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.
Saturday, October 5, 2019
Video: 144 MHz moonbounce with 200w and a 9 el Yagi
In a 45 minute video presentation, KC1HTT in the US shows how it is possible to make contacts on 144 MHz by bouncing signals off the moon with 200 watts into a 9 element Yagi.
Link HERE
The complete station and project is costed at $5,000 but many people will have parts of the station anyway for their 2m SSB station.
The video is a good introduction into what is required to try moonbounce on 2 metres.
Thursday, October 3, 2019
Conditions on 28 MHz - Wed 2nd Oct 2019
I left the radio listening to the FT8 frequency on 28 MHz yesterday and I was suprised to see there had been a reasonable opening. Not too bad considering that the solar flux is down at 69 and we're hopping along the bottom of the sunspot cycle.
As per usual, the main workhorse here is Sporadic-E as can be seen from all the European signals. This allowed me to hear DX signals that were reaching the latitude of Spain.
i.e. F2 prop from say Chile to the Azores and then Sp-E to Ireland.
Saturday, September 28, 2019
Tropo path opens on 2m from the UK to Cape Verde Islands - Sat 28th Sept 2019
Just a quick post to say that D41CV in the Cape Verde Islands managed to work G7RAU in the SW of England on FT8 on 144 MHz this morning, Saturday 28th Sept 2019.
The tropo forecast doesn't look great at the northern end of the path but it might be worth checking.
See F5LEN's website.
Thursday, September 19, 2019
Opening on 144 MHz from the Azores results in several contacts over 3,000kms
On the evening of the 14th and the morning of the 15th of September 2019, there was a very good tropo opening on 144 MHz from the Azore Islands in the Atlantic Ocean to parts of the UK, France, Netherlands, Belgium and Germany.
A list of the stations worked by José CU3EQ using the digital FT8 mode is shown below...
Saturday 14th September 2019
20190914 18:30 G7RAU IN79JX JT65 -18 -10 2138km
20190914 18:47 G4LOH IO70JC FT8 -02 +01 2145km
20190914 18:54 F6DBI IN88IJ FT8 -16 -16 2193km
20190914 19:47 ON4KHG JO10XO FT8 -24 -16 2768km
20190914 20:39 F6KHM IN78RJ FT8 -20 -21 2107km
20190914 20:46 GW0KZG IO71LW FT8 -16 -09 2257km
20190914 22:12 G4RRA IO80BS FT8 -19 -23 2263km
20190914 22:15 G4KWQ IO92AQ FT8 +03 +05 2480km
20190914 22:49 M0JDK IO93KH FT8 -24 -19 2563km
20190914 22:57 G8VHI IO92FM FT8 -19 -21 2496km
20190914 23:17 M0CGL JO03BF FT8 -11 -19 2632km
20190914 23:19 G0GMB IO92NB FT8 -21 -19 2513km
20190914 23:20 PA2M JO21IP FT8 -14 -07 2852km
20190914 23:24 PA3FYC JO31AF FT8 -23 -21 2927km
20190914 23:27 ON8KW JO20BW FT8 -14 -16 2790km
20190914 23:28 G4FUF JO01GN FT8 -19 2579km
20190914 23:49 PA3BIY JO22HB FT8 -24 -16 2861km
Sunday 15th September 2019
20190915 00:06 DJ6AG JO51EQ FT8 -22 -15 3231km ODX of all
20190915 00:08 G3NJV IO70JA FT8 -09 -16 2141km
20190915 00:45 ON4GG JO20AR FT8 -08 -05 2777km
20190915 00:59 PA2M JO21IP FT8 559 559 2852km
20190915 06:53 ON4IQ JO20AR FT8 -24 -04 2777km
20190915 07:10 DG1KDD JO31LE FT8 -22 -20 2988km
20190915 07:15 M0CKM IO90QT FT8 -17 -10 2472km
20190915 07:25 DF2ZC JO30RN FT8 -16 -17 3006km
20190915 07:26 ON4PS JO20KQ FT8 -12 -06 2832km
20190915 07:33 PA0JMV JO21PM FT8 -09 -13 2886km
20190915 07:34 PA5Y JO21VO FT8 -18 +04 2922km
20190915 07:35 PA3CMC JO21WI FT8 -19 -12 2920km
20190915 07:40 ON4LDP JO10UN FT8 -21 -15 2749km
20190915 07:44 G8BCG IO70RK FT8 +01 +00 2204km
20190915 08:00 PA2CHR JO32DB FT8 -15 -20 2970km
20190915 08:06 M0AFJ IO70IC FT8 -13 -03 2140km
20190915 08:36 DK4TG JO31LB FT8 -15 -21 2984km
20190915 08:54 DF1JC JO31OG FT8 -22 -11 3007km
20190915 09:12 DF6PW JO40AQ FT8 -17 -08 3049km
20190915 09:13 DL6YBF JO31OX FT8 -17 -06 3027km
20190915 09:23 PA3PCV JO20VV FT8 -24 -18 2901km
20190915 09:44 PA4EME JO20WX FT8 -17 -02 2909km
This is a more detailed view of the stations worked...
