUS P&P – AUSTRALIA ONLY: $10.00 per order; NZ – $AU12.00 PER BOOK; REST OF WORLD $AU18.00 PER BOOK
PAYPAL (24/7)
INTERNET (24/7)
MAIL (24/7)
PHONE – (9-5, Mon-Fri)
eMAIL (24/7)
FAX (24/7)
To
siliconchip.com.au
Use your PayPal account
www.siliconchip.
Call (02) 2008 95
9939 3295 with
silicon<at>siliconchip.com.au
Your order and card details to Your order to PO Box 139 August
Place
com.au/Shop/Books silicon<at>siliconchip.com.au
Collaroy NSW 2097
with order & credit card details
with order & credit card details (02) 9939 2648 with all details
Your
You can also order and pay for books by cheque/money order (Mail Only). Make cheques payable to Silicon Chip Publications.
Order:
ALL TITLES SUBJECT TO AVAILABILITY. PRICES VALID FOR MONTH OF MAGAZINE ISSUE ONLY. ALL PRICES INCLUDE GST
PRODUCT SHOWCASE
Low-cost video and still capture recorder
from Tenrod
Tenrod has just released their latest
Digital Video Recorder module, the
DVR623. This low-cost module comes
complete with wired camera and
keyboard to make a convenient
start-up system.
It is an easy-to-operate, automatic
and low-cost video and still capture
recorder, able to detect movement
via the camera, enabling automatic video
recording or still capture.
At the same time, it can provide a live output to a TV monitor from its video‑ camera.
It also has an alarm output which can be
utilised to alert an operator, trigger an alarm
or activate other functions.
The module, supplied without enclosure,
needs only a single DC power source to
operate.
Image size is VGA or QVGA, with a variable
frame rate setting of 1, 10 and 30 fps. Recording duration can be set from 1-99 seconds.
Small 4-inch TFT colour LCD screens are also
available for use in conjunction as a small
portable monitor.
Contact:
Tenrod Australia Pty Ltd
1/24 Vore Street, Silverwater, NSW 2128
Tel: (02) 9748 0655 Fax: (02) 9748 0258
Website: www.tenrod.com.au
Voice Activated Universal Remote Control
Want to add voice-activated remote control – to just about anything? This amazing
device allows you to control anything that
has a remote control with voice commands.
No matter if it’s your TV, Stereo, Set-top Box
or even air conditioner, now you can control
them all without even lifting a finger.
Simply set up your voice command and
then press the appropriate buttons on your
original remote control, the voice activated
controller will then “learn” the signals
and reproduce them whenever you trigger
it with your voice
command. Up to
ten signals can
be transmitted
with one voice
command.
Contact:
MicrogramAustralia Pty Ltd
PO Box 8202, Tumbi Umbi, NSW 2261
Tel: 1800 625 777 Fax: (02) 4389 0234
Website: www.mgram.com.au
Microcontroller Development Boards
Arduino is an open-source microcontroller
development board and environment based
on the ATMega168 AVR microcontroller
family and a simple programming language
based on C++. They are available from Ocean
Controls in Victoria.
The Arduino Diecimila USB is ready to be
programmed using a USB port, without the
need for a separate hardware programmer.
The Arduino-compatible Skinny board
shrinks the design by separating the programmer from the board and provides a smaller,
cheaper alternative.
The Arduino LilyPad is like the Skinny, but
is designed to be wearable e-textile technology
by making it washable and incorporating large
connecting pads to allow it to be sewn to clothing with conductive thread. A starter kit and
96 Silicon Chip
many sensor
boards are
available as
well.
There are
free and easyto-learn programming tools compatible with Windows,
Mac and Linux, and
boards starting from
$27.50 + GST.
Contact:
Ocean Controls
3/24 Wise Avenue, Seaford, Vic 3198
Tel: (03) 9782 5882 Fax: (03) 9782 5517
Website: www.oceancontrols.com.au
Superb L-C Meter Kit
Altronics have sent
us their version of the
SILICON CHIP L-C meter
(June 2008) . . . and we
have to say we’re very
impressed!
They’ve gone for a
professional instrument-style case – it’s
larger and flatter than
the zippy box we used
but certainly “feels”
more instrument-ish, with terminals at the
top and the display on the front.
Otherwise, the kit follows the original
design. The kit (Cat K2533), which is available from Altronics stores and dealers, has
a retail price of $84.95.
