"I will do as I told the crew at Elecraft and help the pressure.
At 9:10 AM this morning (Sat) a nice brown truck pulled up in my drive and after I signed for it, gave me a 12"x8"x6" box that said "ELECRAFT KX3 Ultra-Portable HF/VHF Transceiver s/n 0024
Yes ... I got a call yesterday
I am hoping within a hour to be on 20 meters chasing WG0AT on his SOTA trip and putting it thru its paces on digital.
Thank you all at Elecraft ..
The game begins
You will be happy .......
Paul KB9AVO"
Simple QRP projects, 10m, 8m, 6m, 4m, FT8, 160m, WSPR, LF/MF, sub-9kHz, nanowaves and other random stuff, some not related to amateur radio.
31 Mar 2012
Elecraft KX3 - first products delivered
This email appeared on the KX3 Yahoo group today:
8.971kHz VLF earthmode test
30t loop on the ground feeding E-field probe |
far end of the garden and the other end grounded to my copper hot water tank in the house.
At the RX end I was using either (a) a 30t tuned loop feeding either the PA0RDT or G3XBM tuned E-field probe, and (b) the same E-field probes but fed with a 19 inch whip instead of the loop.
Good signals were received at both locations with the loop into both probes but there was no detectable signal when receiving on the 19 inch whip into the EFPs.
It was a struggle to see the difference between the PA0RDT and G3XBM E-field probe/preamps, but I think results with my tuned drain design may have been marginally better on this test.
30 Mar 2012
VLF E-field probe update
Today I compared the PA0RDT E-field probe against my own VLF design (on the sub-9kHz website) that uses an 8-9kHz tuned circuit in the FET preamp drain. To do the test I had my wife hold each E-field probe at arms length above her head in the bottom of the garden whilst I made screenshots on the PC. The S/N on Alpha beacons and 18-22kHz MSK signals is similar with the PA0RDT and mine but the PA0RDT design has a lower noise floor. So, in future I will use Roelof's design. Some measurements made by G3ZJO today compared the PA0RDT design against the narrower band VLF E-field probe by DK7FC and Eddie's results suggest comparable performance within the limits of experimental error.
29 Mar 2012
E-field probe tests
This afternoon I built a version of the PA0RDT E-field probe. In the shack the interference was horrendous, but in the garden with the laptop PC just below it the reception of the VLF Alpha beacons and MSK signals around 18-22kHz was excellent. I need to do more noisefloor measurements and elevate the probe higher, but I think this is going to work well when mounted at the top of my neighbours tree that overhangs into my garden. This is a sycamore which I trimmed back a few months ago. The E-field probe can be mounted "in the clear" some 20m from the nearest house at a height of around 5m off the ground. I now need to rebuild it into a watertight box and think how I am going to get the output and power feed to the shack that is at the wrong side of the house some 30m away. Some have used CAT5 twisted wires for this purpose and I guess this would be a good, simple solution, although less suitable if I want to use the probe at 137 and 500kHz where a coax feed would be better.
ZL9 Campbell Island (near New Zealand)
There is to be a DXpedition to Campbell Island (OC-037) in November this year. See http://dx-world.net/2012/zl9hr-campbell-island-dxpedition/ . This reminds me of the excellent conditions on 20m AM back in the 1960s when I remember hearing a station on Campbell Island working the UK with S9 signals early one morning. In those days I'm sure the prefix was ZL4 though.
Is it just me, or is it much more difficult to hear and work DX stations these days compared with back then? Some believe that the ionosphere has actually deteriorated in the last 40 odd years so that, despite rising sunspot numbers, conditions are not as good as they were years ago.
Is it just me, or is it much more difficult to hear and work DX stations these days compared with back then? Some believe that the ionosphere has actually deteriorated in the last 40 odd years so that, despite rising sunspot numbers, conditions are not as good as they were years ago.
SPRAT 150 is out
The latest edition of the GQRP club's SPRAT quarterly magazine arrived on my doorstep today. As always, this is filled with a variety of interesting articles and this edition even includes one I wrote about 481THz optical comms "over the horizon", but don't let that put you off, HI.
