Regular visitors to the blog will know that I try to promote more interest in the low-VHF part of the spectrum by having a dedicated page related to the new 40 MHz / 8 metre band. If I come across anything of interest that might be related to the band then I post it here on the blog and link to it from the 40 MHz page.
The Clansman is an ex-British army radio that can operate on FM on the low VHF spectrum from 30 to 76 MHz. As such, it is one of the few radios available on the second hand market that can operate at 40 MHz, 50 MHz, 60 MHz or 70 MHz.
Thanks to Steve EI5DD for his permission to post this guest post here....de EI7GL
The Clansman PRC-3512 is an intra-platoon level backpack VHF FM transceiver. The PRC 351 has 4 watt RF power output, and operates in the 30–75.975 MHz range with a possible 1840 channels spaced 25 kHz apart.
This radio is also capable of being mounted on a vehicle in conjunction with the TUAAM (Tuning Unit Automatic Antenna Matching). The PRC 352 is identical, with the addition of a 20 watt RF amplifier and can be used as a ground station also.
The Clansman RT-351 / VRC-351 Back-Pack 4 Watt portable VHF (FM) Radio was made by RACAL BCC Ltd. in England. The PRC-351 was designed to provide command communications at battalion and company level for dismounted troops. It was also used in vehicles by mounted troops. The PRC-351 replaced the older A41 and A42 British VHF radios.
The frequency Range 30 to 76.000 MHz in 25 Khz steps giving a total of 1841 programmable channels. The desired frequency is set by four knobs on the side of the radio which can be operated even while the operator is wearing Arctic mittens, or in the dark by counting clicks from the end-stops.
Friday, November 22, 2019
Thursday, November 21, 2019
More countries in Europe & Africa gain access to 50 MHz
The World Radio communication Conference WRC-19 has just approved an allocation in the 50 MHz band for radio amateurs in Region 1 which includes Europe, Africa and the Middle East.
The entire region will now have an amateur secondary allocation of 50-52 MHz. This is usually granted on basis that secondary users do not cause interference to primary users of the band.
The exception is the Russian Federation, whose administration opted for only 50.080-50.280 MHz on a secondary basis.
This change should make a big difference in areas like Africa where only 11 countries have a primary allocation at present. The secondary allocation now opens the door for more activity from the continent.
According to a press release from the IARU, they state..."The exact manner in which the allocations will be implemented in Region 1 countries will be determined by each administration and may be either more generous or less, depending on national considerations."
So what does this mean??
While 26 countries in Region 1 currently have primary access to 50-54 MHz, the fact is that the vast majority of all 6-metre activity happens between 50 and 52 MHz. By having an official secondary allocation, radio amateurs in countries in Africa, Russia or the Middle East will now have a more valid reason for access to the band. This should result in more activity from those regions and this will be of interest to radio amateurs in western Europe.
It means that there is likely to be more DX related activity on the band which should encourage more activity. Every Summer, there will be multi-hop Sporadic-E from Europe to some of those potentially new countries on the band.
While the current predictions for the next sunspot cycle in a few years time aren't great, it should still result in good north-south paths. For stations in western Europe, this should result in openings to new countries in the Middle East and Africa.
Links...
1) IARU news item dated 21st Nov 2019
2) RSGB News
Sunday, November 17, 2019
Opening on 28 MHz - Sun 17th Nov 2019
Sunday the 17th of November 2019 was an interesting day on 28 MHz. In the morning, there was a modest Sporadic-E opening in Europe with a number of stations being heard on FT8.
The two signals of note were...
5R8VX in Madagascar at 9050 kms. Anything from the Indian Ocean is always of interest on 28 MHz.
F5MYK/MM in the South Atlantic. These are the FT8 signals that I heard...
144945 -18 -0.1 1733 ~ CQ F/MM IH03
145115 -16 -0.1 1734 ~ <...> F5MYK/MM RR73
145215 -15 -0.1 1732 ~ CQ F5MYK/MM
145245 -16 -0.1 1732 ~ CQ F/MM IH03
145315 -17 -0.1 1733 ~ CQ F5MYK/MM
145715 -15 -0.1 1730 ~ EA1AER
It looks as if the strange call was enough to stop it being accepted by the PSKReporter website, hence the lack of a line on the display. An unusual one to hear on the band.
Friday, November 15, 2019
Sixty Symbols video on the simple crystal radio...