Contact:
Altronics Distributors Pty Ltd
174 Rowe Street, Perth, WA 6000
Tel: 1300 797 007 Fax:1300 789 777
Website: www.altronics.com.au
ANTRIM
TRANSFORMERS
manufactured in
Australia by
Harbuch Electronics Pty Ltd
harbuch<at>optusnet.com.au
Toroidal – Conventional Transformers
Power – Audio – Valve – ‘Specials’
Medical – Isolated – Stepup/down
Encased Power Supplies
Toroidal General
Construction
OUTER
INSULATION
OUTER
WINDING
WINDING
INSULATION
INNER
WINDING
CORE
CORE
INSULATION
Comprehensive data available:
www.harbuch.com.au
Harbuch Electronics Pty Ltd
9/40 Leighton Pl, HORNSBY 2077
Ph (02) 9476 5854 Fax (02) 9476 3231
siliconchip.com.au
ASK SILICON CHIP
Got a technical problem? Can’t understand a piece of jargon or some technical principle? Drop us a line
and we’ll answer your question. Write to: Ask Silicon Chip, PO Box 139, Collaroy Beach, NSW 2097 or
send an email to silchip<at>siliconchip.com.au
Garage door
indicator wanted
Do you know of a circuit that tells
me if my garage door is up or down?
I want this done wirelessly, so a
simple magnetic reed switch on the
garage door sends a wireless signal to
a receiver inside the house (say up to
20m) such that if the door is up, a LED
lights up. (B. C., via email).
• We published a Garage Door Indicator in the January 2007 issue. If you
want to run the receiver section from
a 9V battery instead of the specified
12V plugpack, you can omit the 7809
3-terminal regulator, change the two
680W resistors to 1.5kW and change the
LEDs to high brightness types.
Bigger transformer
is a problem
I’m about to construct one of your
fine Studio 350 amplifier modules
(January 2004) to power a subwoofer
system. Unfortunately I am finding it
difficult to obtain the recommended
toroidal transformer with 50V + 50V
output at 500VA. Jaycar and Altronics
used to stock them but now only have
a 55V + 55V transformer. This will give
DC voltages of around ±77V instead of
±70V. I am wondering if this will be
fine with either minimal or no changes
to the design. (J. W., via email).
• The problems with using a 55V +
55V transformer are two-fold. First,
because it gives a 10% higher supply rail, the overall dissipation of the
amplifier can be expected to increase
by about 21%, so it will get quite a
bit hotter. This may or may not be a
problem if you are using 8-ohm loudspeakers and will have an upside in
that the maximum power output will
also go up by about 20%, from 240W
music power to about 290W.
But if you are using a 4-ohm loudspeaker, much higher supply rails
mean that the amplifier could be
driven beyond the safe operating area
(SOA) of the output transistors, as
depicted in the diagram on page 14 of
the article. That might mean that you
blow the transistors and possibly, as
a result, burn out the speaker as well.
That could be extremely costly.
Hence, it would be preferable if you
use the specified 50V + 50V transformer. Contact Harbuch Electronics
at (02) 9476 5854. They should be able
to supply a suitable unit.
Recommended value for
reset pull-up resistor
I have noticed that the pull-up
resistor on the reset pin of the PIC
microcontrollers varies between 1kW
and 100kW, depending on the circuit.
The data sheet on the 16F88 indicates
a circuit with R less than 40kW. Could
you please comment on this? (G. C.,
Mt Dandenong, Vic).
• The recommended value for a
pull-up resistor on the MCLR line
of the PIC16F88 ranges from 1kW (to
limit transient current) through to a
maximum of 40kW. The value used
depends a lot on the designer’s whim
at the time. Typically, we prefer a value
of 10kW because it provides a lower
current into the MCLR pin should a
transient occur or should the supply
go below Vdd. The 40kW maximum is
because leakage current from the pin
could affect reset operation should a
higher value be used.
Charging problems
with tank sender
I recently built the telemetry version
of your rain water tank level meter. It
appears to be working fine, but I’m
having problems with the sender unit’s
power supply. The article says that
it can be powered from a plugpack
provided a rechargeable AA battery
is present (I’m using a NiMH one). It
doesn’t suggest a suitable voltage for
the plugpack, so I chose the smallest I
could find, 6V (switchmode, I believe).
Having connected this up, I saw the
Courtesy Light Delay for Cars
I have built the ‘Courtesy Light
Delay for Cars’ which worked perfectly in my previous car. I now have
a different car with three internal
lights which draw too much current
from the light delay kit. This makes
the lights stay extremely dim for the
set delay time.
Is there any component in the kit
I could change to allow more current during the delay period? If not,
would changing the lights to LEDs
help or allow too much current to
flow? (D. A., via email).
siliconchip.com.au
• The lamp current is effectively
set by the on-resistance of the Mosfet
and this is initially set to a low value
to switch on the lamps fully.
The dimming is due to the resistance of the Mosfet increasing as its
gate voltage decreases over time. At
switch-on the Mosfet should be low
resistance and the lamps should light
fully regardless whether there are three
lights or one.
You may be able to increase the
effective brightness of the lamps by
increasing the C1 value to 1000µF.
This would give more gate voltage
at switch-on. Also increasing R2 to
470kW may help increase the initial
gate voltage.
If you use LED lights, then a 100W
5W resistor would have to be placed
across the courtesy light circuit in
place of the original lamps to provide the circuit supply current. LED
lighting tends to have several LEDs in
series plus a current limiting resistance and so there is too little voltage
for the circuit to work without this
extra resistor.
