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Items relevant to "Reader/Programmer For Smart Cards":
Items relevant to "The SC480 50W RMS Amplifier Module":
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www.siliconchip.com.au
January 2003 1
Contents
Vol.16, No.1; January 2003
www.siliconchip.com.au
FEATURES
7 Receiving TV From International Satellites; Pt.2
How to install your own C-band (free-to-air) system and aim the dish – by
Garry Cratt
82 Chips Monitor Tyre Pressure
Two-chip remote sensing module from Motorola fits inside the tyre to monitor
inflation pressure – by Peter Holtham
PROJECTS TO BUILD
Reader/Programmer For Smart Cards
– Page 16.
16 Reader/Programmer For Smart Cards
Low-cost Phoenix-type reader/programmer lets you program your own Smart
Cards for all kinds of applications – by David Freeman
26 The SC480 50W RMS Amplifier Module
At last! – an amplifier module to replace the venerable ETI-480. It has less
distortion, is much quieter, has inbuilt protection and sounds a lot better – by
Peter Smith & Leo Simpson
34 A “Tiptronic-Style” Gear Indicator
It’s easy to build and indicates the selected gear in both manual and automatic cars on a digital readout – by John Clarke
58 Active 3-Way Crossover For Loudspeaker Systems
Get the very best from your 3-way loudspeaker system with this easy-to-build
high-performance design – by Mick Gergos
SPECIAL COLUMNS
53 Serviceman’s Log
SC480 50W RMS Power Amplifier
Module – Page 26.
When the going gets tough – by the TV Serviceman
71 Circuit Notebook
(1) DC Motor Speed Control With Protection; (2) Magic Wand For 3-Way
Control; (3) Automatic Tape Control For Display Stand; (4) Filter Reduces
Supply Ripple By 40dB.
84 Vintage Radio
Intermediate Frequency (IF) Amplifiers; Pt.2 – by Rodney Champness
COMPUTERS
74 Using Linux To Share An Optus Cable Modem; Pt.3
Masquerading modules and a firewall – by John Bagster
DEPARTMENTS
2
4
81
89
Publisher’s Letter
Mailbag
Silicon Chip Weblink
Ask Silicon Chip
92 Notes & Errata
93 Market Centre
95 Advertising Index
Apology: unfortunately, due to problems debugging the Windows software for
the EPROM Programmer, we have had to hold this project over this month.
www.siliconchip.com.au
“Tiptronic-Style” Gear Indicator
For Cars – Page 34.
Active 3-Way Crossover For
Loudspeaker Systems – Page 58.
January 2003 1
PUBLISHER’S LETTER
www.siliconchip.com.au
Publisher & Editor-in-Chief
Leo Simpson, B.Bus., FAICD
Production Manager
Greg Swain, B.Sc.(Hons.)
Technical Staff
John Clarke, B.E.(Elec.)
Peter Smith
Ross Tester
Jim Rowe, B.A., B.Sc, VK2ZLO
Rick Walters
Reader Services
Ann Jenkinson
Advertising Enquiries
Leo Simpson
Phone (02) 9979 5644
Fax (02) 9979 6503
Regular Contributors
Brendan Akhurst
Rodney Champness, VK3UG
Julian Edgar, Dip.T.(Sec.), B.Ed
Mike Sheriff, B.Sc, VK2YFK
Philip Watson, MIREE, VK2ZPW
Bob Young
SILICON CHIP is published 12 times
a year by Silicon Chip Publications
Pty Ltd. ACN 003 205 490. ABN 49
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©. No part of this publication may
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2 Silicon Chip
Queensland TV repairs now
need an electrical licence
Yep, the Queensland Government, via its union-dominated Electrical Safety Office, has been at
it again. With its new Electrical Safety Act, commencing on October 1st, 2002, any business doing
repairs on electronic or electrical appliances now
needs an electrical contractor’s licence. Previously,
this requirement only applied to those doing electrical installation work but now, after the farcical
electrical safety review at the beginning of 2002,
the vise is tightening.
So if you are in a business in Queensland doing
any sort of electronic or electrical appliance repairs,
you now need an electrical contractor’s licence. The fact that you are more highly
skilled than any electrician cuts no ice – you now need an electrical contractor’s
licence; end of story. This is supposedly all in the interest of reducing death from
contact with electricity but as anyone who knows the true situation can attest,
most people who die in Queensland from electrocution are either electricians or
trades people working on construction sites.
No doubt there will be plenty of people who will bleat about this new licence
requirement but we gave heaps of warning about this nonsense when we had
our long and ultimately futile campaign about do-it-yourself electrical wiring. I
cannot believe that the affected various trade organisations, engineers and businesses have allowed this legislation to be enacted. They have been utterly supine.
Well, the reward for apathy is more government regulation and since there are
Labor governments in every Australian state, this nonsense will probably spread
throughout the country.
The requirement for businesses to have an electrical contractor’s licence takes
effect from 1st February 2003. Furthermore, “If an applicant cannot complete the
necessary competency for the business component (public service speak for shutting you out), an application will be accepted so long as the applicant provides a
certificate of attainment within six months of obtaining their licence and before
1st August 2003”. If you want to read more of this mindless bureaucratic drivel,
go to the website www.eso.qld.gov.au
The net result of this stupidity will not be an improvement in the death rate
from electrocution in Queensland. But as always happens when government
becomes intrusive, there will be lots of unintended consequences and ordinary
people will be worse off. Many small electrical and electronic repair businesses
in Queensland will close. There is not a shadow of doubt about this. These small
businesses already have enough burdens without having to try and satisfy this
unnecessary regulation. Many who have been soldiering on for years will now
close up and take retirement. Can you blame them?
Even larger repair businesses that do warranty work on new appliances will
look askance at this new requirement. I would not be surprised if some of these
decide to give up as well.
So not only will Queenslanders not be able to get their TV, PC, fax machine or
other electronic gear fixed, they won’t get their washing machine, dryer, stove,
vacuum cleaner or other appliances fixed either. Good result, eh? Far more repairable appliances will end up on the tip. And how much hardship will be caused
to those who can ill-afford to buy replacement appliances. Of course, those few
Queenslanders who do manage to find a repairer in the future will sleep much
more soundly because their appliance was fixed by a “licenced electrical contractor”. Won’t that be nice?
Is there any hope? Well, we do still live in a democracy (sort of). If the affected
business organisations get off their behinds and really lobby the government, this
nonsense could be overturned. But I’m not hopeful. Happy New Year.
Leo Simpson
www.siliconchip.com.au
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MAILBAG
Internet Sharing with Linux and
WiFi security
After all these years, you guys still
are the best! Seriously though, I loved
the article about WiFi in the November
2002 issue and intend to try setting up
a test link P2P between my house and
my brother’s sometime soon. However, I am concerned that the writer
is understating the risks involved
in running wireless with standard
security. It is widely accepted within
the IT industry now that 802.11b and
WEP offer little practical security for
the modern business.
So serious is the issue that companies like Cisco systems are now selling
their wireless products with “temporary” additional security measures to
enhance the defaults until a suitable
new standard is finally settled upon.
I feel that security issues need a better
airing, perhaps in a future issue of
SILICON CHIP.
I also loved the article in November
2002 about using a Linux box for sharing a cable modem. This is something
I haven’t tried yet. I thought, however,
that you may want to have a look at
a ready built Linux based firewall/
sharing software kit. I have been
playing with and actively promoting
(to anyone who will listen) the IPcop
firewall project for the last six months
or so. IPcop is a spinoff of the early
GPL code used in the now commercial
Smoothwall firewall.
The IPcop team have made significant changes to the original code over
recent months and are now close to
releasing their second revision (0.1.2).
What makes these firewalls stand
out is that the system installs via a
self-booting CD (supplied as an ISO
image), formatting and setting up any
suitably fitted old PC as the gateway
machine. The build asks a few simple
questions to establish its interfaces for
the trusted network, DMZ and Internet, etc, and then after the first reboot
is fully managed via a Web browser on
the internal network. No more editing
lots of config files!
IPcop is free software as for most
Linux distributions and the development team are friendly and engaging to
4 Silicon Chip
all the folk who use the system.
I have had one running for six
months or so now and have set up a
few for friends who use ADSL. The
firewall is easy to manage, reliable and
even lends itself to modifications and
tweaks via the SSH remote access for
adding extra features.
Have a look at www.ipcop.org for
more information.
Ray Ellison,
Adelaide, SA.
Comment: We agree that wireless security (or lack of it) is a big issue.
Thanks for the Linux articles
A big thank you for the articles on
Linux. I would like to see more, especially for those of us who use ADSL.
I have tried to use Linux for some
time now but get so frustrated because
no one has easy to read help (in plain
Eng
lish) until you started to print
some. I have been an avid reader of
SILICON CHIP for years and sweat on
the copy to arrive each month in the
post. Keep up the good and informative work.
Robert Carnes,
via email.
Subwoofer saga with
an ETI-480 amplifier
I have been meaning to write for
some time and congratulate you on
an excellent magazine. I have an extensive library of every EA since 1965,
every ETI and almost every SC (just
missed a few of the early ones).
I find that SC projects are of the
highest standard and this was brought
home recently when I decided to
build a self-powered subwoofer for
a recently purchased DVD player. I
obtained a suitable speaker and made
a substantial box based on its Thiele &
Small parameters and various designs
published on the Internet.
I just happened to have a half-finished ETI480 amp and power supply
lying around so thought this would
be suitable. I finished off the amp and
installed it along with a kit sub-bass
processor purchased from Dick Smith
Electronics, based on the design in EA
September 1999. When finished, I ini-
tially connected the new subwoofer to
my existing stereo and was amazed at
how bad it sounded on some program
material.
To cut a long story short, I made literally dozens of changes to the internal
bracing of the box, the power supply,
the sub-bass processor and finally, the
ETI-480 itself and although I improved
the sound somewhat there was still
distortion and instability on certain
low-level tracks.
I had almost given up and decided
to buy a commercial unit when I read
your article on the problems school
students were having with the ETI480. I knew as soon as I read it that the
power amplifier was the problem so I
raced down to my local Dick Smith
store again and bought the last SC
50W amplifier module (based on the
LM3876 and published in February
1994) and a power supply they had
in stock. The subwoofer now sounds
first class.
Tony Lohrey,
via email.
Cat.5 tester is a beaut
My thanks to Craig Stephen. His
simple Cat.5 network tester on page
72 of the November 2002 Circuit Notebook is a beaut. I have wanted to build
something like that for ages since I got
a crimper and started making Cat.5
cables. It’s a pain testing them with a
multimeter. I found that the stop/step
was really start/step, but whatever!
It cost about $15 for the parts; mostly
$10 for a bag of 50 LEDs. I got a couple
of microswitches out of a dead mouse
and used an old token ring network
cable converter for the remote assembly. I know you can buy the whole
thing brand new from DSE ($90 on
www.siliconchip.com.au
special for November) but half the fun
is building it out of old bits.
Ray Haverfield,
via email.
CD deterioration
due to foam packing
I wonder if other readers have experienced the same problem of major
deterioration of music CDs that I have
had?
I am aware of the literature on CD
“bronze” corrosion, after being guided to the appropriate website http://
personal.riverusers.com/~manderso/
uhjdisc/bronzing.htm However, my
problem does not appear to be a bronzing of the disc. Rather it is “decay”
of the silver (aluminium) reflective
surface.
It happened on Disc 1 of a 2-CD set of
the opera “La Boheme”, from EMI. The
last two tracks on the disc would not
read and when I examined the disc, I
found two holes in the reflective layer,
about 2-3mm in diameter on the outer
edge of the disc.
I also noticed that the label surface
of the disc felt sticky and gritty, and
realised that the foam plastic sheet
often put in CD sets to hold the disc
in place had rotted and bits of it had
stuck to the label surface.
When I took Disc 2 out of its case,
I found the foam plastic sheet stuck
hard to the label side. I managed
to remove it but the surface is still
sticky and gritty, and when I hold this
Disc up to the light, it appears to be
peppered with thousands of tiny pin
holes, which seem to correspond to
the places where the foam plastic had
stuck to the surface. Disc 2 plays but
with jumps.
I now relate this to similar reflective
layer breakdowns in two other single CDs which I also found with the
foam plastic liner stuck to their label
surface. I am dreading going through
my entire collection of a couple of
thousand CDs, wondering how many
more might have been affected.
My CDs are stored in special shelves
in a cool, dry room, with no direct
sunlight and I believe my storage
arrangements meet the general recommendation.
Since the literature on CD corrosion,
dealing largely with discs pressed in
Europe by Philips and Du Pont from
www.siliconchip.com.au
1998 to 1993, says the corrosion was
caused by inappropriate inks and gels
which attacked the disc itself, I am
wondering if the rotting of the foam
plastic could have released chemicals or corrosives which attached
themselves to the disc surface and
damaged it?
Incidentally, the La Boheme was
a remaster from 1986 (out
side the
generally accepted time frame of
faulty pressings) and was mastered by
Nimbus. It does not have the “PDO”
legend, around the centre-hole, which
identifies the Philips-Du Pont press
ings.
Not being a chemist, I don’t know
what reactions might occur between
the foam and the surface of the disc
but I imagine a breakdown of the
foam is probably a chemical action
and could well cause some kind of
reaction. I am told the damage is
irreparable.
In any event, I feel some exposure
should be given to the fact that not
all CDs are born equal and that, especially in the case of particular press
ings from a specific time and place,
deterioration is likely. People who
have large collections might be wise
to check discs which still have foam
packed with them, and also to inform
themselves of the bronze corrosion
phenomenon.
We have been led to believe that
CDs last for anything up to 100 or 200
years and are virtually indestructible.
It appears, to the contrary, that they
might be very mortal.
Knowing your propensity for taking up thorny issues, I can think of
no better vehicle than your excellent
magazine for informing people about
this danger.
John Tingle MLC,
Parliament House, Sydney.
Comment: most plastic foams will be
corrosive when they perish and break
down, so the label is at risk. Most
plastic foams will not last beyond 1015 years in Australia – the heat does
it. Even a slight scratch on the label
can cause serious tracking problems.
Our recommendation is to go through
all your discs and root out any plastic
foam packing. Nothing should be in
contact with the label surface or the
underside.
Apart from that, there could be a
The Tiger
comes to
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The BASIC, Tiny and Economy
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Intelligent RS232 to RS485
Converter
The JED 995X is
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Several models available, inc. a new DIN rail
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$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
January 2003 5
Mailbag: continued
wider consumer issue here, with record
companies being obliged to replace
faulty discs.
Amateur radio articles
still wanted
I am just catching up with the last
couple of issues of SILICON CHIP and
would like to support G. J. Wilson of
Tasmania, for his letter in Mailbag
in the October 2002 issue. This is a
wonderful opportunity you have at
the moment to enrich your magazine
with amateur radio articles.
Indeed since the demise of “Electronics Australia” and other radio magazines, all “radio-interested” people,
including me, are left in limbo. Your
magazine will definitely increase its
readership by a fair bit if you were to
grab this chance and present a much
richer magazine with a much better
variety of articles.
In the last few years, I stopped
buying every issue of your magazine
simply because it is getting more and
more into computers.
In the recent AGM of the Australian
Radio DX club, the general consensus
was that everybody would buy your
magazine if they found a few articles
on amateur radio. And this club does
have about 300 financial members.
I do hope my mild criticism will be
very constructive,
Peter Theodorakis,
via email.
Comment: if you looked at SILICON
CHIP over the last 10 years or more,
you would not find any increased emphasis on computers – we’ve always
covered them.
Publisher’s letters endorsed
I have subscribed to SILICON CHIP
since a trip to Oz in 1992. I also
subscribe to “Everyday Practical
Electronics” here in the UK. I completely disagree with your Mailbag
subscriber Doug Thwaites and many
of his comments in December’s issue
– particularly in reference to the Publisher’s Letter.
I anxiously await the arrival of SILICON CHIP each month by airmail and
it is read religiously in the following
order:
6 Silicon Chip
(1). Publisher’s letter.
(2). Mailbag.
(3). Ask Silicon Chip.
(4). Serviceman’s Log.
(5). Jaycar and Dick Smith’s adverts,
mainly to compare them with things
here in the UK.
(6). The rest – word by word!!
I am usually most disappointed if
Leo Simpson writes solely on matters
electronic! To me, his asides reflect
the character of the man and I hope
he does not change things. You will
never please everyone but it’s a good
magazine pleasing 95% of its readers,
I am sure.
G Wilsher,
via email.
Easy labelling method
for cables
I’ve just solved a problem that had
been bugging me for some time. When
faced with the problem of labelling
18 audio and video cables linking
the various parts of my video editing
suite, I came to the conclusion that
the paper labels I had originally used
were not durable enough. So I sought
something better.
Some time ago I had made a series
of transparencies for an overhead projector and I still had left a few sheets
of clear acetate film. So I composed
the requisite labels on my computer
and printed them on the acetate sheet.
I then backed the clear labels with
plain white adhesive tape, punched
the necessary mounting holes and
cut out each of the 36 labels, one for
each end of the cables. They look
quite professional and I expect that
they will greatly outlast the previous
labels.
The labels are best if slipped onto
the wires before the plugs are attached
but where this was not feasible, I cut
into the side of the holes, slipped the
label over the wire and closed the gap
with a piece of adhesive tape.
By the way, this method is unsatisfactory if acetate sheet is used with
an inkjet printer. The ink takes a long
time (30mins) to dry on the acetate
sheet and afterwards tends to crack
and flake off.
The alternative is to print the la-
bels on paper with the inkjet printer.
Then copy them onto acetate sheet in
a photocopying machine. After that,
the procedure is exactly as described
above.
Jim Lawler,
Hobart, Tas.
Double fuses
for extra safety
May I revisit the issue of fuses in a
circuit? Should it be on the positive
supply or negative earth? The air force
teaches its technicians to disconnect a
battery’s earth before the power lead.
Consider for a moment, that while
disconnecting a power lead with earth
still attached, your spanner touches
the earthed chassis or frame. The little
blue spark can have rather nasty consequences in certain circumstances.
Power inverters or circuits dealing
in larger currents are normally fused
in the positive supply in contrast to
the above principle. In my experience,
failure of this sort of equipment often
leaves the fuse intact, with power
supply capacitors fuelling the fire, so
to speak.
My point is that a fuse rated to
protect a power circuit provides no
protection whatsoever for control
circuitry that needs protection of a
different order altogether.
This leads me to believe that a good
practice is to provide a fuse on the
earth side of a logic or control circuit
of a power supply to allow the circuit’s
potential to float; ie, to reduce the potential difference between power and
control circuits.
Two fuses allows protection of circuitry used to control power supplies,
inverters, voltage cut-outs and so on.
The large fuse would relate to the
maximum current in the power circuit,
which offers no protection for the
control circuit, while the small fuse
would be rated at 1.5 times the design
current for the control circuitry.
A blown small fuse would allow
the control circuit to protect itself by
letting its potential float; ie, to minimise the potential difference between
power and control circuits.
The resistance of the small fuse
would result in negligible shift in
voltage values.
Stephen Butcher,
SC
Masterton, NZ.
www.siliconchip.com.au
International
satellite TV
part 2. . .
by Garry Cratt*
Last month we discussed the basic principles of satellite TV
reception, equipment required and the type of free-to-air
programming that is available. This month we explain, in
detail, how to install your own C-band (free-to-air) system.
T
he most important aspect of installation is dish
placement. Obviously the dish must be able to point
in the right direction to receive a satellite signal.
With satellite dishes, “near enough” is most definitely not
“good enough.” An error or 1°– or even less – can make all
the difference on Earth (or off it!).
The “view” to the satellite must be clear of all obstructions. Generally this means locating the dish away from
trees, fences and buildings that might obstruct the line of
sight to the satellite. As we mentioned last month, a dry
tree usually makes only a marginal difference to satellite
reception. The smallest rain shower, though . . .
In order to find the best location, a decision has to be
made as to which satellite(s) are to be received. The pointing co-ordinates for the desired satellite can be determined
mathematically. These days, computer software makes this
task relatively simple. We’ll look at software shortly.
Azimuth and elevation
The dish pointing co-ordinates will comprise two parts:
an azimuth bearing, or the direction the dish must face
to point at the appropriate satellite (for Australia that’s
somewhere between 270° and 90°) and a value of dish
elevation, or the angle between the vertical and the axis of
the parabolic dish. At the equator, the dish points straight
up but the angle increases as you get further south.
Typical values for the most popular satellites and capital
cities are shown in Table 1. That’s all the information you
need to point your dish for a single satellite.
Many people, though, want to look at a range of satellites. As all geo-stationary satellites are located above the
equator and as the earth is round, the satellites aren’t in
a straight line across the sky; rather they follow what is
known as a geostationary arc.
To view more than one, a motor is attached to the dish,
designed to follow the curve of the arc. It is important to
locate the dish so that all wanted satellites are visible to
the dish at its extremeties of travel.
A motorised installation is a bit beyond the scope of
this article – that’s when you really do need professional
STEP-BY-STEP: Putting in your own C-band system
Open up the box of accessories
which is supplied along with
your dish box. You should find
a set of instructions (which will
vary from gibberish to excellent, depending on the brand
of your dish – and even then
not always constant), a plastic
bag of nuts and bolts and a
mounting plates.
Along with the four dish panels (petals), you should get four
feedhorn struts (inside the long box) and an LNB cover.
www.siliconchip.com.au
January 2003 7
help. So we will concentrate on viewing the signals from
just one satellite.
Councils and neighbours
Most local councils now require a development application to be submitted for the installation of any satellite dish
over 1m in diameter (some councils even smaller) and it
is wise to check your local council’s policy. It’s also good
policy to install the dish where it will have the smallest
impact on the neighbours.
While it might be possible to install the dish in a location not visible to the neighbours (or council), it should
be remembered that councils can issue demolition orders
for illegally erected satellite dishes (especially big ones!).
One other point about neighbours: it’s amazing how paranoid some can get about those nasty microwaves jumping
off your dish and curdling the milk in their fridge, causing
untold cancers and even rotting the wooden legs on their
tables and chairs.
Of course, none of your assurances that it is for receiving
only, that it doesn’t emit any microwaves, will satisfy them.
One bloke we know finally placated a whining, threatening neighbour by telling him he was actually doing the
whole neighbourhood a favour, collecting all the stray
microwaves from space in his dish and piping them away.
The overall result was less harmful microwaves in the
neighbourhood, not more. Yes, it is stupid. But most people
are when it comes to things they don’t understand. (And
yes, the neighbour swallowed it hook, line and sinker).
Site survey
Assuming a position can be found that is both unobtrusive and has a clear view of the sky, the next step should
be a site survey. Professional satellite companies always
perform a site survey to ensure that there is good access
to the satellite signals and just as importantly, that there is
no terrestrial interference to the desired satellite signals.
Unfortunately, C band (3.4-4.2GHz) is shared with terrestrial microwave services. Such services can be the source
of interference and in some cases, completely prevent the
reception of satellite signals.
The site survey is done using a small (1.2m) dish with
LNBF and a spectrum analyser. By pointing this small dish
using the correct azimuth and elevation values for the desired satellite, the satellite signal can be verified and any
interference can easily be seen.
Dig your post-mounting
hole deep enough to
accommodate half
the post length. For a
2.4m dish, that means
1.2m concreted into the
ground. Standard
mounting pipe is
galvanised 76mm (OD).
When you concrete in
the post, it is vital that it
be exactly vertical AND
it stays that way until the
concrete has well and
truly cured. We normally
use standard concrete,
not quick-set, because it
gives a stronger job.
8 Silicon Chip
The table at right
Pointing data for major Australian and S-E Pacific
capitals. The figure immediately after the city is its
magnetic deviation, while the figures underneath are its
exact location (usually the major airport). These are given
for those who wish to use dish pointing software. To use this
chart, select capital city, then satellite number from list below.
First data line is magnetic azimuth, second line is elevation.
The main satellites listed are prime signal sources. The
other satellites (listed underneath) have marginal footprints and may also be received on an itinerant basis.
N/A means that the particular satellite is below the
horizon for that city and is therefore unviewable.
Even though this size dish is too small to connect to a
digital satellite receiver for decoding, it allows the satellite signals – and any interference – to be viewed on the
spectrum analyser. Where a dish is not available, even
using a standard LNB to detect interference is better than
no check at all.
Where interference is detected, it can sometimes be
eliminated by using the building itself as a shield. Where
a satellite dish is to be installed in a location where there
is known interference (eg, near airport radar), the value of
using quad shielded coaxial cable can be appreciated. This
simple step (choosing quad shielded over the cheaper dual
shield) can mean the difference between perfect reception
and no reception.
In extreme cases, the coaxial cable can be run inside
steel water pipe for even greater immunity to an interfering
RF field.
Now we are not expecting you to own a spectrum analyser
but you may be able to find a local satellite TV company
who will do this for you, albeit at a price.
Digging the hole
The most common installation and perhaps the most
manageable is the backyard pole mount.
There is one logical rule that applies here: whatever
length of pipe that is above the ground should also be
below the ground.
This means that if you plan to install a 2.4m (diameter)
dish, you’ll need to leave a length of pipe at least half the
diameter of the dish (1.2m) protruding out of the ground
and another 1.2m buried in the ground. So it’s pretty easy
to remember – mounting pipe length equals dish diameter.
Butt up two dish panels and finger-tighten just the outermost and
innermost bolts with a flat washer under every bolt-head and nut.
www.siliconchip.com.au
www.siliconchip.com.au
JANUARY
anuary 2003 9
276
29.2
266.1
5.2
267.3
5.8
275.3
27.1
N/A
N/A
266.0
4.1
273
18.8
N/A
N/A
N/A
N/A
269.1
7.2
280.1
15.8
267.8
5.6
278.8
14.2
N/A
N/A
Azimuth
Elevation
Azimuth
Elevation
Azimuth
Elevation
Azimuth 273.6
Elevation
7.7
Sydney (12.6E)
Canberra (11.9E)
Adelaide (8.0E)
273.3
9.9
306.8
35.3
270.1
6.8
272.0
8.4
304.9
33.8
268.6
5.4
N/A
N/A
Azimuth 298.0
Elevation 27.4
N/A
N/A
Azimuth
Elevation
Perth (2.5W)
1.
2.
3.
4.
5.
Azimuth
Elevation
N/A
N/A
263.1
4.1
268.1
17.2
N/A
N/A
273.4
10.0
311.4
38.7
276.5
13.4
283.3
19.4
271.9
10.8
270.0
9.5
268.3
9.2
277.5
33.9
83.0
4
261.4
3.0
266.4
21.8
272.4
35.6
260.2
4.0
287.9
22.0
334.6
49.2
290.3
26.6
298.0
32.9
284.6
24.7
282.0
23.8
278.3
24.8
286.7
52.2
100.5
5
287.6
35.8
292.8
33.5
296.0
34.0
312.0
41.1
302.8
35.0
354.7
52.7
300.2
29.7
268.5
13.8
277.2
49.0
269.6
34.9
281.7
29.2
286.0
27.7
288.8
28.6
303.2
36.4
295.0
30.1
343.0
51.1
292.6
25.2
263.4
7.9
274.0
40.9
267.6
27.0
265.7
14.9
300.3
64.8
291.0
57.4
263.1
7.7
113.0
7
105.5
6
Satellite Number Index – with type and launch date
6. Asiasat 3, HS 601HP 1999 11. Optus B1 HS 601 1992
Panamsat 10, HS 601HP 2001
7. Palapa C2, HS 601 1996
12. Optus A3, HS 376 1987
Apstar 2R, FS 1300 1997
13. Panamsat 8, FS 1300 1998
Thaicom 3, Spacebus 3000A 1997 8. JCSat 3, HP 601 1995
9. Measat 2, HS 376HP 1996 14. Panamsat 2, HS 601 1994
Insat 2e, ISRO 1999
10. Optus B3, HS 601 1994
15. Intelsat 701, FS 1300 1993
Asiasat 2, GE 7000 1995
(18°S, 178°E)
Suva (12.7E)
N/A
N/A
N/A
N/A
(9°S, 156°E)
Honiara (9.2E)
(9.5°S, 147°E)
N/A
N/A
N/A
N/A
N/A
N/A
Azimuth 265.4
Elevation
2.8
Pt Moresby (6.6E)
(37°S, 175°E)
N/A
N/A
267.2
12.7
266.8
10.6
Azimuth
Elevation
Auckland (19.4E)
Azimuth
Elevation
N/A
N/A
N/A
N/A
N/A
N/A
Azimuth
Elevation
(43°S, 147°E)
Hobart (14.7E)
(32°S, 116°E)
(38°S, 145°E)
Melbourne (11.5E)
(35°S, 138.5°E)
(35°S, 149°E)
(34°S, 151°E)
(27.5°S, 153°E)
Brisbane (10E)
Azimuth
Elevation
Darwin (3.5E)
(12°S, 130.5°E)
78.5
3
76.5
2
68.5
1
Orbital Location (°E)
Satellite No.
272.0
29.7
275.6
51.1
289.0
65.1
280.1
25.4
318.1
36.8
024.2
50.5
321.9
42.8
333.8
47.9
313.8
43.3
309.9
43.4
303.5
47.7
344.0
75.1
128.0
8
294.6
56.7
327.0
77.8
036.9
74.7
311.1
42.8
358.0
39.7
059.9
33.1
006.1
44.7
020.6
45.4
359.4
48.4
356.0
50.2
355.3
57.7
62.1
57.4
156.0
10
300.7
60.0
349.7
78.8
047.7
71.3
316.9
44.4
003.6
38.8
063.4
29.9
012.1
43.5
026.3
43.5
006.0
47.4
003.0
49.4
003.7
57.0
65.6
53.2
160.0
11
308.0
63.1
012.8
77.9
055.0
67.4
323.1
45.7
009.1
37.7
066.7
26.7
017.8
41.9
031.6
41.3
012.3
46.0
009.6
48.2
011.6
55.6
068.4
49.1
164.0
12
312.3
64.4
022.4
76.9
057.7
65.3
326.2
46.2
011.7
37.0
068.2
25.0
020.5
41.0
034.1
40.1
015.3
45.2
012.8
47.5
015.4
54.8
69.6
47.0
166.0
13
319.5
66.1
034.0
74.8
061.2
62.2
331.1
46.7
015.6
35.8
070.4
22.5
024.5
39.5
037.6
38.2
019.2
43.9
017.4
46.2
020.6
53.3
71.3
43.8
169.0
14
LM-1, A2100AX 1999, 75 E
Gorizont 28, NPO 1993 96.5E
Apstar 1A, HS 376 1994 138E
Apstar 1, HS 376 1996 138E
Agila 2, FS 1300 1997 146
352.7
68.6
056.2
64.4
069.2
50.4
349.3
46.8
028.6
30.6
077.6
13.3
037.3
33.1
048.9
30.5
033.6
37.6
032
40.0
036.6
46.2
76.0
32.2
180.0
15
Gorizont 33, NPO 2000 145E
ntelsat 802, GE 7000 1997 174E
Intelsat 702, FS 1300 1994 176E
Other itinerant satellite source (craft, launch date & position)
285.5
49.4
298.3
71.9
358.8
78.8
300.6
38.8
346.3
40.5
051.9
39.2
353.3
46.1
008.0
16.1
345.6
49.0
341.7
50.4
338.1
57.4
051.9
65.2
148.0
9
Table 1: Dish Pointing Guide for Capital Cities
In practice its best
to add 100mm or so
out of the ground, so
that even if the dish
is tilted down for
maintenance (rarely
required), the lower
rim of the dish cannot quite touch the
ground, avoiding any
possibility of damage.
