SolderSmoke Podcast #157: Peter Parker on Phasing Rigs

SolderSmoke Podcast #157 is available for download.
http://soldersmoke.com/soldersmoke157.mp3

December 27, 2013

-- Santa Report:  Rigol Scope at SolderSmoke HQ.  Kites at VK3YE.
-- Project updates:   Bill's BITX 40/20 build. 
-- Peter finishing up BITX40  (in a big box)
-- BITX 17 (5 watts SSB) works JA, ZD7, ZS!
-- The mystery, elegance, and gentleness of phasing SSB
-- Phasing explained in 1970 ARRL SSB book
-- Phasing SSB: From Hallicrafters HT-37 to SDR
-- The SP5AHT Phasing Rig
-- I & Q for you:  The Binaural Experience
-- Direct Conversion receivers and Software Defined Radios
-- Simple DC receivers plugging into sound cards 
-- The joy of receiver building
-- 144 MHz aircraft bounce (Melbourne to Sydney)
-- VHF Across The Great Australian Bight  

HAPPY NEW YEAR TO ALL!

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Santa Arrives at SolderSmoke HQ! Rigol and Black&Decker

Santa Claus obviously heard my distress call when the TEK 465 gave up the ghost.  This morning it was replaced by a RIGOL digital scope.   I'm going through the tutorials.  Wow, lots of features.  A Black&Decker jig saw also arrived -- this will help in my cabinetry efforts. 

Last night just before dinner I talked to Kiyo, JH1MDJ, in Tokyo on 17 meter SSB with the 5 watt BITX.   I kind of broke through a small pile-up and we then had one of those "please repeat your power level... I can't believe that is 5 watts to a dipole" conversations.  

Happy Holidays to all!

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How they took the iconic Apollo 8 Earthrise Photo (Amazing Video)

I was ten years old and totally obsessed with the space program.  This video brought back a lot of the magic. Wow. You really have to see this one.


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Where to send all those LM386 chips: Make them BEAM robot brains!

Over in the BITX20 yahoo group there have been some comments about the shortcomings of the widely used LM386 audio amplifier chip.  Many people don't like it because it is noisy.  I don't like it because it is a chip. (In my BITX rigs I have replaced it with a simple discrete component audio amplifier.)  So this morning I was pleased to find this video on the Maker blog that presents a very good use for all those LM386 devices:  We can turn them into robot brains!

Make's video and web page on this project are both very good.   One paragraph in the page kind of captures the reasons I dislike the LM386:

How It Works

The core of the “Herbie” circuit is the LM386 power amplifier chip. To simplify a bit, we can think of the chip as a “black box” with inputs and outputs that respond in predictable ways, and don’t have to completely understand what’s going on inside. 

 http://makezine.com/projects/sunbeam-seeker-bot/

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Christmas Eve Fessenden Memorial Broadcast on 486 KHz

Imagine it is Christmas Eve, 1906 and you are on the air, listening to the harsh buzz of Ol' Spark Morse Code.  Suddenly, in the headphones you hear a human voice and music.

Brian Justin  has set up an experimental station that recaptures that magical "birth of radio telephony" moment.   He will be on the air this Christmas Eve, Christmas Day and New Year's day.   Here is what W4DEX heard during last year's event:

http://www.w4dex.com/500khz/wf9xih/wf9xih_24dec11.mp3


Experimenter to Honor Early Wireless Pioneers with Longwave Transmissions

Fessenden

As he has over the past several years, Brian Justin, WA1ZMS/4 -- as experimental station WG2XFQ -- will transmit voice and music on 486 kHz on Christmas Eve and Christmas Day and again on New Year's Eve and New Year's Day. Transmissions will begin at 0001 UTC and end at 2359 UTC. Justin, who may be better known for his microwave exploits on ham radio, will use an AM audio loop modulating his vintage-style, homebrew transmitter to honor Reginald Fessenden's Christmas Eve 1906 AM voice transmission.