August 2008 97
Making Relay Selector More Flexible
I found a “Circuit Notebook” item
in the January 2006 issue that will be
useful for me. It is a pushbutton relay
selector. I was wondering if someone
could leak the identity of IC1 to me.
I promise I’ll keep it a secret. Is there
a way this circuit could be modified
so that it does not trip one relay off
before activating the next (ie, to give
the option of multiple ‘lives’? (D. M.,
Camden, NSW).
• As shown on the circuit diagram
to which you refer, IC1 is a 4093B
quad CMOS Schmitt NAND gate.
In order to modify this circuit to
allow more than one relay to be activated at a time, you’d need to use
diodes (eg, 1N4148) to gate the relay
voltage displayed on the LCD of the
reader unit climb to somewhere over
1.5V. However, at some point after
that the voltage began to drop until
the sender was no longer able to communicate with the reader unit.
I then checked the plugpack output
with a multimeter and found that it
was producing only about 0.7V with
no load. Has the sender unit destroyed
the plugpack? Replacing the NiMH
battery with an alkaline one made
the sender unit operational again, but
I’d prefer to not have to change the
battery. I’m also not particularly keen
to use a solar panel because the tank
is a fair way from natural light. Any
suggestions would be appreciated. (J.
B. Umina Beach, NSW).
• The Schottky diode D2 must be
replaced with a 1kW resistor as mentioned in the article. The plugpack
can be any voltage from 3V to 12V. If
the cell does not stay charged, then
the charge current is not sufficient. A
lower resistor value may be required.
Typically you need about 1/10th of
the full charging current for the cell,
as listed on the cell itself.
Calculate the current by subtracting
1.25V from the plugpack voltage and
dividing by the resistor value. A 6V
plugpack with a 1kW limiting resistor
should charge at about 4.8mA.
IR decoding for
slave flash
I have constructed the digital slave
flash trigger from the July 2003 issue
98 Silicon Chip
driver transistors from more than
one output of IC2. For example, in
order to have both relay 1 and relay
2 on together, you’d need to have
an additional selector pushbutton
switch connected between (say)
IC2’s output 5 (pin 1) and pin 9 of
IC1c, to create a fifth (1+2) selection
setting. Then you’d also use a pair of
1N4148 diodes to connect between
the O5 output of IC2 and the gates
of Q1 and Q2, with a 100W resistor
in series with each diode.
Then when you press S6 the extra
selector button, the counter will stop
at the O5 position and both relay
drivers Q1 and Q2 would be turned
on together.
but am wondering whether it can be
modified for infrared transmitter operation. I have a Canon 430EX flash
unit with optional slave unit function
for IR control. (Y. H., via email).
• It would not be possible without
major modifications so that the slave
trigger could decode and respond to
the IR code from your flash gun. In
any case, the slave flash should be
directly compatible with your flash
gun as it is.
Noise cancelling for
Kenwood Chef Mixer
My wife’s Kenwood Chef mixer
is very noisy. I Googled “noise” and
“Kenwood Chef” in an effort to find
out if having such a noisy machine is
normal (it is, apparently).
What I need is for someone to invent
a noise-cancelling device for the Kenwood Chef. Because I am not technical
I can’t do it myself but surely someone
could tell me how to set up a microphone and speaker to sit next to the
noisy mixer, with a noise-cancelling
circuit to kill the noise!
Would it work “in the open” or
does the technique only work with
headphones? (I guess one problem in
the open might be that the microphone
would also pick up the “out of phase”
sound from the speaker. (T. J., Gordon,
NSW).
• The Kenwood Chef must be one of
the noisiest kitchen appliances ever
invented. Noise-cancelling does not
work in the open. You need closed
chamber such as in Bose headphones,
the cabin of car (eg, Honda Legend) or
an appliance cupboard. It would be
possible to do noise-cancelling in an
appliance cabinet but really, if you are
using a mixer you do need to be able
to open the cupboard while you use
it and that action would destroy the
noise-cancelling.
Ultimately, we don’t think such a
project is viable. We have pulled a
Kenwood mixer apart to see where
the noise was coming from. It is a
combination of motor and gearbox
noise which is exacerbated by the
speed control which has a tendency
to “hunt” back and forth, regardless
of the speed setting.
In reality, they should give away
a free set of ear protectors whenever
they sell this appliance! Failing that,
the best approach is to shut the mixer
in an appliance cabinet while it is in
use.
Upgrade for 3-way
Active Crossover
I was wondering, since you have
produced the new ultra fidelity preamp and various new amplifier modules, whether there might be plans to
offer an upgraded version of this 3-way
Active Crossover kit featured in the
January 2003 issue?
The TL074 op amps featured in
the circuit are now outdated. Would
the new National Semiconductor
LME49740 op amps drop in without
any circuit modifications?
If a total upgrade was planned I
would like to see level controls for the
various output bands available on the
front panel, plus an overall input level
adjustment and a buffered full range
input/output loop. (D. B., via email).