GQRP club membership, with SPRAT 4 times a year, remains the best bargain in amateur radio in my opinion. More details on the GQRP club at www.gqrp.com .
I note that GQRP club sales is now selling fundamental crystals for 28.060MHz (suitable for my Chirpy rig) at just £2 each. This is a useful source of QRP related parts for club members.
Join!
GQRP club membership, with SPRAT 4 times a year, remains the best bargain in amateur radio in my opinion. More details on the GQRP club at www.gqrp.com .
I note that GQRP club sales is now selling fundamental crystals for 28.060MHz (suitable for my Chirpy rig) at just £2 each. This is a useful source of QRP related parts for club members.
Join!
28 Mar 2012
Amateur radio postage stamps
The excellent Southgate Amateur Radio News page today mentioned that Luxemburg is bringing out a postage stamp to commemorate the 75th anniversary of the Luxemburg radio society. See http://www.southgatearc.org/news/march2012/amateur_radio_stamp_for_luxembourg.htm . This got me wondering how many other countries have issued stamps with an amateur radio theme? I recall the USA doing a ham radio stamp in the mid-1960s.
Wondering if there were others I did a search on Google images for amateur radio postage stamps. Interesting.
Wondering if there were others I did a search on Google images for amateur radio postage stamps. Interesting.
VLF E-field probes compared?
Both
the PA0RDT and DK7FC E-field probes antennas are suitable for detecting weak VLF amateur signals around 8-9kHz when used with the right PC software. See https://sites.google.com/site/sub9khz/antennas for the schematics of these and others.
What I'm wondering is has anyone done a "like-for-like" test to compare their performance? With a near identical test set-up (same height above ground, same ground and PSU noise conditions) it should be possible to compare noise floor, sensitivity (S/N of Alpha beacons, VLF MSK signals), and by looking for the intensity of the intermod line at 9kHz from broadcast signals in Europe get an indication of dynamic range. Has anyone done this test at VLF? If not, it looks like I shall have to do it and "suck it and see".
Incidentally, the PA0RDT voltage probe antenna makes an ideal antenna for shortwave, medium wave and long wave DX SWLs. It is essentially a high dynamic range wideband receive antenna which is tiny, yet capable of excellent results if mounted in the clear in a low noise environment ideally away from house electrical interference.
What I'm wondering is has anyone done a "like-for-like" test to compare their performance? With a near identical test set-up (same height above ground, same ground and PSU noise conditions) it should be possible to compare noise floor, sensitivity (S/N of Alpha beacons, VLF MSK signals), and by looking for the intensity of the intermod line at 9kHz from broadcast signals in Europe get an indication of dynamic range. Has anyone done this test at VLF? If not, it looks like I shall have to do it and "suck it and see".
Incidentally, the PA0RDT voltage probe antenna makes an ideal antenna for shortwave, medium wave and long wave DX SWLs. It is essentially a high dynamic range wideband receive antenna which is tiny, yet capable of excellent results if mounted in the clear in a low noise environment ideally away from house electrical interference.
More optical tests looking for elusive GB3CAM
This evening, thinking it would be a good opportunity to look for the GB3CAM
optical beacon (yet again) I took the trip to nearby Nine Mile Hill (32km from the beacon) with the kit
recently used to detect G4HJW's Phatlight beacon over the horizon at 8.6km. My RX is now pretty sensitive. However, I
failed yet again to detect anything of GB3CAM. Actually it was a little
hazier than my first tests (when I had sensitivity issues) but I was
disappointed not to detect a thing. All I managed was a chat with
the farmer in whose field gate I'd set up my optical kit and PC: he seemed happy with
my explanation.
I've asked the beacon keeper if the beacon was actually on-air - it could have been off I guess.
My other question of Bernie G4HJW, the beacon keeper, is what the ERP of the GB3CAM beacon is compared with his phlatlight beacon at home that I'm consistently
able to copy at 20-30dB S/N in 0.17 - 0.67Hz
bandwidths non line-of-sight, whereas I've so far been unsuccessful receiving the Wyton optical beacon
line-of-sight. At 32km haze will matter more and it may
just be that on the occasions I've tried I've either had insensitive kit
or poor optical conditions. I did try very carefully scanning the
horizon this evening after sundown for a good 15 minutes without
detecting a thing and I had a very good idea where to aim.