For mounting most
2.4m dishes, 76mm
OD (outside diameter)
This magnetic mount Anglemeter
pipe, available from
has 0.1° accuracy and a large dial
larger hardware and
face, allowing dish elevation to be
plumbing stores, is
read directly.
used. For a few dollars
more the store will even cut the pipe. In fact, it’s quite likely
that you will be buying an offcut length anyway, as pipe
tends to come in 6m lengths.
Dig a hole at least 300 x 300mm, 1.2m deep and stand
the pipe vertically in the centre. To keep the pipe vertical,
wedge bricks, rocks, etc between the pipe and the wall of
the hole, and check that the pipe is perfectly vertical by
using a spirit level.
Check the alignment at two positions 90° apart around the
circumference of the pipe. In some circumstances it will be
necessary to brace the pipe with two “starposts” or similar.
A 300 x 300 x 1200mm hole is a little over 0.1m3. You can
either use ready-mixed concrete or mix it yourself. For the
latter, you will need four bags of standard concrete mix. (If
you wanted a really strong mount, a 440 x 450 x 1200mm
hole will take about 0.25m3 of concrete; 10 bags).
Pour the concrete into the hole until it reaches a level
50mm below the ground level. This allows enough room
for topsoil to allow grass to grow under the dish. Leave
the concrete to set for two days, ensuring that the pipe
remains untouched for that period (that includes making
sure the kids don’t come out and give the pole a jiggle to
see if it has set!).
You might be tempted to use rapid set concrete but for
maximum strength, ordinary concrete mix is used and
allowed to dry normally.
If you are digging the hole in an area comprised mainly
of backfill (ie, low density soil) it may be necessary to weld
a piece of flat bar across one side of the bottom end of the
pipe, to ensure the pipe remains bonded to the concrete.
A larger hole would also be more prudent.
Repeat for the second pair of panels. They will happily stand up like
this if there is no wind. But don’t risk it in ANY breeze!
Sit both halves on a milk crate or small garbage bin and bolt them
together. Now insert the missing bolts and tighten them all up.
10 Silicon Chip
Dish assembly
Once the pipe has been set in the ground, the dish can be
assembled. Most mesh dishes are supplied as four pre-assembled panels which must be bolted together to form the
parabolic reflector surface. Also supplied are four steel or
aluminium tubes called “feed struts”. These hold the feed
horn assembly at the focal point of the dish.
In addition, there is a dish mount. This is the mechanical
assembly that connects the reflector to the pipe. It is very
cleverly designed so that elevation, azimuth and declination can all be separately adjusted. This is necessary for
a motorised dish system, where a single motor makes the
dish track in an arc, not a straight line!!
All dishes come with some instructions. Depending
on the brand, they may be very comprehensive or almost
non-existent.
Here are some “generic” instructions based on our experience. Much of the assembly can be performed by one person
but several steps require at least two, if not three people.
The main thing to remember is that the performance of the
dish is dependent on the accuracy of the surface. So dents
and rips in the mesh, apart from not looking at all aesthetically pleasing, will cause a reduction in dish performance
and should be avoided at all costs. Even small dents can
cause significant degradation and sometimes mean the difference between a good picture and a noisy (or no) picture.
Take two of the dish panels (also known as quadrants)
and stand them on their edge. Provided there is no wind (!),
and the surface is flat (a concrete driveway is often useful)
the panels will stand on their edge, the curve of the panel
preventing it from falling over.
Butt up the two panels and insert just the outermost and
innermost bolts. Use a flat washer under every bolt-head
and nut to prevent crushing the aluminium ribs of the dish
panels. Do the nuts up “finger tight”. Place this “half dish”
assembly to one side and make another half dish from the
two remaining mesh quadrants.
Once both halves of the reflector have been assembled,
lie them face down on a horizontal surface (perfectly flat
if available) with an inverted plastic garbage bin (or something similar) supporting the centre of the dish while you
assemble it.
www.siliconchip.com.au
Then butt the two halves together and insert the outermost and innermost nuts and bolts. Do these up finger
tight. You should now have a reflector lying face down on
the ground.
Insert all bolts and nuts (don’t forget the flat washers),
working from the perimeter of the dish to the centre in a
clockwise direction, tightening them with two spanners as
you go. There are four mounting holes for the dish mount,
so leave them vacant. Don’t forget to tighten the nuts you
originally had only finger-tight.
Find an assistant, then carefully pick up the reflector and
turn it over so it is lying face up. Be very careful if there is
any wind: even a mesh dish can get away from you.
The feed struts
The next step is to bolt the feed struts onto the feedhorn.
Do this a short distance away from the reflector to eliminate
the possibility of accidentally piercing the reflector mesh.
The feed struts should be spaced 90° apart and are secured
to the feed ring using four bolts and nuts.
Using that same friendly assistant (or two of them if
available), pick up the feed assembly complete with struts,
and carefully position it over the reflector, making sure
that none of the struts damage the mesh.
Two people can hold up the feed assembly (each holds
the assembly by two struts), while the third person inserts a
bolt, washers and nut, at the location point on the reflector.
You should now have a reflector lying face up, with four
feed struts bolted to the rim, holding the feed ring at the
focal point of the dish. As soon as the feed assembly is
secured, there is a noticeable improvement in the rigidity
of the entire assembly, as it is secured in both axes.
The dish mount
The next step is to place the dish mount on the pipe
protruding from the ground.
As long as the pipe does not protrude more than about
1.5m, one person can generally lift the mount onto the
pipe. But it’s always better with two. That mount is heavy!
First a few precautions: Ensure that the securing bolts on
the outside of the mount sleeve (designed to clamp onto the
pipe) are loosened off so that the mount can slide onto the
pipe. Fix an azimuth bar (supplied with the dish) to lock the
east /west movement of the mount. This prevents the mount
rolling around the horizontal axis as you lift it onto the pipe.
Once the mount has been lifted onto the pipe, rotate it
Hopefully your completed dish looks something like this! Be even
more careful now you’ve got this far; from now on it’s a 2-man job!
www.siliconchip.com.au
such that it is in a position where the dish can be lifted
(by two people) onto the mount, then tighten up the mount
securing screws to hold it solid.
This is not the final position of the dish, merely a convenient position to finish the assembly. Adjust the mount
elevation to about 30°. This will enable you to lift the
reflector up against the mount, rather than lifting it above
the mount.
Up she goes!
We now need to lift the reflector (dish) onto the mount,
orienting it so that the four lugs on the mounting ring
correspond with the four double ribs formed by bolting
the quadrants together. We also need to consider the LNB
securing bolt on the feed horn. This needs to be facing
downwards (towards the ground), so it is easier to adjust
once the dish is mounted.
With the mount clamped to the pipe, the azimuth bar
in place, and using two or three people, carefully lift the
upturned reflector and feed assembly onto the mount,
positioning the four lugs on the mount and corresponding
double ribs.
While one person holds the reflector in place against
the mount, another person must insert the four securing
bolts. It’s necessary to operate from behind the dish to do
this, inserting the uppermost bolts first. Don’t forget the
flat washers under the bolt heads and nuts.
Once the two uppermost bolts have been inserted, the
reflector will sit on the mount without support, while the
remaining two bolts are inserted.
Now tighten all bolts, making sure the mesh is not damaged by the action of the spanner against the securing nuts.
The dish is now ready to have the LNB added and to be
pointed towards the satellite.
Pointing the dish
There are four critical parameters that must be determined for every dish installation. They are dish azimuth,
dish elevation, LNB orientation and dish focal point.
Fortunately, the focal point is almost always determined
by the length of the feedarms. When the feedhorn/LNB is set
in correct position, no further adjustment should be needed.
The azimuth and elevation of the dish need to be mathematically calculated. All satellites are given an orbital
location, which in the case of Asiasat 2 is 100.5° east longitude. This means that the satellite is located 37,000km
Connect the feed struts to the LNB hardware – do this away from the
dish so you don’t risk damaging the dish mesh.
January 2003 11
This satellite signal indicator comprises a broadband
amplifier and diode detector, intended to be used at the
dish to assist in signal peaking.
up, at the intersection of the equator and 100.5° east line
of longitude.
From a map you’ll see that this location is over Indonesia.
For Sydney, even the most rudimentary geography indicates
that the dish will be facing somewhere in the western sky.
Ummmm – west – that’s away from the coastline in Sydney.
Fortunately, there are plenty of computer programs available that simply require the latitude and longitude of the
dish, together with the longitude of the satellite.You can find
a variety of software on the net, some of it freebies.
One such program, GEOSAT.EXE, is one we use at
Avcomm Pty Ltd – in fact, we wrote it!
Alternatively, a quick “Google” will find any amount of
similar programs, such as SMW Link, from Swedish Microwave AB (www.smw.se/smwlink/smwlink.htm). Make sure
you get the latest version (3.05) because earlier versions
had a southern hemisphere calculation bug!
But it’s often even easier than that, because most modern
receivers have a dish pointing menu, where these parameters can be entered to calculate the desired azimuth and
elevation of the dish.
has at least one (and usually more) latitude and longitude
reference on the side.
Alternatively, if you have ’net access you can Google
something like “latitude longitude Gulargambone” – especially handy if you happen to live in Gulargambone.
You should find several websites which will give you the
exact (to the minute and sometimes even second) location
of your town/city, especially if it has an airport. Beware,
though, in big cities, the figures are likely to be that of the
main airport – and if you happen to live on the opposite side
of the city, you could be out by as much as a degree or so.
One further alternative is a very useful book called “The
Dick Smith GPS Guide”. Available from DSE stores or
Australian Geographic, this lists over 16,000 locations in
Australia and the corresponding latitude and longitude.
If using this book, its important to remember that most
dish pointing programs require latitude and longitude in
degrees and tenths of degrees (eg, 34.5) not in the format provide by the book: degrees, minutes, seconds (or 34°30’0”).
Fortunately the book does have a conversion chart – and
even mental calculations aren’t rocket science. (Rocket
science? Satellites? Get it . . . ? Oh, don’t bother . . .)
Azimuth
You probably don’t know the exact latitude and longitude of the dish site. To work out the exact (to the minute)
location, we normally use either a good map or GPS.
Detailed topographic maps of your area will enable you
to extrapolate your exact location because the grid always
One further parameter is required to calculate the dish
azimuth – remember, that’s the direction it points.
But there is a little wrinkle here called magnetic variation.
That’s the difference between what you read on a compass
as north, and true north (ie, lines of longitude from pole
to pole). Magnetic variation varies all over the place depending on the specific place you are at, while computer
software invariably works on true north – and you have
to add or subtract the local magnetic variation to achieve
the desired result.
Magnetic variation can usually be found for any particular location on a specific map called a “WAC” (World
Aeronautical Chart), often used by pilots. These charts are
available at all good map shops and pilot supply centres.
Magnetic variation is also listed on topo maps.
A point to note: as well as varying by location, magnetic
variation changes over time. The map may give a misleading
figure if it is more than a few years old. Once again, Google
is a great way to find out magnetic variation (which is,
by the way, also known as magnetic declination). Google
‘“magnetic variation” Sydney’ and you’ll find several sites
giving the result: 12.6° E.
Very carefully bolt the struts onto the dish using the mounting holes
provided. Place the dish assembly somewhere safe.
Here’s what the dish
mounting hardware looks
like straight out of the box
(albeit photographed here
almost upside down).
The cylindrical section with
the four bolts at right actually points vertically down
(it’s the bit which slips over
the top of the in-ground
76mm pipe “post”). Those
bolts are tightened against
the post to ensure the dish
cannot “windmill” in strong
winds. The ring (on the
ground in this pic) is the
part which bolts on to the
assembled dish.
Where am I?
12 Silicon Chip
www.siliconchip.com.au
Recalling the rhyme “east is least” reminds us to subtract
lines of magnetic variation marked “E” from the calculated
true azimuth. In the case of Sydney the magnetic variation
is 12.6° E, so we need to subtract 12.6° from the calculated
“true” azimuth. The magnetic variation for Perth is around
2.5° W, so we must add 2.5 to that “true” azimuth.
Elevation
The dish pointing software calculates elevation directly
in degrees. Fortunately, this is much easier to measure and
set. The simplest method is to use a protractor and a piece
of cotton and a weight but if this is too much trouble a
simple analog inclinometer can be purchased reasonably
cheaply. This type of instrument has an oil filled chamber
with a pivot and a counterweighted pointer.
A far more sophisticated digital instrument is used by
professional installers, as the dish geometry of a motorised
system must be set to within one tenth of one degree, or
six minutes.
The reality is that most home installers will be able to
set up a system to look at any single satellite but without
sophisticated measuring equipment, the alignment of a
motorised system will require professional help.
Where’s the satellite?
Now that we have been able to work out the dish azimuth
and elevation, we can get to work.
Let’s use the example of Sydney and the Asiasat 2 satellite. We know the latitude of Sydney is 34° south, and the
longitude is 151° east. We also know that the longitude of
Asiasat 2 is 100.5° east.
Our software tells us that the dish elevation must be
23.87°, and the true azimuth is 294.75°. Subtracting 12.6°
from the true azimuth gives 282° magnetic. This is the
required compass heading.
A cheap and nasty compass won’t cut the mustard here:
it needs to be a decent, fluid-filled model graduated in individual degrees. Good orienteering compasses are usually
a reasonable compromise between cost and usefulness.
Also remember when aiming a dish that the compass
itself is likely to be affected by close metal (usually steel)
objects. Just keep that in mind if your compass readings
keep changing as you move about.
The elevation is somewhat easier to set. Assuming the
mounting pipe has no elevation (just like a dish standing
on the rim), calibrate the inclinometer for zero degrees.
Up the right way: the threaded rod in the centre of the pic adjusts
the dish elevation, while the rod at right adjusts declination.
www.siliconchip.com.au
When you get really serious (!) this digital inclinometer
has one degree accuracy and resolution. It’s a must for
setting up motorised dishes.
Place the inclinometer on the centre plate of the dish (from
behind), so that the counterweight is vertical. The elevation
of the dish can be directly read.
Adjust the threaded rod until the elevation reaches 24°.
This should be close enough, once the dish is pointed in
the right direction, to acquire a signal.
One tip – before setting elevation, run the spirit level over
your pipe one last time to make sure it hasn’t moved before
the concrete had a chance to harden. It happens!
Installing the LNB
Now is the time to install the LNB into the feed rings. Do
this by slipping the LNB through the ring assembly, so that
the front edge of the waveguide protrudes 20mm past the
level of the concentric rings. Rotate the LNB so that the flat
part of the housing is vertical. This is a good starting point
for further adjustments once the system is operational.
This brings us to the next point: how do we measure
the signal?
Fortunately, there exists simple in-line signal strength
meters for this task. One popular (and economic) type is
called, logically enough, a “Satellite Finder”.
The meter has an input port that requires DC voltage
from the satellite receiver and an output port that feeds
that DC voltage to the LNB and reads the amount of signal
being sent from the LNB to the receiver.
Basically, it is a simple broadband amplifier and a rectifier driving an analog meter movement and a tone generator.
As the signal gets stronger (as we peak up the dish), the
meter deflection becomes greater and the tone gets louder.
The meter also has a sensitivity adjustment.
Now, having set the dish elevation, set the LNB orientation and calculated the magnetic azimuth of the dish,
rotate the entire reflector and mount assembly on the pole
The completed
mount. The solid
bar (arrowed at
left) locks the
dish azimuth (set
by rotating on the
pole). This bar
can be replaced
by a suitable
motor to enable
the dish to track
any number
of (viewable)
satellites. But
for single-bird
systems, this bar
is bolted in place
as shown here.
January 2003 13
until it points in the desired direction.
At this point, connect the LNB to the signal meter and
the signal meter to the receiver via short lengths of coaxial
cable. Because you are not trying to display a picture right
now, you don’t need any monitor so setup is most easily
done close to the dish with the receiver on a suitably long
power cord.
Adjust the meter sensitivity to maximum and turn the
receiver on. As the dish assembly is rotated on the pole, the
signal strength meter will begin to respond. As the meter
reaches full scale, back off the sensitivity while continuing
to move the dish, until the signal is peaked.
Carefully adjust the clamping screws on the dish mount
so that they are all tightened evenly, clamping the mount
to the pole without causing any skew in the vertical
plane. It may be necessary to optimise this adjustment
several times.
Once this has been done, the elevation adjustment should
be optimised for maximum signal, by slowly turning the
elevation rod. When this is peaked, lock it in place.
At this stage, select the desired channel on the satellite
(most receivers come pre-programmed) and carefully rotate
the LNB (with the meter still connected) until the signal is
peaked. This adjustment will only be in the order of 10-15°.
Making adjustments greater than this will mean the LNB
is peaking on signals of the opposite polarity, as most satellites have signals of both horizontal and vertical polarisation
(and sometimes on the same frequency). This adjustment
is called cross polarisation optimisation.
Connecting up your system.
Like most pieces of audio visual equipment, a digital satellite receiver has several different outputs for connection
to a TV set, VCR or hifi system.
For best results, especially where a recording facility
is desired, it is normal practice to connect the direct line
audio and composite video outputs from the satellite
receiver to the VCR and then use either the RF or (again
preferably) the A/V output of the VCR to connect to the
TV set.
Most satellite receivers have two or more A/V outputs,
allowing separate connections to a hifi system for enhanced
audio. However, many overseas stations broadcast in dual
mono and often in different languages. In some cases the
redundant audio channel is used to carry a separate radio
service.
Place the dish on the
mount. This is definitely a
two-man job (the missing
man in this picture was the
photographer!) The double
edges (joins between
the dish panels) slot into
the U-shaped brackets
on the mount. Place the
upper-most bolts and nuts
first. Some to-ing and
fro-ing of the dish panels
might be necessary to get
the bolts to go right through
the holes in the double-thickness joins. Make
sure all dish panel and
mounting bolts are tight.
14 Silicon Chip
For this reason, satellite receivers allow the user to
determine which output will be routed to the sockets on
the rear panel.
Assuming there is coaxial cable supplying TV wall outlets
in several rooms in the house, the RF output of the satellite
receiver can be combined with the existing internal TV
cabling to provide a “satellite” channel. While the limitation of this system is that only one channel is fed into the
system, it does mean that satellite TV can be enjoyed in
many rooms. Anyway, you can only watch one channel at
a time, no matter which room you are in!
Channel surfers (or those with the remote control permanently super-glued to their hands) need not apply!
If the ability to record is not required, best results are
obtained by running the line audio and composite video
outputs of the satellite receiver, directly in to a spare
A/V input on the TV set. This is an easy way to switch
from normal terrestrial TV to satellite TV.
Most modern TV sets are multi-system, meaning they
have the ability to convert an NTSC video signal into a PAL
signal. If you don’t have one of these, and the station you
want to watch broadcasts in the American (NTSC) video
format, you may need a video systems converter.
Countries using the NTSC format include USA, Canada, Mexico, Japan, Taiwan and Korea – in fact pretty well
anywhere where there has been a US influence in the
development of the country, use NTSC.
All other countries use PAL these days (even digital
signals from Russia use PAL!). PAL or Phase Alternating
Line, is of course the system used for analog TV transmission in Australia.
Analog converters start at $99, while fully fledged digital
converters (that allow recording on a PAL VCR) range from
$750 to $2000 for a top-of-the-line model (near broadcast
quality).
As a digital satellite system is capable of delivering very
high quality video, the appropriate quality cables should
be used. This means going to a reputable electronics outlet
to obtain them.
In the old analog days it might have been possible to
put up with the video performance of audio cables, such
as the inexpensive twin RCA-RCA types we have all seen.
However, to preserve the quality of the video performance from the satellite receiver, it is important to use
well-screened, moulded, three-conductor low capacitance
cables, which can normally be identified by the larger
There are four possible adjustments for maximum signal:
azimuth, elevation, declination
and LNB polarity/focal point.
These must be set as explained
in the text. In this shot, Erin is
setting the elevation – the angle
in the sky to which the dish
points. Turning the elevation rod
raises and lowers the top of the
dish with respect to the vertical
mounting pole. Azimuth is
adjusted even more easily – by
rotating the dish on the mounting
pole. The focal point is almost
always fixed. Don’t worry about
declination unless setting up a
motorised system.
www.siliconchip.com.au
A typical digital
satellite receiver
– in fact, this or
one very similar is the
one in the special offer at right.
diameter of the video cable. The effect of using inferior
cables will be colour smearing, ringing along the leading
edge of the video and generally poor definition.
Do I leave the receiver on?
Most satellite receivers have a standby function, putting
the receiver to sleep but allowing voltage up to the LNB.
This has the effect of keeping the LNB stable and at a constant temperature. For this reason, it is wise to leave the
receiver in the standby mode when it is not being used.
This also eliminates the possible ingress of moisture into
the receiver itself.
Like all electronic equipment, keep the receiver well
ventilated. This is particularly so when several pieces
are stacked together in a typical hi fi cabinet. Spacing
equipment apart with small blocks of wood can help in
this aspect.
Avoid the practise of some people (let’s not be sexist here)
of putting doilies on top of the receiver (or VCR or CD or
DVD or anything else for that matter) and putting a pot plant
or vase of flowers on top, “to make it look more attractive”.
Apart from the fact that this may well cover the ventilation
slots and cause overheating, there is always the danger of
the vase being knocked over and the internals taking an
unwanted and probably highly damaging shower.
For the same reason, empty video sleeves, CD/DVD/
cassette cases, etc, should never be placed on top of electronic equipment.
SC
EXCLUSIVE
SPECIAL OFFER FOR
S ILICON CHIP
READERS
Av-Comm Satellite Equipment has a very
special offer, exclusively for SILICON CHIP
readers: a complete, brand new, state-of-theart DIGITAL satellite receiving system ready
to put together, connect up and turn on!
Here’s what you get:
A 2.4m 4-panel mesh dish complete with all
mounting hardware (except the post!)
A dual polarity, low noise, block downconverter (LNB)
A high efficiency feedhorn
A Digital Satellite TV Receiver with remote
control, MPEG-2 and digital DVB compliant.
25m RG-6 (satellite grade) coaxial cable and
two “F” connectors
An analog inclinometer
A “SatFinder” in-line signal strength meter
Current Av-Comm catalog price for all this is
$1450.00 – but until February 28 2003, if you tell
Av-Comm you’re a SILICON CHIP reader, you can
have the complete package for just $1295.00 –
that’s better than 10% off. And remember, all this
equipment is brand new, with full warranty.
Order direct from Av-Comm (do not call SILICON
CHIP!) Phone Av-Comm on (02) 9939 4377, fax
9939 4378, email cgarry<at>avcomm.com.au or use
the special SILICON CHIP SYSTEM order form on
Av-Comm’s website (www.avcomm.com.au).
* Director, Av-Comm Pty Ltd
The LNB is a friction-fit into
the feed horn (at the junction
of the struts). After fitting
and connecting the coaxial
cable, you need to adjust the
LNB polarity for maximum
signal by rotating it in the
feed horn. You will probably
need to re-adjust elevation
and azimuth. To complete
the job, run the coax down
one of the struts and secure
it with black cable ties (white
ones will break down over
time due to UV). Make a loop
around the back of the dish
and cable-tie the coax to the
mounting post.
www.siliconchip.com.au
And now it’s finished. We’ve
left the LNB cover off for
clarity (quite often they are
left off anyway!). The coax is
connected to the LNB and
secured to the strut and post –
now it is just a matter of
connecting it to your satellite
receiver, tuning in the required
channel and watching your
satellite programs. After the
dish has settled in, it might
pay you to re-peak the azimuth,
elevation and LNB output as
previously detailed. But if you
have wall-to-wall signal, it’s
probably not worth the bother.
Enjoy!
January 2003 15
READER/
PROGRAMMER
FOR
SMART CARDS
Since blank smart cards are now available at attractive
prices, it’s quite feasible to program them with your own
software and data for all kinds of applications. Here’s a low
cost and easy to build ‘Phoenix type’ reader/programmer,
which can be used with most of the programming software
available on the Web to suit this type of serial-port device.
W
ith their embedded microcontroller and serial
EEPROM combination, today’s ‘smart cards’ have many more
uses than dumb cards which merely
have a magnetic stripe.
Smart cards are already used for
pay TV set-top box and mobile phone
authorisation but these applications
really only scratch the surface of their
potential.
You could use them to build your
own personalised security access system, for example, or to provide a ‘plugin brain and memory’ for small robots
and digitally controlled machines.
Or to provide plug-in schedules for
16 Silicon Chip
automatic control of a model railway,
or pointing data for a computer-positioned telescope, or whatever...
Using smart cards for your own
applications is now quite feasible because blank smart cards and matching
‘sockets’ are now available at quite
reasonable cost.
For example, Jaycar stores are
offering blank cards with an embedded PIC16F84A micro and 24LC16B
EEPROM for $19.95 (Cat ZZ-8800).
Jaycar can also supply suitable ‘sockets’ in both through-hole (PS-0012)
By David Freeman
and SMD (PS-0010) versions for only
$8.75 each.
By the way, the PIC16F84A micro-controller chip (made by Microchip Technology) is used in many
of the commonly used smart cards.
Although only an 8-bit processor it’s
quite powerful, with 1024 words of
program memory, 68 bytes of data
RAM and 64 bytes of data EEPROM.
It is even smarter when it’s teamed
up with the 24LC16B serial EEPROM
(which has a capacity of 16K bytes);
the combo is capable of a surprising
range of applications.
Other smart cards team up the PIC16F84A micro with a 24C64 EEPROM
www.siliconchip.com.au
which offers 64K bytes of memory.
They can, of course, because the for reading and programming. (Note
The Atmel AT90S8515 micro is also
cards are available over the coun- that the card’s EEPROM is read and
used in some smart cards. Usually it’s
ter as well as being used in pay TV programmed ‘through’ the micro, with
teamed up with either the 24C64 or
set-top boxes and mobile phones. its ‘cooperation’.)
24C128 (128K bytes) EEPROM.
So because the matching sockets
In this article, I’m describing a
Fig.1 shows what’s acsimple reading/programtually inside a common
ming interface which is
smart card, of the type
quite low in cost and
using the PIC18F84 with
easy to build. I can’t
a 24LC16. Because both
claim it involves any
chips use serial commugreat design innovation.
nication, all of the conIn fact, it’s very simnections to the ‘outside
ilar to quite a few deworld’ are made via only
signs that have been
five of the tiny array of
available on the Internet
eight gold-flashed conand like them, based on
tacts.
what seems to be called
Contact C1 is used to
the ‘Phoenix’ configusupply the chips with +5V,
ration.
C2 to reset the micro, C3
(I haven’t been able
to provide the micro with
to find out where that
clock signals (3.75MHz
name came from – perFig.1: here’s what is inside that innocuous-looking piece
or 6.0MHz), the large ‘L
haps the person who
of plastic. There’s a lot more to it than meets the eye!
shaped’ C5 for ground and
came up with the first
C7 for serial data input
design lived in Phoenix,
amd output.
Arizona!)
This kind of card makes a compact
are readily available as well, it has
The main advantage of using this
(86 x 54 x 0.8mm) and cost effective
become quite feasible to use them in kind of design is that it’s compatible
package containing such a useful
your own projects.
with a lot of the smartcard reading
micro and EEPROM. How they can
All you really need for this is a small and programming software available
fit those chips, bonding wires and hardware interface to connect the card for free downloading from many sites
contacts inside a card with a total
up to your PC, and suitable software to on the internet.
thickness of only 0.8mm is beyond me!
allow you to ‘talk’ to the card’s micro
By the way, SILICON CHIP will NOT
The smart card reader/programmer is
assembled on a single PC board. Basically, it
is just an interface between the card, which
slides into the slot at right, and the PC.
www.siliconchip.com.au
January 2003 17
Fig.2: the complete circuit. There’s not much to it – just a couple of crystal oscillators, an RS-232 chip and power supply.
be able to provide you with any software to go with the hardware, because
according to Australian federal law
this combination of hardware and
software is capable of being ‘used for
the purpose of defeating encryption
systems’, and is accordingly deemed
illegal.
Needless to say, we are certainly not
describing this project with the idea
that you would use it to defeat any
encryption systems. In fact we must
warn you that it should NOT be used
for this purpose, because doing so
would be illegal and make you liable
to be prosecuted.
All we can do with regard to helping
you find suitable software is list the
URLs for some of the web sites where
you may be able find some, and leave
the rest to you.
These are shown in the accomp-anying panel. Be warned again,
though: some of the software on these
and other sites MAY be designed
specifically for illegal smart card
applications.
So let the user beware!
Incidentally, we understand that
kits for this hardware interface will
be available from Jaycar Electronics.
So you shouldn’t have any problems
building up the interface itself or get18 Silicon Chip
ting blank smart cards for use with it.
Free-standing board
As you can see from the photo,
there’s very little in the project and
all of its components fit on a small
freestanding single-sided PC board.
The board measures only 89 x 76mm,
and is coded 07201031. It’s supported
on four small rubber feet and has the
smart card socket on the front, flanked
by two LEDs: one (green) to indicate
when the unit is powered up, the other
(red) to show when the PC is reading
from or writing to the card.
Here’s a selection of “blank” smart
cards showing different types of
contacts available. This reader/
programmer suits only the 8-contact
version, as shown on the left.
Along the back of the board are a
DB9F socket for a standard RS-232C
serial link cable to the PC serial port,
plus a 2.5mm concentric DC power
connector to accept the cable from a
9-12V plugpack power supply. Everything else is on the board itself.
Circuit description
The hardware of this project is
designed to perform just three main
functions: (a) to provide +5V DC to
the smart card plugged into its socket;
(b) to provide the card with a clock
signal of either 3.75MHz or 6.0MHz,
selectable via a jumper shunt; and (c)
to provide a serial communications
interface between it and the PC’s software, to allow reading and writing.
Referring to the circuit diagram,
power for the interface is derived from
a 9-12V DC plugpack, connected to
the unit via CON3. Series diode D1
prevents damage due to an accidental
reverse polarity connection, while
low power regulator REG1 provides
smoothed and regulated 5V DC for
both the smart card and the rest of the
interface circuitry. LED1 is the green
power indicator, which runs directly
from the unregulated input.
Clock signals for the smart card are
provided by the circuitry around IC2, a
www.siliconchip.com.au
Full-size view of the completed PC board. . .
low-cost 74HC00 quad gate. Two of its
gates (IC2c/d) are connected as crystal
oscillators, one for 3.75MHz using
crystal X1 and the other for 6.0MHz
using X2. Which oscillator runs at
any particular time is determined by
the position of the jumper shunt in
the 3-pin header LK1, because this
applies +5V to the second input of
either IC2c or IC2d.