• We have no immediate plans to
upgrade the Active 3-way Crossover. It
does appear as though the LME49740
could be a direct drop-in replacement
for the TL074s and is a far superior op
amp. However, given the circuit configuration used, there is no guarantee
that the overall noise performance and
distortion would be much improved.
PIC-based tank level
meter has surges
I have built the PIC Based Water
Tank Level Meter (SILICON CHIP, November & December 2007 and January
2008). All works well in general but I
siliconchip.com.au
CD-ROM Playback Adaptor Fault
I have recently completed a CDROM Audio Playback Adaptor kit
(SILICON CHIP, November 2007) but
I cannot get the LCD module to initialise properly. It merely displays a
single line of 16 blocks of dot matrix
patterns. The supply rails indicate
the correct voltages and pins 1 & 2
on the LCD module also show +5V
and 0V respectively, which I believe
is correct for the Jaycar supplied
module.
I have tested this with three different CD-ROMs, two of them pulled
from working PCs so I don’t imagine
that this is a compatibility problem.
I have done the usual checks of the
board for broken tracks and shorts,
resoldering any suspect joints etc
but to no avail.
Would this problem indicate that
the micro supplied has not been
programmed or that I have somehow
accidentally erased the program or
should I look elsewhere for a solution?
(S. R., Hastings, Vic).
• The symptoms you describe could
be caused by a number of factors,
including:
(1) the LCD module connection to
the board is not good (some of the 16
connections may be bad);
(2) the microcontroller has not
been programmed with the correct
fuse bits;
(3) the microcontroller is faulty or
not programmed properly (unlikely)
or (4) the LCD module is faulty (unlikely).
The first item is the most likely
cause of your problems, so we suggest that you double-check that all
16 connections from the board to the
LCD module are actually good. If you
have access to an oscilloscope, you
should check the relevant lines like
E (enable) at the LCD module and
you should see short pulses when
the microcontroller is trying to write
to the LCD module.
The relevance of (2) is that if the
fuse bits on the microcontroller have
not been programmed correctly, the
microcontroller may not be running at the correct clock frequency
of 7.3728MHz. If this was the case,
since the LCD module you have is
sensitive to small timing discrepancies, it would give the symptoms you
are describing. In other words, the
micro must be running at 7.3728MHz
or very close to it, for the software to
work correctly.
Given a preprogrammed microcontroller, it is very difficult to erase
it simply by handling it, so unless
the microcontroller was faulty or not
programmed properly then points (3)
and (4) are unlikely.
have a few questions.
In the telemetry version I find that
when I calibrate the tank level, sometimes I get sudden display surges of up
to 10%. For example, when I calibrate
at 85% tank level, the value transmitted and displayed remains at 85% for
a while, the suddenly may jump to
94%, and after another 15 minutes or
so, returns to the original, true value
of 85%.
I am using the shortest update interval of approximately 16 seconds.
I use the version where the sensor is
mounted in a separate box outside the
tank, fed by a T-piece in the outflow
line.
I think that these surges are caused
by the water pressure pump fed from
the tank. But why does it then not
return to 85% soon after the pump
has switched off? Is there something
like hysteresis or friction in the sensor? Or does the software cause this
delay effect?
The battery voltage shown on the
receiving end is 1.3V or more, even at
night. This would be about 0.1V too
high. Where can I calibrate it? (K. F.,
Munster, WA).
• The water tank level meter receiver
may show a higher level for a long
period because the signal from the
transmission is not received reliably.
So a valid signal may only occur every
15 minutes. You can check whether the
receiver detects a valid signal within
16 seconds by switching off power to
the receiver then switching on. The
display should show the correct levels
within 16s. Transmission and reception is improved using an external
antenna, as discussed in the articles.
Sensor hysteresis is 0.1%.
The voltage across the cell could
be 1.3V. Check this with a multimeter. Rechargeable cells that are
charged can show 1.3V when lightly
loaded.
The cell readings are taken with
the water level meter powered up
and accuracy is set by the 5V calibration for the switchmode regulator output using VR1. There is no
other adjustment since the analog
to digital converter for the reading
is referenced to the 5V supply. It is
accurate to within about 5mV.
the battery when starting the bike. I
have already assembled the kit, bench
tested it, set it appropriately and all
works fine but I do have a question to
do with the signal input.
I would like to use a direct connection to the battery as the signal input.
I figured this would be OK as when
the bike is off, the battery outputs between 12.5 - 13.2V, whereas once the
bike is actually running, the regulator
increases the voltage to 14V - 15V. Will
using a direct connection to the battery
as a signal input be OK?
I’m worried that the Universal Switch
might get fried or something since the
signal input is connected directly to
the battery. Should I be worried about
anything else if I do set it up this
way? I plan to connect the ignition
siliconchip.com.au
Uncertainty about
Voltage Switch kit
I recently purchased a Universal
Voltage Switch kit from Jaycar (Performance Electronics for Cars). I intend
to install the switch on my motorbike,
to stop the headlights from turning on
until the engine has started.