26 Mar 2012
160m WSPR this evening
If JT65 is hard going on 160m this definitely cannot be said about WSPR: having switched on just a few minutes ago I am seeing and have been seen by plenty of stations in northern Europe with my 5W to the tiny loft vertical.
MSF 60kHz off air until April 6th
If you use the 60kHz LF signal from MSF Anthorn to lock your frequency reference or digital watch you may have a problem for a couple of weeks: it is off the air! It is scheduled to be off air until 20:00 UTC on April 6th. See http://www.npl.co.uk/science- technology/time-frequency/ time/products-and-services/msf-outages.
PA1B's QRPp website
Bert PA1B has an excellent website describing his experiments with very low power on HF. Using his FT817 with various simple attenuators he has been able to work some remarkable DX with powers ranging from 1mW to 500mW. His website explains how he has achieved this. It is an inspiring page showing just what is possible.
QRP JT65 to HB9 on 160m with indoor antenna
Just seen that HB9FX has copied my 160m QRP JT65 signal at -24dB S/N. Still finding it hard to make 2-way QSOs with this mode on 160m, but it proves the tiny indoor loft vertical antenna is radiating OK. Best DX report on JT65 is still the SP station about 10 days ago at over 1000km.
10m DX
This evening there were some interesting west African stations coming through on 10m. 6V7Z in Senegal on SSB and J52HF in Guinea Bissau on CW. I did not try to break pile-ups with my QRP and instead worked CT9/DL3KWR on QRP CW. Following this I moved down to 12m and worked N1WPU on CW also with QRP.
First ever 2-way international ham QSO on VLF
From Marcus DF6NM via the RSGB LF reflector earlier today:
"Today between 7:30 and 14:00, Lubos OK2BVG and I successfully completed a two-way contact on 8.97 kHz. We believe that this is the first international QSO ever on VLF.
The distance between Breclav (JN88KS) and Nuernberg (JN59NJ 69es) is approximately 424 km. The weekend before, Lubos and I had found that we could see each other's VLF transmissions from our small home antennas in a slow spectrogram, using about 0.45 millihertz FFT resolution ("DFCW-6000"). This long integration requires about 2000 seconds of continuous non-interrupted carrier to reach full sensitivity.
We decided to use absolute frequency encoding of characters ("MFSK-37" mode), which has a simple structure but is significantly more efficient than two-frequency DFCW. The software signal generators in SpecLab were used to create 30 minute dashes by editing the frequency in 1 mHz steps every half hour. This can be automated by opening a textfile which is read by the "periodic actions" function. Between transmissions, additional half-hour gaps were inserted to let the FFT ring down, and allow for TX-RX reconnections.
Characters are identified by reading the frequencies above 8970.000 Hz, with 8970.000 to .009 assigned to the numbers, .010 idle or space, and .011 to .036 the letters A-Z. Lubos used a Rubidium standard to lock his transmit samplerate, while both receivers and my TX were synchronized by military MSK signals from GQD (22.1 kHz) and DHO (23.4 kHz).
With about 80 watts from an audio amplifier, I could get up to 0.38 A antenna current into my top-loaded vertical 9 m above the roof, radiating on the order of 10 to 15 microwatts. I believe that Lubos is using similar equipment, perhaps a couple of dB stronger. For receive, my soundcard was connected straight to the loading coil and antenna, whereas Lubos has an active probe at a quiet site remote from his TX location.
We wanted to go for a "full QSO" format with reports and confirmations, beyond the rudimentary three-dash "micro-QSO" format which was used in June 2009 between DJ2LF and myself. With single-letter suffixes, we ended up proceeding as follows:
07:30-08:30 "NB" ;Lubos' call: df6Nm de ok2Bvg
09:00-10:30 "BNM" ;my reply and report: Bvg Nm M
11:00-12:00 "RO" ;his confirmation and report
12:30-14:00 "RTU" ;my confirmation and thank you
Although today the noise was not as low as it had been before, we managed to exchange the essential information in 5.5 hours until 13 UT, after which QRN from lightning in southeast Europe became strong enough to obliterate further copy.