Each oscillator only operates when
its second gate input is taken to +5V,
so the oscillator whose second input
is held low via the 10kΩ resistor is
disabled.
The outputs of the two oscillators
are fed into IC2a, used here as an OR
. . . along with the matching component overlay.
gate. Then the clock signals are passed
through IC2b, used as a buffer, before
being fed to the CLK pin of the smart
card socket (C3).
The rest of the circuitry forms the
interface between the smart card and
the serial port of the PC (via CON2).
The heart of the interface is IC1, a
standard MAX232 dual RS-232C serial bus transceiver. This chip is very
handy because it contains internal
‘charge pump’ circuitry which generates the correct RS-232C voltage levels
from a standard +5V supply rail, using
the four 1µF capacitors connected to
pins 1-6.
One of the two receivers of IC1
has its input (pin 8) connected to the
transmit data line from the PC (TxD,
pin 3). The output of this receiver (pin
9) is used to operate LED2, the Read/
Write indicator. The same output is
also used to pull down the Data I/O
pin on the smart card socket (C7) via
Schottky diode D2, to send data to the
card during write operations.
The smart card pin (Data I/O) is normally pulled high by a 10kΩ resistor
to +5V but can easily be pulled low by
pin 9 of IC1 because of the very low
voltage drop in D2.
When the smart card micro itself
pulls the Data I/O pin low during
a read operation, this is fed back to
Fore and aft close-up views of the business ends of the smart card reader/programmer, showing the RS232 and power
supply connections (left photo) and the smart card slot (right photo)
www.siliconchip.com.au
January 2003 19
Parts List – Smart Card Reader/Programmer
1
1
1
1
1
1
1
4
2
6
4
PC board, code 07201031, 89 x 76mm
3.57MHz crystal (X1)
6.00MHz crystal (X2)
3-pin SIL header strip with 2-way jumper shunt (J1)
ICA-700 DIP smart card socket (CON1)
DB9F connector, 90° PCB mount (CON2)
2.5mm DC power connector, PCB mount (PS-0520) (CON3)
M3 x 6mm cheesehead machine screws
M3 x 9mm cheesehead machine screws
M3 hex nuts
small rubber feet, screw attachment type
PC via the ‘carrier detect’ line (CD, pin
1) of the serial comms port, this allows
the software to monitor when a card
is present in the socket.
Putting it together
You shouldn’t have any trouble
putting the interface together if you
follow the board assembly diagram
carefully, as a guide to positioning
the various components and their
orientation.
I suggest that you fit the card socket,
the DB9 connector and the DC power
socket to the board first, as all three
Semiconductors
of these may need a small amount of
1 78L05 low current regulator(REG1)
board hole ‘tweaking’ before their pins
1 MAX232 or ST232CM interface (IC1)
all mate with the board correctly. It’s
1 74HC00 quad NAND gate (IC2)
easier to do this before you add all of
1 3mm green LED (LED1 — power)
the other components.
1 3mm red LED (LED2 — read/write)
Note that the card socket mounts
1 1N4004 power diode (D1)
with its card entry slit towards the
1 1N5819 Schottky signal diode (D2)
front(!), and that as well as the various contact connection pins it also
Capacitors
has a couple of 3mm diameter plastic
1 10µF 16V RB electrolytic
locating spigots which sit in matching
4 1µF tantalum
holes in the board.
3 100nF metallised multilayer ceramic (code 100n or 104)
Once the three connectors are fitted
4 22pF NPO disc ceramic
and soldered in place, you can then
Resistors (0.25W 1%)
add the remaining components in the
2 1MΩ
(brown black green brown or brown black black yellow brown)
usual order. That is, wire links first
4 10kΩ (brown black orange brown or brown black black red brown)
(there are only two), then the 3-pin
1 1.5kΩ (brown green red brown
or brown green black brown brown)
SIL header, then resistors, capacitors
3 1kΩ
(brown black red brown
or brown black black brown brown)
and crystals. Finally come the diodes,
regulator, LEDs and ICs.
As always, make sure you fit all pothe serial port (CON2) via one of the
in card sensing switch. The other larised parts with the correct polarity
IC1 transmitters, as pin 10 is also
side of the switch is connected to as shown in the diagram.
connected to this point. The output +5V, so when a card is inserted into
Both LEDs have their cathode ‘flat’
from pin 7 of IC1 is connected to pin the socket and pushed right in, the
side towards the front of the board,
2 of CON2 which is
while both ICs
the RS-232C receive
have their notch
data (RxD) line.
end towards the
The second reback. Take special
Here are some website links where software compatible with this smart
ceiver of IC1 has its
care with the pocard reader/programmer is available for free download:
input (pin 13) conlarity of the four
www.adteknik.se/english/
nected to the Ready
1µF tantalum cawww.angelfire.com/space/aussiemulate/
to Send (RTS) line
pacitors on the outfrom the PC (CON2
er side of IC1.
www.maxking.co.uk
pin 7), and its output
When the board
www.maxkingtunisia.com
(pin 12) to the Reset
is fully assembled,
www.skyvisiontech.com/card_reader.htm
pin of the smart card
the four small rubNote that neither SILICON CHIP nor the author of this article can accept
socket. This allows
ber feet can be
responsibility for the operation of any of this software or its potential to
the software in the
attached to it usbe used for unlawful purposes.
PC to issue a reset
ing M3 x 6mm
command to the
mach-ine screws
micro in the smart
and nuts.
card whenever this
The feet are important with this kind
switch operates and pin 11 of IC1 is of ‘naked board’ assembly because
is required.
The input of the second transmitter pulled high.
they give the board proper support
The output of this transmitter (pin while lifting the solder joints away
section of IC1, pin 11, is connected
14) thus swings to RS-232 ‘mark’ level,
via a 10kΩ resistor to ground but also
from whatever surface the interface
to one side of the card socket’s built and as this output is passed back to the
may be placed on.
Where to look for software
20 Silicon Chip
www.siliconchip.com.au
That’s about it. Your smart card
interface should now be ready to use,
but before hooking it up to one of the
serial comms ports of your PC you
might want to give it a quick check-out.
1-minute checkout
To do this, connect the output cable of the 9V plug pack to CON3, and
apply power to the plugpack.
Power indicator LED1 should immediately light — if not, remove the
power and check that you’ve fitted it
the right way around.
The only other reason for ‘no glow’
is that you may have wired in diode
D1 in wrong way around, or the plug
is fitted to the plug pack output cable
with the connections reversed.
Assuming the LED is happily glowing, check the DC voltage at pin 14
of IC2 and pin 16 of IC1 with your
DMM. In both cases you should get
a reading within a few millivolts of
5.0V, and you should also be able to
measure the same voltage at the ‘+5V’
pin of the card socket and/or the end
of the 1kΩ resistor right next to it (and
alongside D2).
If these voltages measure OK, you
must have connected the regulator in
the correct way around.
At this stage your interface is probably working as it should. However, if
you have access to a scope (CRO) you
might also want to check the crystal
oscillators.
This too is very straightforward.
With the unit powered up, try fitting
the jumper shunt joining the centre
and lefthand pins of the SIL strip (looking from the front). With the scope
probe on pin 6 of IC2, you should
find a 5V peak-peak square wave of
3.75MHz.
If you shift the jumper shunt to join
the centre and righthand pin instead,
the waveform at pin 6 should simply
change in frequency to 6.0MHz.
Assuming this is what you find, you
can conclude that your smart card
reader/programmer is all present and
correct.
All you need now is a cable to con-
nect it to a spare comms port of your
PC and of course some software so that
your PC knows how to talk to a card
plugged into the front socket. Plus a
card or two, of course...
Incidentally there’s a lot of specialised knowledge and jargon associated with some areas of smart card
technology.
You’ll find a lot of this explained
in some of the documentation files
available on the Angelfire website.
If you’d also like more information
on the PIC 16F84A micro and the
24LC16 EEPROM, this can easily be
downloaded from the Microchip website (www.microchip.com).
There are applications notes available as well as device data sheets —
most of them in PDF file format.
So once you have the interface, your
future with smart card technology will
SC
await. Over to you!
Where from, how much. . .
This project was designed for Jaycar
Electronics and is only available
through Jaycar Electronics stores,
dealers and mail order service.
Expected retail price is around $29.95.
Jaycar also have blank smart cards
available for $19.95 each. Contact your
nearest Jaycar Electronics store.
ELECTRONICS
Do You Eat, Breathe and Sleep Technology?
Jaycar is a leading electronics retailer with over 6,000 products from electronic components to computer accessories.
Management Opportunities plus Full and Part Time Sales Positions
Available Nationwide
We are growing rapidly with 30 stores and we have an expansion programme to open many more. Backed by mail order and a
fully interactive website, we need dedicated individuals to help achieve our goals.
You need to be customer focused, with an eye for detail and empathy for the products we sell. Ideally you will have some
experience in retailing, coupled with management experience for the senior positions. You will also need to be energetic,
enthusiastic and have excellent interpersonal skills.
Career opportunity with full training is available if you have the drive and ambition to make your future at Jaycar.
We offer a competitive salary, sales commission and many other benefits.
To apply for any of the above positions please ask in-store for details or alternatively send a full C.V. indicating the roll you
are interested in, location and details of current salary to;
Retail Operations Manager
Jaycar Electronics Pty Ltd
P.O. Box 6424
Silverwater NSW 1811
Fax: (02) 9741-8500
Email: jobs<at>jaycar.com.au
www.siliconchip.com.au
January 2003 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
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
E
R
U
FEATJECT
PRO
Build the
–– aa new,
new, high
high perform
perform
By LEO SIMPSON
& PETER SMITH
The transmogrification of an amplifier.
Many readers will recognise the
venerable (26-year-old!) ETI-480
top left. But the SC480 (bottom right)
is as modern as tomorrow –
with performance to match.
Performance
into 4Ω
50 watts into 8Ω; 70 watts
Output Power
tts into 4Ω
77 watts into 8Ω; 105 wa
Music Power
1W – see Fig.1)
B at 14Hz and 70kHz (at
Frequency response -1d
0.875V for 50W into 8Ω
Input sensitivity
typically <.003%
5% from 20Hz to 20kHz;
d,
Harmonic distortion <.0
22kHz); -119dB A-weighte
4dB unweighted (22Hz to
-11
io
Rat
ise
-No
-to
nal
Sig
into 8Ω
both with respect to 50W
t PTC thermistor
h respect to 8Ω and withou
wit
z,
1kH
&
Hz
100
at
>140dB
Damping factor
thermistor
es plus “Polyswitch” PTC
Protection fus
26 S
ilicon Chip onditional
Stability unc
www.siliconchip.com.au
SC
ETI-480
mance
mance amplifier
amplifier module
module
Have you built one – or more – of the popular ETI-480 power
amplifier modules over the years? Here is the module to
replace that old design. The SC480 produces a great deal
less distortion, is much quieter and has inbuilt protection.
It also sounds much better.
B
ack in the October 2002 issue we noted that we
intended to produce a replacement module for the
very popular ETI-480 amplifier module which was
published back in December 1976 – 26 years ago.
In the same note we stated, somewhat controversially,
that the ETI-480 was a dog of an amplifier and that it was
not a good performer, even by 1976 standards.
Having made that outrageous statement (to some readers,
at least), we had to come up with the goods. Fortunately,
we were pretty confident that we could, and we are pleased
to state that this new module is even better than we had
hoped. It uses the same power output transistors as in the
ETI-480 and just one more low-cost transistor has been
added to the overall component count. Kit cost should be
about the same as for the ETI-480.
When this project was first mooted, we decided to base
it on TIP3055 and TIP2955 plastic
power transistors. These are
60V 15A 90W
transistors in the
TO-218 (SOT-93)
encapsulation.
We i n t e n d e d
to produce a new
version of a 100W
module which was
published in the December 1987 issue of
SILICON CHIP. That design was based on a Hitachi
amplifier circuit and used
2N3055/MJ2955 power
www.siliconchip.com.au
transistors in TO-3 metal encapsulation.
Accordingly, we produced a PC board pattern for the new
module and while we waited for it to be produced by RCS
Radio Pty Ltd (thanks Bob), we realised that a substantial
number of readers who had built countless ETI-480 modules
would probably like to “graduate” to our new design but
would wish to at least reuse the TO-3 power transistors
from their ETI-480s on the new board.
Hence, the idea of a TO-3 version of the new module
also came to pass, as is featured here.
The plastic version of the module has the power transistors lined up along the back edge, making it easy to mount
them to the vertical surface of a finned heatsink.
The TO-3 version is larger and has the four power transistors mounted on the horizontal shelf of a cast heatsink
or on a rightangle bracket which can then be mounted on
a vertical heatsink.
Why publish both modules? The simple answer is that
we had produced them both, so why not? However, each
module has its own advantages.
Version 2, using the TO-3 transistors, is rugged but takes
up more space and is likely to be less convenient to mount
in a typical chassis. There is also more work in assembling
Version 2 with the TO-3 transistors.
Version 1, with the plastic power transistors is quite a
bit more compact and less trouble to mount in a typical
chassis but the module assembled onto a heatsink is not
quite as rugged to handle.
By the way, if you decide to build Version 1, don’t be
tempted to substitute the (usually) cheaper MJ“E”... versions of the transistors. These TO-220 transistors are rated
lower (only 75W) and will inevitably cause you great pain
and suffering.
January 2003 27
Which version to build?
Our preference is for Version 1 but we have a sneaking
suspicion that Version 2, with the TO-3 power transistors,
will be the more popular module (especially amongst
those looking for a somewhat look-alike ETI-480 substitute).
Depending on the particular brand of power and driver
transistors used, both modules will give virtually identical
performance.
Regardless of which version you decide to build, the
performance will be vastly better than the old ETI-480
design.
And that is as it should be. After all, we should have
learnt quite a bit about amplifier design in 26 years or so,
shouldn’t we?
Performance
Power output is 50 watts RMS into a 8Ω load and 70
watts into 4Ω load, before the onset of clipping. Music
power is around 77 watts into 8Ω and 105 watts into 4Ω.
Hang on a minute! Wasn’t the ETI-480 claimed to be 100W
into 4Ω? Well, it was but the distortion graph published by
ETI back in December 1976 shows the amplifier heading well
into clipping at around 70W RMS. This is to be expected
since both the ETI-480 and the new SC480 use the same
voltage rails and the same output transistors.
A particular feature of the SC480 is low distortion.
Distortion for all power conditions, up to clipping, into
an 8-ohm load, is less than .05% for the full range of frequencies from 20Hz to 20kHz.
Similarly, with a 4-ohm load, total harmonic distortion
is less than .07% for the full audio frequency range.
In reality, this is a very conservative rating as the distortion will typically be .003% or less for both load conditions.
And for very lower power levels, less than 100mW, where
noise becomes a significant part of the measurement, the
distortion is really low, down to as low as .0005%. This is
two orders of magnitude better than the ETI-480!
Signal to noise ratio is better than -114dB (unweighted,
22Hz to 22kHz) with respect to full power into an 8Ω load.
Frequency response is just 1dB down at 14Hz and 70kHz
(see Fig.1).
Fig.1: this is the frequency response of both versions of the
new amplifier, taken at a power level of 1W into an 8Ω load.
Transistor quality
As in most things, you get what you pay for and it is no
different with these modules.
The plastic version (Version 1) of the amplifier was built
with the output and driver transistors in what we would
call the premium brands: Philips, Motorola (On Semi) and
ST Micro.
Version 2 was built with second rank power and driver
transistors (Mospec). We did this to compare performance
and we are pleased to report that although the premium
branded transistors do give slightly better performance,
there is a not a lot in it.
Refer to the distortion graphs of Figs.2-9 to make the
comparisons.
Either way, the performance of these modules is very
good, especially considering that we are not using expensive transistors such as Motorola MJL21193/4 or the even
more expensive MJL1302A & MJL3281A.
In fact, in some respects the measured performance challenges that of our popular and more powerful Plastic Power
module published in the April 1996 issue. Interestingly, a
These two oscilloscope screen grabs show just how clean this new amplifier is. The first screen (left) shows a 1kHz output
waveform at a level of 40W into 8Ω at top. The lower trace is the distortion waveform which has been “averaged” by the
scope to remove noise. Note that it is mostly second harmonic distortion. The same process has been applied to the screen
shot at right except that it is a 10kHz signal. Again, the distortion is mainly second harmonic.
28 Silicon Chip
www.siliconchip.com.au
key part of that performance standard comes about because
of improved PC board and wiring layout.
We’ll discuss these vitally important aspects in more
detail later in this article.
Oh, and we should state that the SC480 Version 1 and
Version 2 modules are a drop-in replacement for the ETI480 modules but will sound a great deal better.
While nominally of the same rating, they will deliver
more power, they’re quieter and as already detailed, much
lower in distortion.
By the way, these modules are not suitable for driving 2Ω
loudspeakers as used in car sound systems. We do not have
space to publish the load/line curves in this article but suffice
to say that attempting to drive 2Ω loads will blow the fuses
and may blow the output transistors as well.
Protection
The trouble with all high-power amplifiers is that, if a
transistor fails, there is a big chance that the loudspeaker
system could be damaged, despite having fuses in the
power supply.
The problem is that the fault condition may place a large
DC voltage across the speaker’s voice coil and the resulting
current may not blow the fuses. The speaker’s voice coil
then gets red hot and may actually set the speaker cone on
fire! Once that happens and if you’re not there to kill the
power to the amplifier, you can have a raging fire in your
home and enormous amounts of smoke being generated by
the burning of the filling material in the cabinet.
Our normal approach to this problem is to incorporate
relay protection which will disconnect the loudspeaker in the
event of a large DC fault condition occurring in the amplifier.
Relay protection works as far as the speaker is concerned
but it doesn’t protect the amplifier itself if the loudspeaker
leads are shorted. Here again the fuses may not blow before
the output transistors are damaged.
Neither do fuses protect the speakers if you seriously
over-drive the amplifier. This is a particular risk for tweeters
but even woofers can have voice coil damage by serious
over-drive.
Complete protection
The method we have used to provide protection to both
the loudspeaker and amplifier is to connect a high current
positive temperature coefficient (PTC) thermistor (known
commercially as a “Polyswitch”) in series with the output
circuit. This is the same method of protection as we used
in the original module published in December 1987.
The PTC thermistor normally has a very low resistance
but when the current through it rises to high value, it immediately switches to a high resistance state and stays in
that condition until the fault is fixed or power is removed.
The resistance of the PTC thermistor is so low (typically
0.1Ω or less), it has a negligible effect on amplifier performance, apart from the fact that it does cause a reduction
in damping factor.
In practice, it works extremely well. It allows you to
drive the amplifier to full power on program signals but
the moment a short circuit is applied or the amplifier is
seriously over-driven, the PTC thermistor goes high in
resistance to cut off the fault current.
After the protection thermistor has switched to its high
state, it takes some time to revert to its low resistance condition, after the fault current has ceased. This depends on
how much current is passing through it. If the drive level
is maintained after a fault has occurred, the protection
thermistor will stay high in resistance.
Circuit description
Now let’s have a look at the circuit of Fig.10. 13 transistors
and three diodes make up the semiconductor complement.
The input signal is coupled via a 1µF bipolar electrolytic
capacitor and 2.2kΩ resistor to the base of Q2. Q2 & Q3
make up a differential pair. Q1 is a constant current source
which sets the current through Q2 & Q3 and renders the
amplifier largely insensitive to variations in its supply rails
Just to confuse you, Version 2 of the SC480 amplifier (with TO-3 transistors) is on the left, while Version 1 (with TO-218
transistors) is on the right. There is only a small difference in performance between the two versions.
www.siliconchip.com.au
January 2003 29
Fig.2: THD versus power at 1kHz into an 8Ω load for
Version 1 (TO-218).
Fig.3: THD versus power at 1kHz into a 4Ω load for
Version 1 (TO-218).
(power supply rejection).
Signals from the collectors of Q2 & Q3 drive another
differential pair, Q4 & Q5 which have a “current mirror”
as their collector loads. The current mirror, comprising D3
and Q6, ensure that this second differential stage has high
linearity (ie, low distortion).
The output of Q5 is then used to drive class-AB output
stage consisting of drivers Q8 & Q9 and power transistors
Q10, Q11, Q12 & Q13.
Q7 is a Vbe multiplier, so-called because it multiplies
the voltage between its base and emitter to provide a fixed
voltage between its collector and emitter, regardless of
the drive current delivered to the output stage by Q5. The
voltage is adjusted by trimpot VR1.
The function of Q7 is to set the DC voltage applied
between the bases of Q8 & Q9. By doing this it sets the
“quiescent current” in the output stage (ie, the current
when no signal is present). This is to minimise crossover
distortion. In fact, our tests did not reveal any signs of
crossover distortion.
The complementary output transistors are connected in
parallel to give high output current capability. Each transistor has its own 0.22Ω emitter resistor. These are included
to ensure that the output current is shared reasonably well
between the output transistors.
Negative feedback is applied from the output stage back
to the base of Q3 via a 22kΩ resistor. The level of feedback, and therefore the voltage gain, is set by the ratio of
the 22kΩ resistor to the 1kΩ at the base of Q2. The 47µF
bipolar capacitor in series with the 1kΩ sets the DC gain
to unity and sets the -3dB point of the frequency response
to about 3Hz. The other determinant of the amplifier’s low
frequency response is the 1µF input capacitor and the
22kΩ base bias resistor feeding Q1 and these set a -3dB
point at about 7Hz.
The 330pF capacitor together with the 2.2kΩ resistor
feeding Q2 form a low pass filter to roll off frequencies
above 200kHz.
The 68pF capacitor between the base and collector of
Q5 and the 10pF capacitor between base and collector of
Q2 roll off the open-loop gain of the amplifier to ensure
stability with feedback applied. Note that the 68pF capacitor can be a ceramic or polystyrene type and must a have
a voltage rating of 100V or more. Other capacitor types are
not recommended.
Another important factor in the amplifier’s excellent
Fig.4: THD versus power at 1kHz into an 8Ω load for
Version 2 (TO-3).
Fig.5: THD versus power at 1kHz into a 4Ω load for
Version 2 (TO-3).
30 Silicon Chip
www.siliconchip.com.au
Fig.6: THD versus frequency at 40W into an 8Ω load
(Version 1).
Fig.7: THD versus frequency at 60W into an 4Ω load
(Version 1).
stability is the output RLC network consisting of the 6.8µH
choke, a 6.8Ω resistor and a 150nF capacitor. Not only does
this network ensure stability but the capacitor is an effective
killer of any RF and mains-interference signals which can
be picked up by long loudspeaker leads.
As noted earlier, the design of the PC board is a very
critical part of the overall circuit. The placement of the
components and the way that heavy currents flow in the
tracks is all arranged to minimise the radiation of harmonics
into the input stage involving Q1 & Q2.
This board is yet a further refinement of the topology
we first introduced in the Ultra-LD amplifier featured in
March, May & August 2000 and then again in November
& December 2001. The PC board for version 2 and the
component placement is shown in Fig.12.
It incorporates “star earthing” whereby all earth currents
come back to a central point on the board, thereby avoiding
any flow of output, supply and bypass currents flowing in
the signal earths.
Furthermore, placement of the copper tracks to the output
stages is arranged, as far as possible, to cancel the magnetic
fields produced by the asymmetric currents drawn by each
half of the output stage.
By way of explanation, when the positive half of the
output stage (Q10 & Q12) conducts, the DC current drawn
is effectively a positive half wave (ie, rectification takes
place) of the signal waveform. And when the negative
half conducts (Q11 & Q13), the DC current is the negative
half wave.
A major cause of harmonic distortion in class-B amplifiers is the magnetic fields produced by these asymmetric
Fig.8: THD versus frequency at 40W into an 8Ω load
(Version 2).
Fig.9: THD versus frequency at 60W into an 4Ω load
(Version 2)
Power supply
The power supply circuit is shown in Fig.11. This uses
a centre-tapped 56V transformer driving a bridge rectifier
comprising four 1N5404 diodes and two 4700µF 50V filter capacitors. This produces unregulated supply rails of
about ±40V.
Depending on the mains AC voltage, the rails will drop
to around ±32V or less when the amplifier module is delivering full power into a 4Ω load.
We have also provided a ±15V DC supply for a preamplifier. This is derived with 2.2kΩ resistors and two 15V
1W zener diodes.
PC board topology
www.siliconchip.com.au
January 2003 31
Fig.10: this direct-coupled amplifier module uses a differential input stage (Q2,Q3) with a constant current tail (Q1). This
drives another differential amplifier (Q4,Q5) with current mirror load (D3,Q6). Quiescent current in the output stage is set
by VR1 and Q7. The output stage is a complementary class-AB configuration using Q8 & Q9 as drivers and Q10 to Q13 as
the output devices. Voltage readings are taken with no signal applied.
currents inducing unwanted signals into the input stages,
in this case involving Q1 & Q2.
So we have tried to cancel these fields as much as possible
(in a single sided PC board).
For example, notice how the positive fuseholder (F1) is
placed close and parallel to the emitter resistors for Q10 &
Q12. So what happens is that the magnetic field produced by
the asymmetric current in fuse F1 is more or less cancelled
as the same current flows back in the emitter resistors. This
is the main reason why the layouts for these two modules
is much tighter than our designs of recent years.
You will see the same method employed in the Version
1 of the board, with the heavy collector and emitter tracks
32 Silicon Chip
placed close together but we think this has been more
fortuitous on Version 2 than on Version 1.
It is then most important to arrange the DC supply cables
to the amplifier to further this cancellation process. We’ll
detail this in the construction description.
To make the input stage less vulnerable to spurious magnetic fields from the output stage, we have concentrated it
into as small an area of the PC board as possible.
Another trick is the location of the takeoff point for the
22kΩ resistor and its orientation at rightangles to the output
stage emitter resistors.
Finally, the signal earth for the input stage is separated
from the main amplifier earth by a 10Ω resistor.
www.siliconchip.com.au
Fig.11: the power supply is very simple but adequate. The ±15V
preamplifier supply is optional.
This is not so important when a single module is in use
but it is most important when two modules are used in a
stereo system.
In that situation, the joining of the two signal earths back
via the input cables to a single program source such as a
CD player will cause an earth loop and a resulting major
degradation in the separation between channels and lesser
degradation in the distortion performance.
Well, that’s probably enough discussion of the PC board
but suffice to say that the overall design has been carefully
arranged to minimise distortion and leave as little to chance
in the wiring layout so that constructors are certain to get
excellent results.
Next month, we’ll give the full details of assembly, wiring and setup of both versions, the parts list and the PC
SC
board patterns.
Fig.12: version
2 of the SC480
amplifier with
the TO-3 (steel)
transistors.
We’ll be
presenting this
again next month
as part of the
constructional
details but it is
reproduced here
to demonstrate the
attention we have
paid to the PC
board design
to achieve the
exceptional
performance
figures depicted
on earlier pages.
www.siliconchip.com.au
January 2003 33
•
•
•
•
•
•
Indicates up to 9 gears
•
Display dimming
Neutral indication
Reverse indication
Easy gear calibration
Adjustable parameters
Adjustable reverse gear
switch level
A “Tiptronic-style”
Gear Indicator
Do you know what gear your car is in at any
given time? “Just look at the gear stick”, you
say. Actually, it’s not that easy, especially if
you have a 4-speed automatic or a 5 or 6-speed
manual gearbox. And what if you ride a
motorbike? So you need the Gear Indicator – it
will give you the answer on a digital readout.
By JOHN CLARKE
I
F YOU’RE DRIVING in traffic, it is
quite easy to be in the wrong gear,
especially as the noise of the traffic
can drown out the engine. And if you
have your stereo system blaring as
well, then what chance have you got?
Yes, you can deliberately look at the
gearstick but you’re not likely to do
that unless you suspect you might be
in the wrong gear.
34 Silicon Chip
Why would you be in the “wrong
gear” in the first place? If your car is
stuck in heavy traffic you might easily
continue on for some time in 2nd or
3rd after the traffic clears, particularly
if your engine is not noisy.
Much the same can happen with an
automatic, if you are in the habit of
“flicking” back to 3rd or 2nd (eg, when
going up a hill or for engine braking
downhill). It’s all too easy to forget
to flick it back into Drive later on. As
a result, you could finish up driving
quite some distance in a low gear and
that’s not good for fuel consumption.
The same problem can happen if
you ride a motorbike. Wouldn’t it be
nice to have a digital display to show
the gear you’re in? In fact, when driving an automatic it can still be useful
to know which gear you are in, even
if Drive is correctly selected. Modern
automatics are so smooth that it can
be difficult to “pick” the changes. Now
you can “see” what the transmission
is doing.
This idea is not new, of course. All
cars with Tiptronic transmissions and
the latest Honda Jazz with its 7-speed
gearbox have a digital gear indicator
on the dashboard.
Main features
Basically, the Gear Indicator consiliconchip.com.au
sists a small box which incorporates
a single-digit LED display. This can
show gear selections from 1-9, Neutral
(which is shown on the display as a
dash; ie, “-”) and Reverse (which is
shown as an “r”).
Inside the case are several switches
which allow the unit to be calibrated
and set up for best gear detection
results. Once it’s all set up, that’s it –
there are no user controls on the front
panel to fiddle with.
As presented, the unit is designed
to be mounted on the dashboard. Alternatively, you could hide the unit
under the dashboard and mount the
LED display separately, if space is a
problem. A 9-strand cable (eg, rainbow cable) would then be required to
connect the display back to the main
circuit.
The right gear
The Gear Indicator works by monitoring both the speed of the vehicle
and the engine RPM. It then decides
which gear has been selected by
feeding the results into a lookup table
that’s programmed into an internal
microcontroller. And that means that
the unit must first be calibrated, so
that it knows what the results are for
each gear.
Note, however, that neutral (-) is
always shown when the unit is first
powered up and also if the vehicle is
stationary (or almost stationary) while
the engine is running. By contrast,
reverse (r) is shown when ever the
vehicle’s reversing lights are activated.
One thing you should note is that
the Gear Indicator does not work by
detecting gear changes – eg, by fitting
switch actuators to the gearstick. This
method would not only be unreliable but would also be a mechanical
nightmare to set up. What’s more,
the position of the gear selector in an
automatic car doesn’t tell you which
gear the transmission is in (unless 1st
gear is manually selected).
That’s because the transmission can
still select any one of the lower gears in
the remaining positions. For example,
if the gear selector is set to 3rd, 2nd
and 1st can also be selected.
Of course, it is conceivable that
the signals from an elec
tronically
controlled automatic transmission
could be used to drive a gear display.
However, we have not provided for
this in the Gear Indicator because these
signals would be different on each
siliconchip.com.au
Fig.1: block diagram of the Gear Indicator. It works by counting the
number of ignition pulses that occur during a fixed number of pulses
from a speed sensor and comparing the result with a “lookup” table
that’s stored in memory.
type of vehicle and may be difficult
to utilise effectively.