At the moment, they turn on automatically as soon as you put the key
in and switch the bike to ‘ON’. I want
to do this so that there is less strain on
Ozitronics
Tel: (03) 8677 1411 Fax: (03) 9011 6220
Email: sales2008<at>ozitronics.com
Rolling Code 2-Channel
UHF Remote
K157 - $80.30
Momentary or
latching relays
with indicator
LEDs and reset
inputs. Up to
15 Tx can be
linked to one
Rx. 12VDC.
Also available assembled: K157A - $95.70
Extra 2 and 4 button remotes also available
More kits & documentation available on website:
www.ozitronics.com
:
August 2008 99
switch +12V to an accessories wire
and of course, ground the switch to the
chassis. (S. S., via email).
• The Voltage Switch is protected
for operation from a bike battery, with
zener diode ZD2 at the signal input and
with zener diode ZD1 at the supply input. The unit is therefore suited to your
application without danger of damage
to the electronics in the circuit.
LED ammeter
for a genset
I would like to use the LED Bargraph
Ammeter (SILICON CHIP, January 1999)
on a portable genset. It would need
to go across a 50mV shunt and start
at 0V, LED 1. What mods would be
needed please? How about a project
combining the above and the Battery
Monitor featured in Electronics Australia in the May 1987 issue? (H. B.,
Wynyard, Tas).
• The LED Ammeter is capable of
displaying a 20A range with a 0-40mV
input. The range and offset from zero
is adjustable and no changes to the
circuit should be necessary. There is
no reason why you could not incorporate the EA display with the LED
Ammeter display.
MPLAB not needed for
dsPIC programmer
Regarding the PIC programmer project described in the May 2008 issue of
SILICON CHIP, I assume it requires the
MPLAB program as well as WinPic to
operate. If this is the case, which of
the MPLAB programs is required? (A.
D., via email).
• The dsPIC programmer in the
May 2008 issue works with WinPIC,
as described in the article. You do not
need MPLAB to use it. You simply load
a .hex file into WinPIC and program
your PIC/dsPIC that way.
The only reason you may need
MPLAB is to compile your source code
into a hex file. For that, almost any
version (including the most current)
is suitable.
Trouble-shooting
an ignition kit
I have just completed repairing a
high energy ignition kit that my son
built some years ago. He blew it up
accidentally by hooking it up incorrectly. I have replaced Q1 with the
TO-3 package and have also replaced
the MC3334 and Q3. All the other
components have been checked.
My problem is that Q1 stays on,
regardless of the points being open
or shut. I recently purchased the back
issue of SILICON CHIP to help me set
it up. The kit does everything as per
instructions. Originally the car did not
have a ballast resistor but I have since
installed one. It still does not work.
Do you have any idea what could be
wrong? I have built the points version.
(J. C., via email).
• The transistor will appear to
remain on with points open because
this transistor only opens (goes off) for
a short 0.9ms period before switching
on again. This is the dwell extension
feature of the ignition circuit.
You can temporarily alter the circuit so that the transistor will follow
the action of the points by placing a
short across the C1 (0.1µF) capacitor
at the collector of Q2 that passes signal through to pin 5 of IC1 via a 22kΩ
resistor.
If the transistor still remains on with
this test, perhaps the transistor’s case
Notes & Errata
UV Light Box, November 2007: the
4.7kW resistor shown connected
between pin 3 & 10 of IC1 is incorrect. It should be between pin 10
and +5V, as on the PC board.
is shorted to the metal box or the zener
diodes are shorted.
Aid wanted for setting
pendulum clocks
I have some difficulty in setting several pendulum clocks vertical so that
the pendulum beats correctly. Listening to the “tick-tock”, as advised by
Mr Eckles (not a joke), the horologist
to the National Trust, and adjusting the
vertical position from the “tick-tock--tick-tock”, is quite difficult.
Could you consider a project that
would listen to the beat and display
the timing and difference in the beat
so that the pendulum length could
also be adjusted to beat seconds?
Could this project be used for other
audible timing measurements? (J. H.,
via email).
• That is really quite a specialised
application so we would not do it as
a project. In any case, it would be
more practical to have the pendulum
work with a photo-interrupter and
an accurate period counter. However
it would need to be very accurate, of
the order of several parts per million
to usefully set pendulum length for
good time-keeping.
As an aside, part of the charm of
keeping old clocks is the trial and error
process of adjusting pendulum clocks.
It can take months to get it right, as
you have found.
SC
WARNING!
SILICON CHIP magazine regularly describes projects which employ a mains power supply or produce high voltage.
All such projects should be considered dangerous or even lethal if not used safely.
Readers are warned that high voltage wiring should be carried out according to the instructions in the articles.