Normally the Sixty Symbols video channel on YouTube from the University of Nottingham covers some serious subjects on physics and astronomy.
In a recent edition however, they looked at a simple crystal radio.
Wednesday, November 13, 2019
Galway Radio Club Newsletter - Issue 1 - Winter 2019
Galway Radio Club in the west of Ireland have recently launched a new 48 page newsletter which covers some some recent club activities as well as a number of items which may be of interest to a wider audience.
These include...
1) An overview of how an amateur radio digital network was developed in the west of Ireland.
2) An overview of the experimental 5 MHz / 60m band.
3) Antennas for portable operation.
4) Understanding the Ionogram.
5) 160m top band operation.
6) G4HOL multi-band HF horizontal loop.
7) Operating the DVstick 30 - How to communicate on D-Star and DMR without a radio.
The newsletter can be seen HERE
For more information on the Galway Radio Club, visit https://www.galwayradio.com/
Monday, November 11, 2019
Opening on 28 MHz to North America - Mon 11th Nov 2019
Monday the 11th of November 2019 was a pretty quiet day on 28 MHz for the most part. Other than a handful of European stations, the best DX to the south on FT8 was ZD7MY on St.Helena. The three exceptional signals however were WU1ITU, K0TPP and KC4QX in the USA.
On the lower bands like 18 MHz, 21 MHz or even 24 MHz, it's no big deal to hear an East-West signal outside of the Sporadic-E season. On 28 MHz and at the bottom of the sunspot cycle, it is.
When the solar flux is very low at the bottom of the sunspot cycle, propagation on 28 MHz via the F2 layer in the ionosphere is usually via North-South paths. As a result, hearing South Africa or South America from Europe on 28 MHz at the moment is nice but not exceptional. Hearing North America is unusual though.
I got just two FT8 decodes today from K0TPP in Missouri. He was 6,267 kms from here which is more than one F2 hop so perhaps there was some Sporadic-E helping to extend the path at one end or the other?
WU1ITU by contrast was much stronger and was at least +14dB here. That's a kind of level where a CW or SSB contact should be easily possible. It was a bit strange that these were the only two US stations that I heard.
KC4QX in Florida was heard much later at 18:43 UTC, about two hours after local sunset. Looking at the PSK Reporter website, it seems as if I was the only one in Europe in Europe to hear him.
Some of the my FT8 decodes are shown below. As you can see, WU1ITU was working Greece, France, Denmark and Spain.
103015 -15 -0.3 862 ~ CQ MM3NRX IO86
113300 -12 -0.5 1366 ~ CQ RA2FL KO04
121145 -12 -0.0 976 ~ CQ IZ2MHO JN45
151515 -11 -0.2 664 ~ WB2PYN K0TPP -03
151545 -10 -0.2 664 ~ WB2PYN K0TPP RR73
Sunday, November 10, 2019
Lack of activity from Africa on 28 MHz...
Sunday the 10th of November 2019 was a pretty quiet day on 28 MHz with only one South African station being heard on FT8 here as well as a handful of Europeans.
I did a check of all the FT8 stations on 28 MHz from 9am to 9pm on the 10th of November and the map is shown above. I'm not sure if all the stations are shown but you can see very clearly where most of the activity is located.
It just highlights the fact that while there is plenty of activity from Europe, there is nobody active in most of Africa. This means that the 10-metre band may well be open from Europe to Africa at times but we can't tell.
Saturday, November 9, 2019
Opening to South Africa on 28 MHz - Fri 8th Nov 2019
An interesting day on 28 MHz with some mixed propagation on the band. There seems to have been some Sporadic-E between Ireland and Spain to the south. This then linked to what was probably F2 propagation from the latitude of Spain down to South Africa and Mauritius in the Indian Ocean.
Thursday, November 7, 2019
28 MHz opens up to the Indian Ocean - Thurs 7th Nov 2019
There was an interesting opening on Thursday the 7th of November 2019 with 3B8CW in Mauritius in the Indian Ocean being heard on FT8 on 28 MHz.
The distance was around 10,200 kms.
Sunday, November 3, 2019
SDRplay announce release of new SDR receiver
On the 1st of November 2019, SDRplay announced the release of their new RSPdx model. This is a software defined radio intended for reception only and replaces their RSP2 and RSP2 PRO models.