WA1ZMS constructed his MOPA transmitter from 1920s-vintage components. [Brian Justin, WA1ZMS, photo]

"While his original transmissions used a set of carbon microphones in the antenna lead to modulate the signal," Justin explained, "WG2XFQ will be utilizing true Heising modulation in honor of Raymond Heising, who developed this early form of amplitude modulation during World War I.Justin constructed his 5 W master oscillator power amplifier (MOPA) transmitter using 1920s-vintage components. He said a modern 500 W FET linear amplifier allows him to meet his WG2XFQ ERP limit of 20 W. An RF engineer, Justin collects pre-1920 wireless gear and has a World War I Heising-modulated aircraft transmitter he's planning to restore. Justin was an active participant in the ARRL's WD2XSH 600 meter experimental project.

(From the ARRL Newsletter)

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BITX 2040 Build Update #2: Of Spreadsheets and VFOs

I continue to tweak the capacitors in my new BITX 20/40 VFO (scroll down to see it).  On Sunday I added a little relay that will switch in some additional capacitance to move the VFO about 500 kHz.  Without the additional cap, the VFO will be on frequencies suitable for 40 meters -- with the additional cap it will be on frequencies needed for tuning 20 meters. 

I calculated that I'd need an additional 220 pf to make this shift ( I later went with 100 pf).  In went the needed cap and relay.  It worked.  But there was a problem:  On 40 I had the desired 175 kHz frequency range.   But I found that with this arrangement on 20 I could only cover 95 kHz.   Obviously my variable air cap with 44 pf in series was being "diluted" by the additional 220 pf being switched in by the relay -- with the additional capacitance, the change in total capacitance produced by the variable cap (with series cap) was smaller in the 20 meter range than it was in the 40 meter range. 

Clearly, one solution was to play with the value of the cap that I had in series with the variable cap -- increasing it would increase the freq spread (both on 40 and 20).  But how much should I increase it?

By this point I was getting tired of all the manual calculations.  Time for a spreadsheet! I created one, and threw in the values of all the caps and of the coil,  and the resonant frequency formula.  I set it up to display and the resulting freq coverage. 

The freq ranges in the actual ham bands is a bit off -- there may be some stray capacitance and inductance in the circuit that is not being captured in my numbers.   But the important thing was the spread.  The spreadsheet allowed me to see that with a 100 pf cap switched in by the relay and a 74 pf cap in series with the variable, I could cover 180 kHz on 40 and 123 kHz on 20.  That's OK.  This little exercise shows the usefulness of spreadsheets in dealing with this kind of calculation.

You can see my spreadsheet here:
https://docs.google.com/spreadsheet/ccc?key=0Ak4BJL1-oWiJdElieDY5Y2xVWUtSNDl0anRYLVBBeGc&usp=drive_web#gid=0

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20/40 BITX Build Update #1: VFO Success

I've started construction on my second BITX transceiver, this one for 20 and 40 meters.  As with the previous rig, I decided to take the VFO first, but this time I pledged not to surrender, not to wimp out with a VXO or (worse!) a DDS.   No, this time it would be a real LC VFO.

I took seriously all the admonitions in the tech literature about the fickle permeability of ferrite and iron powder, so this time I used an old-fashioned air-core coil.  It is wound around a cardboard tube.  The tube was previously the bottom portion of a coat-hanger from the dry cleaner.  I wound 40 or so turns on this core, then measured the inductance:  5.6 uH -- that looked about right.

For the oscillator stage I used a Colpitts circuit very similar to the one in the original BITX schematic (but I am hoping I won't need the varactor diode fine tune mechanism).   I had on hand a nice Heathkit 19-146 pf variable cap with an internal 4:1 reduction drive.  Not wanting to pluck rotor places out of this beautiful part, I had to calculate the series capacitance that would yield a frequency spread of about 175 kHz.  It turned out to be 40 pf.  Then I had to figure out how much capacitance to put in parallel with the variable.  Well, it all ended up like this:

There was a bit of trial and error in the process of getting the VFO to cover the desired range.  A big help in all this was an on-line reactance calculator.  I found this one to be very useful:

  
http://www.1728.org/resfreq.htm

I found that the VFO is more stable if I reduce the voltage from 12 volts down to about 8.  Also, I found that when evaluating the stability, it is better (psychologically!) just to use a stable superhet receiver instead of the frequency counter.  The counter may appear to be jumping around a lot, especially if the signal you are monitoring is not very strong.  Just listening to it at zero beat on the superhet is very reassuring.