When working on these projects use extreme care to ensure that you do not accidentally come into contact with
mains AC voltages or high voltage DC. If you are not confident about working with projects employing mains voltages
or other high voltages, you are advised not to attempt work on them. Silicon Chip Publications Pty Ltd disclaims
any liability for damages should anyone be killed or injured while working on a project or circuit described in any
issue of SILICON CHIP magazine. Devices or circuits described in SILICON CHIP may be covered by patents. SILICON
CHIP disclaims any liability for the infringement of such patents by the manufacturing or selling of any such equipment. SILICON CHIP also disclaims any liability for projects which are used in such a way as to infringe relevant
government regulations and by-laws.
Advertisers are warned that they are responsible for the content of all advertisements and that they must conform to the Trade Practices Act 1974 or as subsequently amended and to any governmental regulations which are
applicable.
100 Silicon Chip
siliconchip.com.au
MARKET CENTRE
Cash in your surplus gear. Advertise it here in SILICON CHIP
CLASSIFIED ADVERTISING RATES
Advertising rates for these pages: Classified ads: $29.50 (incl. GST) for up to 20
words plus 85 cents for each additional word. Display ads: $54.50 (incl. GST) per
column centimetre (max. 10cm). Closing date: 5 weeks prior to month of sale.
To book your classified ad, email the text to silicon<at>siliconchip.com.au and
include your name, address & credit card details, or fax (02) 9939 2648, or post
to Silicon Chip Classifieds, PO Box 139, Collaroy, NSW, Australia 2097.
Enclosed is my cheque/money order for $__________ or please debit my
o
Visa Card o Master Card
Card No.
Signature_____________________________ Card expiry date______/______
Name _________________________________________________________
Street _________________________________________________________
Suburb/town ______________________________ Postcode______________
Phone:______________ Fax:______________ Email:___________________
FOR SALE
TECH REPAIRS SERVICE MANUALS:
www.techrepairs.org
Thousands of manuals for all brands,
makes and models including: Vintage
Radio, PDP, LCD, VCR, DVD, CTV,
Laptops, Monitors, Sewing Machines,
Washing Machines, Dryers, Fridges
and many more. An absolute must have
website for any Tech!
RCS RADIO/DESIGN is at 41 Arlewis
St, Chester Hill 2162, NSW Australia
and has all the published PC boards
from SC, EA, ETI, HE, AEM & others. Ph
(02) 9738 0330. sales<at>rcsradio.com.
au; www.rcsradio.com.au
LEDs! Nichia superbright oval LEDs
and 5mm Agilent (HP) LEDs - brandname quality LEDs at Chinese LED
prices! Osram surface mount range and
other NOS standard and superbright
brand name LEDs from just a few cents
each. Cree XR-E LEDs, LED drivers,
kits and other interesting stuff. www.
ledsales.com.au
FACTORY OUTLET: flexible neon wire.
Sheet (Backlight cuttable) flower. LGP
Backlight. EL products. Phone 041
771 8607 Fax (07) 3397 5787. Email:
cjappliance<at>gmail.com
DOWNLOAD OUR CATALOG at
MicroByte Electronics: PIC Micros
– Development Board – Development
tools & Components. Phone: (03) 9378
4288. info<at>microbyte.com.au; www.
microbyte.com.au
WORLDWIDE ELECTRONIC COMPONENTS
PO Box 631, Hillarys, WA 6923
Ph: (08) 9307 7305 Fax: (08) 9307 7309
Email: worcom<at>iinet.net.au
PCBs MADE, ONE OR MANY. Any
format, hobbyists welcome. Sesame
Electronics Phone (02) 9593 1025.
sesame<at>sesame.com.au
www.sesame.com.au
www.iinet.net.au/~worcom
siliconchip.com.au
CUSTOMERS: Truscotts Electronic
World – large range of semiconductors
and passive components for industry,
hobbyist and amateur projects including Drew Diamond. 27 The Mall, South
Croydon, Melbourne. (03) 9723 3860.
electronicworld<at>optusnet.com.au
WANTED
WANTED: A REINARTZ COIL, Aegis
type M12. Please contact Nathan on (02)
9586 3017 or email me nsamuels1<at>
bigpond.com
KIT ASSEMBLY
KEITH RIPPON KIT ASSEMBLY &
REPAIR:
* Australia & New Zealand;
* Small production runs.
Phone Keith 0409 662 794.
keith.rippon<at>gmail.com
August 2008 101
VIDEO - AUDIO - PC
Degen 1103 Pocket Receiver
distribution amps - splitters
digital standards converters - tbc's
switchers - cables - adaptors
genlockers - scan converters
bulk vga cable - wallplates
Range 100kHz
- 29,999kHz,
direct entry,
digital display.
Listen to SSB,
amateur radio,
marine weather,
HF aircraft, shortwave and many
more. Supplied with rechargeable
AA batteries, approved charger, 10m
longwire, carry case and earphones.
$159.00 + P/H
Contact Av-Comm Pty Ltd 02 9939
4377 email: michael<at>avcomm.com.au
DVS5c & DVS5s
High Performance
Video / S-Video
and Audio Splitters
MD12 Media Distribution Amplifier
QUEST
®
Quest AV®
VGA Splitter
VGS2
C O N T R O L S
HQ VGA
Cables
faster with the
world’s easiest controllers!
best v
alue!