It is described as follows..."The SDRplay RSPdx is a complete redesign of the popular RSP2 and RSP2pro multi-antenna receiver. It’s a wideband fullfeatured 14-bit SDR which covers the entire RF spectrum from 1kHz to 2GHz. Combined with the power of readily available SDR receiver software (including ‘SDRuno’ supplied by SDRplay) you can monitor up to 10MHz spectrum at a time.
The RSPdx provides three software selectable antenna inputs, and an external clock input. All it needs is a computer and an antenna to provide excellent communications receiver functionality."
This particular model retails for about €200 / $200 which is twice the price of the RSP1a version.
SDRPlay seem to have a reputation for good SDR receivers at reasonable prices. The RSP1a looks like good value but I guess it depends on what you are looking for. The RSPdx has a metal enclosure with more sockets which might appeal to some.
More info in the video below and on the SDRplay website... https://www.sdrplay.com/
Saturday, November 2, 2019
Jump in numbers for the IRTS Autumn 80m Counties Contest...
The IRTS 80 Metres Evening Counties Contest was held on the 8th October 2019 and the results show an increase in numbers taking part.
While the numbers may be small compared to other contests, it's good to see some local activity going in the right direction.
See www.irts.ie/results for full details.
Friday, November 1, 2019
Opening to Africa on 28 MHz - 1st Nov 2019
It wasn't the best of days for propagation on 28 MHz but it was still interesting to see stations from Africa coming through on 10-metres.
Besides TR8CA in Gabon, four stations in South Africa were heard.
I suspect the band is often open to others part of Africa except that there is no-one on from those countries.
Besides TR8CA in Gabon, four stations in South Africa were heard.
I suspect the band is often open to others part of Africa except that there is no-one on from those countries.
Thursday, October 31, 2019
Comparison of the FT8 and WSPR modes on 28 MHz - 31st Oct 2019
For the months of May & June 2019, I left the radio listening to FT8 signals on 28 MHz and fed the reception reports up to the PSK Reporter website. With the Summer Sporadic-E season in full swing, it kind of got very repetitive in terms of what was being heard with each days list of stations looking pretty much the same as the previous days.
For the second half of the Summer, I spent a lot more time listening to the WSPR frequency on 28 MHz and uploaded those spots instead. Once we got to September however, the number of reports really began to diminish.
FT8 V WSPR... As an experiment, I tried out both modes today on 28 MHz. My objective was to listen at a time when the band was open and see how the activity on each mode compared.
Session 1... 30 mins of FT8. There seemed to be plenty of signals around 12:00 UTC and this is what I heard on FT8....
Session 2... 30 mins of WSPR. I went to the WSPR frequency and I heard nothing. I could see the odd bit of a signal on the waterfall but no decodes.
Session 3... 30 mins of FT8. I switched back to the FT8 frequency for 30 mins and heard the following...
Obviously conditions had declined a bit from session 1 but I was still hearing signals.
Session 4... 30 mins of WSPR. I switched to the WSPR frequency for 30 mins and heard nothing.
I checked the WSPRnet website and it said that there were 84 stations active worldwide on 10-metres during this period. If I take out the receive only stations then there were just 21 stations in all of Europe transmitting on WSPR on 28 MHz.
Conclusion... Even though WPSR is a fascinating mode, it does require enough users to be operating on the band to make it useful. I'm of the opinion that outside of the summer Sporadic-E season, that critical mass doesn't exist for WSPR on 28 MHz.
Maybe things will be different as we leave the sunspot minimum but it seems to me as if that on 28 MHz at least, FT8 is the only mode that has a critical mass of users.
Addendum : Later in the evening, I heard Mauritania, Argentina and the Falkland Islands on 28 MHz FT8.
For the second half of the Summer, I spent a lot more time listening to the WSPR frequency on 28 MHz and uploaded those spots instead. Once we got to September however, the number of reports really began to diminish.
FT8 V WSPR... As an experiment, I tried out both modes today on 28 MHz. My objective was to listen at a time when the band was open and see how the activity on each mode compared.
Session 1... 30 mins of FT8. There seemed to be plenty of signals around 12:00 UTC and this is what I heard on FT8....
Session 2... 30 mins of WSPR. I went to the WSPR frequency and I heard nothing. I could see the odd bit of a signal on the waterfall but no decodes.
Session 3... 30 mins of FT8. I switched back to the FT8 frequency for 30 mins and heard the following...
Obviously conditions had declined a bit from session 1 but I was still hearing signals.