Attached image contains captures from Lubos' grabber at Apollons temple (top) and my receiver (bottom), with screenshots from the DK7FC and OE3GHB grabbers pasted inbetween. The original captures are at http://df6nm.bplaced.net/VLF/ok2bvg_df6nm_120325/. All spectrograms were stretched to the same timescale (5 min/pixel). On the left hand side, you can see a MFSK pre-test from Lubos, sending his call to hs own grabber at very low power. There was also a long dash from OE3GHB on 8970.030, and a carrier from DJ8WX on 8970.022 is visible at DK7FC.
The rightmost part of the captures shows the essential eight dashes from our QSO. You can see that I had almost lost Lubos' "B" when my noise blanker triggered heavily on local QRM, inducing me to give an "M" rather than "O" report. But hovering the cursor to 8:15 UT does show the peak at 8970.012 Hz in the spectrum graph. My final "R" is just barely visible at .028, whereas the following "TU" at .030 and .031 ended up drowning in the increasing noise.
During the lowest noise period (9 - 12 UT), the dashes were visible (though not decodable) in 4.5 mHz "600" spectrograms. At that time, our symbols also appeared on Paul Nicholson's spectrogram http://abelian.org/vlf/fbins.shtml#p=1332712800&b=110&s=sp
Thanks again to Lubos for the effort and patience! Although exchanging half-hour symbols is tedious and may sound boring to some, both of us enjoyed it and actually found it quite exciting.
Best 73,
Markus (DF6NM)"
"Today between 7:30 and 14:00, Lubos OK2BVG and I successfully completed a two-way contact on 8.97 kHz. We believe that this is the first international QSO ever on VLF.
The distance between Breclav (JN88KS) and Nuernberg (JN59NJ 69es) is approximately 424 km. The weekend before, Lubos and I had found that we could see each other's VLF transmissions from our small home antennas in a slow spectrogram, using about 0.45 millihertz FFT resolution ("DFCW-6000"). This long integration requires about 2000 seconds of continuous non-interrupted carrier to reach full sensitivity.
We decided to use absolute frequency encoding of characters ("MFSK-37" mode), which has a simple structure but is significantly more efficient than two-frequency DFCW. The software signal generators in SpecLab were used to create 30 minute dashes by editing the frequency in 1 mHz steps every half hour. This can be automated by opening a textfile which is read by the "periodic actions" function. Between transmissions, additional half-hour gaps were inserted to let the FFT ring down, and allow for TX-RX reconnections.
Characters are identified by reading the frequencies above 8970.000 Hz, with 8970.000 to .009 assigned to the numbers, .010 idle or space, and .011 to .036 the letters A-Z. Lubos used a Rubidium standard to lock his transmit samplerate, while both receivers and my TX were synchronized by military MSK signals from GQD (22.1 kHz) and DHO (23.4 kHz).
With about 80 watts from an audio amplifier, I could get up to 0.38 A antenna current into my top-loaded vertical 9 m above the roof, radiating on the order of 10 to 15 microwatts. I believe that Lubos is using similar equipment, perhaps a couple of dB stronger. For receive, my soundcard was connected straight to the loading coil and antenna, whereas Lubos has an active probe at a quiet site remote from his TX location.
We wanted to go for a "full QSO" format with reports and confirmations, beyond the rudimentary three-dash "micro-QSO" format which was used in June 2009 between DJ2LF and myself. With single-letter suffixes, we ended up proceeding as follows:
07:30-08:30 "NB" ;Lubos' call: df6Nm de ok2Bvg
09:00-10:30 "BNM" ;my reply and report: Bvg Nm M
11:00-12:00 "RO" ;his confirmation and report
12:30-14:00 "RTU" ;my confirmation and thank you
Although today the noise was not as low as it had been before, we managed to exchange the essential information in 5.5 hours until 13 UT, after which QRN from lightning in southeast Europe became strong enough to obliterate further copy.