AWP1
A-V Wallplate
Come to the
specialists...
You get results
Do you have wireless problems?
Telelink has wireless solutions!
If you want the right ‘wireless’ ingredients for a
successful project recipe, THINK Telelink! Don’t
want to be confused by wireless gobbledegook
and confusing buzz words? TALK to Telelink!
We will give you honest advice so that you
can make the right purchase decision for
your OEM low power wireless requirements.
Browse our website for more information about
our products. If you have any questions speak
with a Telelink Communications representative.
At Telelink we sell solutions, not problems!
01010101
Telelink Communications
www.telelink.com.au
e-mail Jack Chomley – jack<at>telelink.com.au
or call (07) 4934 0413 or 0428 199 551
®
Quest Electronics® Pty Limited abn 83 003 501 282 t/a Questronix
ELNEC IC PROGRAMMERS
Products, Specials & Pricelist at www.questronix.com.au
fax (02) 4341 2795
phone (02) 4343 1970
email: questav<at>questronix.com.au
MS120OEM216
$149 1-off
Developer’s Kit $193 includes programming cable & software
Made in Australia - enthusiastic users world-wide
www.dontronics.com has 300 selected
hardware and software products available from over 40 world wide manufacturers, and authors.
Olimex Development Boards & Tools:
ARM, AVR, MAXQ, MSP430 and PIC.
Atmel Programmers And Compilers:
STK500, Codevision C, Bascom AVR,
FED AVIDICY Pro, MikroElektronika Basic
and Pascal, Flash File support, and boot
loaders.
PICmicro Programmers And Compilers:
microEngineering Labs USB programmers, adapters, and Basic Compilers, DIY
(Kitsrus) USB programmers, MikroElektronika Basic, Pascal, DSpic Pascal Compilers,
CCS C, FED C, Hi-Tech C, MikroElektronika
C, disassembler and hex tools.
CAN: Lawicell CANUSB, CAN232
FTDI: USB Family of IC ‘s. FT232RL,
FT2452RL, also BL and others.
4DSystems LCD/Graphics: Add VGA
monitor, or OLED LCD to your micro. Simple Serial I/F.
Heaps And Heaps Of USB Products:
TTL, RS-232, RS-485, modules, cables,
analyzers, CRO’s.
Popular Easysync USB To RS-232
Cable: Works when the others fail. Only
one recommended by CBUS. Money back
guarantee.
www.dontronics-shop.com
102 Silicon Chip
splat-sc.com
ISM
ISM Tx/Rx + 8051 Modules
eRF-PoB. 433, 868 or 915MHz
Programmable On Board Via RF
Use any 8051 Assembler/Compiler
Nordic Semiconductors nRF9E5
8051 Processor: 32K Eeprom:
8 I/O:SPI:RS232:16MHz XTL etc.
Mini RF Programmer Development Platform
1 off Module
Price $59.00
Plus GST
High quality
Realistic prices
Free software updates
Large range of adaptors
Windows 95/98/Me/NT/2k/XP
CLEVERSCOPE
USB OSCILLOSCOPES
2 x 100MSa/s 10bit inputs + trigger
100MHz bandwidth
8 x digital inputs
4M samples/input
Sig-gen + spectrum analyser
Windows 98/Me/NT/2k/XP
IMAGECRAFT C COMPILERS
ANSI C compilers, Windows IDE
AVR, TMS430, ARM7/ARM9
68HC08, 68HC11, 68HC12
GRANTRONICS PTY LTD
www.grantronics.com.au
ellert-technologies.com.au
Battery Packs & Chargers
Siomar Battery Engineering
www.batterybook.com
Phone (08) 9302 5444
siliconchip.com.au
Do You Eat, Breathe and Sleep TECHNOLOGY?
Advertising Index
Opportunities for full-time and part-time positions all over Australia & New Zealand
Jaycar Electronics is a rapidly growing, Australian
owned, international retailer with more than 39 stores in
Australia and New Zealand. Our aggressive expansion
programme has resulted in the need for dedicated
individuals to join our team to assist us in achieving our
goals.
We pride ourselves on the technical knowledge of our
staff. Do you think that the following statements describe
you? Please put a tick in the boxes that do:
Knowledge of electronics, particularly at component level.
Assemble projects or kits yourself for car, computer, audio, etc.
Have empathy with others who have the same interest as you.
May have worked in some retail already (not obligatory).
Have energy, enthusiasm and a personality that enjoys
helping people.
Appreciates an opportunity for future advancement.
Have an eye for detail.
Why not do something you love and get paid for it? Please
write or email us with your details, along with your C.V.
and any qualifications you may have. We pay a
competitive salary, sales commissions and have great
benefits like a liberal staff purchase policy.