A list of the stations worked by José CU3EQ using the digital FT8 mode is shown below...
Saturday 14th September 2019
20190914 18:30 G7RAU IN79JX JT65 -18 -10 2138km
20190914 18:47 G4LOH IO70JC FT8 -02 +01 2145km
20190914 18:54 F6DBI IN88IJ FT8 -16 -16 2193km
20190914 19:47 ON4KHG JO10XO FT8 -24 -16 2768km
20190914 20:39 F6KHM IN78RJ FT8 -20 -21 2107km
20190914 20:46 GW0KZG IO71LW FT8 -16 -09 2257km
20190914 22:12 G4RRA IO80BS FT8 -19 -23 2263km
20190914 22:15 G4KWQ IO92AQ FT8 +03 +05 2480km
20190914 22:49 M0JDK IO93KH FT8 -24 -19 2563km
20190914 22:57 G8VHI IO92FM FT8 -19 -21 2496km
20190914 23:17 M0CGL JO03BF FT8 -11 -19 2632km
20190914 23:19 G0GMB IO92NB FT8 -21 -19 2513km
20190914 23:20 PA2M JO21IP FT8 -14 -07 2852km
20190914 23:24 PA3FYC JO31AF FT8 -23 -21 2927km
20190914 23:27 ON8KW JO20BW FT8 -14 -16 2790km
20190914 23:28 G4FUF JO01GN FT8 -19 2579km
20190914 23:49 PA3BIY JO22HB FT8 -24 -16 2861km
Sunday 15th September 2019
20190915 00:06 DJ6AG JO51EQ FT8 -22 -15 3231km ODX of all
20190915 00:08 G3NJV IO70JA FT8 -09 -16 2141km
20190915 00:45 ON4GG JO20AR FT8 -08 -05 2777km
20190915 00:59 PA2M JO21IP FT8 559 559 2852km
20190915 06:53 ON4IQ JO20AR FT8 -24 -04 2777km
20190915 07:10 DG1KDD JO31LE FT8 -22 -20 2988km
20190915 07:15 M0CKM IO90QT FT8 -17 -10 2472km
20190915 07:25 DF2ZC JO30RN FT8 -16 -17 3006km
20190915 07:26 ON4PS JO20KQ FT8 -12 -06 2832km
20190915 07:33 PA0JMV JO21PM FT8 -09 -13 2886km
20190915 07:34 PA5Y JO21VO FT8 -18 +04 2922km
20190915 07:35 PA3CMC JO21WI FT8 -19 -12 2920km
20190915 07:40 ON4LDP JO10UN FT8 -21 -15 2749km
20190915 07:44 G8BCG IO70RK FT8 +01 +00 2204km
20190915 08:00 PA2CHR JO32DB FT8 -15 -20 2970km
20190915 08:06 M0AFJ IO70IC FT8 -13 -03 2140km
20190915 08:36 DK4TG JO31LB FT8 -15 -21 2984km
20190915 08:54 DF1JC JO31OG FT8 -22 -11 3007km
20190915 09:12 DF6PW JO40AQ FT8 -17 -08 3049km
20190915 09:13 DL6YBF JO31OX FT8 -17 -06 3027km
20190915 09:23 PA3PCV JO20VV FT8 -24 -18 2901km
20190915 09:44 PA4EME JO20WX FT8 -17 -02 2909km
This is a more detailed view of the stations worked...