Attached image contains captures from Lubos' grabber at Apollons temple (top) and my receiver (bottom), with screenshots from the DK7FC and OE3GHB grabbers pasted inbetween. The original captures are at http://df6nm.bplaced.net/VLF/ok2bvg_df6nm_120325/. All spectrograms were stretched to the same timescale (5 min/pixel). On the left hand side, you can see a MFSK pre-test from Lubos, sending his call to hs own grabber at very low power. There was also a long dash from OE3GHB on 8970.030, and a carrier from DJ8WX on 8970.022 is visible at DK7FC.
The rightmost part of the captures shows the essential eight dashes from our QSO. You can see that I had almost lost Lubos' "B" when my noise blanker triggered heavily on local QRM, inducing me to give an "M" rather than "O" report. But hovering the cursor to 8:15 UT does show the peak at 8970.012 Hz in the spectrum graph. My final "R" is just barely visible at .028, whereas the following "TU" at .030 and .031 ended up drowning in the increasing noise.
During the lowest noise period (9 - 12 UT), the dashes were visible (though not decodable) in 4.5 mHz "600" spectrograms. At that time, our symbols also appeared on Paul Nicholson's spectrogram http://abelian.org/vlf/fbins.shtml#p=1332712800&b=110&s=sp
Thanks again to Lubos for the effort and patience! Although exchanging half-hour symbols is tedious and may sound boring to some, both of us enjoyed it and actually found it quite exciting.
Best 73,
Markus (DF6NM)"
25 Mar 2012
DX reports with JT65 on 10m QRP
This evening I called CQ on JT65 on 10m as the band was closing (I thought) and was surprised to see a couple of reports appear from LW9DC (Argentina) at 11272km. No QSO resulted, but a report of -16dB was quite good with the 5W and halo antenna. A little later I got reports from LU2XPK (13419km) and LU2XPL (13426km). Again no QSOs, just reports from these stations on http://jt65.w6cqz.org/freceptions.html.
24 Mar 2012
VLF activity this last week
Whilst I was away on holiday there was considerable activity around 8.970kHz from Europe with Henny PA3CPM now putting a consistant signal from his small home station antenna on the G3ZJO grabber. Activity is continuing this weekend.
One of my priorities in the next 2 weeks is to get my VLF receive set-up back in full working order as this has been off-air for a couple of months. I will try a new E-field probe this time around and see how results compare with my 80m square wire loop. The PA0RDT or DK7FC E-field probes are well proven designs that work well if mounted high and in a low noise environment. See https://sites.google.com/site/sub9khz/antennas for details. Antenna size is less important than S/N and dynamic range on VLF RX. This is why tiny voltage probe antennas can work so well.
160m WSPR
Just back from a week away on holiday and sorting out things like washing, post etc. So, whilst this is going on I have set the WSPR beacon running with my 5W into the short loft vertical to see what is about. In the next couple of weeks I have some work to do on antennas in the garden.
21 Mar 2012
Holidays and light
Starehole Bay near Salcombe today |
So do I, but I find myself looking out to sea and thinking how would a 481THz light signal scatter off waves in the sea? Would my beacon be copyable around the coast by aiming a few miles out to sea and aiming a receiver (located down the coast) at the same spot in the sea? How would my QRSS3 light beam beacon signal scatter off those metamorphic schist cliff formations?
I need a holiday .....oh, I'm on one!
20 Mar 2012
All for the want of an SMA-BNC adaptor
This week my wife and I are on holiday at my brother's home in South Devon. I don't bring much ham gear with me these days, but I packed my VX2 dual bander and a small mag-mount to erect when static on the car roof. Packed the rig, charger, several whips, mag mount ......but I forgot to put in the essential SMA-BNC adapter.
Never mind, there are plenty of things to do instead of amateur radio including seeing the house in Island Street, Salcombe where my dad used to live in back in the 1920s now on sale as a second home for rich bankers at £325k. The house has no views, is tiny, has nowhere to park the Rolls and floods when there is a very high Spring tide.
Never mind, there are plenty of things to do instead of amateur radio including seeing the house in Island Street, Salcombe where my dad used to live in back in the 1920s now on sale as a second home for rich bankers at £325k. The house has no views, is tiny, has nowhere to park the Rolls and floods when there is a very high Spring tide.