I followed the Colpitts oscillator with the FET buffer and two stage BJT amplifiers from page 50 of Doug DeMaw's QRP Notebook (page 50).  I now have the requisite 7 dbm signal.  And it appears to be quite stable. 

I plan using this with an 11 MHz IF, with the VFO running at around 3.875--3.700 for 40 meters and 3.175 -- 3.355 for 20.   I plan to use a small relay to switch in some additional capacitance to move the VFO down to the range for 20 meters.


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University of Twente's Online Receiver

Wow, I played with this on-line SDR receiver a few years ago and thought it was fantastic.   It is now even better.  I'm sitting here listening to 40 meters in the Netherlands.  Great stuff.   Check it out.  It is really amazing:

http://websdr.ewi.utwente.nl:8901/

Thanks to Bob, KD4EBM for letting me know about the updates. 

Our book: "SolderSmoke -- Global Adventures in Wireless Electronics" http://soldersmoke.com/book.htm Our coffee mugs, T-Shirts, bumper stickers: http://www.cafepress.com/SolderSmoke Our Book Store: http://astore.amazon.com/contracross-20

Circular Polarity and The Water Wheel in Dale's Moonbounce Amplifier

Bill:

 

I'll attach some pix of the feedhorn and LNA for you.

The importance of circular  feeds is that as a linear wave passes through the ionosphere, it undergoes Faraday rotation. So it may arrive at  the station you are talking to having been twisted 90 degrees. This  is a slow progressing process and  on  all bands except 23cM, may cause EU for example to be locked out for hours at a time for linear stations.

With circular polarity, Faraday is a non issue. The feedhorn almost all of us use is a VE4MA that has separate TX and RX probes. The circular polarity is synthesized as the linear wave propagates down the circular waveguide and encounters sets of  capacity stubs. The exact opposite occurs for waves entering the waveguide. The result is we get CW and CCW without having to use any relays (loss) and phasing  lines (loss).

My LNA has a noise figure of under 0.24dB and uniquely connects to a protection relay with no cable or adapters (loss).

The position of the feedhorn and its scalar ring is tediously adjusted by measuring the difference between sun noise and cold sky. W4SC developed a very accurate and repeatable process that uses an SDR RX for this.

I use  a modified C band satellite drive system known as a polar mount so I only need one motor drive to track the moon.

Anyway, hearing my own echoes off the moon was and still is the highlight of my amateur career. 

 

The photos are the feedhorn + LNA, My first water cooled 500W  tube amp, my previous 400W solid state amp (mounts right at the dish). My current design is 600W solid state and will also mount at the dish.

BTW, that little circle in the middle of the tube amp is a paddle wheel that turns as long as water is flowing. A tachometer on the wheel sounds an alarm and shuts down plate voltages   should the wheel stop turning.

I'll keep  you up to date on my BB RX progress- thank you again Bill.

Dale W4OP

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The NASA Juno Fly-by "Hams say HI to Juno" Video (very nice)

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The QRP Mojo Ceremony

More from Lobstercon (from N2HTT): 
 http://n2htt.net/2013/11/24/there-are-lobsters-in-the-woods/
And thanks to Pete, VE2XPL, for alerting me to all this. 

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Need help with part construction...

Please take a look and see if you can help me figure out how to make this thing.  The diagram is eschpecially illuminating.

 

 

THE DIE-CAST DROP-FORGED PLASTIC

TRICHOTOMETRIC INDICATOR-SUPPORT

          Inquiries concerning the mounting of the Trichotometric Indicator

          Support indicate that some difficulty is being experienced with the

          brackets which attach the support. As an aid toward fabricating the

          support brackets, the accompanying illustration is provided to show

          the type of material as well as the dimensional data needed. It will

          be noted that in attaching the bracket to the support a special ambi-

          melical hexnut is used. The application of this nut is unique in that

          any attempt to remove it in the conventional manner only tightens it.

          Because of this design, the nut must be fully screwed on before it can

          be screwed off.

 

DRAWN BY	FRED SPOON	SCALE ¼”=1 MILE
NO. 43906		FILE – BAR NONE

 Thanks to ZL2DEX for bringing this to our attention.

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