Wednesday, September 18, 2019
US Government Report on 32-42 MHz from 1998
Thanks to Rob, PE9PE who sent on an interesting link recently about a US government report about the low VHF spectrum from 32 to 42 MHz.
After a bit of research, I established that the report titled "NTIA Special Publication 98-36 SPECTRUM REALLOCATION REPORT" was from February 1998.
The report looked at who the existing users were in this part of the spectrum and whether some of the frequencies could be reallocated to commercial interests.
While the full report looked at several different bands, we'll concentrate on the low VHF spectrum here.
I have included sections of interest from the report below with certain key points highlighted in bold.
It might be worth pointing out that antennas for low band VHF tend to be very large compared to those for the higher VHF and UHF bands. For example, a full size quarter wave ground plane antenna is roughly 2.5 metres on 30 MHz and 2 metres on 40 MHz.
While the report is over 20 years old, it does show that even back then there was little commercial interest in the 30 to 50 MHz spectrum.
*****
SECTION 3 ASSESSMENT OF REALLOCATION OPTIONS
INTRODUCTION In the previous section, the bands to be considered for reallocation for non-Federal use were identified. All of the bands being considered for reallocation are used by the Federal Government agencies, in varying degrees, to support Presidential and Congressionally mandated missions. A band-by-band assessment of these factors is presented and recommendations are made as to which bands will be included in the spectrum reallocation plan.32-33, 34-35, 36-37, 38-39, AND 40-42 MHz
Band Usage
The Department of Defence (DoD) uses the frequency bands between 32-42 MHz for tactical communication using the Single Channel Ground and Airborne Radio System (SINCGARS) and other land mobile radio (LMR) assets (e.g., Scope Shield II) as well as some non-tactical intra base radio functions.
After a bit of research, I established that the report titled "NTIA Special Publication 98-36 SPECTRUM REALLOCATION REPORT" was from February 1998.
The report looked at who the existing users were in this part of the spectrum and whether some of the frequencies could be reallocated to commercial interests.
While the full report looked at several different bands, we'll concentrate on the low VHF spectrum here.
I have included sections of interest from the report below with certain key points highlighted in bold.
It might be worth pointing out that antennas for low band VHF tend to be very large compared to those for the higher VHF and UHF bands. For example, a full size quarter wave ground plane antenna is roughly 2.5 metres on 30 MHz and 2 metres on 40 MHz.
While the report is over 20 years old, it does show that even back then there was little commercial interest in the 30 to 50 MHz spectrum.
*****
SECTION 3 ASSESSMENT OF REALLOCATION OPTIONS
INTRODUCTION In the previous section, the bands to be considered for reallocation for non-Federal use were identified. All of the bands being considered for reallocation are used by the Federal Government agencies, in varying degrees, to support Presidential and Congressionally mandated missions. A band-by-band assessment of these factors is presented and recommendations are made as to which bands will be included in the spectrum reallocation plan.32-33, 34-35, 36-37, 38-39, AND 40-42 MHz
Band Usage
The Department of Defence (DoD) uses the frequency bands between 32-42 MHz for tactical communication using the Single Channel Ground and Airborne Radio System (SINCGARS) and other land mobile radio (LMR) assets (e.g., Scope Shield II) as well as some non-tactical intra base radio functions.
Friday, September 13, 2019
Watch out for VHF path to Cape Verde Is
Just a note to say that there is a nice high pressure system over the eastern part of the Atlantic at the moment and there is a possibility of a VHF opening to Cape Verde Islands from the UK and Ireland.
As always, it's a long shot but keep an eye on the tropo prediction website of F5LEN.
As always, it's a long shot but keep an eye on the tropo prediction website of F5LEN.
Wednesday, September 4, 2019
Tom EI4DQ completes an 11 band DXCC!
Congrats to Tom EI4DQ who recently achieved an 11 band DXCC!
While a number of EI stations have 10 band DXCC, Tom is the only one to get the magic 100 countries confirmed on eleven bands.
The key difference of course is that EI4DQ has managed to get DXCC on 144 MHz (2 metres) as well primarily by bouncing signals off the moon.
It's probably no exaggeration to say that it's easier to get an 8 band DXCC from 10m-80m than it is to get DXCC on 2m!
Here is an excerpt of Tom's 11 Band DXCC journey....