17 Mar 2012
KX3 - more pictures
Some nice shots of the new Elecraft KX3 QRP transceiver at http://www.worldwidedx.com/elecraft-kx3/134267-elecraft-kx3-hands-preview.html. This rig has still to start shipping nearly 12 months after first announced although the first units should be on their way to happy customers within weeks now. There were some late changes following extensive field testing and some supplier issues.
QRM on VLF?
DK7FC, PA3CPM and DF6NM have all been TXing today around 8.970kHz with reception reports coming in from many of the western European grabbers. DF6NM is running some 20dB less ERP than Stefan yet is appearing on UK grabbers quite well just HF of DK7FC. PA3CPM is a much weaker signal although he has been copied by Paul Nicholson in Todmorden UK. Activity is likely to continue over the weekend. Here is a screen grab from Eddie G3ZJO's VLF grabber today showing 2 of the active stations quite clearly. Notice the timescale on Eddie's grabber: between markers it is 4 hours in his DFCW6000 window, so don't expect snappy QSOs on VLF.
Dropbox Windows Registry issue - NOT fixed!
Having struggled to get Dropbox files sharing working on my main WinXP PC I today did a full uninstall and loaded a new version 1.1.45.exe from http://dl-web.dropbox.com/u/17/Dropbox%201.1.45.exe and I was back in business for the first time in 3 months. Within 10 minutes though, the same "unable to access vital Windows registry data" message reappeared! What the heck is going on???
16 Mar 2012
iPod Touch external audio - success!
Thanks to some input from Robin G7VKQ I have now managed to get an external mic to work with my iPod Touch 4g. He referred me to http://www.blackcatsystems.com/ipad/iPad_iPhone_iPod_Touch_Microphone_Wiring.html which shows that a resistor to ground is needed to make the device recognise the external mic is in place. In the end I found a couple of ways to make the connection work (shown below).
When used with the Spectrum View app from Oxford Wave Research I was able to connect my lightbeam receiver to my iPod Touch 4g and record QRSS3 and CW transmissions. This is 10wpm CW being received at home between rooms by scatter in broad daylight.
When used with the Spectrum View app from Oxford Wave Research I was able to connect my lightbeam receiver to my iPod Touch 4g and record QRSS3 and CW transmissions. This is 10wpm CW being received at home between rooms by scatter in broad daylight.
15 Mar 2012
iPod Touch 4g repair video
iPod Touch, SpectrumView and external mic input
A few days ago I mentioned SpectrumView as being a very useful package for the iPhone and iPod Touch 4g for audio measurements and spectrum analysis. Well, I've now got a 4 pin jack plug and wired it up (according to the best published data I can find) as an external mic input. To my great disappointment nothing happened and the internal mic was still being selected. I am wondering if something has to be asserted to select the external mic input? Anyone know please? What did I do wrong? The ring nearest the jack body is the mic input and the next ring down is supposed to be the ground. I checked the plug was correctly wired. Help!
New personal DX record on 160m JT65
SP3CUG has just spotted my 5W QRP 160m JT65 signal from my tiny loft antenna at a distance of 1063km. This beats my best DX so far (a report at 1007km from SM on WSPR) on 160m using the small indoor antenna. I cannot see him TXing which is a pity as he may be able to work me.
14 Mar 2012
VLF E-field probe design from DK7FC
DK7FC's VLF E-field probe antenna |
Further 481THz G4HJW reception "over the horizon"
G4HJW received on 481THz over an 8.63km non line-of-sight path |
On 3 attempts copying G4HJW's optical signal it has been (1) 30dB S/N, (2) no copy and (3) today 20dB S/N in 0.67Hz bandwidth over an 8.63km NLOS path. I am still using the BPW34 detector in 100mm optics.
13 Mar 2012
160m JT65 QSO with loft vertical
160m loft antenna diagram
12 Mar 2012
160m JT65
My 4 year old grandson having gone home now, I have my shack back again so am able to play amateur radio again. I've several things to catch up on including:
- Trying for a first 160m JT65 QSO.