Block diagram
Fig.1 shows the basic operation of
the Gear Indicator. There are three
external inputs: speed sensor pulses,
ignition coil pulses and the reversing
switch input.
The speed sensor pulses can be
obtained from a rotating magnet and
coil assembly mounted on the tailshaft. Alternatively, you can use the
digital speed signal that comes from
the vehicle’s engine computer, if this
can be identified (and accessed). The
ignition pulses can either be obtained
from the ignition coil or you can use
the low-voltage tachometer signal from
the engine management computer if
this is available.
The reversing input is obtained,
naturally enough, from the reversing
switch. When this switch is closed
(ie, when reverse gear is selected), the
display will show an “r” for reverse
as indicated previously. Conversely,
when the switch is open, the display
will show either neutral (when the
unit is first powered up or if there are
no pulses) or a gear number.
If the vehicle is moving, the circuit
counts the number of ignition coil
pulses that occur during a fixed number of speed pulses. If a low gear is
selected (eg, 1st gear), it follows that
there will be more ignition pulses
counted for a given speed compared
to those counted at the same speed in
a higher gear.
The gear selection number is shown
on the 7-segment LED display. This
number is obtained by comparing the
number of ignition pulses counted
with the stored values (in a microcon
troller). These stored values are obtained during calibration of the Gear
Indicator.
Fig.2 shows how the Gear Indicator
compares the ignition pulse counts
with the calibration values. These
calibration values are different for
each gear and are obtained by driving
the vehicle in each gear during the
initial setup.
This means that comparing the
counted pulses with the calibration
values should give the correct gear
number. However, in practice, the
calibration number may differ from
the value ob
tained during driving.
That’s because the number of ignition
pulses counted may vary by up to
several counts for the same number of
speed pulses, depending on the phase
difference between the two.
To counter this effect, a set amount
of hysteresis is added to each gear
range – see Fig.2. This can be varied
to suit the vehicle during calibration
and also corrects for any slippage in
the transmission – either in the clutch
or in the torque converter.
As a further refinement, a slight
January 2003 35
IC2a’s output is fed to pin 6 of IC1 via
a 3.3kΩ resistor. The signal on pin 6
is then clamped by pin 6 (via internal
diodes) to 0.6V above IC1’s supply rail
(5V), as before.
In operation, IC1’s pin 6 input is
set as an interrupt – ie, the microcontroller’s embedded software increments the count each time pin 6
goes low.
Display brightness
Fig.2: a small amount of hysteresis is added at the end of each gear range
to correct for phase errors and transmission slippage. This is set to suit the
vehicle and is one of several parameters that are adjusted during the setup
procedure.
delay is added between each display
update. This delay prevents the display from behaving erratically during
gear changes, when clutch slippage
and changes in engine RPM could
otherwise produce an incorrect gear
indication.
Circuit details
Refer now to Fig.3 for the circuit
details. As indicated above, it’s based
on a PIC microcontroller (IC1). This
device accepts inputs from the various
sensors and switches and drives the
7-segment LED display.
OK, let’s start with the speed sensor
circuit. This consists of a sensing coil
which mounts on the chassis, plus four
magnets which mount on a drive shaft
(or tail shaft). As the magnets spin
past, they induce a voltage into the
coil and this is detected by comparator
stage IC3.
One side of the speed sensing coil
connects to a 2.5V sup
ply, derived
from a voltage divider consisting of
two 2.2kΩ resistors between the +5V
rail and ground. This 2.5V rail is decoupled using a 47µF capacitor and
biases pin 3 (the non-inverting input)
of IC3 via a 22kΩ resistor. It also biases
pin 2 of IC3 via the coil and a series
1kΩ resistor. Diodes D1 & D2 clamp
the input signal from the coil to 0.6V,
while the associated 10nF capacitor
filters the pickup signal.
IC3 is wired as an inverting Schmitt
trigger comparator. Its hysteresis is set
by a 1MΩ positive feedback resistor,
which prevents false triggering due
to noise.
The output signal from the speed
sensor is a 250mV peak-to-peak pulse
waveform and this is fed to pin 2 of
IC3. Each time the input swings nega36 Silicon Chip
tive, IC3’s output (pin 1) goes high (ie,
to about 10V).
This output is fed to pin 12 (RB6)
of IC1 via a 3.3kΩ current limiting resistor. The internal diodes at RB6 then
clamp the signal voltage to about 5.6V.
Note that the feedback signal for IC3
is derived from this point to ensure a
consistent hysteresis level, regardless
of the 12V supply level.
Ignition coil pulses
As shown, signals from the ignition
coil are first fed to a voltage divider
consisting of 22kΩ and 10kΩ resistors.
The associated 68nF capacitor then
shunts any signals above 700Hz to
ground to eliminate noise.
From there, the signal is AC-coupled
via a 1µF capacitor to diode D3 and
thence to pin 2 of op amp IC2a. Zener
diode ZD2 limits the signal amplitude
at D3’s anode to 20V, while D3 prev
ents negative signals from being fed
into IC2a. The associated 10kΩ resistor
pulls pin 2 low in the absence of a
signal input via D3.
A low input (LOW IN) has also
been provided at the junction of D3
and ZD2. This input allows the tachometer signal from an engine management computer to be applied instead
of using the ignition coil input. The
signal level at this input can be any
where from 2.3V up to a maximum
of 20V.
IC2a is wired as an inverting comparator with hysteresis. Its pin 3 input
is nominally biased to about 1.6V via
a voltage divider connected to the 5V
rail, while the 47kΩ feedback resistor
provides the hysteresis to set the high
and low trigger points (1.7V and 1.5V
respectively).
The resulting square-wave signal at
Trimpot VR1, light dependent resistor LDR1 and op amp IC2b are used
to control the display brightness. As
shown, IC2b is connected as a voltage
follower and this drives buffer transistor Q1 (which is inside the negative
feedback loop) to control the voltage
applied to the anode of the 7-segment
LED display.
When the ambient light level is high,
LDR1 has low resistance and so the
voltage on pin 5 is close to the +5V
supply rail. As a result, the voltage on
Q1’s emitter will also be close to +5V
and so the display will operate at full
brilliance.
As the light level falls, the resistance
of the LDR increases and the voltage
on pin 5 of IC2b decreases. As a result,
Q1’s emitter voltage also falls and so
the display operates with reduced
brightness.
When it’s completely dark, the
LDR’s resistance is very high and the
voltage on pin 5 of IC2b is determined
solely by VR1. This trimpot is adjusted
to give a comfortable display brightness at night.
The 7-segment LED display is driven via the RA1, RB1-RB5 and RB7
outputs of IC1 via 470Ω resistors. A
low output on any one of these output
lines lights the corresponding display
segment, with the output at RA4 controlling the decimal point.
Switch inputs
Pushbutton switches S1, S2 and S3
are monitored using the RA2 and RA3
inputs. These two inputs are normally
tied high via 10kΩ resistors and are
only pulled low when the switches
are pressed.
When S1 (Mode) is closed, RA2 is
pulled low and this is recognised as
a closed switch by the software. Similarly, when S2 (Number) is closed,
RA3 is pulled low, while pressing S3
(Store) pulls both RA2 & RA3 low to
ground (via diodes D4 & D5). As a result, the software can recognise which
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Fig.3: the complete circuit of the Gear Indicator. The PIC microcontroller (IC1)
processes the signals from the various inputs and drives a single 7-segment LED
display (DISPLAY1) to show the result. IC2b, Q1 & LDR1 automatically dim the
display at night, so it is not too bright.
switch has been pressed and respond
accordingly.
Clock signals
Clock signals for IC1 are provided
by an internal oscillator and a 4MHz
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crystal (X1) connected between pins
15 & 16. The two associated 22pF
capacitors are there to provide the
correct loading and to ensure that the
oscillator starts reliably.
The crystal frequency is divided
internally to produce clock signals for
the internal circuitry and the various
parameters used in the software. It is
also used to give a precise time period
to count the speed pulses.
Power
Power for the circuit is derived from
the vehicle’s battery via a fuse and
the ignition switch. This supply line
January 2003 37
Table 2: Capacitor Codes
Value
100nF (0.1µF)
68nF (.068µF)
10nF (.01µF)
22pF (22p)
IEC Code EIA Code
100n
104
68n
683
10n
103
22p
22
to power IC1. IC2 and IC3 derive their
power directly from the de
coupled
+12V rail.
Construction
Fig.4 shows the assembly details.
Most of the work involves building
two PC boards: a microcontroller board
coded 05101031 and a display board
coded 05101032. These two boards
are then stacked together piggyback
fashion using pin headers and cut
down IC sockets, so that there is very
little external wiring.
Begin by carefully checking the PC
boards for defects, by comparing them
with the published patterns. It’s rare to
find problems these days but it doesn’t
hurt to make sure.
The microcontroller board can
be assembled first. Install the three
wire links first, then follow with the
resistors and diodes. Table 1 shows
the resistor colour codes but we also
recommend that you check each value
using a digital multimeter as some
colours can be hard to decipher.
Note that the six 470Ω resistors are
mounted end-on to save space. Take
care when installing D1 & D2 as they
face in opposite directions. Similarly,
watch the orientation of ZD1.
REG1 can go in next. It is mounted
with its metal tab flat against the PC
board. As shown, its leads are bent
Fig.4: install the parts on the two PC boards as shown here. Note that
all the electrolytic capacitors must be mounted so that their bodies lie
parallel to the board surfaces (see photos), so that the boards can later be
stacked together.
is decoupled using a 10Ω 1W resistor
and filtered using a 47µF electrolytic
capacitor. ZD1 provides transient protection by limiting any spike voltages
to 16V. It also provides reverse polarity
protection – if the supply leads are
reversed, ZD1 conducts heavily and
“blows” the 10Ω resistor.
The decoupled supply is fed to
3-terminal regulator REG1 to derive a
+5V rail. This rail is then filtered using
10µF and 100nF capacitors and used
Table 1: Resistor Colour Codes
o
No.
o 1
o 2
o 2
o 5
o 2
o 2
o 3
o 2
o 7
o 1
38 Silicon Chip
Value
1MΩ
47kΩ
22kΩ
10kΩ
4.7kΩ
3.3kΩ
2.2kΩ
1kΩ
470Ω
10Ω
4-Band Code (1%)
brown black green brown
yellow violet orange brown
red red orange brown
brown black orange brown
yellow violet red brown
orange orange red brown
red red red brown
brown black red brown
yellow violet brown brown
brown black black brown
5-Band Code (1%)
brown black black yellow brown
yellow violet black red brown
red red black red brown
brown black black red brown
yellow violet black brown brown
orange orange black brown brown
red red black brown brown
brown black black brown brown
yellow violet black black brown
N/A
siliconchip.com.au
down at right angles so that they pass
through their respective mounting
holes. This is best done by slipping
an M3 screw through the hole in the
device tab, positioning it on the PC
board and then gripping one of the
leads with a pair of needle-nose pliers,
just before it reaches the mounting
hole. The device is then lifted clear of
the PC board and the lead bent down at
right angles, after which the procedure
is repeated for the next lead.
Next, install a socket for IC1, taking
care to ensure that it is the right way
around. Don’t plug the microcontroller in yet – that step comes later, after
you’ve checked out the power supply.
IC3 can then be installed, followed by
the capacitors.
Note that the 47µF capacitor near the
speed sensor input must be installed so
that it lies parallel with the PC board
– see photo. Similarly, the adjacent
47µF & 10µF capacitors below REG1
lie over the regulator’s leads. In each
case, it’s simply a matter of bending the
capacitor’s leads at right angles before
installing it on the PC board.
Crystal X1 mounts horizontally on
the PC board and can go in either way
around. It is secured by soldering a
short length of wire between one end
of its case and an adjacent PC pad.
Finally, you can complete the
assembly of this board by fitting PC
stakes to the external wiring points
and fitting the 7-way single in-line
(SIL) sockets. The latter are made by
cutting down two 14-pin IC sockets
into in-line strips using a sharp knife
or fine-toothed hacksaw.
Clean up any rough edges with a
file before installing them on the PC
board.
Checking the supply rails
Before plugging in IC1, it’s a good
idea to check the supply rails (note:
you don’t need to have the display
board connected to do this). All you
have to do is connect a 12V supply to
the board and check that there is +5V
on pins 4 & 14 of the socket (use the
metal tab of REG1 for the ground connection). If this is correct, plug IC1 in
as shown in Fig.4 – ie, pin 1 towards
bottom right.
Display board
Now for the display board. Install
the wire link first, followed by the
resistors, diodes D3-D5, ZD2 and
transistor Q1. The three capacitors can
siliconchip.com.au
This is the fully-assembled microcontroller board. Note particularly how the
three electrolytic capacitors are mounted – ie, so that they lie horizontally
across other components.
The pin headers on the underside of the display board plug into the in-line
sockets on the microcontroller board. Take care to ensure that the 7-segment
LED display is correctly oriented.
then be installed, along with trimpot
VR1 and the 7-segment LED display.
Note that the 1µF bipolar capacitor is
installed so that it lies across ZD2 –
see photo.
Watch the orientation of the LED
display – its decimal point goes towards bottom right.
LDR1 can go in next. It’s mounted so
that its top face is about 3mm above the
face of the 7-segment display. Once it’s
in, you can install switches S1-S3 and
PC stakes at the external wiring points.
The three 7-way SIL pin headers are
installed on the copper side of the PC
board with their leads just protruding
above the top surface. You will need
a fine-tipped soldering iron to install
them. Note that you will have to slide
the plastic spacers along the pins to allow room for soldering, after which the
spacers are pushed back down again.
Final assembly
Work can now begin on the plastic
case. First, remove the integral side
pillars with a sharp chisel, then slide
the microcontroller board into place.
That done, mark out the two mounting holes on the base – one aligned
with the hole in REG1’s metal tab and
the other diagonally opposite on the
lefthand side.
Now remove the board and drill
January 2003 39
Parts List
1 microcontroller PC board, code
05101031, 78 x 50mm
1 display PC board, code
05101032, 78 x 50mm
1 plastic utility case, 83 x 54 x
30mm
1 dark red transparent Perspex
or Acrylic sheet, 14 x 16 x
2.5mm
1 4MHz parallel resonant crystal
(X1)
1 LDR (Jaycar RD-3480 or
equivalent)
4 or 6 button magnets
1 coil former, 15mm OD, 8mm ID
x 7mm
1 20m length of 0.18mm enamelled copper wire
1 6mm x 25mm steel bolt, 2
washers and nut
6 PC stakes
3 7-way pin head launcher
2 DIP-14 low-cost IC socket with
wiper contacts (cut for 3 x
7-way single in-line sockets)
3 PC-mount tactile membrane
switches (S1-S3) (Altronics S
1120 or equivalent)
2 6mm long M3 tapped spacers
1 10mm Nylon spacer or 2 x
6mm spacers with one cut to
4mm
1 9mm long untapped metal
spacer
2 M3 x 6mm countersunk screws
2 M3 x 15mm brass screws
1 100mm length of 0.8mm tinned
copper wire
1 2m length of single core
shielded cable
1 2m length of 7.5A mains rated
wire
1 2m length of red automotive
wire
1 2m length of black or green
automotive wire (ground wire)
1 2m length of white automotive
wire
these two holes to 3mm. Once drilled,
they can be slightly countersunk on
the outside of the case to suit the
mounting screws.
In addition, you will have to drill
two holes in the back of the case to accept the power leads, the shielded cable from the speed sensor, the ignition
coil and the reversing switch. These
40 Silicon Chip
1 200kΩ horizontal trimpot (VR1)
Semiconductors
1 PIC16F84P microprocessor
programmed with gear.hex
(IC1)
2 LM358 dual op amps (IC2,IC3)
1 7805 or LM340T5 5V 1A
3-terminal regulator (REG1)
1 BC337 NPN transistor (Q1)
1 HDSP5301, LTS542A common
anode 7-segment LED display
(DISP1)
5 1N914, 1N4148 signal diodes
(D1-D5)
1 16V 1W zener diode (ZD1)
1 20V 1W zener diode (ZD2)
Capacitors
2 47µF 25VW PC electrolytic
1 10µF 16VW PC electrolytic
1 1µF bipolar electrolytic
3 100nF MKT polyester
1 68nF MKT polyester
1 10nF MKT polyester
2 22pF ceramic
Resistors (0.25W 1%)
1 1MΩ
2 3.3kΩ
2 47kΩ
3 2.2kΩ
1 22kΩ
2 1kΩ
1 22kΩ 1W
7 470Ω
5 10kΩ
1 10Ω 1W
2 4.7kΩ
Alternative speed sensor
1 PC board, code 05101033, 14
x 30mm.
1 UGN3503 Hall senosr
1 100nF MKT polyester capacitor
1 2m length of twin-core shielded
cable
3 PC stakes
Miscellaneous
Automotive connectors, heatshrink tubing, aluminium bracket,
self-tapping screws
holes should be located so that they
line up with the relevant PC stakes.
The display PC board can now be
plugged into the microcontroller board
and the assembly fastened together
and installed in the case, as shown
in Fig.5. Once it’s all together, check
that none of the leads on the display
board short against any of the parts on
the microcontroller board. It may be
necessary to trim some of the pigtails
on the display board to prevent this.
The panel artwork can now be used
as a template for marking out and drilling the front panel. You will need to
drill a hole for the LDR plus a series
of small holes around the inside peri
meter of the display cutout.
Once the holes for the display cutout
have been drilled, knock out the centre-piece and clean up the rough edges
using a small file. Make the cutout just
big enough so that the red Perspex is a
tight fit. A few spots of superglue along
the inside edges can be used to ensure
that the window stays put.
That done, you can affix the front
panel label and cut out the holes with
a utility knife.
Testing
Now for the smoke test! First, apply power and check that the display
shows “-”. If it doesn’t, switch off immediately and check for wiring errors
and solder faults.
Assuming that everything is OK,
you can test the dimming feature by
holding your finger over the LDR.
Adjust VR1 until the display dims to
the level you want at night.
Next, connect the leads from the
ignition coil (or low level input),
the reversing switch and the speed
sensor. These leads all connect to the
underside of the PC board and the
ignition and reversing switch wires
pass through to the base of the case via
notches cut in the side of the microcontroller PC board. These notches are
located on either side of the adjacent
7-way socket and their positions are
marked on the PC board using a fine
track outline.
Speed sensor
Two different speed sensors can be
made up, one based on a coil pickup
and the other using a Hall sensor pickup. However, both rely on the use of
an adjacent rotating magnet assembly .
The coil pickup is likely to be more
rugged and less prone to water damage
but the Hall sensor will allow for very
low speed operation. That’s because its
output voltage doesn’t depend on the
speed at which the magnets rotate past
the sensor. It’s just a matter of waterproofing it correctly, using heatshrink
tubing and silicone sealant.
The coil sensor version is shown in
Fig.6. It is made by winding about 400
siliconchip.com.au
Fig.5: this diagram shows how the two PC boards are
stacked together and secured to the bottom of the case
using screws, nuts and spacers. Be sure to use nylon
spacers where specified.
Fig.6: the pickup coil used in the speed sensor is mounted
on a L-shaped bracket that’s secured to the vehicle’s
chassis. Position the coil so that it is no more than 10mm
away from the magnets as they pass, to ensure sufficient
signal pickup. Note that the magnets must all be installed
with the same pole facing outwards – either North as
shown here or South.
turns of 0.18mm enamelled copper
wire onto a plastic bobbin measuring
15mm OD x 8mm ID x 5mm. Use
electrical tape to secure the turns and
leave about 10-20mm of lead length
at each end.
Once the coil has been wound,
solder its leads to a suitable length of
shielded cable – ie, one lead goes to
the shield wire and the other goes to
the core. Secure this lead to the side of
the coil with some tape, then cover the
coil with silicone sealant (preferably
the non-acid type such as roof and
gutter sealant).
Finally, cover the coil with a short
siliconchip.com.au
Fig.7: the alternative speed sensor
uses a Hall effect device mounted
on a small PC board.
This is the completed PC board assembly, ready for mounting in the plastic
case. Note that the various external leads are all soldered to PC stakes on the
copper side of each board, with the leads from the display board resting in
small grooves cut into the microcontroller board.
January 2003 41
Adjustable Parameters For The Gear Indicator
Because each vehicle is different,
the Gear Indicator must be correctly
set up in order to obtain the best
results. Consequently, the unit has
been designed to cater for up to nine
gears and there are various parameters that can be adjusted to control
its operation.
Table 3 shows the details of the
various parameters. These are as
follows:
(1) The first parameter that can
be set is the number of speed pulses used to gate the ignition pulses.
This is adjustable from 4-36 pulses
in increments of 4, using numbers
from 1-9. The initial setting is for 12
pulses but this may have to be varied
to cater for various speed sensor
characteristics.
(2) Next is the amount of hysteresis
for each gear comparison. In practice,
this value is made just large enough
so that the display does not sometimes briefly show the next highest
gear number. The default value
is 6% of the ignition pulse count and
this should be suitable in most cases.
This value will have to be increased
if the display shows a tendency to
occasionally jump to the next highest
gear. Conversely, it should be made
length of heatshrink tubing and shrink
it into place using a hot-air gun
The sealant should now be left to dry
for about eight hours. A 100mm-long
cable tie can be placed around the coil
to secure the lead in place.
The alternative Hall sensor is assembled on a small PC board coded
05101033. Fig.7 shows the assembly
details. Apart from the Hall sensor
itself, there’s just a single 100nF capacitor to be installed.
Note that the UGN3503 Hall sensor
is mounted flat against the PC board
with the label side up. The connecting lead to the main unit is run using
twin-core shielded cable.
Installation
Be sure to use proper automotive
cable and connectors when installing
the unit into a vehicle. The +12V supply is derived via the ignition switch
and the fusebox will provide a suitable
42 Silicon Chip
Table 3: Adjustable Parameters
Display
Value
Speed Puls- Hysteresis
es (S)
Delay (d)
Timeout (-) Reverse (r)
Clear (C)
1
4
2%
0.1s
0.5s
12V = r*
-
2
8
4%
0.2s*
1s
0V = r
-
3
12*
6%
0.3s
1.5s
12V = r*
-
4
16
8%
0.4s
2s
0V = r
-
5
20
10%
0.5s
2.5s*
12V = r*
-
6
24
12%
0.6s
3s
0V = r
-
7
28
14%
0.7s
3.5s
12V = r*
-
8
32
17%
0.8s
4s
0V = r
-
9
36
20%
0.9s
4.5s
12V = r*
-
Note: an asterisk (*) denotes the default value.
lower if this tendency is not apparent
and then adjusted back the other way
until the effect disappears.
In practice, you can adjust the
hysteresis over a range from 2-20%.
The lower the value the better, since
this gives the greatest range of
ignition pulses that are counted for
each gear.
The third parameter is the delay
between gear changes. Without this
delay, the display could show the
incorrect number since the engine
RPM can vary widely when changing
gears.
The initial setting for this is 0.2s
which should be suitable for most
cars. However, depending on the
driver, the 0.1s setting may be better for cars with manual gearboxes.
Conversely, a longer delay may
be needed for cars with automatic
transmissions.
You can set the delay to any value
between 0.1s and 0.9s.
The fourth parameter is the timeout
connection point. Be sure to choose the
fused side of the supply rail, so that
the existing fuse is in series.
You should also be able to access
the reversing switch connection at
the fusebox. The ground connection
can be made by connecting the lead to
the chassis using a solder eyelet and
self-tapping screw.
Fig.6 shows the mounting details for
the speed sensor. Note that the four
magnets must all be installed with
the same pole facing outwards – ie,
they must all have either their north
pole facing outwards or their south
pole facing outwards (it doesn’t matter
which).
This is done by attaching the magnets together in a stack. This will
either give an N-S-N-S, etc stack or
an S-N-S-N, etc stack. You then mark
the outside face of the top magnet and
remove it from the stack, then mark
the next magnet and remove it and so
on until all the magnets are separate.
The magnets can then be attached to
the driveshaft with the marked faces
on the outside.
The magnets should be equally
spaced around the driveshaft and can
be affixed using builder’s adhesive (eg,
Liquid Nails, Max Bond, etc). Covering
the magnets with some neutral cure
silicone sealant will protect them from
damage due to stones and other debris
thrown up by the wheels.
Mounting the pickup coil
The pickup coil can be secured by
bolting it to an L-shaped bracket which
is then fastened to the chassis. Position
it so that there is about a 10mm maximum gap between it and the magnets
as they pass.
Alternatively, you can use a Hall
sensor instead of the pickup coil, as
shown in Fig.7.
The ignition coil input is connected
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period. Normally, the ignition pulses
are counted during a set number of
speed pulses. However, if the vehicle
is moving very slowly or is stopped,
the speed pulses may not reach the
count setting. Instead, the timeout
stops the count and places a neutral
(-) reading on the display.
The timeout parameter is initially
set at 2.5s but can be set anywhere
in the range from 0.5-4.5s, using
numbers from 1-9. Its setting is a
compromise between showing neutral only when stopped or at a very
low speed (long timeout) and getting
a fast neutral indication after coming
to a stop (short timeout).
The next parameter is the reversing
switch sense. Setting an odd number
between 1 and 9 (1, 3, 5, 7 or 9) will
cause the display to show reverse
when the reverse input goes to +12V.
Conversely, setting an even number
(2, 4, 6 or 8) will cause reverse to
show when the reverse input goes
to 0V.
This selection is simply made so
that the unit shows reverse (“r”) when
the reversing lights come on.
The final parameter is “clear”,
which clears all the gear calibration
values. The gear ranges will then
need to be recalibrated. This “clear”
operation should be carried out if the
unit is fitted into another vehicle.
directly to the switched (negative) side
of the ignition coil using a 250VAC
rated cable.
Using computer signals
As mentioned earlier, instead of
making you own speed sensor, you
may be able to obtain the speed signal
from the engine management computer. This signal is simply fed to the 1kΩ
resistor at the speed input.
If the car’s speedometer stops
operating after connecting the Gear
Indicator, increase the 1kΩ resistor on
the speed input to 10kΩ and remove
the 10nF capacitor.
Similarly, you can use the low-voltage tachometer signal from the computer instead of ignition coil pulses
if this is available. In fact, it will be
necessary to do this if your car uses
several double-ended coils to fire the
spark plugs, rather than a single coil.
The low-voltage tachometer signal
siliconchip.com.au
Setting The Parameters
The various parameters are set by
first pressing (and holding down) the
Mode switch while the Gear Indicator
is powered up. The display decimal
point then lights to indicate that the
unit is in the “setting mode”.
The first parameter shown is an
“S” which refers to the speed pulses.
If the Mode switch is then released,
the display will show the value stored
(from 1-9) after 1s. Conversely, if the
Mode switch is held down, the other
parameter indicators will appear in
succession, at a 1s rate.
The parameter values are altered
by pressing the Number switch. Each
press increments the number by one,
while holding the Number button
down causes the value to automatically increase at a 1s rate – ie, the
numbers cycle from 1-9 and then
back to 1 again. When the required
value is selected, you simply release
the Number switch and press the
Store switch to store the value in
memory.
Once the “S” (speed) parameter
has been set, the other parameters
are selected and set in turn. These
are “H” (hystere
sis; “d” (delay); “-”
(timeout) and “r” (reverse). These
are all modified and stored exactly
as before.
Note that no changes are stored
until the Store switch is pressed.
This enables you to cycle through
the parameters to check their values
without making any changes.
The last parameter to be selected
simply shows a “C” on the display,
without any value. Pressing Store will
clear all the gear settings.
Finally, you exit from the Param
eter Mode, by switching off and then
reapplying power. The display will
then show a “-” (ie, the neutral gear
indication) and the decimal point will
be off.
Gear Calibration
Pressing the Mode switch after
the unit has powered up places the
unit into the “Calibrate Mode”. The
decimal point will light to indicate this
mode and the number shown initially
will be a “1” (ie, 1st gear).
To calibrate the unit, just follow
these step-by-step instructions:
(1) Drive the vehicle at light
throttle with 1st gear selected (for
automatics, you have to select 1st
gear rather than Drive). After a few
seconds, press the Store button and
the calibration for 1st gear is saved.
Note that it may be necessary
to drive relatively fast in 1st gear to
ensure that the speed pulses are
counted within the timeout period.
Also, with an automatic, be sure to
drive along a flat section of road without accelerating to eliminate torque
converter slip.
(2) Next, press the Number button
so that the unit shows a “2” (ie, 2nd
gear). Now drive at light throttle in
2nd gear for a few seconds and
press the Store switch to calibrate
the 2nd gear.
Note that it is not necessary to
drive at a fast speed in this gear to
achieve calibration. If the car is an
automatic, be sure to select 2nd gear
and drive fast enough to ensure that
the car is in this gear (ie, not 1st).
The remaining gears are calibrated
in exactly the same manner.
(3) Once you have calibrated all the
gears, press the Mode switch again
and the decimal point will extinguish.
The unit will now revert to the “Gear
Indicator” mode.
If you make a mistake during
cal-ibration, or if the unit is to be used
in a different vehicle, the data should
be cleared using the “C” parameter
before re-calibrating the unit.
Note too that if you subsequently
change the speed pulses parameter
after calibration, the gears will need
to be recalibrated. Also, if you don’t
obtain a successful 1st gear calibra
tion, this gear can be recalibrated
after extending the timeout delay. In
that case, the Store button should
be pressed after about 10 seconds
to ensure a suitable count for the
ignition pulses.
Note that some automatics start in
2nd gear rather than 1st when light
throttle settings are used.
January 2003 43
Fig.8: this full-size artwork can be used as a drilling
template for the front panel. You will need to make
cutouts for the LDR and the 2-segment LED display.
Fig.9 (right): check your etched PC boards
against these full-size patterns before any
of installing the parts. The smallest board
(ie, 05101033) is for the optional Hall speed
sensor.
The corners of the two PC boards must be cut away to clear the mounting pillars
inside the case. This should be done before any parts are installed.
should be applied to the low input
terminal on the Gear Indicator (not to
the ignition coil terminal).
On-road testing
Once fitted to the vehicle, the various parameters can be set and the
unit calibrated as described in the
44 Silicon Chip
accompanying panels.
The speed pulses setting for the parameters can be made a larger value as
described earlier. This will give more
ignition pulses to be counted and give
a better resolution for the differences
in counts for each gear ratio.
The larger value will also provide
less tendency to show a lower gear due
to clutch or torque converter slippage.
The compromise is that the time
required to count the pulses will be
longer and the display will have a
tendency to show the neutral (-) indication at a higher speed compared to
using a smaller speed pulses number.
This is because the timeout period will
occur before the pulses are counted at
slower speeds.
Gear change response will also be
slower with a higher speed pulse count
number.
In general, use 16 or more speed
pulses if you use four magnets on the
tailshaft and use 12 or less if you use
magnets on the wheel shaft. Use of
the speedometer sensor signal should
require 28 or more speed pulses but
this may need to be smaller if the
response at slow speeds is too long,
causing neutral indication at not so
slow speeds.
