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Wednesday, September 9, 2009

Hubble Space Telescope: New and Improved!

I know, I know, it is not exactly ham radio, but look at it this way: electromagnetic waves from far, far away! REAL DX. And some very cool gear to receive the signals. And some recent repair and modification work... So you see, this is really not so far afield after all.

I've been a big fan of the Hubble Space Telescope for a long time. When I was closer to the equator (in Santo Domingo) sitings of the HST were quite common. I'm glad to see that the recent repairs and mods worked out so well. Here is a really nice video on the new and improved Hubble: Hubble Space Telescope Video

Saving the world, finding comets....

Well I guess the hours are not great, but how about the job satisfaction! Rob McNaught works at the Sliding Spring Observatory about 400 km from Sydney, Australia. The observatory searches for comets and asteroids that could do to us what they may have done to the dinosaurs (see below). A significant fringe benefit of this job is that Rob gets to discover new comets. He recently set world record by finding his 50th. Congrats Rob!

The mission of the Siding Spring Survey is to contribute to the inventory of near-earth objects (NEOs), or more specifically, the potentially hazardous asteroids (PHAs) and comets (PHOs) that may pose a threat of impact and thus harm to civilization. The identification of the iridium anomaly at the Cretaceous-Tertiary boundary (Alvarez et al., 1980) and associated Chicxulub impact crater (Hildebrand et al., 1991) and perhaps recently the Australian Bedout crater (Becker et al., 2004) associated with the Permian- Triassic "great dying" (although the presence of shock metamorphism has not yet been adequately demonstrated), strongly suggests that impacts by minor planets play an important role in the evolution of life. These are a natural result of the accretionary process that formed the Earth and planets. Indeed, the 1994 impact of D/Shoemaker-Levy 9 on Jupiter provided tangible evidence of this. Although the collision frequency is much lower than in the past, the question is not whether there will be other impacts, but when.

Tuesday, September 8, 2009

Early Crystal Set in Altoids-like Box


Even way back then, British homebrewers had an affinity for Altoids-like boxes!
David, M0VTG, sent me the above pictures, and this description:

I enclose some pictures of a kit produced in the early to mid 1900s of crystals and a holder for use in a crystal radio; unfortunately the cats whisker is missing! The box is marked:

Front: NEUTRON Back: Neutron Ltd
Trade Mark Sicilian House
Wireless Crystal Southhampton Row
1/6 Phone Museum 2017
Catswisker and
Directions Enclosed

The 1/6 refers to the price (one shilling and six pence) pre-decimalization and converts to seven and a half pence today (although the half pence has been dropped thorough inflation). I should add that the box measures about an inch and a half in length.

Saturday, September 5, 2009

Carrington Flares, Aurora, Where were you on August 4, 1972?

Greg, KC2DWF, sent me a really interesting story about the work of the English solar astronomer Richard Carrington. He discovered a kind of solar flare (named for him) that comes along every few centuries and could knock us all off the air.

As I was reading the article, I started to think about a childhood event that I think I mentioned in one of the podcasts. I have vivid memories of a summer night in which the skies were filled with really bright colorful lights. The article about Carrington notes that there was a major solar flare (but not of Carrington levels) on August 4, 1972 that caused auroral displays far into the southern part of the USA. The year is a bit later than I thought (I was 13 at that time) but the time of year is correct. And that flare was big enough to have caused really vivid aurora over New York.
The NASA site "Brushfires in the Sky" provides this very helpful list for people, like me, trying to figure out what we saw, and when:

The Aurora Watchers Handbook lists the following "Great Geomagnetic Storms" of the 20th century when auroras were seen much farther south than usual. If you have a childhood memory of aurora borealis, it may have come from one of these storms.

  • October 31 - November 1, 1903
  • September 25, 1909
  • May 13-16, 1921
  • April 16, 1938
  • February 11, 1958
  • July 8, 1958
  • August 4, 1972
  • December 19, 1980
  • March 13-14, 1989
Looks to me like my event was August 4, 1972. Anyone else have memories of this storm?

Here is the article that Greg sent:
http://science.nasa.gov/headlines/y2008/06may_carringtonflare.htm

The Transistor Museum

Wes, W7ZOI, relayed to us this great site found by from Jeff Damm, WA7MLH. This is a real treasure trove of transistor history:
http://semiconductormuseum.com/Museum_Index.htm

Thursday, September 3, 2009

Alaska QRSS Grabber Controlled from CHINA!

Our friend Laurence leads an interesting life...

http://www.kl1x.com/

Hi Bill and greetings from the NE coast of still summery China - actually its cooling down a bit from boiling over to just cooking.