Send to:
Retail Operations Manager - Jaycar Electronics Pty Ltd
P.O. Box 6424 Silverwater NSW 1811
Email: jobs<at>jaycar.com.au
Jaycar Electronics is an equal opportunity employer and
actively promotes staff from within the organisation.
RFMA RF Modules Australia
Low Power Wireless Connectivity Specialists
Applications: Parani-SD100
Laptop/PDA
Bluetooth Serial Adapter
OEM Bluetooth Module
comms,
control In Stock NOW!
In Stock NOW!
AT Interface & measurement. Range 100m to 1Km
Rural
No drivers
Power: +18dBm
Class 1
Industrial
Range of upto 1Km
Data rate: upto 115200bps
Bluetooth Spec: V2.0+EDR
Commercial
SENA: OEM Bluetooth Modules and Serial Adapters
Parani-ESD1000
RF Modules Australia. P.O. Box 1957 Launceston, TAS., 7250.
Ph: 03-6331-6789. Email: sales<at>rfmodules.com.au. Web: rfmodules.com.au
HIGH QUALITY VALVE/TUBE KITS
MUDLARK
VALVE AMP KITS
THE A205
a u d i o
NX-14 RETRO NIXIE CLOCK
s y s t e m s
IMPROVED VERSION
EVEN BETTER SOUND
& LOOKS
SC July-Aug
2007
Kit: $899.00
Built: $1299.00
New Models
The A2.1 Series Stereo Valve + Subwoofer Amp
The best of SE triode sound with a built-in powerful
bass subwoofer amp. Total 60W power!
3 KIT VERSIONS FROM $399.00
With genuine NOS valves. Ask for the A2.1 brochure.
LIMITED
PRODUCTION
These amazing clocks are loved by technical and
non-technical people alike. Features retro vintage
Nixie tubes & crystal control for accurate time.
FULL KIT: $259.00 with transparent housing & blue
LED uplighting. LESS HOUSING: $199.00
GLESS AUDIO: 7 Lyonsville Ave, Preston 3072.
SPK360Email:
3/5/06
1:10 PM Page 1
Phone: (03) 9442 3991 Mob: 0403 055 374
glesstron<at>msn.com
The long-time supplier of PC boards to
enthusiasts is finally calling it a day and
needs to make arrangements to keep this
valued service to readers in operation.
The prospective buyer will need to be
an enthusiast and also happen to have a
large shed, 3-phase electricity supply and
broadband internet. For more info on plant,
SAV etc, contact Bob Barnes at sales<at>
rcsradio.com.au
siliconchip.com.au
20 years experience!
HI-FISPEAKER REPAIRS
YOUR EXPERT SPEAKER REPAIR SPECIALISTS
Specialising in UK, US and Danish brands.
Speakerbits are your vintage, rare and collectable speaker
repair experts. Foam surrounds, voice coils, complete
recone kits and more. Original OEM parts for Scan-Speak,
Dynaudio, Tannoy, JBL, ElectroVoice and others!
tel: 03 9647 7000 www.speakerbits.com
PC Boards
SPK360
RCS Radio Pty Ltd is
FOR SALE
Agilent Technologies......................... 3
Altronics..................................... 74-77
Aztronics........................................... 6
Av-Comm...................................... 102
CJ Appliance................................. 101
Computronics................................ 102
Dick Smith Electronics............... 22-23
Dontronics..................................... 102
Ecowatch...................................... 101
Ellert Technologies........................ 102
Emona Instruments........................... 7
Force Electronics.............................. 6
Front Panel Express.......................... 7
Furzy Electronics.............................. 4
Futurlec........................................... 10
Gless Audio................................... 103
Grantronics................................... 102
Harbuch Electronics........................ 96
Instant PCBs................................. 101
Jaycar............................IFC,49-56,103
JED Microprocessors........................ 5
Keith Rippon................................. 101
LED Sales..................................... 101
Microbyte Electronics.................... 101
Ocean Controls................................. 8
Ozitronics........................................ 99
Quest Electronics.......................... 102
RCS Radio.................................... 101
RF Modules...........................103,OBC
Sesame Electronics...................... 101
Silicon Chip Binders........................ 57
Silicon Chip Bookshop..... 31,93,94-95
SC Perf. Electronics For Cars......... 60
Silicon Chip Subscriptions.............. 17
Siomar Battery Industries............. 102
SOS Components........................... 47
Soundlabs Group............................ 10
Speakerbits................................... 103
Splat Controls............................... 102
Tech Repairs................................. 101
Tekmark Australia.................. 104,IBC
Telelink.......................................... 102
Tenrod Pty Ltd................................. 11
Truscotts Electronic World............. 101
Wagner Electronics...................... 9,45
Worldwide Elect. Components...... 101
Printed circuit boards for SILICON CHIP
designs can be obtained from RCS
Radio Pty Ltd. Phone (02) 9738 0330.
Fax (02) 9738 0334.
August 2008 103
siliconchip.com.au
104 Silicon Chip
siliconchip.com.au
August 2008 105
|