Note also that using magnets and
a coil pickup will not provide gear
indication at very slow speeds since
the output from the sensor will be too
low to register. The Hall effect pickup
will be much better at slow speeds and
will provide gear indication down to
where the speed pulse count takes
SC
longer than the timeout.
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SERVICEMAN'S LOG
When the going gets tough
When the going gets tough, the tough get going
or so the old saying goes. But in my case, when
the going gets tough, I compromise, by taking on
unusual service jobs – like a couple of 20-year
old reel-to-reel tape recorders and a Sony set
intended for South Africa.
There are times when I swear blind
that I will never touch any equipment
that’s over 10 years old again. That’s
because of all the warranty implications when something else inevitably
fails and because you often cannot
get a critical part or it is prohibitively
expensive.
www.siliconchip.com.au
But then I reach a quiet business
patch and in a panic I accept not one
but two 20-year old units for repair.
Yes, I regret to say that muggins was
guilty of this when two unrelated people brought in Sony TC-366 reel-to-reel
tape recorders.
These Sony TC-366s are nicely built
3-speed machines. They have one
motor, their fastest speed being 7.5ips
(inches per second), and all the tape
action is controlled via a large single
knob. In both instances, the symptoms
were no or little play torque but each
fault was different.
Removing the covers involved unscrewing five Philips screws, undoing
two special poles which also hold the
head cover, and removing the Pause/
Instant Stop switch knob. This round
knob is about 1mm larger that the
slot it is meant to go through when
removing the tape deck escutcheon.
It is screwed onto its shaft and one
has to manually unscrew it in order
to release the escutcheon from the
machine.
Unfortunately, some 20 years later,
this knob refused to unscrew, so I had
to gingerly widen the slot with a round
file. I really don’t know why they
couldn’t have made it pass through
when it was manufactured!
When I could finally see inside
the mechanism, it was obvious that
the large play idler wasn’t moving to
engage the motor and capstan shafts.
Lubricating the bearings of the associated levers solved this problem on
one of the machines.
The second was more complicated.
The motor wasn’t rotating at all until
I gave it a little nudge. But although I
could get it going, it didn’t have much
get up and go about it. In fact, it kept
slipping, especially in fast forward,
and was also getting very hot.
As a matter of interest, this particular machine had been imported
from the USA and was connected
to our 240V mains by a stepdown
transformer. The machine was rated
at 117V 60Hz and the AC motor at
100V 50/60Hz.
The 1.5µF starter capacitor (PN 117034) looked to be the main culprit. As
luck would have it, when I rummaged
through an old box of capacitors I
found not one but two original re
placements still sealed in plastic bags.
The only difference was that they had
an additional 0.5µF terminal on them
as well (PN 117-036).
This fixed the problem immediately
but not being a rocket scientist when
it comes to AC motors, I wasn’t really sure whether to simply connect
the 1.5µF section of the replacement
capacitor or connect the 1.5µF and
0.5µF sections together to make 2µF
January 2003 53
for 50Hz (as opposed to 1.5µF for
60Hz).
Well, I initially left it at 1.5µF and
put the machine on soak test. Three
hours later, I revisited it and was horrified to find that the motor was nearly
too hot to touch and had stopped. The
replacement capacitor had failed and
I had only one left.
This time I connected the two sections in parallel, lubricated the motor
and soak tested it again. Fortunately,
this one held and, hopefully, will continue to do so. If not, it means ordering
in a very expensive industrial one.
Anyway, I finished up with two satisfied customers, so my gamble with
these 20-year old machines paid off.
An interesting Sony
An interesting TV set came in
the other day. It was a 1990 Sony
KV-2184SA (GP-1A). So what is interesting about that? Well, the “SA”
designation in the model number
(rather than AS) indicated that it was
from South Africa. In addition, it had
a built-in FM radio on the lefthand
side of the cabinet for simulcast
transmissions.
This surprised me because I thought
the whole purpose of simulcast transmissions was to receive stereo and
yet this was fed into the monaural
TV sound system and only one small
elliptical loudspeaker. So I really can’t
quite see the point; perhaps some expat can enlighten me, as there is no
instruction book or service manual
54 Silicon Chip
available for this model in Australia.
The set was dead, with an IC
link fuse (PS801) open circuit. This
led me on a merry dance as I was
using my old service manual for a
KV-2184AS and there was an extra
transistor circuit (Q622) that wasn’t
marked. This supposedly monitors
the current through R621 and turns
off the horizontal drive from pin 27
of the jungle IC (IC301, CXA-12135)
by biasing pin 22.
First, I found the D608 R2M safety
zener to be short circuit, which implied the 115V rail had risen high
enough to destroy it. So I replaced
this, along with IC601 (STR50115,
B version). I then found that R621
(1Ω) had gone high, as well as R622
(470kΩ).
I was getting closer but the set gave
a high-pitched squeal when I switched
it on and the 115V rail was at 87V. Yet
when connected via a 100W globe,
with a clip lead between base and
emitter of the horizontal output tran-
Items Covered This Month
•
•
•
•
•
Sony TC-366 reel-to-reel tape
recorders.
Sony KV-2184SA (GP-1A) TV
set.
AWA 65850 S/T TV set.
Grundig ST70-755 TOP/LOG
TV set (CUC 6360 chassis).
AWA C5105 TV set.
sistor, the voltage was spot on at 115V
and there was no squealing.
When I re-enabled the horizontal
output stage, I could get sound and a
white raster. And when I subsequently
replaced R851 1.2Ω (200V supply to
the CRT), I could get a coloured picture, albeit small and distorted due to
the low HT.
From this, I deduced that the horizontal output stage might possibly
be drawing too much current. But it
wasn’t and it took a very long time to
work out that R609, a 33Ω 3W resistor,
was open circuit in the power supply
and that this was part of a feedback
circuit to pin 2 of IC601.
By now, I had a good picture and
sound when I connected a video recorder to the AV inputs. However, that
wasn’t the case off air.
The reason for that wasn’t hard
to figure out. South Africa uses the
CCIR system with a 6MHz sound IF
and with no Band I VHF (V-L). This
meant removing the IF module IF201
(IFB-389SA) and replacing the three
6MHz ceramic filters with 5.5MHz
units (CF01 for D5.5E, CF02 5FE5.5MB
and CF03 T5.5B). The set now gave
good sound and colour for all stations
except for the ABC (Ch2, Band I).
Now all that was left to be done was
to fit the extra band switching transistor (Q151, DTA114ES) – along with
6.8V zener D152 and C150 (1µF 25V)
– and link it to pin 7 of microprocessor
IC002 via a 2.2kΩ resistor (R098). I did
all this but it still didn’t work. The tranwww.siliconchip.com.au
sistor would still only scan high-band
VHF (ie, no Band I) and UHF.
Initially, I thought this was
due to the microprocessor being
a PCA84
C 640P/037 instead of
PCA84C640P/016 as in the cir
cuit
diagram. However, this was just a
red herring as I discovered that the
Australian module also used the same
“037” suffix and worked OK.
What I did discover was an extra
diode (D005) fitted in the South African model that connected pin 22 to
the vertical pulse going to Q005 from
the vertical output stage. Removing
this diode breaks the TV scan mode
into VL, VH and U and the set could
now be tuned like an Australian TV
receiver.
Obviously, the easiest way to solve
the above problem would have been
to fit an Australian tuner and an the
IF module as well (as they would be
better matched). However, I hadn’t
scrapped any of these sets lately, so I
couldn’t scrounge the necessary parts
and fitting new units would not have
been cost-effective.
Finally, to select the simulcast FM
radio, it is necessary to rotate the system switch inside the front control
panel and then tune the knob on the
side. The tuner is connected via CN302
and CN201 to the de-emphasis pin
(pin 10) on the IF module and pin 7
of analog switch IC702.
AWA TV set
AWA is now used as a brand name
on a series of TV sets imported from
China. These sets are very similar to
those of Teac, Akai and Masuda, and
are probably produced by the same
ONWA factory.
www.siliconchip.com.au
In fact, the 1993 66cm AWA 6850ST
on my bench could easily have been
mistaken for a Teac CT-M711 or a
Masuda 28AV. And it was completely
dead.
After removing what seemed like an
unnecessary quantity of screws, the set
was seen to consist of a motherboard,
a Teletext board, a stereo decoder and
a power supply. And a quick examina
tion soon revealed that two capacitors
in the power supply had spilled their
guts.
I replaced the two culprits – namely
C910 47µF 25V and C908 10µF 50V
– before replacing the parts they had
destroyed: Q909 (2SD1403), R944
(2.2Ω, 5W), C925 (1000µF, 25V), R916
(0.68Ω, 1W) and C925 (22µF, 160V).
Judging by the soldering, I wasn’t
alone in going down this path. I also
checked the HT voltage and set it to
143V at TP B+.
Intermittent flicker
The next problem was the picture
which was intermittently flickering
horizontally with colour problems.
Sometimes the picture would tear
and sometimes it would shift horizontally. It’s not only a horrible fault
to describe but was equally hard to
diagnose and fix. And it was somehow
temperature related, the set getting
better when hot.
By trial and error, I discovered
that the fault seemed to be located
around IC102 (TDA8305A). This is
predominantly an IF detector processor but also a jungle IC and is located
underneath the stereo decoder board
in a soldered-in metal cage. There
was a lot of black silicone rubber all
over this set which, like the brown
PCB POWER
TRANSFORMERS
1VA to 25VA
Manufactured in Australia
Harbuch Electronics Pty Ltd
9/40 Leighton Pl. HORNSBY 2077
Ph (02) 9476-5854 Fx (02) 9476-3231
glue before it, tends to conduct after
many years.
Well, I had to start somewhere so I
scraped off the black silicone rubber
and replaced the IC. This didn’t work,
so I started replacing the capacitors.
Fortunately, I struck gold with C127
(3.3µF), which is a decoupling capacitor for the AGC detector and sync
demodulator.
At this time, I didn’t have a remote
control but fortunately I had a Remote
Master RM0900 Universal remote
control and tuned that into this set’s
command set. This was a good idea,
as I found then that the remote control
power on/standby function wasn’t
switching off.
This set used a relay for switching
the 143V on and off to the rest of the
set, so it was just a matter of tracing
it back to the microprocessor. How-
January 2003 55
Serviceman’s Log – continued
ever, the fault turned out to be a lazy
momentary contact on the main on/
off switch (S512) that was sticking in
the on position. A little lubrication
soon fixed that and the set was back
in operation.
Grundig day
I don’t see many Grundig TV sets
these days, probably due to the dealer
network set up by Grundig in recent
years. I normally try to avoid house
calls but when Fred Schmidt called
and gave me his address as being
only a block away, I bent the rules
and arranged to “have a look” at his
10-year old Grundig ST70-755 TOP/
LOG (CUC 6360 chassis). The fault
complained of was intermit
tent no
picture and it was the “intermittent”
bit that worried me.
When I arrived, the set gave no
picture but a green raster with retrace
lines. After it had been on for sometime, the picture flashed on.
56 Silicon Chip
I removed the back – there were
only four screws to undo (other manufacturers please note) – and checked
for faulty joints or anything obvious.
The only thing I learnt was that by
varying the CRT screen control
SG/VG2 clockwise to give a very
bright green raster and then
slowly reversing it anticlockwise, the picture would return.
However, it was too bright and
too green and turning the brightness control down on the remote
control still couldn’t make the
blacks black.
Basically, if the screen control is turned too far anti
clockwise, the picture loses
definition and gives poor
colour contrast.
This looked to me like
the RGB video output stage
was producing signals that
were outside the optimal
characteristic curve sections
of the CRT guns. I told Fred that
it had to go to the workshop
and though it was a fine
TV set, perhaps he ought to
think about updating it considering its age. However,
being rather short of cash, he
decided to have the set fixed
rather than dumped.
Back on the workshop bench, I
first replaced the RGB video output
IC (IC790, TEA5101A/D), which is a
very complex FET amplifier. Initially,
I fitted a generic IC from my local supplier but later, when I became more
desperate, and at Grundig’s sugges
tion, I ordered and fitted a genuine
replacement but it made no difference
either way.
This type of circuit is used in a lot
of European-designed sets like Philips
and the fault can quite often be caused
by a low-emission tube. To prove this
one way or another, I decided to test
the Philips A66 EAK71X01 picture
tube thoroughly. First, I connected
my CRT analyser directly to the tube
and, at 6.3V RMS, I measured an even
0.62mA emission from each gun,
which is reasonably good.
Next, I measured the voltage across
the CRT filaments with my RMS voltmeter and that too was spot on at 6.3V.
Finally, I connected an external power
supply to the heaters and wound it up
to 8V to see if it made any difference
but it didn’t.
I now concentrated on the diodes
and electrolytic capacitors on the CRT
module (29305-022.48). Note that this
differs from the one in the service
manual (29305-022.44) – it has four
more diodes fitted, as well as other
modifications.
I tried replacing all the 1N4148 diodes with higher-rated BAV21 (used
mostly as clamps) but that didn’t help.
I also measured all the voltages around
the CRT socket but of course, the voltage for each colour was not consistent
and besides, the service manual does
not give voltages.
The thing I did notice was that the
voltage drive for each colour from the
colour decoder module was 4V for
red and blue and 5V for green. I also
measured the beam limiting SB voltage
from the horizontal output transformer
(A) on pin 1 of the module to be 16V
and the SW voltage on the CRT RGB
pin 1 plug to be 0.63V in the fault
condition. I should also add that it
was not possible to set up the screen
control according to the alignment instructions, as the picture would be far
too bright (in AV mode, there should
be 172.5V on each cathode). The EHT
was spot on.
Colour module
All this was very time consuming
and all I had really achieved was
to confirm that the CRT and socket
were probably OK. So now I shifted
my attention to the colour module
– 29504-105.67 – which also differs
from the 29504-105.56 module in the
service manual.
The other drama with this double-sided module concerned the access to its surface-mount components.
About all I could measure were the
voltage supplies (12V, 8V) and the
inputs and outputs. Fortunately, the
service manual gave a pretty good
explanation of the circuit.
The circuits I was interested in
were mostly in IC5040 (TDA8376)
and the 10 surface-mount transistors
after it. I pulled the module out and
using an ohmmeter, checked all the
transistors to be OK. I then replaced
all the electros and measured all
the diodes. An exchange module (if
available) would cost $227.25 trade
and the TDA8376 $119.70 plus freight
charges of $11.
www.siliconchip.com.au
I gambled on the latter and ordered
it. A few days later, after replacing
this 52-pin high-density IC, I discovered I had lost and blown all my
money!
So far I wasn’t doing very well. If
only I had had another set to compare
it with. As I had the necessary ICs in
stock, I replaced all the other ICs on
the Chroma Module but even that was
a waste of time.
Finally, I decided to replace the
surface mounted transistors, starting
with CT5127 (Red), CT5128 (Blue)
and CT5129 (Green) – all BC858s.
Naturally, with my luck, these are no
longer available, so I fitted BC858Cs.
This fixed one problem – the green
caste was gone and the grey scale was
correct even if it was too bright.
I surfed the net and found one German site for TV and Video Service
Repair Tips that had to be translated,
suggesting I replace CT5066, another
BC858. This I did and I noticed a
small improvement. Thus encouraged,
I moved along and replaced CT5060
as well. This finally produced an
acceptable picture after realignment.
These transistors are part of the beam
limiting current circuit to pin 22 of
IC5040 (3-4V).
I couldn’t fault any of the PNP
transistors I replaced but because of
their size and position, it was almost
impossible to hook up complicated
test gear to test them. I have even had
cases where the glue used to cement
these components onto the board affected their characteristics.
Anyway, the picture was now quite
acceptable but will Fred go ahead with
my quote? How could I possibly guess
at the likely cost beforehand?
And to finish off, here is another
reader contribution. It is from A. B.
of Glen Waverley, Victoria. He has
titled it:
The perils of modern test gear
Mr Smith staggered up the path
clutching an AWA C5105 TV set,
moaning “I couldn’t find the place”.
I resisted the temptation to ask if he
had seen the sign out the front but in
this game you soon learn that the customer has a good reason for whatever
they say.
“Its dead, just stopped – is it the
picture tube?” he puffed on. After
reassuring him it was unlikely, I
booked it in and shoved it onto the
“look at” pile.
www.siliconchip.com.au
I got to it a few days later. It
was a 51cm AWA set of Chinese
manufacture and only about 18
months old. The first thing you
do in these sets is go straight for
the power supply, in this case
the electrolytic capacitors in
the primary circuit (C614
and C615). Both measured
faulty on the ESR meter and
were promptly replaced. As
well, the EHT circuit was
checked for shorts and a DC
resistance measurement to
chassis showed no obvious
faults.
The set was then powered
up and I fully expected it to
burst into life. Alas, it was
not to be – the red standby
LED was on but no amount
of prodding at the usual user
controls made any difference.
At this point, you start to wonder if
the remote control is needed to start
the set – most modern TV sets are
switched on by firing a start-up pulse
from the remote using the on/off button or a channel button. I worked on
this assumption and turned the chassis
upside down on the workbench to access the underside of the board.
It was soon established that the HT
rail was at 110V – a figure I assumed
to be OK on a set this size. After
diligently studying the circuit, a 5V
regulator and an 8V regulator were
also found to be functioning. As
well, there was HT on the collector
of the horizontal output transistor
and about 85V on the collector of the
driver transistor.
However, a quick check with the
CRO revealed that there was no drive
waveform to the base of the driver
transistor. Unfortunately, the relevant
track soon disappeared into a mess
of similar tracks wandering all over
the board.
At this point, it was decided to obtain a circuit diagram. Unfortunately,
when this turned up, it proved to be a
15th generation copy (or thereabouts),
plus a booklet full of useless (in a
practical sense) information on how
to do alignments, etc.
The circuit was of limited help as all
the figures were unreadable. However,
I did manage to locate the jungle IC
and I checked that this had supply
volts. I also discovered that there was
no horizontal drive waveform on the
relevant output pin.
So what was going on? All the routine tests had been done to no avail.
After staring at the board, I decided to
measure all the high-wattage low-value resistors. All checked OK (or as near
as could be judged given the useless
circuit diagram) with the exception of
R320, the dropping resistor to the horizontal driver circuit - it was reading
about 6MΩ! However, the HT on the
transistor measured OK at 85V!
Suddenly the penny dropped, and
I mentally kicked myself around the
workshop. I pulled the resistor out
and replaced it with a 2.7kΩ 5W unit,
switched on the power and the set
came to life.
What happened?
So what had happened – easy, and
if I had remembered basic theory I
would have found it a lot quicker.
What happened was this – at switch
on, the start-up pulse gives enough
energy to kick the set into life and all
is well. In this case, because the set
wasn’t running, my high impedance
digital multimeter was indeed reading
a nearly correct voltage across the driver transistor because the thing was still
stuck in standby mode, the transistor
not drawing any current.
By contrast, an old, cheap analog
meter with its higher loading would
have shown a lower voltage at this
point and the true fault would have
been revealed at once!
Ah well, that’s the problem with
getting older – what was once routine
is now new if you haven’t seen it for
SC
awhile.
January 2003 57
This stereo 3-way active crossover is for those enthusiasts who
want the very best from their 3-way loudspeaker systems. It
avoids the disadvantages of passive crossover networks and
allows the power levels to the speakers to be optimised.
W
hat is an active crossover
and why would you want
one?
Most hifi enthusiasts are aware that
2-way and 3-way loudspeaker systems
contain passive networks to split
up the audio spectrum into two
frequency bands in the case of
2-way systems and three bands in
the case of 3-way systems.
Passive crossover networks use
inductors, capacitors and resistors
to split the audio into the various
bands and set the signal levels to
the various speaker drivers.
For example, the woofer is often
less sensitive than the midrange
driver and tweeter and so the signals
58 Silicon Chip
to the latter drivers have to be reduced
so that the overall output from the
three drivers is equal.
In the higher performance speakers,
the crossover networks are often very
complex and they can be very difficult to design and optimise. And because they usually do attenuate
the midrange and high signals,
that means they do waste ames
ur
at
Fe
plifier power.
1-unit rack case
They also interpose a com Single PC board
plex
network between the
r
transforme
speakers and the amplifier
15V+15V 20VA toroidal
which means a loss of damping
Stereo module
stages
t
tpu
ou
d
factor, particularly for the lowan
ut
inp
Buffered
impots)
(tr
ts
er frequencies where it is most
tpu
ou
ble
ria
va
Individually
needed, if you are to achieve
ly
pp
su
r
On-board powe
tight, clean bass and midrange
tors
On-board RCA connec onents
reproduction.
mp
OK, so that’s the passive ap Made from standard co
proach. It involves just one stewww.siliconchip.com.au
An active
3-way
crossover
for
loudspeaker
systems
Design by Mick Gergos
reo amplifier to drive the two speaker
boxes in a stereo system.
In an “active” system, we eliminate the passive crossover networks
and electronically split each of left
and right channel signals into three
frequency bands: low, midrange and
high. This is the job of the “active
crossover”.
Its output signals are fed to six (yep,
six) separate amplifiers to drive the
woofer, midrange and tweeter units
in each loudspeaker enclosure. The
overall system layout is shown in the
block diagram of Fig.1.
So you end up with a lot more amplifiers than in a conventional system
but it gives you a lot more flexibility.
And ultimately, you can end up with
a system with higher performance,
including much higher power levels.
This shot inside the box reveals the simplicity of construction. Everything except the transformer is on one PC board!
www.siliconchip.com.au
January 2003 59
Fig.1: the block diagram shows the overall system
layout. It replaces the crossover currently in the
speaker enclosure.
The active crossover approach also
means you can mix 4Ω and 8Ω drivers in the same system and match the
levels easily, without power wastage.
Active crossover
The Active Crossover presented
here is housed in a 1-unit high rack
case with just the power switch on
the front panel.
There are no user controls for the
crossover; no switches to alter the
crossover frequencies nor external
level controls for the output signals.
To alter the drive to the loudspeakers,
you will need to adjust the volume
controls of the driver amplifiers.
On the rear panel there are four pairs
of RCA sockets, one pair for the stereo
input signals while the other three are
for the stereo low (woofer), midrange
and high (tweeter) signals.
Also on the rear panel is the IEC
mains power socket and a fuseholder
for the primary circuit of the power
transformer.
Inside the case, all the circuitry is
on a PC board measuring 219 x 99mm
and this includes the dual RCA input
and output sockets. The only external
wiring to the board are the secondary
connections to the toroidal power
transformer.
Circuit description
Now let’s have a look at the circuit
of Fig.2. Since both channels are identical, this shows only the left channel.
While the power supply is also on the
PC board, it is shown in Fig.3.
In total, the left channel uses 12 op
amps, in three TL074 quad FET-input
op amp packages.
Four op amps, IC1a, IC1b, IC5a &
IC5b, act as input or output buffers
while the remaining eight op amps
are Linkwitz-Riley active filter stages
with 12dB/octave filter slopes.
In each case, two 12dB/octave filters
are cascaded to give an overall filter
slope of 24dB/octave. This is far steeper than is normally used in passive
crossover networks.
The voltage gain of all these filter
stages in the passband is unity.
Low pass, high pass
Before we go any further we should
explain some terms which often confuse beginners: low pass, high pass
and bandpass.
A low pass filter is one that allows
low frequencies to pass through and it
blocks the higher frequencies. Hence,
a circuit to drive a subwoofer would
be called a low pass filter since it only
delivers frequencies below 200Hz or
thereabouts.
Similarly, a high pass filter is one
that allows high frequencies to pass
through and it blocks low frequencies.
Hence, the part of a crossover network
which feeds a tweeter is said to be a
high pass filter, even though it may
consist of only one capacitor.
If we cascade (ie, connect in series)
a high pass filter with a low pass filter,
the combination will pass a band of
Specifications
Voltage gain: Unity
Frequency response
Within ±1dB from 10Hz to 20kHz (see Fig.5)
Filter attenuation slope 24dB/octave
Total harmonic distortion
Typically .003% at 1V RMS
Signal to noise ratio
-94dB unweighted (22Hz to 22kHz) with respect to 1V RMS
Separation between channels Typically better than -100dB from 10Hz to 20kHz
Input impedance 47kΩ
Output impedance
60 Silicon Chip
less than 200Ω
www.siliconchip.com.au
www.siliconchip.com.au
January 2003 61
Fig.2: just 12 op amps and a few other components make up each channel of the active crossover. The six
outputs (three only shown here; three more in the right channel) each drive separate power amplifiers for the
tweeter, midrange and bass drivers in your loudspeakers.
Fig.3: the power supply is entirely conventional, using positive and negative 15V regulators to give ±15V rails. Everything
from the bridge on is mounted on the PC board. The seven 100nF capacitors are bypasses distributed around the PC board.
frequencies and we then refer to it as
a bandpass filter. We use a band-pass
filter for the midrange output in this
active crossover circuit.
The other points you need to know
about high and low pass filters are the
so-called cut-off frequency and the
filter slope.
The filters used in this circuit have
an attenuation of 12dB/octave; this
is the filter slope and it applies for
frequencies after the cut-off frequency.
The cut-off frequency is where the
signal output is -3dB down on the
normal level.
For example, in a low pass filter we
might have a cut-off frequency of 1kHz
(ie, -3dB point) and from there on the
filter slope could be 12dB/octave. In
theory, this means that the response at
2kHz (ie, one octave above 1kHz) will
be -15dB although in practice it might
not be quite that good.
The filters used in our circuit are
of the Linkwitz-Riley configuration
and we use eight of these filters, four
high pass and four low pass, in each
channel. Each filter consists of an op
amp connected as a voltage follower,
preceded by two RC networks.
As already noted, for each high pass
and low pass filter we are using two
12dB/octave filters cascaded, to make
the total roll off 24dB/octave (4th order) per filter stage.
The basic filter configurations are
shown in Fig.4, together with the
formula for calculating the crossover
frequency. In this particular case, the
crossover frequency is at the -6dB
point and the reason for this is that
we are cascading two filters for each
section (2 x 3dB = 6dB).
Note that the capacitors in the low
pass filter are shown with values of C
and 2C while in the high filter we have
resistors with values of R and 2R.
In the main circuit of Fig.2 you will
note two capacitors of equal values
have been used for the 2C component,
as it is difficult to obtain capacitor
values exactly double that of another.
On the other hand, resistors are much
easier and so we have values of 10kΩ
for R and 20kΩ for 2R.
Now after that little diversion, let’s
refer back to the circuit of Fig.2.
The input to the left channel is fed
via an RC filter, to roll off frequencies
above 100kHz, and then to op amp
IC1a which is connected as a unity
gain buffer (or voltage follower).
It drives two high pass filter stages
associated with IC1d & IC1c, and two
low pass filters associated with IC3a
& IC3d. Both these low pass and high
pass filters have cutoff frequencies set
to 5.1kHz.
The output of the second high pass
filter, IC1c, is fed to the level setting
trimpot VR1 and then to op amp IC1b
which is connected as a non-inverting
amplifier with a gain of two. It drives
the left treble output (tweeter). Hence
the tweeter only gets frequencies above
5kHz.
Midrange band-pass
Fig.4: the basic arrangements for the low pass and high pass filters.
62 Silicon Chip
The output of low pass filter IC3d
www.siliconchip.com.au
feeds high pass filters based on IC3c &
IC3b, both with cut-off frequencies of
239Hz. The output of high pass filter,
IC3b, is fed to trimpot VR2 and then to
op amp IC5a which has a gain of two.
This drives the left midrange output
which gets the band of frequencies
between 239Hz and 5.1kHz.
As well as driving high pass filters
IC3c & IC3b, op amp IC3d also drives
the cascaded low pass filters based on
IC5d & IC5c, again with a cut-off frequency of 239Hz. IC5c drives trimpot
VR3 and then op amp IC5b which has
a gain of two. It drives the left bass
output which only gets signals below
239Hz.
All the outputs from each stage
are in phase at the crossover points.
Voltage gain at the crossover frequency
for each section is -6dB (ie, half the
reference level).
Thus when the response curves of
all three sections are added together,
the result is an extremely flat frequency response with an overall gain of
unity.
Just how well this works is shown
in the response curves of Fig.5. We’ve
plotted the three filter responses and
then the resultant curve is plotted
along the top. The adder circuit we
used to do this is shown (for interest
only) at the end of this article in Fig.8.
Power supply
The power supply circuit is shown
in Fig.3. It uses a 20VA toroidal power
Parts List – 3-Way Active Crossover
1 1RU rack-mounting case, Altronics H-5011 or equivalent
1 PC board, code 01101031, 219 x 99mm
1 IEC power socket
1 chassis-mount safety fuseholder (3AG or M205 type)
1 0.5A fuse (3AG or M205 type to suit fuseholder)
1 DPST rocker switch with inbuilt neon (S1)
1 20VA toroidal transformer with 2 15V secondaries
1 3-way insulated terminal block
4 dual gold-plated RCA PC-mounting sockets, Altronics P-0212 or
equivalent
6 multi-turn 100kΩ trimpots (VR1-VR6), Altronics R-2382A or equivalent
Semiconductors
6 TL074 quad FET-input op amps (IC-IC6)
1 7815 positive 3-terminal regulator
1 7915 negative 3-terminal regulator
4 1N4004 silicon diodes (D1-D4)
Capacitors
2 1000µF 25V PC electrolytic
2 100µF 25V PC electrolytic
2 1µF 50V bipolar electrolytic
14 100nF (0.1µF) multi-layer ceramic
(code 100n or 104)
20 47nF (.047µF) metallised polyester (code 47n or 473)
20 2.2nF (.0022µF) metallised polyester (code 2n2 or 222)
2 220pF ceramic
Resistors (1% metal film)
2 47kΩ
(yellow violet orange brown or yellow violet black red brown)
8 20kΩ
(red black orange brown or red black black red brown)
38 10kΩ
(brown black orange brown or brown black black red brown)
4 100Ω
(brown black brown brown or brown black black black brown)
transformer with two 15V secondaries
driving a bridge rectifier (diodes D1 D4) and two 1000µF 25V capacitors
to derive unregulated DC supplies
of around ±22V DC. These are fed to
3-terminal regulators REG1 and REG2
to produce supplies of ±15V DC. These
are each bypassed by a 100µF 25V capacitor and seven 100nF multi-layer
ceramic capacitors distributed around
the PC board.
Construction
Fig.5: this graph shows the three filter response curves which were plotted
separately. The overall response curve at top (red) was plotted using the mixer
circuit in Fig.8. The overall response curve is extremely smooth.
www.siliconchip.com.au
As already noted, all the circuitry
is on a single PC board measuring
219 x 99mm, so construction is very
straightforward.
The only complication will occur if
you you wish to set your own crossover frequencies. If so, you will need
to select values from Table 1.
For example, if you decide you
want a tweeter crossover frequency of
around 3kHz, go to Table 1, run your
finger down the righthand column
until you get to 3100 and the R and C
values are in columns 1 & 2.
In practice, the 2.2nF capacitors
in the high- pass and lowpass filters
associated with IC1 and IC3 now have
to be changed to 3.3nF, while the 10kΩ
January 2003 63
Fig.6: the component overlay, as viewed from above the PC board.
Note the polarity of electrolytic capacitors and ICs when soldering
them in!