Just been home to Alaska. Whilst and between lumberjacking 20 dead trees on the property I had a few mins to throw up a K9AY and connected it via 250ft of Walmarts best RG6U into the R75 - with a little help of Ham radio delux, Citrix and Skype I have control of the radio from here in China - Mostly on 30m but really shoved it up for the winter lf/mf season but of course WSPR and visual modes have proved very popular. So until a moose walks thru, a Wolf chews threw or wife cuts thru the antennae wire it will be up.

Here in China I'm sporting the second r75 and this supplements the SDR IQ - my antennae are gradually getting blocked towards the states and Eu by every rising high rises just in front and I can actually measure the increasing losses at LF and HF as the beast rise. Still looking for your WSPR signal and keep up the good work.

Regards
Laurence G4DMA et al - KL1 X and in BY3A

Tuesday, September 1, 2009

A Good Old VFO (by Rick, KK7B)

Here is another really great message from Rick, KK7B, sent to the emrfd yahoo group: [emrfd] A Good Old VFO Saturday, August 22, 2009 10:29 PM From: Rick To: emrfd@yahoogroups.com For several critical receiver applications in my lab I've used old Collins PTOs converted to solid state (I just replace the triode in the classic Hartley circuit with a J310 and run the circuit from a 9 volt regulator). I have half a dozen of them in dedicated propagation study receivers, and one SSB exciter I occasionally use on UHF. The other day I was changing something else in one of my receivers and connected the solid-state PTO to the frequency counter on my bench. The PTO was set to 3.100000 MHz. From a cold start (it hadn't been turned on for years) it drifted three Hz over the first ten minutes, and then a total of 10 Hz over the next few hours. When I calibrated one of my 144 MHz propagation study receivers 25 years ago, total frequency drift was <18Hz/hour. I expect most of that was aging of the overtone crystal oscillator in the premix circuit. Old Collins PTOs are common (someone at Dayton this year had a box of unknown ones in decent shape for $10 each, and there are R390 PTOs in the current Fair Radio flyer). I've never had one fail, tuning resolution is infinite, phase noise is low, digital noise is zero, and once I build one into a receiver, that part of the project is done--no improvements, software upgrades, needed. My research receivers are connected to a baseband Fourier analyzer (yes...even 25 years ago). The finest resolution I've used for serious experiments is 10 milliHertz, but more often I use 1 Hz resolution, with 1024 channels in the output spectrum. I often average spectra for more than a minute, so frequency drift needs to be less than 1 Hz per minute. The solid-state Collins PTO is much more stable than needed even for those critical experiments. This is not a fluke. Every Collins PTO I've converted to solid state using a U310 or J310 has had similar performance. Sometimes it is useful to remember that the major benefit of digital frequency synthesis is that it is quick, cheap, and frequency agile. No commercial manufacturer could afford to build a transceiver with a Collins Mil-Spec PTO in it these days. But for an amateur with mechanical skills or access to surplus hardware who needs just one good oscillator, the venerable Hartley with a temperature compensated tuned circuit and a JFET can provide outstanding performance. In music, art, architecture, automobiles, motorcycles. .. there are recognized "golden eras" where some combination of factors resulted in technical hardware that is widely recognized as being superior to what is being produced today. Often the difference is directly related to the amount of skilled labor needed during production. As technical hobbyists, we automatically assume that new is better, but as experimenters, we should be open to the idea that sometimes the technology, ideas, and block diagrams of an earlier era are superior to the cost-driven disposable technology coming off fully automatic assembly lines in some out-of-the-way place with inexpensive labor and attractive business tax codes. The idea that old technology designed decades ago by retired guys might be better than new technology is a radical concept in electronics. But NASA is using a brand new, hand built, Traveling Wave vacuum tube in the current Moon exploration mission. After 100 years of radio experiments- -it is fun to look back and find old technology that might actually work better than some of the new things we've been inventing recently. Best Regards, Rick KK7B

Sonya's Rig

Stewart, G3YSX, provided us with Part II of his article on the espionage radio work of the Soviet spy Sonya (who had the Knack).

Sonja Continued

A few days after my article on Sonja the Spy was published in the September 2004 edition of the CARC newsletter, I received a letter from club member Eddie Ramm
DK3UZ filling in a few additional details.

The Fuchs antenna that Sonja used was first described by Dr Josef Fuchs, OE1JF, in 1928 and is a half-wave end-fed design.

End-fed half-wave antennas are very efficient and do not need a particularly good ground, but they are very high impedance and need a suitable matching circuit. For a spy the use of a simple, but efficient, antenna of this type would have its attractions.