- Measuring the performance of my ST-3 JRC headphones that AA1TJ managed to find for me recently.
- Another over-the-horizon 481THz test looking for G4HJW's beacon and my own.
- Testing my iPod Touch SpectrumView application with an external audio input.
8 Mar 2012
10m good despite the flare
Today all the propagation forecasts were showing poor conditions on HF. Despite this, 10m was well open this afternoon to the Middle East, Africa and South America with good signals received. My only QSO so far has been with JY5HX when running 5W CW here.
The lower part of 10m had several Russian (?) CB stations including one operating almost on 28.060MHz, the CW QRP frequency. Use it or lose it folks.
The lower part of 10m had several Russian (?) CB stations including one operating almost on 28.060MHz, the CW QRP frequency. Use it or lose it folks.
7 Mar 2012
160m JT65
As I appear to be having some success with WSPR on topband, I have decided to try JT65 on the band to see if I can manage a few QSOs.
UPDATE: after calling for around 15 minutes I gave up!
UPDATE: after calling for around 15 minutes I gave up!
My 160m WSPR analysis
Since erecting my tiny 160m loft mounted vertical this last weekend I've used it on WSPR a few evenings with great success. The following tables show the unique reports received and sent on the band using (mostly) 5W. Most stations copying me can be copied here, despite the horrendous noise issues on the band at night.
So far, reports have been received from 9 countries with best DX being 1007km. Not bad with an antenna which is essentially a 1m long coil, a couple of top capacity wires and about 3m of feed wire from the loft to the upstairs shack and tuned against my central heating system copper pipes as a ground.
160m WSPR reports received |
160m WSPR reports given |
6 Mar 2012
Elecraft KX3 manual
The soon to be released KX3 QRP transceiver |
5 Mar 2012
VLF test by OE3GHB
OE3GHB's VLF loading coil and transmitter |
3 Mar 2012
Mixed results on 160m
The small loft antenna for 160m has produced some impressive results tonight with spots from all over NW Europe of my QRP signal. Best was GM4SLV in Shetland at 5W and OZ7IT at 2W.
But the real reason for erecting the antenna was to allow QSOs on QRP AM over a 3km path to G6ALB so we could use topband for a talkback link when doing other tests. Now, at 9.30pm we went onto 1.973MHz AM to see how easy it would be. It wasn't easy at all! In fact it was very hard work copying even a few watts of AM. The killer is the noise floor that is around S9 both at Andrew's home and mine. On WSPR, with its much narrower bandwidth this is not such an issue, but on AM it ruins the band for what we'd intended. There is no way that 0.25W of AM would make it, certainly not easily with simple rigs as we'd planned. 10W would be OK, but that defeats the purpose. On 70cm AM (yes AM) we had armchair copy between us with about 1W. On 160m FM it was better copy until we dropped the power down and the signal was drowned by the QRN/QRM.
So, what will we do? There is now no point in continuing with the 160m AM transceivers as this isn't going to work at our noisy QTHs with QRP over 3km, sadly. The most probable choice will be 6m AM using my SixBox rig at my end.
The lower HF bands like 160m are radically different from 30 odd years ago when the noise floor was some 20-30dB lower.
But the real reason for erecting the antenna was to allow QSOs on QRP AM over a 3km path to G6ALB so we could use topband for a talkback link when doing other tests. Now, at 9.30pm we went onto 1.973MHz AM to see how easy it would be. It wasn't easy at all! In fact it was very hard work copying even a few watts of AM. The killer is the noise floor that is around S9 both at Andrew's home and mine. On WSPR, with its much narrower bandwidth this is not such an issue, but on AM it ruins the band for what we'd intended. There is no way that 0.25W of AM would make it, certainly not easily with simple rigs as we'd planned. 10W would be OK, but that defeats the purpose. On 70cm AM (yes AM) we had armchair copy between us with about 1W. On 160m FM it was better copy until we dropped the power down and the signal was drowned by the QRN/QRM.
So, what will we do? There is now no point in continuing with the 160m AM transceivers as this isn't going to work at our noisy QTHs with QRP over 3km, sadly. The most probable choice will be 6m AM using my SixBox rig at my end.