64 Silicon Chip
resistors increase to 11kΩ and the
20kΩ values go to 22kΩ.
Note that it is essential that both the
high pass filters (ICd & IC1c) for the
tweeter and the low pass filters (IC3a
& IC3d) for the midrange must have
exactly the same cut-off frequencies
otherwise you will not get an overall
flat frequency response.
Similarly, if you want to change the
bass cut-off frequency to around 350Hz
(say), run down the righthand column
of Table 1 to 347Hz. The R values then
become 11kΩ and 22kΩ while the C
values become 27nF.
Alternatively, if you want to do
the calculations yourself, visit www.
sherlab.com/filter/filter.htm for a filter
calculator.
Lots more information regarding
Linkwitz-Riley crossovers can be
found at www.rane.com/note160.html
Here they discuss lobing errors,
driver alignment & phase correction,
phase shift vs frequency etc.
Having decided on your crossover
frequencies, you can start assembly
of the PC board by closely checking
it for shorts between tracks, open
circuits etc, against the pattern
opposite.
Then install all the resistors, followed by the capacitors and multi-turn trimpots. Make sure that the
electrolytic capacitors are installed
the right way around. The bipolar
electro-lytics are not polarised and
can go in either way.
Ideally, 1% capacitors should be
used in all of the filter circuitry. As
an alternative, purchase a bag of 100
capacitors of the value you require
and pick the 20 that are the closest
in value to each other, using a capacitance meter or DMM with capacitance
ranges.
Next, install the two regulators
which are laid flat on the PC board. Be
careful not to swap them over otherwise the circuit definitely won’t work
and you may have to replace quite a
few damaged semiconductors. Finally,
you can install the op amps and the
RCA sockets.
You will then need to wire up the
power transformer, using the diagram
of Fig.7. Temporarily install the PC
board into the chassis and you are
ready for some voltage checks.
Voltage check
Apply power and check the regulated supply rails with your digital
www.siliconchip.com.au
This photo of an early prototype PC board shows the general layout of components. It should be noted that there have
been substantial changes since this photo was taken, particularly along the bottom (rear) of the board. The component
overlay (Fig.6) shows the final version.
multimeter. They should be close to
±15V DC.
Then check that +15V is present at
pin 4 of each TL074 and that -15V is
present at pin 11 of each IC. Lightly
touch each IC to ensure that none of
them are getting hot – they should all
be cool.
The next step is to align the whole
circuit using the trimpots. This is
a simple matter of setting up each
output for unity gain in its passband.
This can be done at three frequencies,
say 100Hz for the bass, 1kHz for the
midrange and 12kHz for the treble.
You will need an audio oscillator
and a digital multimeter with an AC
frequency response to 20kHz or better.
Connect your audio oscillator to the
input RCA connector in one channel.
Set the frequency to 100Hz, 1kHz or
12kHz, depending on which section
you wish to align. Set the level of the
oscillator to 1V RMS.
Then measure the signal level at the
output of the stage that you are adjusting. For the treble output, use 10kHz
and adjust trimpot VR1 (left channel)
or VR4 (right channel) to obtain 1V
RMS at the output socket.
Similarly, for the midrange, use
1kHz and adjust VR2 (left channel) or
VR5 (right channel) to obtain 1V RMS
at the output sockets.
Finally, for the bass, use 100Hz
and adjust VR3 (left channel) or VR6
(right channel) to obtain 1V RMS at
the output. That done, it is now a
matter of finally completing the wiring
inside the case and checking it before
connecting the unit to your amplifiers.
Your amplifiers
We mentioned before that six amplifiers are required; one for each of the
bass, midrange and treble speakers,
times two (for stereo). But what amplifiers should you use?
The completed project showing the rear panel arrangement, power supply wiring and PC board placement. Use this in
conjunction with Fig.7 (opposite) during final assembly.
www.siliconchip.com.au
January 2003 65
Fig.7: follow this wiring
diagram and you should
have no problems with final
assembly. Be especially
careful with the mains
wiring – note the heatshrink
covering all the “bitey” bits!
66 Silicon Chip
www.siliconchip.com.au
amplifier module
featured in this
issue for the midrange and treble.
The Ultra LD
(Nov, Dec 2001,
Jan 2002) or even
the Plastic Power module (April
1996) would make
a superb bass amplifier.
Connection
It is simply a
matter of connecting the stereo outputs from
the 3-Way Active
Cross-over to the
appropriate bass,
Fig.8: here is the adder circuit we used to produce the
mid-range and trediagram shown in Fig.5. You don’t have to make one of
ble stereo amplithese unless you are interested in measuring your own
fier inputs, then
circuit.
connecting the
amplifiers’ outTypically, the woofer amplifier puts direct to the appropriate drivers
needs to be about double the power of
in each of the speaker enclosures.
the midrange and tweeter amplifiers,
Needless to say, the existing crossoto take into account the lower sensi- ver network in the speaker enclosures
tivity of the woofers.
is disconnected completely – and you
So if you have been running a 100W will need to put an extra two sets of
per channel stereo amplifier into your
terminals on the back of your enclo3-way speaker system, you will still
sures with each of the three connected
need two 100W amplifiers for the
directly to a driver (and appropriately
woofers (eg, your exisiting amplifier!) labelled).
but you can get away with two 50W
The tone controls should ideally be
amplifiers for each of the midrange
flat on all amplifiers (although that can
and tweeters (ie, four total).
be a matter of individual taste – but the
You may be able to put back into ser- treble control won’t do much on the
vice an amplifier that you pensioned
bass amplifier nor the bass control on
off as “underpowered”.
the treble amplifier!).
Or, if you want to go the whole hog
Volume controls can be individuand build new amplifiers to go with ally adjusted to get the best balance
your new active crossover, you could
between the bass, midrange and treble
SC
do a lot worse than the new SC480 speakers.
There are no screws holding the PC board in place. Instead it sits on selfadhesive holders (as used in many computers) and the RCA sockets on the back
panel are themselves held in by screws.
www.siliconchip.com.au
Table 1: Values for R & C
R
C
2R
Crossover
Frequency
(kΩ) (nF) (kΩ)
(Hz)
15
47
30
160
15
39
30
192
12
47
24
200
11
47
22
218
15
33
30
227
10
47
20
239
12
39
24
240
11
39
22
262
15
27
30
278
12
33
24
284
10
39
20
289
11
33
22
310
7.5
47
15
319
15
22
30
341
10
33
20
341
12
27
24
347
11
27
22
379
7.5
39
15
385
10
27
20
417
12
22
24
426
7.5
33
15
455
11
22
22
465
10
22
20
512
7.5
27
15
556
7.5
22
15
682
15
4.7
30
1596
15
3.9
30
1924
12
4.7
24
1995
11
4.7
22
2177
15
3.3
30
2274
10
4.7
20
2394
12
3.9
24
2405
11
3.9
22
2623
15
2.7
30
2779
12
3.3
24
2842
10
3.9
20
2886
11
3.3
22
3100
7.5 4.7
15
3193
15
2.2
30
3410
10
3.3
20
3410
12
2.7
24
3473
11
2.7
22
3789
7.5 3.9
15
3848
10
2.7
20
4168
12
2.2
24
4263
7.5 3.3
15
4547
11
2.2
22
4650
10
2.2
20
5115
7.5 2.7
15
5558
7.5 2.2
15
6821
January 2003 67
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
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.
Motor speed control
with protection
This DC motor speed controller
provides compensation for the voltage
drop in the armature circuit. Voltage
drop in the armature circuit is mostly
responsible for the poor low speed
running characteristic of small motors.
This characteristic is most noticeable
at start up and when running at low
speed driving a varying load. Small
motors can have an armature resistance of less than one 1Ω to several
tens of Ohms.
From DC electric motor theory:
Vm = Vb + IaRa
where Vm is the applied voltage; Vb is
the back-EMF generated by the armature, proportional to the speed; Ia is the
current in the armature circuit; and Ra
is the armature resistance.
When a motor is running without a
load, it will draw only a small current
and so IaRa will be small. Conversely,
its speed will be high and so Vb will
be high as well. When the motor is
loaded, it draws more current and so
IaRa will be increased. The speed will
therefore reduce and so will Vb.
For a given motor speed, the applied
motor voltage must be increased to
compensate for the increase in IaRa.
This circuit can perform this task. It
works as follows. The speed setting
control VR1 adjusts the base voltage
of Q1 to set the current flow in resistors R2 & R3. The voltage across R3 is
applied to the base of the compound
transistor comprising Q5 & Q6 and this
drives the motor.
Q2, Q3 and VR2 provide compensation for the armature voltage IaRa. The
motor current flows through Q6 and
its emitter resistor R8 and the resulting
voltage is applied to the emitter of Q3
to be reflected at the emitter of Q2 and
applied to trimpot VR2. Varying the
resistance of VR2 thus changes the
voltage across R8.
This means that the voltage across
R3 has two components, the speed
setting from VR1 and the speed compensation from VR2.
www.siliconchip.com.au
VR2 must be adjusted to provide
the correct amount of compensation
otherwise the motor will surge or stall
whenever a load is applied.
VR3 sets the maximum current, to
protect the speed control circuit or
the motor itself from excessive load.
Before adjusting VR2, make sure the
wiper of VR3 is at 0V. Then adjust VR1
to run the motor slowly, say about 200
RPM. Load the motor by pinching the
motor shaft with your fingers. Now
adjust VR2 so that the motor runs
smoothly without stalling or surging.
Depending on the motor, speeds of 60
RPM under varying load should be
easily achievable.
C1 gives the circuit stability. How-
ever, if your motor and
cable capacitance is large,
surging (instability) may
occur. C1 can be inDunc
creased to compensate. is this man Graham
onth’s
Q6 must have a heatsink. ner of the Wavetwinek
Meterman 85XT
For motors with less
tru
e RMS digital
than 6Ω armature resistmultimeter.
ance, change R8 to 1Ω. If
the armature resistance
is greater than 20Ω,
change R8 to 4.7Ω. A
value of 2.2Ω suits
motors in between.
VR3 is adjusted to limit the
current as desired.
Duncan Graham,
Hamilton, NZ.
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January 2003 71
Circuit Notebook – continued
The circuit uses an IR sensor to pick up the reflected light from two IR LEDs, plus two CMOS 7555 ICs (IC2 & IC3) to
debounce the incoming signal and provide timing. Switch S2 is used to select between toggle on/off operation, timed
operation & “press switch” operation (see text).
Magic wand for
3-way control
This was devised to enable handicapped children who lack manual
dexterity to operate electrical toys.
72 Silicon Chip
No doubt it could have many other
applications.
A wave of the hand or a “magic
wand” over the box can operate the
relay in three ways:
(1) as a toggler – one wave on, next
wave off;
(2) as a timer – one wave turns it on
for a set time;
(3) as a press switch – hold the
wave over the sensor and the relay
stays closed.
The circuit depends on infrared
sensor IC1 which sends a coded
signal through two IR LEDs 1 and 2.
IR light from these LEDs is reflected
by a wand or hand back on to the
sensor and this causes its output at
pin 2 to go low.
This “low” is connected to two
7555 timers (IC2, IC3) and to PNP
transistor Q1 which is used as an
inverter. Selector switch S2 determines which of these three devices
is connected to transistor Q2 which
drives relay RLY1.
IC2 is a short time monostable
to debounce the incoming signal
and toggle IC4, a 4013 flipflop. Its
output at pin 1 goes high and low
on alternate input pulses. This is
option 1.
IC3 is another monostable to give
a relay closed time of about 16 sec
onds. This time can be varied by
changing the associated resistor and
capacitor. This is option 2.
In the third switch position, the
inverted low from Q1 becomes a
high and operates the relay for as
long as the hand is held over the
sensor.
A wave can be quite fast and
about 10cm above the sensor, on
each side of which is one IRLED
– about 13mm away. The sensor is
from RS Components (Cat 564-396)
and the relay is from Jaycar – a 500Ω
reed relay (Cat SY-4030).
The wand must be white and
about 15mm in diameter. A rolled
up sheet of A4 paper works well.
The LED in series with the relay indicates when the relay is
operating.
If your selector switch does not
short circuit the contacts when between positions – ie, it is a “breakbefore-make” type – then you can
omit diodes D4-D6. The IRLEDs
should be mounted in bezels to
prevent leakage of IR light to the
sensor.
The 330nF capacitor is a supply
bypass for IC1 and should be as
close to the sensor as possible. Because the signal is coded, the circuit
is immune to ambient light.
A. J. Lowe,
Bardon, Qld. ($45)
www.siliconchip.com.au
Automatic tape control for display stand
This circuit controls an autoreverse Walkman cassette player,
via the relay in a standard security
light unit (about $20 from Kmart).
These units are unsuitable for connection to inductive loads, so to
overcome this and still maintain
isolation from the AC supply, it is
arranged so that the sensor’s relay
activates a pair of NE2 neons with
integral resistors.
These are encased with an LDR
in heatshrink tubing. The LDR
switches on transistor Q1 which
activates the relay. This in turn
switches the supply to the cassette
player which is left with the Play
button permanently activated. A
second set of relay contacts pro-
vides a 12V supply to an audio
amplifier, fed with the signal from
the Walkman.
The duration of operation is set
by the adjustment provided on the
movement sensor which is also set
for daylight operation. Two LM317
adjustable regulators provide the
+12V and +3V supply rails.
Max Walker,
Blackburn, Vic. ($30)
Filter reduces supply
ripple by 40dB
This circuit reduces noise and ripple voltage by 40dB over the 100Hz to
20kHz audio range. It provides a clean
source of 5V power for driving audio
circuits in portable applications such
as cellular phones and multimedia
notebook computers. Most linear regulators reject noise only up to 1kHz or
so, which can be inadequate in many
applications.
When operating, the circuit acts as
a wide bandwidth buf
fered voltage
follower (not a regulator) whose DC
output level is 7% below the input.
R1 and R3 form a voltage divider that
provides the 7% attenuation while
C4 provides filtering. The op amp’s
small input bias current (25nA typical)
allows large resistor values for R1 and
R3, yet limits the maximum DC error
to only 20mV. The result is a low-pass
filter with a 2Hz corner frequency and
20dB of attenuation at 20Hz.
www.siliconchip.com.au
The physical layout can be very
small: one SOT23 transis
t or, one
µMAX (shrink SO-8) op amp and a
few passive components. The largest
capacitor is 10µF and the resistors can
be 0.1W or surface mount 0805 size.
Because the op amp’s common
mode input range extends from rail
to rail, its non-inverting input can
sample the output voltage directly.
The op amp’s supply voltage is filtered
by R2 and C5, providing lower output
impedance and better power supply
rejection for the op amp at high frequencies. This filter’s 300Hz rolloff
augments the op amp’s PSRR (already
impressive at 110dB).
A similar article appeared in the
January 18, 1996 issue of EDN magazine.
January 2003 73
COMPUTERS: masquerading modules & a firewall
Using Linux to Share
an Optus Cable
Modem Internet Connection
Pt.3: masquerading modules & a firewall
In this article, we show you how to load various modules that
are required for effective Internet access, along with a simple
yet effective firewall. We also tell you what you need to do to
connect a cable modem to Telstra Bigpond Advance instead of
to Optus CableNet.
By JOHN BAGSTER
In order to effectively use your Linux box as a gateway, you need to set the machine up so that it loads
some “masquerading modules” on start-up. In addition,
you need to set up a firewall so everything is secure.
After all, you don’t want someone breaking in and
taking over!
We’ll get to our firewall shortly. Let’s deal with the
masquerading modules first.
The various masquerading modules are required so
that the gateway correctly forwards IP packets for various
Internet utilities on the client machines. Basically, these
modules work with IP masquerading (or IP forwarding)
so that it looks as though everything that’s forwarded to
the Internet is coming from a single machine – ie, the
Linux box.
This is done by translating IP addresses from the local
network into a valid Internet IP number before relaying
the packets out onto the Internet. At the same time,
IP masquerading translates any incoming packets into
local addresses before forwarding them to the client
machines.
It’s all really something of a masquerade because the real
IP addresses of the clients are hidden – hence the name
“IP masquerading”.
IP masquerading (forwarding) is carried out using a
program called “ipchains” and this is also used to create
the firewall rules. Recent versions of Linux also include an
updated replacement for ipchains called iptables (although
74 Silicon Chip
ipchains is still included). The firewall described here
is based on ipchains (since this is used by default with
RedHat 7.0) but both are supported in system startup, so
you could use iptables if you want.
Note, however, that the commands for iptables are differ
ent. The differences are well documented in manual pages
if you wish to convert the firewall to iptables.
Loading modules
In most cases, the firewall rules and the rules to load
the various module are all in one script – ie, the firewall
script. However, in this case, they have been separated
into two scripts so that the firewall can be enabled before
networking is enabled. Note that this not only applies to
a cable modem connection – it is equally applicable to a
dial-up modem.
There are quite a few masquerading modules for Linux,
most of which are optional for audio, instant messaging,
and various games, etc. Basically, you only need to load
the modules that you require. This is roughly similar
to selecting which options you want when you install
Windows.
OK, so how do we ensure that these modules are loaded
at start-up? The answer is that we use a file called rc.local
which RedHat Linux stores in the /etc/rc.d folder. This file
is the last thing executed at start-up and you can add your
own commands to it.
You could put all the module loading commands diwww.siliconchip.com.au
Masquerading script: /etc/rc.d/rc.modules
#!/bin/bash
#
# rc.modules
# rc.modules should be called via rc.local
# Load powerswitch so Linux will shutdown neatly when switched off.
# Only works with ATX power supplies. Uncomment the following line and modify to suit
#
#/sbin/insmod /lib/modules/3rdparty/powerswitch.o
# Load all required IP masquerading modules
# Uncomment the modules you need.
/sbin/depmod -a
# Supports the proper masquerading of FTP file transfers
/sbin/modprobe ip_masq_ftp
# Supports the masquerading of RealAudio over UDP.
# Without this module, RealAudio WILL function but in
# TCP mode. This can cause a reduction in sound quality
#/sbin/modprobe ip_masq_raudio
# Supports the masquerading of IRC DCC file transfers
#/sbin/modprobe ip_masq_irc
# Supports the masquerading of Quake and QuakeWorld.
# This module is for multiple users behind a Linux gateway.
# If you are going to play Quake I, II, and III, use the second one.
# Quake I / QuakeWorld (ports 26000 and 27000) :
#/sbin/modprobe ip_masq_quake
# Quake I/II/III / QuakeWorld (ports 26000, 27000, 27910, 27960) :
#/sbin/modprobe ip_masq_quake 26000,27000,27910,27960
# Supports the masquerading of the CuSeeme video conferencing software
#/sbin/modprobe ip_masq_cuseeme
# Supports the masquerading of the VDO-live video conferencing software
#/sbin/modprobe ip_masq_vdolive
rectly into the rc.local file and that would work without
problems. However, it’s far neater to have the commands
in a separate file and then call this from /etc/rc.d/rc.local (we’ll show you how shortly). We’ve called this
separate file rc.modules and placed it in the /etc/rc.d
folder.
The rc.modules file
OK, let’s take a look at the /etc/rc.d/rc.modules file that
you need to create. You can either download this file from
the SILICON CHIP website or type it in on your Linux box
using a text editor. The file is shown in the accompanying
www.siliconchip.com.au
panel and contains the common masquerading modules
that you might need. However, most of these have been
commented out by placing a “#” at the beginning of their
command lines.
All you have to do is “uncomment” the mod
ules that you need by removing the relevant “#”
symbols.
The various lines in the rc.modules file are all self-explanatory except for the “powerswitch” line. To explain,
Powerswitch is a nifty little utility that shuts down Linux
properly (and switches the PC off) when you press the
power switch on the system case – provided you have an
January 2003 75
COMPUTERS: masquerading modules & a firewall
Firewall rules: the cablefirewall.simple script
#!/bin/bash
#
# cablefirewall.simple
# run this to set up the rules, then run
# /etc/rc.d/init.d/ipchains save
# to save the rules to be used every time the machine is started
# modem interface (change to suit)
MODIF="eth1"
# local network (change to suit)
LOCNET="192.168.0.0/24"
# =============================================================================
# blocking rules for the input, output, forward chains respectively
Iblock="DENY" ; Oblock="REJECT" ; Fblock="DENY"
# Flush all existing rules and remove any user defined chains
/sbin/ipchains -F ; /sbin/ipchains -X
# loopback and local interfaces are OK on input and output
/sbin/ipchains -A input ! -i $MODIF -j ACCEPT
/sbin/ipchains -A output ! -i $MODIF -j ACCEPT
# set policies to block everything
/sbin/ipchains -P input $Iblock
/sbin/ipchains -P forward $Fblock
/sbin/ipchains -P output $Oblock
# masquerading timeouts
/sbin/ipchains -M -S 7200 10 160
# =============================================================================
# input chain:
# block and log modem interface claiming to be local network (IP spoofing)
/sbin/ipchains -A input -i $MODIF -s $LOCNET -l -j $Iblock
# allow return tcp packets (those not requesting a connection)
/sbin/ipchains -A input -p tcp -i $MODIF ! -y -j ACCEPT
# allow incoming tcp ftp-data connections (for outgoing active ftp)
/sbin/ipchains -A input -p tcp —sport ftp-data —dport 1024:65535 -i $MODIF -y -j ACCEPT
# allow all udp and icmp in
/sbin/ipchains -A input -p udp -i $MODIF -j ACCEPT
/sbin/ipchains -A input -p icmp -i $MODIF -j ACCEPT
# uncomment to reject and log anything else (required since policies can’t log)
# the policy is the same so leave this line commented out if you’re not logging
#/sbin/ipchains -A input -l -j $Iblock
# =============================================================================
# output chain:
continued next page . . .
76 Silicon Chip
www.siliconchip.com.au
Cablefirewall.simple – continued
# allow everything except local network traffic out to the modem
/sbin/ipchains -A output -i $MODIF ! -s $LOCNET ! -d $LOCNET -j ACCEPT
# set delay and throughput times if using a dial-up modem (ppp interface)
# these are not to be used if using a network card (cable modem)
if [[ $MODIF == “ppp”* ]]
then
# set minimum delays
for p in www ssh telnet ftp pop3 smtp ; do /sbin/ipchains -A output -p tcp —dport $p -t 0x01 0x10 ; done
# set ftp-data for maximum throughput
/sbin/ipchains -A output -p tcp —dport ftp-data -t 0x01 0x08
fi
# reject and log anything else (required since policies can’t log)
# the policy is the same so comment this line out if you’re not logging
/sbin/ipchains -A output -l -j $Oblock
# =============================================================================
# forward chain:
# Masquerade from local network to anywhere on the modem interface
/sbin/ipchains -A forward -i $MODIF -s $LOCNET -j MASQ
# all other forwarding is blocked and logged
# the policy is the same so comment this line out if you’re not logging
/sbin/ipchains -A forward -l -j $Fblock
ATX power supply, that is.
It’s just the shot if you intend operating your Linux gate
way without a mouse, monitor or keyboard.
The powerswitch module does not come with the Linux
distribution. If you intend to use it, you can download
it from http://deadlock.et.tudelft.nl/~joris/powerswitch/
and install it as described in the instructions (more on
this next month). In this case, the powerswitch.o file was
placed in the /lib/modules/3rdparty folder (you will have
to create this).
#!/bin/sh
#
# This script will be executed *after* all the
# other init scripts.
# You can put your own initialization stuff in here if
# you don’t want to do the full Sys V style init stuff.
Modifying rc.local
Once rc.modules is set up, your Linux gateway is
complete except for a firewall. The one described here
offers good security while not compromising access to
the Internet. It is about as simple as you can get and is
easy to set up.
We’ll look at how the various firewall rules operate
first, then give the firewall script and describe how it
works.
RedHat has a start-up script called /etc/rc.d/init.d/
ipchains (not to be confused with the /sbin/ipchains
program). This is run before networking starts and loads
a saved set of firewall rules. Furthermore, to save a new
set of rules, you simply run the firewall script and then
type:
You now have to modify /etc/rc.d/rc.local so that it calls
the rc.modules file during start-up. The start of the rc.local
file initially looks like this:
#!/bin/sh
#
# This script will be executed *after* all the
# other init scripts.
# You can put your own initialisation stuff in here if
# you don’t want to do the full Sys V style init stuff.
if [ -f /etc/redhat-release ]; then
All you have to do is edit it to add a call to the
/etc/rc.d/rc.modules file, so that it looks like this:
www.siliconchip.com.au
/etc/rc.d/rc.modules
if [ -f /etc/redhat-release ]; then
Setting up a firewall
/etc/rc.d/init.d/ipchains save
January 2003 77
COMPUTERS: masquerading modules & a firewall
Once you’ve done that, the firewall is automatically set
up before any networking each time you start the Linux
PC. This not only gives you full security but also saves
you from having to manually modify or add any start-up
scripts yourself!
To reload your saved rules you can type:
/etc/rc.d/init.d/ipchains start
and the previously saved rules are restored! Conversely,
to remove all rules, you type:
/etc/rc.d/init.d/ipchains stop
This flushes all rules and removes all user-defined
chains, thereby disabling the firewall. However, this will
leave your PC wide open to attack, so it is not recommended.
On the other hand, typing
/etc/rc.d/init.d/ipchains panic
does the opposite – ie, it denies everything (including local
network traffic). Don’t do this from a local telnet or ssh
connection – if you do, you will be stuck and will have
to recover from the console!
Firewall rules
The firewall consists of three basic sections, called
“chains”: an input chain, an output chain and a forward
chain. They can be applied to each network card in the
Linux PC but all we are really concerned about here is
the network card connected to the cable modem (no restrictions are usually applied to the local network card,
although they could be if required).
The input chain covers anything coming in from the
Internet. This is the one that the restrictions usually apply
to, as you do not have any control over who or what is
trying to gain access to your PC. The output chain covers
anything being sent out to the Internet.
The forward chain is used to transfer packets from
the input chain of your local network card to the output
chain of your modem network card (ie, to send stuff from
your Linux PC or one of your Windows PCs to the Internet). Anything coming back from the Internet (ie, reply
packets) is simply transferred directly from the input
of the modem card to the output of the internal LAN
card.
A fourth type of chain is one you create yourself. This
is effectively a subroutine, for want of an analogy, and
would normally be used if you want to apply the same
set of rules in more than one place.
Note that in ipchains, the forward chain comes from
the input chain and goes to the output chain. This means
that the forward chain does not usually require any specific blocking rules. Conversely, in iptables the forward
chain does not traverse the input or output chains at
all. As a result, it requires similar security to the output
chain.
All chains can be told to DENY (DROP in iptables) or
78 Silicon Chip
REJECT something. The difference between the two is that
REJECT returns an error message (so the hacker knows
what has happened) while DENY does not return any
messages. This means that DENY is ideal for use with the
input chain as hopefully potential crackers will give up
if they get no response at all.
Another option is called ACCEPT, which means to allow something through. This is not normally used in the
forward chain. Instead MASQ is used, which instructs
the chain to change the internal network addresses to the
external (eth1) address.
The input, output, and forward chains also have a
thing called a “policy”, which is simply what to do
when all else fails. By contrast, user defined chains do
not have a policy – they simply return to the point they
were called from.
For a detailed description on ipchains (with lots
of exam
p les), go to the following Internet site:
http://www.tldp.org/HOWTO/IPCHAINS-HOWTO.html
To find out how iptables works, you can go to:
http://www.linuxguruz.org/iptables/howto/iptables-HOWTO.html
How the firewall works
OK, let’s now take a look at the firewall rules listed
here in cablefirewall.simple. We’ll start from the top and
describe what each rule does:
First, MODIF="eth1" is a variable that defines the network card your cable modem is connected to. Change
the eth1 to eth0 if required, or to ppp0 if you are using a
dial-up modem.
The reason for using a variable is that you can change
it here and then all later references to $MODIF will refer
to the correct network card. This saves you from having
to change it throughout the whole script.
Similarly, LOCNET="192.168.0.0/24" refers to your
internal network. The /24 means the same thing as
/255.255.255.0
Iblock="DENY" ; Oblock="REJECT" ; Fblock="DENY"
are three statements on one line (hence the semicolons).
You can change the DENYs to REJECTs and visa versa if
you want. I have used DENY for the input (so crackers
get no indication) and REJECT for the output so users on
the internal network are warned of any problems with
outgoing traffic.
Next any existing firewall rules are removed by flushing
all existing rules and any user-defined chains.
The local and loopback networks are allowed for both
input and output, so the loopback (required for internal
Linux use) is enabled as quickly as possible. The local
network is allowed to do anything, the theory being that
users on your internal network are friends, not enemies!
This is done by allowing everything except the cable modem interface (the “!” means “anything but”).
Next, the policies for all three chains are defined
to deny or reject everything. The following masquerading timeouts are standard values which are used
everywhere.
The input chain is where we stop crackers getting
in. Here, crackers who are devious enough to supwww.siliconchip.com.au
Connecting To Telstra Bigpond Advance
Unlike OptusNet cable, Telstra Bigpond Advance
requires a login script for full Internet access. Under
Linux, this login script is called bpalogin and several
readers have asked for further information on how this
is installed. Although we haven’t tested it, the following
procedure should work:
(1) Go to http://bpalogin.sourceforge.net/, then click
the “Download BPAlogin” link and select the download you require - eg, “RedHat Linux RPMs v2.0”. The
bpalogin-2.0-1.i386.rpm file that’s download is about
170Kb in length.
(2) Copy this file to the Linux PC and install it by typing:
rpm -i bpalogin-2.0-1.i386.rpm
This creates the following files and directories (as
shown by rpm -q -p -l bpalogin-2.0-1.i386.rpm):
/etc/bpalogin.conf
/etc/rc.d/init.d/bpalogin
/usr/doc/bpalogin-2.0
/usr/doc/bpalogin-2.0/COPYING
/usr/doc/bpalogin-2.0/CREDITS
/usr/doc/bpalogin-2.0/INSTALL
/usr/doc/bpalogin-2.0/README
/usr/sbin/bpalogin
(3) Open /etc/bpalogin.conf in a text editor and
change the following two lines (near the top of the file):
username yourname
password yourpass
ply an internal IP address to try to get through are
stopped.
Now the important one. Anybody trying to break in
must be stopped but you have to be able to get stuff back
from the Internet yourself. The next line achieves this by
allowing TCP traffic that is not a connection (ie, it allows
return packets).
One problem with this is that when you download data
using FTP, it requires a connection! So the next line defines
a rule that allows FTP data connections only.
Next we allow UDP and ICMP packets in. UDP is used
by DHCP and DNS, while ICMP is used for error messages,
pings, etc. This does mean that crackers can ping the PC
but it is possible to prevent this by setting up several ICMP
rules, to be selective.
The last input chain rule blocks and logs anything
else, so you can check who or what is trying to break in.
This is only required if you want to log any blockages.
Since the only thing being blocked is TCP connections,
www.siliconchip.com.au
You obviously set “yourname” and “yourpass” to whatever your Bigpond Advance user name and password
are.