Eddie then pointed out that the design is of current interest to the QRP community by pointing me to the following URL: http://www.qrpproject.de/UK/fuchs_ant_.htm. This describes a 5 band portable QRP antenna designed by Frank, DL7AQT, based on the Fuchs design. The antenna is a 40m to 42m length of wire and the ATU is a parallel tuned circuit using a pair of toroids and a 200pf variable capacitor. It is worth reading the English version of the manual, which discusses the issue of self-resonance in these high impedance matching circuits. Matching circuits of this type only function correctly below the self-resonant frequency. Frank used of a two toroid arrangement to the move the self-resonance from 18MHz to 60MHz, thereby producing an ATU that operated correctly from 80m to 10m.

The second point that Eddie raised was the term “Three Point Oscillator” that Ruth used to describe her (Sonja’s) transmitter. The German term is “Dripunktsender” (three point sender), which Eddie tells me is the term was used to describe both the Hartely and the Colpitts based transmitters. Both oscillator designs are similar in the way that they use the reactive components in the tuned circuit as an impedance transformer to provide the coupling between the tuned circuit and the amplifier, so the use of the common term makes sense. He included an article dated January 1939, which shows a 3W automatic transmitter for maritime use, which is of the Hartley design and is described as a Dripunktsender. The article can be found at http://www.radiomuseum.org/funkschau/1939/funkschau_12jg_0339_1v2.pdf and the Hartley transmitter circuit is shown above.

We have no way of knowing which type Sonja actually used, although, as I suggested before I would suspect that it was the Hartley. This is likely because the Hartley was popular in the amateur radio world at the time and we know that she improved here spy transmitter by using amateur radio techniques. Secondly, because her transmitter had to fabricated, without raising suspicion, using material found in the field, a Hartley would seem to be the preferred design. A Hartley has no critical capacitors, just a coil which can be fabricated out of an “innocent” piece of wire or metal, and adjusted to give both the right inductance and the right feedback.

Stewart G3YSX

Saturday, August 29, 2009

SolderSmoke Podcast 114

A particularly big one. Not the one we heard.

http://www.soldersmoke.com

Roman Forum, Sabina, Snakes! Wild Boar!
Amateur Engineering?
WSPRing again (cheap thrills?)
Trastevere flea and a return to 1995
Electric airplanes
Ether rediscovered?
Galileo!
Sir Douglas Hall
Sonya had The Knack
Altoidism?
MAILBAG

Jean Shepherd and "I, Libertine"

This provides a lot of insight into what Shep was all about:
http://www.bobkaye.com/ilibertine.html

Friday, August 28, 2009

Sonya had The Knack

Stewart, G3YSX, sent us an article that he wrote some time ago for the Crawley ARC. Thanks Stewart. (This is an abridged version of the article. ) Very interesting:

Sonya
Sonya is the code name of Ruth Werner ne Kuczynski 1907 - 2000. Sonja is of interest here because her role in the GRU was as a clandestine radio operator. In her autobiography “Sonya’s Report” she gives a little insight into her work.

Trained in Moscow in the early 1930’s Soviet radio operators had to learn to build their own transmitters on site, using available materials. In rural China she and her accomplice (whom she lived with as husband and wife) set about building their first transmitter using receiver parts. There is an interesting story of how she had her real husband ship the transformer (a heavy 8 inch cube) up from Shanghai in the seat of a chair. Under the stresses of travel this nearly split from the chair which might have terminated her career as a clandestine radio operator before it started. This was the first of many incidents in which only luck prevented discovery of her activities.

Their first transmitter was a “three point” Hartley set, much improved by studying an amateur radio handbook of the time. It is not clear whether this was an oscillator, buffer, PA, whether she meant a Hartley transmitter that used three valves in parallel, perhaps that it was a single stage transmitter, with a two stage receiver in the classic paraset fashion. On the other hand it is known that she had a domestic set and it was not uncommon of them to be shortwave capable at that time. Building and setting up the transmitter must have been something of a challenge because she would not have had access to test equipment. In particular she implies that the transmitter was VFO controlled (presumably crystals were fragile and a security risk, both when making a boarded crossing and being on a fixed frequency). Under these circumstances getting setting set up on frequency must have been really difficult. I would imagine that this must have required her to find a reference frequency sent by control, net her transmitter and then send. Not easy with a power oscillator design and a receive that would be pulled by such a strong signal. The set had to be hidden when not in use. The Morse key was improvised out of a Chinese paperweight (actually a type of steel ruler) and a bolt and was dismantled during the day.