The lower HF bands like 160m are radically different from 30 odd years ago when the noise floor was some 20-30dB lower.
160m loft antenna erected
160m loft antenna |
UPDATE: My first 2 WSPR reports on the new (indoor) antenna were from OZ7IT at 853kms! The antenna must work, HI. Shortly after PA0A spotted me.
2 Mar 2012
DMR products
My old company, Sepura, entered the Digital Mobile Radio market last year (as an addition to the TETRA products they already design and make) and are, as we speak, designing DMR products for sale in the near future. In recent days they've had a wake-up call from their major competitor Motorola in the form of two new DMR radios that set the benchmark. See http://www.motorola.com/Business/XU-EN/Product+Lines/MOTOTRBO/SL4000+Series/SL4000_SL4010. These look very attractive products and I am glad I no longer have the task of trying to beat them! Instead I can tinker with lightbeams and VLF.
Getting Going on "Bottom Band"
Well, guess what, I am a year younger (amateur radio wise) than I thought. Having looked up some old RSGB Bulletins this evening I see that I actually joined the RSGB in 1963 and not 1962, so I've only been a member for the last 49 years. Suddenly I feel a year younger!
I was looking for an article about lightbeam communications that was in the very first RSGB Bulletin (later Radcom) I ever received and this was in April 1963 and not 1962. It was called "Getting Going on Bottom Band". The article was an April Fool's one but I didn't realise this and got the reference books from the library. But, the fascination with communicating a long way over a beam of light was kindled in that very article and only now am I giving the subject proper attention, some 49 (and not 50) years later. I feel as if I have a whole year extra in which to enjoy the hobby, HI.
I was looking for an article about lightbeam communications that was in the very first RSGB Bulletin (later Radcom) I ever received and this was in April 1963 and not 1962. It was called "Getting Going on Bottom Band". The article was an April Fool's one but I didn't realise this and got the reference books from the library. But, the fascination with communicating a long way over a beam of light was kindled in that very article and only now am I giving the subject proper attention, some 49 (and not 50) years later. I feel as if I have a whole year extra in which to enjoy the hobby, HI.
SpectrumView for iPod/iPhone
SpectrumView 0-24kHz displays of waterfall and spectrum |
To make best use of this I need to connect an external audio input into my iPod Touch 4g. A 4-pin jack plug when inserted, rather than a 3-pin one, allows an external audio input (or a mic) to be connected so I can feed my VLF receivers, used for both 8.7-9.1kHz earth-mode comms and for lightbeam baseband/sub-carrier detection, directly into the iPod. Resolution will be down to around 2Hz at best, so this will be of somewhat limited use, but certainly easier than a laptop for quick field tests or quantitative measurements.
The mic input (on a 4-pin jack) is on pin 4 (nearest the plug cover) and the ground is the next one down the connector (pin 3). The tip (pin 1) and pin next to the tip (pin 2) are the two audio outputs for a headset.
UPDATE 16.3.12: to tell the iPod Touch 4g that an external mic is connected you seem to need to have a 4k7 resistor to ground across the terminals. See later post for details.
1 Mar 2012
RSGB member since 1962
Next month is an historic occasion for me as it will be exactly 50 years since I joined the RSGB. In those days applications had to be supported by 2 existing RSGB members and living in the wilds of Devon I had to look hard to find two! One of the two who supported my application was Roger Thorn G3CHN, now SK, who later overhauled my ex-military DST100 radio and thereby opened up the world of shortwave listening to me. Roger worked at the local Decca Navigator station and I remember being thrilled when he showed me around the station.
Many people are critical of the national society, but behind the scenes the RSGB does a LOT for the UK amateur population. A society is only as good as its members and the contributions we make towards its success. A lot of hard work is being done currently to get the society back onto a firm footing after a turbulent period. It deserves our support.
Many people are critical of the national society, but behind the scenes the RSGB does a LOT for the UK amateur population. A society is only as good as its members and the contributions we make towards its success. A lot of hard work is being done currently to get the society back onto a firm footing after a turbulent period. It deserves our support.