Session 4... 30 mins of WSPR. I switched to the WSPR frequency for 30 mins and heard nothing.
I checked the WSPRnet website and it said that there were 84 stations active worldwide on 10-metres during this period. If I take out the receive only stations then there were just 21 stations in all of Europe transmitting on WSPR on 28 MHz.
Conclusion... Even though WPSR is a fascinating mode, it does require enough users to be operating on the band to make it useful. I'm of the opinion that outside of the summer Sporadic-E season, that critical mass doesn't exist for WSPR on 28 MHz.
Maybe things will be different as we leave the sunspot minimum but it seems to me as if that on 28 MHz at least, FT8 is the only mode that has a critical mass of users.
Addendum : Later in the evening, I heard Mauritania, Argentina and the Falkland Islands on 28 MHz FT8.
Opening on 28 MHz - Wed 30th Oct 2019
The 30th of October was one of those days when I could hear some weak FT8 signals coming from the loudspeaker of the radio and not really strong enough to take much notice of them.
It was a bit of a suprise to see later that the band had been open to Africa and South America during the day
Wednesday, October 30, 2019
Local experiments on 23cms...
Every Tuesday evening, we have a local VHF net in Cork and a few of us get together for a chat. We use the the 6m, 4m, 2m and 70cms bands and which one we use depends on which Tuesday of the month it is.
It usually covers the first four Tuesdays of the month and if there happens to be a fifth Tuesday then we gave it a skip. A few weeks back, we thought it might be a good idea to use the fifth Tuesday in a month for experimentation, to try something that we don't usually do.
From this concept came the idea to try the 23cms band, i.e. 1296 MHz.
Denis, EI4KH near Watergrasshill has a Yaesu FT-2312 23cms transceiver running 4 watts on FM only and his antenna is a 26 element Yagi horizontally polarised.
A sked was organised with Don, EI8DJ who was located in a car at Camden near Crosshaven at the mouth of Cork harbour, a distance of 22 kms or 13.8 miles.
While the path wasn't line of sight, both Denis and Don were in good high locations. EI4KH was about 120m above sea level while EI8DJ was at a spot about 45m above sea level.
As the plot shows below, any obstructions on the path were several kms distant which made them less of an obstruction.
For EI8DJ's portable set-up, he was using a scanner for receive with a home made Bi-Square antenna shown below which was sitting on the dash of his car.
Using a frequency of 1290.000 MHz, EI8DJ managed to hear the FM signal from EI4KH at an estimated S'4' signal strength and a successful 23cms to 2m crossband contact was completed.
EI8DJ found the Bi-Square to be suprisingly directive and later peaked the FM signal from EI4KH to a maximum of an estimated S'7' signal strength.
The experiment was repeated with EI8DJ back in his driveway which is some bit lower than his portable location. From his home location, EI8DJ couldn't hear any sign of the FM signal from EI4KH.
While the distanced achieved were nothing special, it was interesting to see some local activity on the lowest of the amateur microwave bands.
Notes:
1) The beam heading for Denis was 170 deg.
Saturday, October 26, 2019
Sporadic-E opening on 28 MHz - Fri 25th Oct 2019
Even though it was late October, there was a Sporadic-E opening on 28 MHz from around Europe.
As can be seen from the map, the band opened up via Sporadic-E to Spain and probably linked up with some F2 propagation down to South Africa.
There were some signals from Eastern Ukraine and SW Russia as well. There were possibly F2 but I'd be inclined to think they were double hop Sporadic-E.
Even though we are at the bottom of the sunspot cycle, the band isn't completely dead.
Monday, October 21, 2019
The remarkable rise of FT8
I came across a news item recently with a chart showing the remarkable rise of FT8.
The data for this chart came from the ClubLog system which is used by thousands of people so I would assume it gives a reasonably representative picture.
The data for this chart came from the ClubLog system which is used by thousands of people so I would assume it gives a reasonably representative picture.
Saturday, October 19, 2019
Conditions on 28 MHz - Sat 19th Oct 2019
An interesting day on 28 MHz. Even though the solar flux was way down at 66 and we're at the sunspot minimum, it does show that the 28 MHz band isn't completely dead at the moment.
While none of the signals were particularly strong and most were buried in the noise, the band was open. Over the last few days, there have been openings as well so it's worth checking the band.
Monday, October 14, 2019
Signs of the next solar cycle starting...