Antennas were not so much a problem because large outside receiving antennas were common. Ruth talks about asking permission from her landlord in Oxford to put up her antenna and receiving help from her unsuspecting host. From here text it seems that antennas were mostly long wires, although she talks about a “Fuch’s” antenna, a type that I am not familiar with.

In one house (in Warsaw I think) she started transmitting and this immediately blew the fuse for the house. She then had to quickly dismantle and hide the apparatus in the dark, lest her rented room be searched looking for the cause of the fault. In another apartment in Switzerland she had to close down and move sites (suddenly move house) because of EMC problems. Luckily (for her) one of her neighbours commented to Ruth that her husband (a Nazi) was sure that someone was operating a transmitter nearby which was causing interference to their radio receiver, and that he would organize a search later that week when he returned from a trip.

Ruth notes in passing that the absence of amateur radio traffic during the war was a problem because Soviet operators used to use it as a cover for their clandestine activities. It is not clear whether she was operating in the amateur bands giving the authorities too many Morse signals to monitor (unlikely because the non-amateur nature of the traffic would have been observed and reported by the radio amateurs), whether she was posing as a radio ham (again unlikely because of the tight regulation) or more likely, in my view, using our activities as a cover for both EMC problems and - to the unskilled – for strong local morse received on the shortwave bands.

In 1937 whilst operating out of Warsaw, Ruth talks of one evening when after setting up the transmitter, she caught here hand across the HT (two 120v batteries in series). She could not remove her hand without the help of an accomplice, by which time it was painfully burnt. She then got a hard time from her controller for failing to get a 50 group message out that night through extreme QRN. It later out that there had been a major solar even that night which had disrupted all radio communications. However she appears to have been working for the sort of organization that trucked no excuse, not even acts of
God.

Ruth would typically transmit at night between two and four times a week. Messages were 60 to 500 groups. Assuming 20 WPM with perhaps 30% time allocated to repeats and other procedure transmissions would have taken at least 45 minutes. In practice however, due to the difficulty of copying, transmissions often took half the night. It is therefore very surprising that she was never caught. In particular, given the hard time that the GPO gave the amateur radio community during the late 1940’s when she was handling the Fuch’s traffic, it would be very interesting to know why they never found her station in rural Oxford.

Ruth’s autobiography, which is out of print, but available from East Sussex libraries, unfortunately lacks much of the detail that one would have expected from a western text written so long after the event. This is undoubtedly a result of the excessive secrecy intrinsic to the other side of the Iron curtain even so long after the events, and which was maintained despite the obvious duplicity of her employers. This is a pity, because it would have interesting but harmless after all these years to have read more technical detail about both the transmitters and the operating procedure used by these agents.

Stewart G3YSX

Thursday, August 27, 2009

WANTED: MEPT Grabbers in S. America, Africa, Asia

Dear Bill,

It Hurts!!.... You have abandoned us visual Beacon Anarchists for the Instant gratification of the WSPR crowd.

Hey, To refresh your memory, Your the one that got me started in this Visual MEPT World. I listened to your podcast and ordered some 10.140 Mhz Crystals and built my Model 1 MEPT transmitter. After that I was hooked. It has gone on to a model 2 and Now started on a DDS driven Model 3 which is all band and right now is crying out for someone to see it at 160 mW. It has made it last week to VK7ZL in Tasmania 8455 miles and ZL2IK in New Zealand 6917 miles. So, as you can see, I have been busy. One of the really extarodinary things is that we are doing this on 40 meters at 7,104,800 Hz. What would really help is to enlist some more monitoring stations with ARGO Spectrum Analyzers on their computers LISTENING. They are sorely needed in South America, Africa, India and the Far East. I have the belief that my signal at 160mW on 7,104,800Hz can be copied in all of those areas at different times of the day, almost every day. The reason it isn't is there is nobody listening and my little FSKCW signal
just keeps looking for a receiver to hear it.

My model 3 transmitter is a thing of beauty. It can work all bands from 160 to 10 meters. It is completely under the control of an Ardunio processor (A great product of Italy). It controls the frequency, the amount of frequency shift, and the CW keying. It is not quite ready for prime time yet. But work is being done on the controlling software and one of these days, It will be done. Then the visual guys will not be chained by a crystal to determine their frequency. They will merely command their Ardunio to control their Direct Digital Synthesizer to the desired frequency, select the desired mode of transmission and hook up the antenna.

So, Please Mr Bill, Don't abandon us visual MEPT beacon guys. We really need your voice and talents to keep the airways of our 100 Hz of spectrum alive and vibrant. You could hang an extra wire out the window and do both!

73 Dave
David R. Hassall WA5DJJ
Website: http://www.zianet.com/dhassall/
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