I notice that the file is set to -rwx------ and is owned
by root, so it already is protected against unwanted
peaking.
The start of the file looks like this:
# Default debug level is 1. Values range from 0-2
# with 0 being silent
# All information goes to the syslog.
debuglevel 1
# The user name you have for your BPA account
username yourname
# Your BPA password
password yourpass
Note that there is also a /etc/rc.d/init.d/bpalogin startstop script. Now type:
chkconfig --list bpalogin
This shows that the rpm installation sets the startup
and shutdown as follows:
bpalogin 0:off 1:off 2:off 3:on 4:on 5:on 6:off
This means that after editing /etc/bpalogin.conf, you
can start bpalogin either by restarting Linux or by
typing:
/etc/rc.d/init.d/bpalogin start
which you should never allow anyway, this line is
commented out.
If you do want to log TCP blockages then remove the
“#” from the start of the line.
The output chain is a lot simpler. Everything is allowed out to the cable modem, except internal IP addresses. This is a simple safeguard in case you make a
mistake configuring any of the services on your local
network.
Next are some delay rules which only apply to a dial-up
modem (delays are optimised for a network card by default). A test is done for the external interface being ppp*
(ie, a modem).
The last thing is to block and log everything else. Since
the output chain policy is to block, you can remove this
if you do not want to log anything but that would not be
a good idea. Anything logged here will be something you
will need to fix.
The forward chain is also quite simple and has just two
January 2003 79
COMPUTERS: masquerading modules & a firewall
rules. First, internal IP addresses are changed (masqueraded) to the cable modem’s IP address. Everything else is
then logged and blocked. Again, if anything is logged here,
it will be a problem you need to fix.
Making the firewall work
To get the firewall rules up and running, you must
have IP forwarding enabled as described in Pt.1. The
local and cable modem networks will also be up and
running at this stage. Note, however, that this means that
the PC is wide open to attack, so have the firewall ready
to roll if you are starting with the cable modem plugged
in.
Actually, only the local network needs to be up for IP
forwarding to be enabled, so a better scheme would be to
unplug your cable modem before starting the PC. In fact,
this is the recommended method as it will keep you safe
while you install the firewall.
You can either type cablefirewall.simple in yourself or,
better still, save yourself the hassle by downloading the
script from the SILICON CHIP website at: www.siliconchip.
com.au
It doesn’t really matter where you save it since it is only
run once to initially set the rules up before they are saved
(see below). However, /usr/local/bin is probably as good a
place as any to store the firewall script.
It’s then just a matter of running the script to activate
the rules. You do that by typing:
/usr/local/bin/cablefirewall.simple
Note that if you have the cable modem unplugged, this
script will take a while to run but it will get there. Follow
this by typing:
/etc/rc.d/init.d/ipchains save
This command saves the firewall rules so that they
are now automatically invoked on system startup,
before networking is enabled. This gives you full
security.
By contrast, if /etc.rc.d/cablefirewall.simple was called
from /etc/rc.d/rc.local, then the networking would be up
long before the firewall was. And that could create security problems.
The interesting thing here is that the saved rules will be
restored before IP forwarding is enabled without a problem.
However, trying to set the rules via cablefirewall.simple
without IP forwarding enabled won’t work! Note that this
isn’t a problem with cablefirewall.simple – it’s simply the
way ipchains works.
Assuming that you unplugged your cable modem for security, you can now plug it back in and
type:
ifup eth1
This will start the cable modem network. Don’t forget
to use eth0 instead of eth1 if this is the cable modem
interface.
And that’s it. If you’ve followed all the instructions so
far, you will now have a working Internet gateway, firewall,
DHCP server and DNS server.
In Pt.4, we will describe a script to enable easy viewing of any firewall logs and show you how to run your
Linux box without a screen or keyboard, including
shutting it down via the power switch (if it has an ATX
power supply). We’ll also briefly discuss a few security
SC
safeguards.
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*Australia only.
Offer valid only
while stocks last.
THAT’S RIGHT! Buy a 1- or 2-year subscription to SILICON
CHIP magazine and we’ll mail you a free copy of “Electronics TestBench”, just to say thanks.
“Electronics TestBench” is a valuable 128-page collection of
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only consumer electronics magazine.
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Contact: Silicon Chip Publications, PO Box 139, Collaroy, NSW 2097
Phone Orders: (02) 9979 5644 Fax Orders: (02) 9979 6503 Email Orders: office<at>silchip.com.au
80 Silicon Chip
www.siliconchip.com.au
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Tel/Fax: (02) 9533 3517
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Tel:(03) 9562-8222 Fax: (03) 9562 9009
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Tel: (03) 9762 3588 Fax: (03) 9762 5499
WebLINK: wiltronics.com.au
JJanuary
anuary 2003 81
Chips monitor
tyre pressure
US electronics giant Motorola is set to introduce computers into
the last electronics-free zone in a car – its tyres. The company has
developed a two-chip remote sensing module (RSM) small enough
and light enough to fit inside a tyre without unbalancing the wheel.
A
sensor chip, code-named
Daytona, measures pressure to
within 7.5kPa (typical car tyre
pressure is 220kPa), and temperature
to within 4° Celsius. Temperature
measurement is necessary to compensate for pressure changes due to tyre
heating during driving.
The Daytona chip is fabricated using low power CMOS technology and
draws just 0.55µA on standby. The second chip in the RSM is a combination
of Motorola’s HC08 microcon-troller
and a UHF radio transmitter in a
32-pin package. It processes the raw
measurements into a tyre pressure
reading and transmits the data to the
in-car receiver.
82 Silicon Chip
The transmitter operates in the 315,
434 or 868MHz bands, sending the
pressure data at up to 9600 baud by
either on/off or phase shift keying.
The HC08 has 2Kb of on-board FLASH
memory and enough I/O and computing power to handle the pressure and
temperature reading task.
It also has built-in power management capabilities to get the most out
of the lithium battery powering the
module. When the car is parked, an
inertial switch can be used to turn off
the transmitter and leave the HC08 in
low power sleep mode.
By PETER HOLTHAM
These power-saving features of the
RSM will ensure a battery life of at
least ten years. A simple PC board
antenna completes the RSM hardware.
It provides a signal strong enough to
be picked up by the receiver inside
the car.
Making the module is one thing,
keeping it alive in the harsh environment inside a tyre is another. Temperatures can range from a freezing -40°C
to a scorching 150°C . The RSM is also
subjected to accelerations as high as
2000G as the wheels rotate.
The computer and transmitter can
be protected but the pressure sensor
must be in contact with the air in the
tyre. Motorola engineers have develwww.siliconchip.com.au
oped a special Teflon filter to protect
it against attack by liquids, dust, and
corrosive gases.
The tyre pressure signal is picked
up inside the car with the same receiver already installed for remote
keyless entry.
The information presented to the
driver will depend on the software
programmed into the HC08 and the
receiver by car component suppliers.
It could be as simple as a dashboard
warning light showing that one of
the five tyres (including the spare)
needs pumping up.
More complex systems will automatically identify each tyre and
provide the exact pressure. Motorola
plans to begin volume production
of RSMs in September this year.
The price will depend on end-user
requirements and will vary based on
volumes and specifications. But with
around 50 million cars produced every
year, demand for remote tyre pressure
monitoring is expected to soar, driving
prices down.
All of which means monitors are
likely to become standard equipment
within the next few years.
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Other Manufacturers Join The Fray
Given the huge global market for
new cars, Motorola was not going
to be left as the sole supplier of tyre
pressure monitors for long.
Now European electronics company Philips has launched a rival
chip to assist in the measurement of
individual tyre pressures.
The P2SC signal-conditioner works
together with pressure sensors built
into the tyre. It mounts directly on the
tyre rim, providing a wireless link to
transmit the pressure to the keyless
entry receiver in the car.
The monitor inside the car sends
a low frequency ‘wake-up’ signal to
www.siliconchip.com.au
each P2SC chip every time the ignition is switched on. The chip returns
pressure information at frequencies
in the 315 and 434MHz bands.
While the car is being driven, the
P2SC chips send regular status reports on each tyre back to the driver.
The low frequency wake-up also
allows the monitor to automatically
identify which tyre is where; even
after tyre position is changed during
maintenance.
Industry analysts expect pressure
monitors to become the fastest growing segment of car electronics over
SC
the next few years.
718 High Street Rd, Glen Waverley 3150
Ph (03) 9802 0788 FAX (03) 9802 0700
ALL MAJOR CREDIT CARDS ACCEPTED
January 2003 83
VINTAGE RADIO
By RODNEY CHAMPNESS, VK3UG
Intermediate Frequency (IF)
Amplifiers; Pt.2
Last month, we looked at how the IF stage
evolved in early broadcast-band AM radios.
This month, we look at high-fidelity IF
amplifier stages and describe how to get rid
of the 9/10kHz whistle.
P
RIOR TO THE introduction of
FM into Australia, some radio
manufacturers produced receivers that were capable of reproducing
the full transmitted audio bandwidth.
Typically, this involved designing
20kHz IF (intermediate frequency)
stages to give a maximum audio frequency response of 10kHz.
However, the use of a wide-bandwidth IF laid the receiver open to
annoying “monkey-chatter” – ie, distorted modulated audio signals from
stations close to the tuned frequency.
It also gave rise to annoying 10kHz
Fig.1: the circuit for a 9/10kHz
audio notch filter. It is designed
to filter out 9kHz or 10kHz
whistles (depending on the
station spacing) in a wideband
AM receiver.
84 Silicon Chip
heterodyne whistles from stations
on adjoining channels. The monkey
chatter couldn’t be eliminated but the
10kHz whistle could be and often was.
Basically, the 10kHz whistle was
“eliminated” by installing a simple
10kHz audio notch filter. This filter
effectively reduced the whistle to an
insignificant level.
The 10kHz filter often took the form
of a narrow-band rejection filter, as
shown in Fig.1. In this case, the filter is
physically tuned to 10kHz by varying
L1 or C1 and C2, while the depth of
the notch was adjusted by VR1. Note
that, with the advent of 9kHz channel
spacing, these filters had to be retuned
from 10kHz to 9kHz.
Variable selectivity IF stages
In most cases, broadband amplifiers did a good job on local stations
and gave an audio output which
was considered high-fidelity at the
time (10kHz compared to FM which
has frequencies as high as 15kHz).
However, listening to more distant
stations was often quite unpleasant
at night, due to fading, noise and interference, monkey chatter and 10kHz
heterodynes.
To counter these extremely annoying problems, most high-fidelity receivers included a switch that reduced
the IF amplifier bandwidth to around
10kHz. This meant that the receiver
could produce audio signals up to only
about 5kHz when the switch was in
the “narrow” position.
Fig.2: a variable bandwidth IF stage. Switching the
resistors across the IF transformer windings increased
the bandwidth, while reducing the gain of the
amplifier.
www.siliconchip.com.au
This photo shows an assortment of 455kHz
IF transformers. They came in a wide range
of sizes.
Of course, this meant that the full
frequency range was no longer reproduced, so listeners had to be content
with less than “hifi” reproduction.
However, on the positive side, the
10kHz whistles, monkey chatter, noise
and interference were all signifi cantly
reduced. This was important because
before the advent of TV, the evening’s
entertainment often involved listening
to the radio.
Variable bandwidth
Taking this a step further, some
manufacturers designed variable
bandwidth IF stages that could be
switched to suit the listeners’ requirements. This was done in a variety of
ways.
One method involved switching
resistors across the IF transformer
windings. This lowered the Q of the
windings and the gain of the amplifier,
while at the same time increasing the
bandwidth of the amplifier – see Fig.2.
Another method involved removing
one IF transformer completely, replacing it with an untuned inductance-capacitance network.
Still another method involved
switching a tertiary winding in and out
of circuit in a special IF transformer.
There were even circuits which automatically adjusted the bandwidth
according to the strength of the received signal – ie, the bandwidth was
www.siliconchip.com.au
controlled by the AGC.
However, although such circuits
were around, very few showed up in
the average domestic receiver. It’s also
interesting to note that specialised
high-fidelity tuners/receivers often
used an IF of 1900kHz (or some other
frequency above the broadcast band)
to achieve good bandpass shape and
20kHz bandwidth.
Unfortunately, fading – and selective fading in particular – remained as
a severe impediment to good quality
reception on distant stations. For those
unfamiliar with selective fading, it
manifests itself as severe distortion
and fading of the received signal. It is
usually due to multi-path reception,
which causes the relative levels and
phase of the carrier and its two side
bands to vary.
Keeping IF amplifiers stable
It is rare to have instability and oscillation problems in well-designed amplifier stages. By using an IF of 455kHz
and normal high-gain IF transformers,
a valve with a mutual conductance of
around 2000 was all that was necessary
to obtain the necessary performance.
Valves such as the 6U7G and the 6N8
fall into this category.
To ensure stability under all circumstances, it is necessary to make
sure that the layout of the amplifier is
such that inputs and outputs are kept
well apart. This particularly applies
if using high-gain valves. In some
cases, such as when using high-gain
valves like the 6BA6 (and more so
with the 6AU6), a shield may need to
be soldered across the valve socket,
isolating the input from the output.
As a matter of interest, I’ve found a
number of Healing sets using the 6AU6
to be marginally stable.
Neutralisation
Fig.3: this diagram shows the
correct positions for the slugs in
an IF transformer. Note that the
coils are tuned with the slugs
towards the outside ends of the
former (not in the centre).
Neutralisation was used in circuit
design back in the 1920s when triodes were used as RF amplifiers. It
was necessary if reasonable gain was
to be obtained without the amplifier
oscillating. However, with the advent
of RF tetrode and pentode valves,
January 2003 85
Fig.4: typical IF, detector and audio stages for an AM broadcast band receiver. The components marked with an
“A” suffix are often missing but their inclusion improves performance (see text).
neutralisation became unnecessary
in most circuits, particularly in IF
amplifiers with their relatively lower
frequency of operation compared to
RF amplifiers.
However, I’ve found that EMI/HMV
have been sticklers for doing things
right. Fig.4 shows a circuit in which
the IF stage is approximately neutralised. The 5pF (C2) capacitor from the
plate of the 6BA6 to the bottom of the
secondary of the IF transformer acts
with the AGC bypass (C1) to form a
bridge neutralising circuit.
I had a Little Nipper receiver to
restore some time back which had an
unstable IF amplifier – it tended to
oscillate if I wasn’t careful with the
alignment. It turned out that someone
had been at the set before it came to
me and had replaced the .01µF AGC
bypass capacitor (C1) with a value of
0.1µF. Replacing this capacitor with
the correct value restored the neutralisation and the IF stage was again
quite stable.
Detector & AGC leads
The leads from the detector and the
AGC diode tend to be treated as having
no RF energy on them. In reality, however, they carry quite a bit of RF (IF)
energy and this needs to be prevented
from radiating and causing instability
within the receiver.
For example, resistors R3 and R4
should have minimal lead length on
the ends connecting to pin 5 of the
6AV6. Similarly, the 47pF capacitor
86 Silicon Chip
(C7) lead from pin 5 of the 6BA6 should
be as short as possible, as should C5’s
lead on the IF transformer terminal. By
observing these precautions, minimal
IF energy will be radiated from the IF
amplifier circuits.
The detector lead to the volume
control can also radiate energy if it
isn’t shielded. However, few receivers
in the later valve radios have this lead
shielded so it isn’t always necessary.
Note too that some receivers have the
volume control di
rectly connected
to the bottom of the IF coil as shown
in Fig.4 (assuming that R2A is a wire
link). In that case, only the 100pF
bypass capacitor (C5) provides RF
filtering.
By contrast, the better receivers
include another section of filtering
based on resistor R2A and capacitor
C6A. This further reduces the level of
RF (IF) energy getting through to the
audio amplifier.
Although the audio amplifier favours audio frequencies, it also amplifies any IF signals that find their way
into this stage. This signal can then
be radiated from the audio amplifier
and picked up by the front-end of the
receiver, or by other receivers nearby, where it can cause some strange
effects.
In some cases, this radiation causes
the receiver to perform poorly at the
low-frequency end of the broadcast
band. It’s difficult to describe the
exact symptoms. However, the set
doesn’t have the sensitivity it should
and also seems to be a little strange in
its alignment, with a certain amount
of “swish” heard as the set is tuned
across a station.
So what can be done to overcome
this problem. The amount of IF signal
getting into the audio amplifier has
already been reduced by the filter consisting of R2A and C6A. In addition,
capacitor C8 from the plate of the 6AV6
to earth also reduces the amount of IF
energy in the circuit.
However, if the lead lengths from
the plate of the 6AV6 to the grid of the
6M5 are short, it would be better to
connect a small-value capacitor (such
as C11A) between the grid of the 6M5
and earth. The combination of R8 and
C11A would then be more effective at
reducing the IF energy applied to the
grid of the 6M5 than using just C8.
Most output stages have a capacitor from the plate to chassis or to the
high voltage supply. This reduces the
amount of IF energy at the output of
the audio amplifier, as well as acting
as a mild top-cut audio filter. The suggested added components that reduce
this problem are shown with an “A”
after them in Fig.4 (R2A is normally a
short circuit in most sets). By carrying
out these modifications, I’ve found
that many receivers offer improved
performance.
Another set I looked at some time
ago had an extremely unstable IF amplifier. It didn’t take long to establish
that RF signals were being amplified
in the audio stage and were being fed
www.siliconchip.com.au
back through the set. In fact, it was so
unstable that even bringing the plastic
handle of a screwdriver near some of
the normal supply wiring caused the
set to either go into oscillation or to
stop oscillating, depending on the state
it was in at the time.
In this case, the problem was found
to be lack of proper filtering of the
high-tension (HT) supply line. In this
particular receiver (from a well-known
manufacturer), R9 was not includ
ed in the circuit design – there was
just a length of wire where a resistor
could (should) have been. I decided
to decouple the HT line by installing
a resistor in this location and the
set imme
diately became stable and
proved to be a really hot performer.
Problems can also occur when IF
cans are not earthed prop
erly or a
shield can is missing from a valve.
These are problems that are easily
fixed.
Despite a few problems, I have
generally found IF amplifi
ers to be
quite reliable. In most cases, all that is
necessary to restore the performance
is to replace leaky paper capacitors
and perhaps the odd valve. The AGC
bypass capacitor(s) are particu
larly
important and these should have no
discernible leakage. If they do, the
normal AGC control voltage will not
be applied and this usually results in
overloading of the IF amplifier.
An IF amplifier with low gain
It’s important that IF transformers
be wired the correct way, as reversing
the connections on one winding can
cause the gain to be quite low. Many
replacement IF transformers, such as
those produced by Aegis, have the
connections marked on the can, so
they are easy to identify.
For unmarked transformers (eg,
those salvaged from derelict receivers),
the windings can usually be identified
by taking the transformer out of its
shield can. The grid winding is the
one furthest from the base. If the performance is poor and you know the
transformer is good, try reversing the
connections. Also, if an IF transformer
is being taken out of a wreck, observe
what each lead is attached to and label
the leads accordingly.
The following information from the
4th edition of the Radiotron Designer’s
Handbook (by Langford-Smith) will
help in identifying IF transformer
windings: “For the capacitance and
mutual inductance coupling to be
aiding, the prim
ary and secondary
windings are arranged so that if the
plate connects to the start of the primary, then the grid (or diode plate) of
the next stage connects to the finish
of the secondary winding; both coils
being wound in the same direction . . .
the grid and plate connections should
be as far from one another as possible”.
Aligning the IF amplifier
The standard IF transformer usually has critical coupling between the
two tuned circuits. Critical coupling
provides maxi
mum gain with the
transformer adjusted by simply tuning
for a peak.
IF transformers employ a variety of
methods when it comes to adjusting
the slug-tuned types. Older types
have an earthed metal screw thread
which can be adjusted with a normal
metal screwdriver. Conversely, if the
tuning tool has to be inserted into the
Looking for an old valve?
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Tel: (03) 5257 2297; Fax: (03) 5257 1773
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Email: evatco<at>mira.net
Premises at: 76 Bluff Road,
St Leonards, Vic 3223
www.evatco.com.au
Subscribe &
Get This FREE!*
*Australia only. Offer valid only while stocks last.
THAT’S RIGHT! Buy a 1- or 2-year
subscription to SILICON CHIP magazine
and we’ll mail you a free copy of “Electronics TestBench”, just to say thanks.
A selection of plastic alignment tools will be necessary if you intend restoring
vintage receivers.
www.siliconchip.com.au
Contact: Silicon Chip Publications,
PO Box 139, Collaroy, NSW 2097
Phone Orders: (02) 9979 5644
Fax Orders: (02) 9979 6503
Email Orders: office<at>silchip.com.au
January 2003 87
Photo Gallery: Eclipse Monarch DKL
Manufactured by Eclipse Radio (Melbourne), the 1947 Monarch DKL is
a good example of the 4-valve reflex superhet designs that were popular
during that period. The set was available in a number of different cabinet
colours, including white as shown here. The following valves were used:
6A8-G frequency changer; 6B8-G IF amplifier/reflexed 1st audio/detector/
AVC amplifier; 6V6-GT output; and 5Y3-GT rectifier. (Photo and information
courtesy Historical Radio Society Of Australia).
IF transformer, you use a non-metallic
alignment tool.
It is also important to use the right
tool here for two reasons: (1) so that the
slugs are not damaged; and (2) so that
the transformer is not detuned by the
presence of a metallic adjustment tool.
Plastic alignment tool kits are available from various electronics stores or
you can use knitting needles which
have their ends filed to a screwdriver
blade shape.
The older type IF transformers that
use trimmer capacitors across the
tuned winding are also best adjusted
with a plastic alignment tool. That’s
because the plate voltage (ie, the HT)
is usually present on at least one trimmer – use a metal tool and you could
get a nasty shock.
The alignment procedure is as
follows: first, with the set turned off,
connect a digital multimeter (DMM)
across C1 on the AGC line and switch
to the 0-20V range. That done, connect a signal generator to the antenna
terminals of your set and tune the
set to the low-frequency end of the
broadcast band.
The next step is to apply a high-level
signal modulated at 1kHz at around
the expected IF frequency and tune
88 Silicon Chip
the generator across the band. If the
set hasn’t had its IF tuning adjustments
fiddled with, a response should be
heard at or near 455kHz (or what ever
the nominal IF of the set is).
If the signal through the set is quite
strong, the DMM will register an extra
-2V along the AGC line. Adjust the
output of the generator so that only
-1V or so of extra voltage is shown on
the meter.
If the frequency is some way away
from the expected IF (eg, 20-30kHz),
it is possible to “walk” the IF adjustments onto the required frequency. To
do this, first tune the signal generator
just to the side of the spot where the
maximum response is (ie, towards
the wanted frequency). That done,
adjust each of the IF slugs for a peak,
then go through the whole procedure
again until the maximum response is at
455kHz (if this is the target frequency).
Now it is necessary to accurately
tune the IF amplifier. Once again,
adjust the signal generator so that
the DMM reads a volt or so above the
standing bias on the AGC line. Adjust
each of the internal slugs or external
screws for a maximum reading on the
DMM, except for the tuned winding
going to the detector diode. This one,
at the top of the transformer, is adjusted for maximum audio, not maximum
meter reading.
If the DMM is connected across
the volume control (VR1), peak all
adjustments for a maximum reading.
Reduce the generator signal level if the
DMM reading is above about -4V, as
the IF amplifier tunes (peaks) slightly
differently with a strong signal compared to a weak signal. Note that for
best performance on weak signals, it
is necessary to align the set on weak
signals.
Note particularly that the slugs or
screws should adjust to the correct
frequency with the slugs and screws
away from the centre of the former,
as shown in Fig.3. If they are close
together (ie, towards the centre of the
former), the coupling between the two
tuned circuits will be upset and the
performance will be compromised.
If you don’t have a signal generator
it’s still possible to align the set, although not quite as accurately. Once
again the DMM is connected to either
the AGC line or to the detector output.
All you have to do then is tune to
a relatively weak sta
tion and peak
the signals as described in the previous paragraph. Of course, you won’t
know if the IF stage is tuned to exactly
455kHz but that doesn’t really matter.
Note that this job should be done in
the middle of the day, to avoid signal
fading which would make it difficult
to accurately align the IF amplifier.
So there you have it – a straightforward method of tuning the IF amplifier
stages in most sets. In times gone by,
when high impedance voltmeters were
scarce, the audio output was measured
and the IF adjustments peaked for
maximum audio. However, I believe
that the method I’ve described is more
appropriate today as it also gives an
idea as to whether the AGC system is
working as it should.
Occasionally, one slug in an IF
transformer will be stuck. If you strike
this, don’t force it as broken slugs are
hard to get out. Instead, just adjust
all the other slugs so that all tuned
circuits are on the same frequency as
the circuit that’s tuned by the stuck
slug. Being precisely on 455kHz isn’t
at all necessary.
Finally, for anyone who wants to
know more about IF amplifiers, take
a look at the relevant chapters in the
“Radiotron Designer’s Handbook” by
SC
Langford-Smith.
www.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
Cheap 12V power supply wanted
I want a power supply to convert
240VAC from the power point to 12V
DC at 3A. I am currently using a car
battery but that is inconvenient. (D.
F., via email).
• The cheapest way to get a high current 12V power supply is to obtain a
computer power supply and tie all the
+12V output leads together and all the
0V leads together (ie, connect the 12V
outputs in parallel). We have not done
a project along these lines.
Problems with LP Doctor kit
I recently completed construction of
the LP Doctor (SILICON CHIP, January
2001) kit but now I find several problems that defy repair. In the “bypass”
switch position, the straight through
phono preamp and output level control work perfectly, however in any
of the “processed” switch positions,
there is no audio output.
I also notice that the left/right LEDs
appear to function normally, although
they flash regardless of the selector
Adjusting mixture
on a VR Commodore
I have just purchased a Fuel
Mixture Display kit. If the vehicle is
running rich, is it possible to adjust
the vehicle’s computer to make it
run in the correct mixture range?
For a VR Commodore, is there room
for adjustment to make it run lean?
(D. G., via email).
• Although it’s possible to change
the “chip” in the engine management computer (eg, to alter the timing curve and/or to change mixture
settings), this really is a job for the
specialist. And generally speaking,
it’s difficult to do better than the
manufacturer’s original chip.
www.siliconchip.com.au
switch position. Is this normal? I have
thoroughly checked my work and can
see no apparent error. I have also successfully completed the voltage adjustment as outlined in the construction
manual. Can you offer any advice? (F.
S., Ingham, Qld).
• It is normal for the click detection
LEDs to operate independently to the
selector switch. The signal is somehow
being lost through IC3, IC7 IC4, IC8,
etc. Check the supply to each of the IC3
and IC7 delays and op amps IC5a and
IC7a. Also check that there is -7.5V at
pin 2 of IC4 and IC8.
Alternatively, the wiring to switch
S2 is incorrect. Check that there is
audio signal directly at the outputs of
IC5a and IC7a.
10-channel remote receiver queries
The following queries relate to
the 10-Channel IR Remote Receiver
published in the February 2002 issue.
Firstly, in forcing IC1 to display its remote control status by connecting pin
1 to the 5V supply (TP2) via a 220Ω
test resistor at power up, can the same
be achieved by connecting the two
If the fuel mixture display indicates that the engine in your VR
Commodore is running rich, then
there are two possibilities: (1) either
the fuel mixture display is incorrectly calibrated; or (2) there is a
fault in your vehicle’s fuel system
which should be corrected by a
specialist service outlet.
Note that there are times when
the engine should run rich – eg,
under acceleration. If your vehicle
is performing normally, then it’s
likely that the fuel system is operating correctly. Note also that the
VR Commodore also runs quite lean
when at speed under light throttle
settings. It can return very good fuel
economy on a trip.
stakes (TP1 & TP2) on the completed
board? Or should another resistor be
employed, so that LED11 does not
blow (ie, does the 100kΩ resistor take
enough of the current)? Is this resistor
best connected from TP2 straight into
the terminal contacts of pin 1 with
IC1 in place.
Secondly, is the decoded signal at
TP2 for all signals received or only
those matching Sat1/Sat2 codes?
Thirdly, if the use for some outputs
is currently unknown, is it OK to just
leave out the 1.8kΩ resistor, which selects toggle or momentary, or do some
other parts need to be left out too? (eg,
respective transistor).
Fourthly, is there a part that comprises a variable resistor on a reversible
motor for volume control? What would
happen if power is supplied to both
directions at once; ie, both buttons
are pressed down by the remote user
or would only signal for one button
be sent from the remote? (D. K., via
email).
• TP1 cannot be directly connected to
TP2 or the LED (LED1) will have 5V
across it with no current limiting and
consequently it will be destroyed. This
is why we use a 220Ω resistor at pin
1 to TP2 instead. Connecting a 220Ω
resistor between TP1 and TP2 will
not bring pin 1 of IC1 high enough as
it will be at about 1.8-2V as set by the
LED voltage.
The decoded signal at TP1 will reflect the incoming code sent by the IR
transmitter. The code does not have to
be SAT1 or SAT2 but the 10 outputs
will not respond unless the code is
correct.
The 1.8kΩ resistors on the outputs
need to be connected to set the momentary or toggle option. If these are
left out of circuit, the output could
be either option, depending on what
level the pins float at when powered
up. Generally, the RA outputs will be
set at momentary and the RB outputs
for Toggle if no resistor is connected.
The decoder can only respond to
one code at a time and so driving the
January 2003 89
SuperCharger vs Multi-Purpose Fast Charger
I have read the SuperCharger
articles with interest and I am keen
to build one, if you can first answer
a couple of questions. I have been
using your Multi-Purpose Fast
Charger II for quite some time now.
It has charged quite a few of the
new high capacity batteries (AA
1800mAh) and seems to do it well.
What is the difference between
the two chargers in their ability to
charge the new high capacity batteries and am I doing my batteries
harm by using the Fast Charger?
I always refresh before charge.
The standard number of AA cells
I charge is four; ie, 4.8V. I always
use the thermistor when charging
and have never had any problems
with overcharged or overheated
batteries.
One advantage of the new charger is it could be used away from a
240VAC power source which is attractive when using a digital camera
on motoring or camping holidays.
(C. N., via email).
• There are a few potential probmotorised potentiometer using the two
outputs will not cause any problems.
And no problems occur if outputs are
in any state as the motor will only have
power (with either polarity) or have no
power with the motor terminals both
at positive or both at ground.
Delayed audio on
parliament broadcast
I am interested in politics and enjoy
watching the daily broadcast, when
parliament is sitting, of Question
Time on ABC-TV between 2:00pm &
3:00pm. Normally, when ABC-TV is
broadcasting the House of Representatives, ABC NewsRadio broadcasts
the entire day’s proceeding from the
Senate and vice versa.
However, on some occasions, both
the TV and radio broadcasts were
from the same House (in this case, the
House of Representatives). On such
occasions, when I have the TV on and
also try to listen to the proceedings of
the same House on the radio, I notice
that there is a delay of a few seconds
in the audio between the TV & radio
broadcast.