On the 21st of August 2019, I finally completed my 11 band DXCC.
I had started my plan of trying to gain the 11 band DXCC goal back in March of 2015, after completing DXCC for the 2 metre and 6 metre bands. I decided it was time to try and get DXCC on the HF bands as well.
The last time I had operated the HF bands was back around 1998. I installed various antennas for all the hf bands i.e. dipoles, verticals, loops, etc. I decided to start at the bottom i.e. 160mtr band (1.8 MHz), and work my way up to 10mtr (28 MHz).
My first 160mtr antenna was a single wire inverted L. It worked ok but I had lots of issues feeding it at the base as it had a very low impedance. I always had to use some type of tuner at the base to feed it and make it work.
I then made a folded Marconi L antenna out of 450 ohm open wire feeder, i.e. 4x impedance transformation. Wow what a difference!
Direct 50 ohm feed, no tuner, 1:1 vswr, and hearing and working DX much better. I also had about 60 radials down of various lengths.
I started to listen to all the 160mtr contests picking off needed DXCC both on cw and ssb and then on FT8. I also started monitoring the Reverse Beacon Network, and the DXsummet DX cluster for any new DXCC countries that were about. I was about to install a separate receive antenna for 160mts in late 2017, but when I purchased a ICOM IC7610, its noise reducing capabilities and receive were so good that I did not need any receive antenna. I completed DXCC on 160mtr in late February of 2019.
80mtr / 40mtr / and 30mtr DXCC were all completed by March of 2019. 20mtr and 17mtr were completed by April of 2019. 15mts was completed in June of 2019 and 10mtr was completed in July of 2019.
All contacts were confirmed via Logbook of the World (LOTW). I could have used some of my QSL cards from previous activity in the 1970's to 1990's period when I was very active on the HF bands but chose not to do so. I also tended to only pick out stations who were in the LOTW program.
The last band 12mtr (24 MHz) was completed in August of 2019. This band was the most frustrating band to work DX! It was a pain to hear DX on 15mtr and 10mtr and sweet nothing on 12mtr. It took me 2 months just to dig out the last needed DCXX to make 100 on this band. My final total on this band was 112 DXCC but only 100 of them uploaded to LOTW.
So at last on the 21st of August 2019, the 11 band DXCC was completed. All together it took me just over 4 years to complete the needed HF DXCC.
All my antennas are homebrew vertical dipoles, loops or verticals, modes used cw / ssb / ft8.
Now its back to 6mtr, 4mtr and 2mtr! ... Tom, EI4DQ
Monday, September 2, 2019
Study suggests 11 year Solar Cycle is “Powered By Tidal Forces of Venus, Earth, Jupiter”
I recently across this news item based on a scientific paper which was released in May of 2019. Despite the huge differences in size, the study suggests that the planetary alignment of the planets Venus, Earth and Jupiter is large enough to effect the sun and its sunspot cycle.
"As with the gravitational pull of the Moon causing tides on Earth, planets are able to displace the hot plasma on the sun’s surface. Tidal forces are strongest when there is maximum Venus-Earth-Jupiter alignment; a constellation that occurs every 11.07 years."
The lead author of the study, Frank Stefani is quoted as saying...“There is an astonishingly high level of concordance: what we see is complete parallelism with the planets over the course of 90 cycles.”
If it is true then perhaps it might allow for better computer models to be built to predict future sunspot cycles?
Not only is the solar cycle of interest for radio propagation but it is hugely relevant to the large number of satellites in orbit in terms of drag and radiation.
More info on the study in the links below...
1) Scientific Paper... A Model of a Tidally Synchronized Solar Dynamo
2) Daily Galaxy... Sun’s 11-Year Cycle –“Powered By Tidal Forces of Venus, Earth, Jupiter”
3) Newsweek... SUN'S SOLAR CYCLE IS GOVERNED BY THE ALIGNMENT OF THE PLANETS, SCIENTISTS DISCOVER
Sunday, September 1, 2019
Failure of a $14,000 antenna project
I came across this website recently which I think some readers might find of interest. It's a story of one persons antenna project in the USA which cost $14,000 and its eventual failure.
You can read it here... http://w6dsr.com/LP1005AA/index.html
Subscribe to:
Posts (Atom)