Courtesy of NASA/SDO and the AIA, EVE, and HMI science teams. |
At the moment in October of 2019, we are the bottom of the sunspot cycle and conditions on the HF bands are pretty awful. Recent observations of the Sun however show that things are changing.
The image above shows the active regions of the Sun's corona, the outer atmosphere of the Sun. Active regions, solar flares, and coronal mass ejections will appear bright here.
On the 6th of October, two regions with different magnetic polarity were spotted which are part of the next solar cycle.
Back in April, I had a post about a report from NOAA/NASA which said that the end of Cycle 24 and start of Cycle 25 will occur no earlier than July, 2019, and no later than September, 2020. The latest observations tie in with this report.
These observations don't mean that conditions on the HF bands are going to improve all of a sudden. This is a slow process. Over the next year or so, we should begin to see more and more regions with the magnetic polarity of the new solar cycle 25 and fewer with the solar cycle 24 signature.
It's only after we have passed the solar minimum for sure that scientists can pinpoint exactly when it happened.
I would suggest that it will probably be late 2020 before we start to see any real enhancement in the HF bands. Even then, it will be a case of more openings on the likes of 21 MHz rather than 28 MHz.
Links...
https://sdo.gsfc.nasa.gov/data/
Saturday, October 12, 2019
Example of BBC TV signal at 45 MHz being heard in South Africa
The BBC recently released this old television clip from 1949 explaining how an amateur radio station in Cape Town, South Africa had received TV signals from the UK.
The map below shows the path which is about 9,700kms or 6,000 miles...
The TV transmitter mentioned in the video was a 405 line transmission from Alexandra Palace in North London. This was vertically polarised with a power of 500 kilowatts (ERP?).
This TV signal had a video carrier on 45.0 MHz and a sound carrier down at 41.5 MHz.
The reception report in 1949 was near the peak of solar cycle 18. As can be seen from the chart below, that was a really good sunspot cycle and conditions were probably excellent on all the HF bands and well up into the low VHF region.
The most likely mode of propagation at 45 MHz was probably multi-hop from the F2 layer in the ionosphere. The maximum usable frequency was probably above 50 MHz so the signals on 45 MHz should have been very good.
It's likely however that with a video signal spread out over three and a half megahertz, the picture was probably very distorted and constantly changing. It should have been possible however to have very good reception of the sound on AM on 41.5 MHz with a dedicated radio receiver.
The radio contact shown in the clip between G8IG in England and ZS1PK in Cape Town, South Africa was probably on 28 MHz AM (note the beam at the start of the clip).
The South African station mentioned that signal were better when things were calm which might infer some sort of tropo ducting. That is unlikely to have been the case as it was very probable that all propagation was via the ionosphere and the weather conditions would have no impact.
All the same, it's an interesting example of early low band VHF TV reception.
#OnThisDay 1949: England and South Africa were linked through the magic of radio. pic.twitter.com/BpTODBlaRZ— BBC Archive (@BBCArchive) October 6, 2019
The map below shows the path which is about 9,700kms or 6,000 miles...
The TV transmitter mentioned in the video was a 405 line transmission from Alexandra Palace in North London. This was vertically polarised with a power of 500 kilowatts (ERP?).
This TV signal had a video carrier on 45.0 MHz and a sound carrier down at 41.5 MHz.
The reception report in 1949 was near the peak of solar cycle 18. As can be seen from the chart below, that was a really good sunspot cycle and conditions were probably excellent on all the HF bands and well up into the low VHF region.
The most likely mode of propagation at 45 MHz was probably multi-hop from the F2 layer in the ionosphere. The maximum usable frequency was probably above 50 MHz so the signals on 45 MHz should have been very good.
It's likely however that with a video signal spread out over three and a half megahertz, the picture was probably very distorted and constantly changing. It should have been possible however to have very good reception of the sound on AM on 41.5 MHz with a dedicated radio receiver.
The radio contact shown in the clip between G8IG in England and ZS1PK in Cape Town, South Africa was probably on 28 MHz AM (note the beam at the start of the clip).
The South African station mentioned that signal were better when things were calm which might infer some sort of tropo ducting. That is unlikely to have been the case as it was very probable that all propagation was via the ionosphere and the weather conditions would have no impact.
All the same, it's an interesting example of early low band VHF TV reception.
Subscribe to:
Posts (Atom)