90 Silicon Chip
lems charging small (AA/AAA)
cells with the Multipurpose Fast
Charger II. Of most concern is its
high fixed charge rate. You may
find that you can charge Nicads
at this rate (using the thermistor
for temperature sens
ing) but it
will depend greatly on the type of
battery. Look specifically for “high
discharge rate” types, intended for
R/C applications and the like.
For NiMH-chemistry types, we’re
not aware of any small (AA/AAA)
types that can be safely charged
at 6A. You mention that you are
currently doing this without problems. While it’s true that thermistor
temperature sensing should prevent
catastrophic cell failure, we doubt
that the cells will be fully-charged
before the charge terminates. You
may like to verify this by doing a
cell capacity test.
We may publish a simple “addon” circuit for the Multipur
pose
Fast Charger that allows you to reduce the charge current at the flick
of a switch. No promises though!
Can you explain the reason or reasons for this delay? I can only assume
that it may have something to do with
the physics of the propagation of
radio waves as, I suspect, both transmissions here in Canberra come from
local transmitters. I suppose another
question might be should there be a
delay in the reception of the audio for
a simulcast program received on both
TV and radio? (P. M., Queanbeyan,
NSW).
• The delay has nothing to do with
the propagation of radio waves and
everything to do with the way the
ABC routes signals between its various
studios and transmitters.
We would guess that the TV signals
come direct from Canberra to the
relevant station transmitter while the
audio signal may go via the ABC radio
studios in Adelaide (or wherever).
There may even be a satellite link
involved.
Mic for measuring
frequency response
I would like to know if there is a
cheap way of making a microphone
and (preamp) with a known frequency
response, to use in conjunction with
the RTA spectrum analyser shown in
the August 2002 issue. If not, I believe
it would make a great project because
being able to see the problem areas
in the frequency response of a sound
system setup would be very handy.
I know you can buy calibrated
microphones but these all seem to
be quite expensive and for the small
amount of use they might get places
them out of reach of most people.
Could SILICON CHIP do a project
using an easy to get and cheap electret
microphone and plot its response,
etc, to use with RTA software? (B. B.,
Runaway Bay, Qld).
• Producing a calibrated microphone
is not a simple task – we have looked
at it as a project but cannot see an easy
way of doing it.
Faulty speed control
blows FETs
I have built two 20A Speed Control
kits from the June 1997 issue. One
works OK while the other worked for
one week and then the battery was
put in reverse polarity. It blew one
FET.
I replaced the faulty parts and it
worked for one week and then both
FETs blew. I replaced both FETs but
now I can’t vary the speed – always
near flat out. (S. G., via email).
• Strictly speaking, the circuit should
not have been damaged by battery
reversal. The fuse should have blown
with diode D1 forward biased.
However, since the FETs were destroyed, it may be that the transistors
and IC were also damaged. This would
explain the full-speed only operation.
It may be wise to replace the FETs,
transistors, IC1 and the regulator, plus
the diodes at the battery supply and
across the motor.
ETI pH meter
wanted
In the December 1980 issue of ETI a
digital pH meter project was featured.
This used an Intersil 7106 driver and
a 3.5-digit LAD204 display. Do you
know if this display is still available?
The driver and display were sold by
Intersil as part of an evaluation kit.
Perhaps an updated version of the pH
meter could be considered as a SILICON
CHIP project? (T. S., via email).
www.siliconchip.com.au
•
The ETI pH meter is no longer
available. SILICON CHIP described a
pH meter based on an LM324 quad
op amp and an analog meter, in the
April 1988 issue. It would probably
be much easier to source the parts for
it but you would need to make sure
you could get pH electrode before
proceeding further.
We can supply a photostat copy
of the April 1988 article for $10, in
cluding airmail postage.
Splitting a
line level signal
Could you please advise me, if I
split a line level stereo output signal
(left & right channel) using two “RCA
Y adaptors”, will it affect the level/
quality of the input signal at either of
the destination components (power
amplifiers in this case)? G. M., via
email).
• That’s not an easy question to answer. Superficially, it would seem that
splitting line level signals would not
cause a problem but there are a number
of factors to consider.
Factor one is the input impedance of
the amplifiers, etc. Normally, this will
be high and should not cause a problem but if it is low (say below 5kΩ), it
could reduce the signal level, as well
as degrade the frequency response and
distortion performance.
Two, if one of the amplifiers is
driven into overload, the resulting
distortion artefacts may be superimposed on the line signal to the other
destination device.
Three, if one of the destination
devices and the signal source is
earthed via the mains (rather than
double-insulated) an earth loop will
result which again could degrade the
performance.
From this, you will see that we are
not keen on Y-connectors. Provided
Hum in Plastic Power
amplifier
I have built the Plastic Power
amplifier module described in the
April 1996 issue of SILICON CHIP
and it passed all the tests. However,
I am getting hum. When I turn the
power supply off, the hum stops and
the amplifier continues to function
for about 10 seconds or so.
Do you have any suggestions to
get rid of the hum or would bigger
filter capacitors do the job? (S. G.,
via email).
• The hum could be due to the
filter capacitor value not being suffi
ciently large but this is unlikely.
Instead, hum at low levels is more
likely due to a hum loop, due to
the ground connections not being
the input impedances of your two
destination devices are high, a better
way is to make up a splitter box with
RCA connectors and feed the signal to
the two devices via isolating resistors
of, say, 4.7kΩ. That way, if something
naughty happens in one destination
device (say overload), it won’t degrade
the rest of the signal chain.
Generating different
audio tones
I am about to start a project that requires two different audio tones, one
having a positive sound like a “ping”,
the other having a negative sound like
“baamp”. If you imagine, like a board
game that has “yes” and “no” answers.
I would like to know what I need
for creating these two tones. I want
to be able to trigger each tone with
a microcontroller. (B. C., via email).
• We suggest using Twin-T oscillators
connected to the one point.
To minimise hum, the ground
connections for the capacitors
should all connect to a single
point with the 0V wiring from the
transformer also connecting to this
point. The amplifier output (speaker) ground then connects to this
common ground. The input ground
of the amplifier is not connected
to the common ground as this is
connected to the speaker ground
on the PC board.
In addition, the rectifier (+) and
(-) outputs should connect to the
capacitors first, with the amplifier supply rails connecting to the
capacitor leads rather than the
rectifier terminals. Use heavy gauge
wiring for these power supply
connections.
set to different frequencies and also set
just below the point of oscillation; they
can then be shocked into oscillation
by a short pulse.
SILICON CHIP has not published anything on this subject but there were
two relevant articles in EA: “Electronic Bongos” in December 1979 and
“Twin-T Oscillators” in May 1976. We
can supply photostats of these articles
for $8.80 each, including postage.
How to suppress
contact arcing
I have a question about how to reduce the arcing across relay contacts.
I’m switching a 240VAC 1A solenoid
with a 24V DC relay. What is more
reliable, using a Triac or relay? (Y. G.,
via email).
• The normal way to suppress contact
arcing when switching DC is to use a
reverse-biased diode with a current
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.
www.siliconchip.com.au
January 2003 91
Notes & Errata
40W Fluorescent Inverter, September 2002: Mosfets Q1 & Q2
have been found to be prone to
overheating when the PC board
is placed within the confines of
a slimline 36W fluorescent tube
batten. To correct this, the inverter
has been altered to improve efficiency without reducing the lamp
brightness.
Changes include reducing the
334V DC supply to 280V and winding transformer T1 differently.
The voltage change requires replacing one of the 270kΩ resistors
leading to pin 1 of IC1 with a 180kΩ
resistor. The changes to T1 involve
using 130 turns on the secondary.
For the primary use figure-8 7.5A
wire with a polarity stripe. Insert
one end of the figure-8 wire in the S1
& F1 holes nearest to Q2 and wind
on five turns, starting up through the
centre of the core and anticlockwise
towards S2 & F2. Insert the wire
ends into S2 & F2 with continuity
(same wire) between S1 and S2 and
the second wire between F1 and F2.
This means that if the polarity stripe
on the figure-8 wire is at S1, it then
terminates into S2.
rating of more the than load current
being switched. This should suppress
any contact arcing across the relay
contacts.
When switching 240VAC with
a solenoid, it is usual to connect a
250VAC-rated capacitor across the (solenoid) contacts. Try a 47nF (.047µF)
250VAC capacitor across the contacts.
High input impedance
amplifier wanted
I would like a suggestion for a high
input impedance ampli
fier circuit.
What I need is to be able to intercept
a line level signal and basically split
it in to two line level signals. I need it
high impedance so that it doesn’t load
the line too much.
I want to build five of these amplifiers and then use them to provide
line-level outputs from each channel
of my Boston Acoustics BA7500G
Speaker system so I can feed external
amps, without disturbing the internal
92 Silicon Chip
Set the current drain from the
battery at 3A (300mV across the
0.1W resistor used in the current
measurement set-up in Fig.8).
As noted in December 2002, it is
recommended that the maximum
current delivered to the fluorescent
tube be adjusted using a trimpot.
The 100kΩ resistor connecting between pin 2 of IC3 and the top of
the dimming potentiometer (VR1)
should be replaced with a 50kΩ
trimpot and series 82kΩ resistor.
The 1.2Ω resistor between the
source of Q4 and ground should be
changed to 2.2Ω to allow the full
dimming range available from VR1.
Using the current measuring
setup of Fig.8, the trimpot should
be adjusted for the 300mV, corresponding to 3A when the dimming
pot (VR1) is turned fully clockwise.
Note that this adjustment should
be made after the inverter has been
running for some time and is fully
warmed up. Once adjusted, the
trimpot and 82kΩ resistor can be
swapped for a single resistor that
is the same value as the total series
combination.
When testing the current (using
amplifier. Any help would be greatly
appreciated. (M. R., via email).
• You really don’t need a high input
impedance. What you need is a buffer
amplifier that can drive a series of low
impedance outputs. We have already
published a suitable circuit – the audio
portion of the Audio/Video Distribution Amplifier in November 2001.
This circuit is based on an LM833
dual op amp.
If you decide to use it, make sure
you install 1kΩ resistors in the outputs instead of the 47kΩ resistors
mistakenly specified in the original
article.
Speed control in
cordless drills
I recently bought a variable speed
cordless drill/screw
d river (Black
& Decker) and would like to know
what method is used to provide the
variable speed feature. I guess I could
open the drill and look inside but
the setup of Fig.8), it is important
not to have the 0.1Ω 5W resistor
in series with the supply for any
appreciable length of time as the
current drain will begin to increase.
To prevent this, short out the 0.1Ω
resistor (with a clip lead) when not
making the measurement. Remove
the clip lead briefly to make the
current measurement.
In addition, use heavy gauge wire
rated at 7.5A or more to connect the
inverter to the 12V battery.
It is recommended that the inverter not be used while the battery is
being charged from a high current
charger such as an automotive
alternator or mains-powered unit.
If the inverter Mosfets still run
excessively hot, it is recommended
to reduce the current drain to 2.5A
(250mV across the 0.1Ω resistor)
which will reduce the lamp brightness slightly.
With slimline batten holders,
ventilation can be improved by
drilling some holes in the side of
the batten adjacent to the Q1 and
Q2 heatsinks and some extra holes
at the other end of the batten to
SC
allow air flow.
that will void my warranty. (H. P., via
email).
• Cordless drills are usually permanent magnet motors with a Mosfet
switchmode power control, usually
running at about 1kHz or so. In fact,
you can usually hear the 1kHz tone at
very low speed settings.
Temperature
controlled fan
I want a circuit for a temperature-controlled fan for the heatsinks
of an amplifier I’m working on. I am
positive SILICON CHIP published one
in the not-too-distant past but for the
life of me I can’t find it in my back
issues, nor can I locate it on your
website. Can you recall where the circuit appeared please? (G. B., Scotland
Island, NSW).
• The circuit was associated with
the Ultra-LD Amplifier in the August
2000 issue. There were two options: a
SC
thermistor or thermal cutout.
www.siliconchip.com.au
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Enclosed is my cheque/money order for $__________ or please debit my
❏ Bankcard ❏
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Signature__________________________ Card expiry date______/______
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Street ______________________________________________________
Suburb/town ___________________________ Postcode______________
www.siliconchip.com.au
FOR SALE
WEATHER STATIONS: Windspeed &
direction, inside temperature, outside
temperature & windchill. Records highs
& lows with time and date as they occur.
Optional rainfall and PC interface. Used
by Government Departments, farmers,
pilots, and weather enthusiasts. Other
models with barometric pressure, humidity, dew point, solar radiation, UV, leaf
wetness, etc. Just phone, fax or write for
our FREE catalogue and price list. Eco
Watch phone: (03) 9761 7040; fax: (03)
9761 7050; Unit 5, 17 Southfork Drive,
Kilsyth, Vic. 3137. ABN 63 006 399 480.
UNIVERSAL DEVICE PROGRAMMER: Low cost, high performance,
48-pin, works in DOS or Windows incl.
NT/2000. $1364. Universal EPROM
programmer $467.50. Also adaptors,
(E)EPROM, PIC, 8051 programmers,
EPROM simulator and eraser.
Dunfield C Compilers: Everything you
need to develop C and ASM software
for 68HC08, 6809, 68HC11, 68HC12,
68HC16, 8051/52, 8080/85, 8086, 8096
or AVR: $198 each. Demo disk available.
ImageCraft C Compilers: 32-bit Windows IDE and compiler. For AVR, 68HC
08, 68HC11, 68HC12, 68HC16. $385.00
Atmel Flash CPU Programmer: Handles the 89Cx051, 89C5x, 89Sxx in
both DIP and PLCC44 and some AVR’s,
most 8-pin EEPROMS. Includes socket
for serial ISP cable. $220, $11 p&p.
SOIC adaptors: 20 pin $132.00, 14 pin
$126.50, 8 pin $121.00.
Full details on web site. Credit cards
accepted.
GRANTRONICS PTY LTD, PO Box 275,
Wentworthville 2145. (02) 9896 7150 or
http://www.grantronics.com.au
CENTRAL COAST FIELD DAY, SUNDAY 23rd FEB: Don’t miss Australia’s
biggest Amateur Radio exhibition
and sale of new and used radio and
communication equipment at Wyong
Race Course, just 1 hour north from
Sydney. Gates open 8.30am. Special
Field Day bargains from traders and
tons of disposals gear in the flea
January 2003 93
Silicon Chip
Binders
New New New
Mark22-SM
Slimline Mini FM R/C Receiver
REAL
VALUE
AT
$12.95
PLUS
P&P
These binders will protect your copies of SILICON CHIP. They feature
heavy-board covers & are made
from a dis
tinctive 2-tone green
vinyl. They hold up to 14 issues &
will look great on your bookshelf.
80mm internal width
•
•
•
•
•
6 Channels
10kHz frequency separation
Size: 55 x 23 x 20mm
Weight: 25gm
Modular Construction
Price: $A129.50 with crystal
Electronics
PO Box 580, Riverwood, NSW 2210.
Ph/Fax (02) 9533 3517
Satellite TV Reception
International satellite
TV reception in your
home is now affordable.
Send for your free info
pack containing equipment catalog, satellite
lists, etc or call for appointment to view.
We can display all satellites from 76.5°
to 180°.
AV-COMM P/L, 24/9 Powells Rd,
Brookvale, NSW 2100.
Tel: 02 9939 4377 or 9939 4378.
Fax: 9939 4376; www.avcomm.com.au
Need prototype PC boards?
We have the solutions – we print electronics!
Four-day turnaround, less if urgent; Artwork from your own
positive or file; Through hole plating; Prompt postal service; 29
years technical experience; Inexpensive; Superb quality.
Printed Electronics, 12A Aristoc Rd,
Glen Waverley, Vic 3150.
Phone: (03) 9545 3722;
Fax: (03) 9545 3561
Call Mike Lynch and check us out!
We are the best for low cost, small runs.
email: youngbob<at>silvertone.com.au
Website: www.silvertone.com.au
SILICON CHIP logo printed in
gold-coloured lettering on spine
& cover
Buy five and get them postage
free!
Price: $A12.95 plus $A5.50 p&p.
Available only in Australia.
Silicon Chip Publications
PO Box 139
Collaroy Beach 2097
Or fax (02) 9979 6503; or ring (02)
9979 5644 & quote your credit
card number.
Use this handy form
Enclosed is my cheque/money order for
$________ or please debit my
❏
Bankcard
❏
Visa ❏ Mastercard
Card No:
_________________________________
Card Expiry Date ____/____
Signature ________________________
Name ____________________________
Address__________________________
__________________ P/code_______
94 Silicon Chip
For price list, write Acetronics
5/32 Seton Rd, Moorebank 2170 or email
acetronics<at>acetronics.com.au
Phone (02) 9600 6832
www.acetronics.com.au
market. Exhibits by clubs and groups
with interests ranging from vintage
radio, packet radio, scanning, amateur
TV and satellite. www.ccarc.org.au
Ph (02) 4340 2500.
ROBOT KITS, books, accessories.
Check them out at: www.robotics.com.
au Free catalogue 1800 000 745.
KITS KITS AND MORE KITS! Check
’em out at www.ozitronics.com
LABJACK USB DATA ACQUISITION
MODULE features 8 12bit analog inputs, 20 digital I/O, 2 analog outputs
and high speed counter. Free software
and ActiveX component. DAS005
Parallel Port Data Acquisition Module features 8 12bit Analog inputs,
4 digital I/Ps & 4 digital O/Ps. Free
windows software. FAB Programmable Logic Controllers. Low cost, high
performance. Programming software
and SCADA software free. Heaps of
features. Full details and credit card
ordering available at:
www.oceancontrols.com.au
PCBs MADE, ONE OR MANY. Any
format, hobbyists welcome. Sesame
Electronics (02) 9586 4771.
sesame777<at>optusnet.com.au; http://
members.tripod.com/~sesame_elec
RCS HAS MOVED to 41 Arlewis St,
Chester Hill 2162 and is now open,
with full production. Tel (02) 9738 0330;
Fax 9738 0334. rcsradio<at>cia.com.au;
www.cia.com.au/rcsradio
www.siliconchip.com.au
Subscribe &
Get This FREE!*
*Australia only. Offer valid only while stocks last.
Positions At Jaycar
We are often looking for enthusiastic staff
for positions in our retail stores and head
office at Silverwater in Sydney. A genuine
interest in electronics is a necessity. Phone
02 9741 8555 for current vacancies.
Microzed.com.au
PIC CHIP SPECIALIST
PO Box 634 ARMIDALE 2350 (296 North Cooke’s Rd)
(02) 6772 2777 – may time out to Mobile 0438 277 634
(02) 6772 8987
Advertising Index
Acetronics....................................94
Altronics................................. 68-70
Av-Comm Pty Ltd.........................94
Clarke & Severn...........................81
Dick Smith Electronics........... 22-25
Elan Audio....................................83
Do you have a good circuit idea? We pay
up to $60 for contributions to Circuit
Notebook. Silicon Chip Publications, PO
Box 139, Collaroy, 2097.
THAT’S RIGHT! Buy a 1- or 2-year
subscription to SILICON CHIP magazine
and we’ll mail you a free copy of “Electronics TestBench”, just to say thanks.
Contact: Silicon Chip Publications,
PO Box 139, Collaroy, NSW 2097
Phone Orders: (02) 9979 5644
Fax Orders: (02) 9979 6503
Email Orders: office<at>silchip.com.au
FLUKE 123 SCOPEMETER: 60MHz,
still in box, as new with battery charger
+ all accessories $1100, ONO. Ph: 0412
621822 or (02) 9831 1673.
Audio, Video, S-Video and VGA cables
distribution amps, switchers, adaptors,
price lists at:
www.questronix.com.au
HALF RETAIL PRICE! Used Solar
Panels, Inverters, Batteries, Surplus
Components and more. See our specials pages at www.kcsolar.com.au
USB KITS: Stepper Motor Controller,
DTMF Transceiver, Thermometer, DDS
HF Generator, Compass, 4 Channel
Voltmeter, I/O Relay Card. Also available
Digital Oscilloscope, Temperature Loggers, VHF Receivers and USB OCXs
to control our kits from your application.
www.ar.com.au/~softmark
ADD SPEECH, SONAR OR DIRECTION SENSING to your next project.
Fully contained modules. Full specs on
website www.robotparts.com.au Ph
0412 350671
Evatco..........................................87
Grantronics..................................93
Harbuch Electronics.....................55
Instant PCBs................................94
Hy-Q International........................81
Jaycar ......................... 21,45-52,95
JED Microprocessors................5,81
Kalex............................................83
Microgram Computers...................3
MicroZed Computers..............81,95
Printed Electronics...................... 94
KIT ASSEMBLY
Procon Technology.......................81
KIT ASSEMBLY & REPAIR. Small production or one off. Phone Robin Frost
08 8357 4441.
Email: patrob<at>bigpond.com.au
Procopy........................................81
NEVILLE WALKER KIT ASSEMBLY
& REPAIR:
• Australia wide service
• Small production runs
• Specialist “one-off” applications
Phone Neville Walker (07) 3857 2752
Email: flashdog<at>optusnet.com.au
RF Probes....................................83
Quest Electronics.........................71
RCS Radio...................................94
Silicon Chip Binders............55,OBC
Silicon Chip Bookshop..........96,IBC
Silicon Chip TestBench..............IFC
Silvertone Electronics.............81,94
NOW
AVAILABLE
FROM
Soundlabs Group.........................81
www.siliconchip.com.au
Project Reprints
Limited Back Issues
Limited One-Shots
If you’re looking for a project from ELECTRONICS AUSTRALIA, you’ll find it at SILICON CHIP! We
can now offer reprints of all projects which have appeared in Electronics Australia, EAT, Electronics
Today, ETI or Radio, TV & Hobbies. First search the EA website indexes for the project you want
and then call, fax or email us with the details and your credit card details. Reprint cost is $8.80 per
article (ie, 2-part projects cost $17.60). SILICON CHIP subscribers receive a 10% discount.
We also have limited numbers of EA back issues and special publications. Call for details!
visit www.siliconchip.com.au or www.electronicsaustralia.com.au
www.siliconchip.com.au
Telelink Communications.............81
Wiltronics.....................................81
_________________________________
PC Boards
Printed circuit boards for SILICON
CHIP projects are made by:
RCS Radio Pty Ltd. Phone (02) 9738
0330. Fax (02) 9738 0334.
January 2003 95
REFERENCE
GREAT BOOKS FOR
ALL PRICES INCLUDE GST AND ARE
AUDIO POWER AMPLIFIER DESIGN HANDBOOK
PIC Your Personal Introductory Course
A handbook for professionals and students
from one of the world’s most respected
audio authorities. New edition is more
comprehensive than ever with a new
chapter on Class G amplifiers and
further new material on output coils,
thermal distortion, relay distortion,
ground loops, triple EF output stages and
convection cooling. 427 pages in paperback.
Concise and practical guide to getting up and
running with the PIC Microcontroller. Assumes no
prior knowledge of microcontrollers, introduces
the PIC’s capabilities through simple projects.
Ideal introduction for students, teachers, technicians and electronics enthusiasts – perfect for
use in schools and colleges. 270 pages in soft
cover.
by Douglas Self 3rd Edition 2002
89
$
by John Morton – 2nd edition 2001
NEW
NEW
NEW
NEW
46
$$
VIDEO SCRAMBLING AND DESCRAMBLING
AUDIO ELECTRONICS
If you've ever wondered how they scramble
video on cable and satellite TV, this book tells
you! Encoding/decoding systems (analog
and digital systems), encryption, even
schematics and details of several encoder
and decoder circuits for experimentation.
Intended for both the hobbyist and the
professional. 290 pages in paperback.
For anyone involved in designing, adapting and
using analog and digital audio equipment. It
covers tape recording, tuners and radio receivers,
preamplifiers, voltage amplifiers, audio power
amplifiers, compact disc technology and digital
audio, test and measurement, loudspeaker
crossover systems, power supplies and noise
reduction systems. 375 pages in soft cover.
By John Linsley Hood. First published 1995.
Second edition 1999.
FOR SATELLITE AND CABLE TV
by Graf & Sheets
2nd Edition 1998
4th
EDITION
$
70
87
$
EMC FOR PRODUCT DESIGNERS
3rd
EDITION
UNDERSTANDING TELEPHONE ELECTRONICS
By Stephen J. Bigelow. 4th edition 2001
Based mainly on the American telephone system, this book covers conventional telephone
fundamentals, including analog and digital
communication techniques. Provides basic information on the functions of each telephone
component, how dial tones are generated and
how digital transmission techniques work.
402 pages, soft cover.
103
$$
By Eugene Trundle. 3rd Edition 2001
3rd
EDITION
Eugene Trundle has written for many years in
Television magazine and his latest book is right
up to date on TV and video technology. includes
both theory and practical servicing information
and is ideal for both students and technicians.
382 pages, in paperback.
Widely regarded as the standard text on
EMC, provides all the key information needed
to meet the requirements of the EMC Directive.
Most importantly, it shows how to incorporate
EMC principles into the product design process, avoiding cost and performance penalties,
meeting the needs of specific standards and
resulting in a better overall product. 360 pages
in paperback.
63
$
By Ian Hickman. 2nd edition1999.
Essential reading for electronics designers and
students alike. It will answer nagging questions
about core analog theory and design principles
as well as offering practical design ideas. With
concise design implementations, with many of
the circuits taken from Ian Hickman’s magazine
articles. 294 pages in soft cover.
by Dogan Ibrahim. Published 2000.
by Steve Roberts. 2nd edition 2001.
Based mainly on British practice and first published in 1997, this book has much that is relevant to Australian systems as a guide to home
and small business installations. A practical
guide to installation of telephone wiring, ranging
from single extension sockets to PABX, with the
necessary tools, test equipment and materials
needed by installers. 178 pages in soft cover.
89
$$
Microcontroller Projects in C for the 8051
TELEPHONE INSTALLATION HANDBOOK
69
By Tim Williams. First published
1992. 3rd edition 2001.
ANALOG ELECTRONICS
GUIDE TO TV & VIDEO TECHNOLOGY
$
92
$
$
73
Through graded projects the author introduces the
fundamentals of microelectronics, the 8051 family,
programming in C and the use of a C
compiler. The AT89C2051 is an economical chip with re-writable memory.
Provides an interesting, enjoyable and
easily mastered alternative to more theoretical
textbooks. 178 pages
in paperback.
BOOKSHOP
ENQUIRING MINDS!
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Power Supply Cookbook
Analog Cct Techniques With Digital Interfacing
by T H Wilmshurst. Published 2001.
by Marty Brown. 2nd edition 2001.
An easy-to-follow, step-by-step design framework for a wide variety of power supplies. Anyone with a basic knowledge of electronics can
create a very complicated power supply design .
Magnetics, feedback loop, EMI/RFI control and
compensation design are all described in simple
language. 265 pages in paperback.
99
VIDEO & CAMCORDER
SERVICING AND TECHNOLOGY
by Steve Beeching (Published 2001)
$
69
$
$
Provides fully up-to-date coverage of the whole
range of current home video equipment, analog
and digital. Information for repair and troubleshooting, with explanations of the technology of
video equipment. 318 pages in soft cover.
69
Antenna Toolkit
by Joe Carr. 2nd edition 2001.
Together with the CD software included, the reader
will have a complete solution for constructing or using an antenna - bar the actual hardware. The software is based on the author’s Antler program, which
provides a simple Windows-based aid to carrying
out the design calculations at the heart of successful
antenna design. 253 pages in paperback.
NEW
NEW
NEW
NEW
PIC IN PRACTICE
O
R
D
E
R
H
E
R
E
by Howard Hutchings. Revised by Mike James.
2nd edition 2001.
63 $$63
$
Anyone interested in ports, transducer interfacing,
analog to digital conversion, convolution, filters or
digital/analog conversion will benefit from reading
this book. The principals precede the applications
to provide genuine understanding and encourage
further development. 302 pages in paperback.
PRACTICAL RF HANDBOOK
by Ian Hickman 3rd Edition 2002
by D W Smith Published 2002
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 microcon-trollers for hobbyists, students and professionals.
255 pages in paperback.
87
$
Interfacing With C
Electric Motors And Drives
by Austin Hughes. 2nd edition 1993.
Reprinted 2001.
For non-specialist users – explores most of the
widely-used modern types of motor and drive, including conventional and brushless DC, induction,
stepping, synchronous and reluctance motors. 339
pages, in paperback.
Covers all the analog electronics needed in a wide
range of higher education programs: first degrees
in electronic engineering, experimental science
course, MSc electronics and electronics units for
HNDs. Text is supported by numerous worked
examples and experimental exercises. 312 pages
in paperback.
52 69
$$
$$
A guide to RF design for engineers, technicians,
students and enthusiasts. Covers all of the key
topics in RF: analog design principles, transmission lines, transformers, couplers, amplifiers,
oscillators, modulation, transmitters and receivers,
propagation and antennas. 279 pages in paperback.
NEW
NEW
NEW
NEW
TAX INVOICE
ANALOG CIRCUIT TECHNIQUES W/DIGITAL INT............$69.00
Your Name_________________________________________________
ANALOG ELECTRONICS..................................................$89.00
PLEASE PRINT
ANTENNA TOOLKIT.........................................................$87.00
Address ___________________________________________________
AUDIO ELECTRONICS.....................................................$92.00
___________________________________ Postcode_______________
AUDIO POWER AMPLIFIER DESIGN...............................$89.00
Daytime Phone No. (______) __________________________________
ELECTRIC MOTORS AND DRIVES..................................$63.00
STD
EMC FOR PRODUCT DESIGNERS.................................$103.00
Email___________________<at>_________________________________
GUIDE TO TV & VIDEO TECHNOLOGY............................$63.00
INTERFACING WITH C.....................................................$63.00
❏ Cheque/Money Order enclosed OR
M'CONTROLLER PROJECTS IN C FOR 8051..................$73.00
❏ Charge my credit card – ❏ Bankcard ❏ Visa Card ❏ MasterCard
PIC IN PRACTICE............................................................$52.00
PIC - YOUR PERSONAL INTRODUCTORY COURSE........$46.00
No:
POWER SUPPLY COOKBOOK..........................................$99.00
PRACTICAL RF HANDBOOK............................................$69.00
Signature______________________Card expiry date
TELEPHONE INSTALLATION HANDBOOK.......................$69.00
UNDERSTANDING TELEPHONE ELECTRONICS.................$70.00
PLUS P&P (if applic): $...........................
TOTAL$ AU..............................
VIDEO & CAMCORDER SERVICING/TECHNOLOGY........$69.00
VIDEO SCRAMBLING/DESCRAMBLING..........................$87.00
Orders over $100 P&P free in Australia.
POST TO: SILICON CHIP Publications, PO Box 139, Collaroy NSW, Australia 2097.
AUST: Add $A5.50 per book
OR CALL (02) 9979 5644 & quote your credit card details; or FAX TO (02) 9979 6503
NZ: Add $A10 per book, $A15 elsewhere
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P&P
ALL TITLES SUBJECT TO AVAILABILITY. PRICES VALID FOR MONTH OF MAGAZINE ISSUE ONLY. ALL PRICES INCLUDE GST
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