Monday, February 13, 2023

14,588km opening on the 40 MHz band from Quebec to New Zealand - 12th Feb 2023


Sunday 12th February 2023: In recent posts, I've reported on how Bob, ZL1RS in New Zealand had heard 3 of the 7 special experimental stations in the USA on the 40 MHz (8m) band as well as PJ4MM on the island of Bonaire in the Caribbean. Reports linked from the 40 MHz page.

On the 12th of February, ZL1RS managed to decode the WSPR and FT8 signals from Bernard, VA2CY in Quebec, Canada on 40.680 MHz, a distance of 14,588 kms. Bernard was granted the experimental license CYA373 by the Canadian authorities to carry out tests on the 40 MHz band.

These are the WSPR reports...

 Local   (y-m-d) TX txGrid RX rxGrid MHz W SNR drift km
2023-02-12 21:04 VA2CY FN46lw ZL1RS RF64vs 40.681457 100 13 -4 14588
2023-02-12 20:52 VA2CY FN46lw ZL1RS RF64vs 40.681454 100 17 -4 14588
2023-02-12 20:44 VA2CY FN46lw ZL1RS RF64vs 40.681454 100 16 -3 14588
2023-02-12 20:28 VA2CY FN46lw ZL1RS RF64vs 40.681469 100 -3 -1 14588

Note the signal reports that range from -3dB to a whopping +17dB, well into the region where a comfortable SSB contact would have been possible.

When I was preparing this post, I noticed that the path was also open on the 13th of February.

2023-02-13 20:24 VA2CY FN46lw ZL1RS RF64vs 40.681467 100 -16 -4 14588

Bob also reports that he also heard several US signals as well as VA2CY on FT8 as well.

Bob, ZL1RS writes... "Some thumping signals received on 8m from VA2CY in Quebec this morning ... +17 in WSPR and +15 in FT8 !

Here are today's decodes (12th Feb) from my WSJT-X  ALL_WSPR . txt and ALL . txt files ...

15,700km opening on the 40 MHz band between Ireland and Australia - 12th Feb 2023


12th February 2023: With the solar flux just above the 200 mark, some interesting paths are beginning to appear on the 40 MHz (8m) band. On the 12th of February 2023, Lloyd, VK4TVL in the north-east of Australia received the FT8 signals on 40.680 MHz from Tim, EI4GNB and Robbie, EI2IP in Ireland.

 Txmtr Band Mode Distance Time (UTC) SNR
EI2IP 8m FT8 15766 km 11:11:44 -16
EI4GNB 8m FT8 15587 km 11:00:14 -17

The signal reports of -16dB and -17dB suggest that the signals were very weak indeed and just below what is really audible to your ear. It is however stronger than what would be required for a successful FT8 contact.

Lloyd reports using an off-centre fed dipole for the 80m band up about 6-metres. No doubt with a dedicated antenna for the band, the signals would have been even stronger.

Analysis... This opening happened just after sunset in NE Australia and that no doubt was a factor in the opening. The primary mode of propagation was likely F2 with possibly some help from TEP to the north of Australia.

The distances of 15,587 kms and 15,766 kms are the longest paths that have been reported on the 40 MHz band so far for amateur radio or experimental stations. Could it go further?

The next obvious step is for someone down around Sydney & Melbourne to receive the 40 MHz DX signals. Even though it's about an additional 1000kms or so, the path is a little more southerly so the chances of success are high.


New Zealand to Europe on 40 MHz??? The problem here is that the short path and long path start getting close to the polar regions. This is especially true for stations in the UK or Ireland.

The path above shows the path from the centre of England to the north tip of New Zealand. i.e. location of ZL1RS. The path from Ireland is even worse. From the UK, the SE of England looks like the best spot i.e. G9PUV.

Perhaps a 40 MHz path from New Zealand to the OZ7IGY beacon in Denmark or the stations in Slovenia or Croatia might be more likely? The short path and long path routes certainly don't get as close to the poles.

Link: For more information on the 8m band, visit my 40 MHz page.

Sunday, February 12, 2023

Signals heard on the 40 MHz band - Sun 12th Feb 2023



Sunday 12th February 2023: Due to interference from some silly RTTY contest, I had to abandon listening on the 28.1246 MHz, the frequency for WSPR signals on the 10m band. Instead, I turned my attention to the 40 MHz band and had a listen there for a change.

The signals heard on FT8 over a 2-hour period are shown above including ZS6WAB and ZS6OB from South Africa. If this was on the HF bands, I'd be thinking 'whatever' but there is something special about hearing a signal from South Africa on a VHF band. And when I say 'hear', I really mean hear. Both the South African FT8 signals were audible to my ear.

All of the signals were on FT8 although I was able to hear Robbie, EI2IP and Willem, ZS6WAB have a contact on SSB as well. ZS6WAB was quite weak with me, maybe peaking 4/1 but still very audible. Robbie by contrast is 62kms away and is audible all of the time with a 5/2 signal report.

I was a bit surprised to hear the EI4GNB. EI9KP and G9PUV was well. At 200-600kms, they're in that kind of skip zone for signals. As for the mode of propagation, I think it was F2 layer backscatter. I see a lot of debate about aircraft scatter but most of these 'close in' radio signals on the 40 MHz band during the daytime can be easily explained by F2 layer back-scatter.

To close off the reception report, I had a listen for the EI1KNH 8m beacon as well and it was easy to hear, again probably via backscatter. There was no sign of EI1CAH in the west of Ireland or of GB3MCB in Cornwall.

In conclusion: An interesting day but the takeaway message here is that I was just using a simple CB type vertical half-wave antenna for reception. As it is tuned for 28 MHz, it's performance at 40 MHz probably isn't great.

I think anyone in Europe would be able to hear these 40 MHz signals with any sort of reasonable antenna and a special dedicated 40 MHz antenna is not required.

WM2XCS/B 40 MHz beacon heard 4000kms away on the west coast of the USA - 7th to 11 Feb 2023


George, N2CG in New Jersey has one of the seven special experimental permits for the 40 MHz band -  call WM2XCS. He has a 30-watt beacon on 40.685 MHz which beams towards Europe. The following report is about recent reception of his beacon on the 8m band.

George writes... "This week I received two WM2XCS/B 40.685 MHz CW Beacon reception reports from over 2k miles away from CA and WA as follows:

Report 1 from K6YK: I've been checking 8 meters now & then to see if I hear anything.  Yesterday and the day before I heard you! Feb. 7 and 8  your beacon was in for hours! And fairly strong at times on 40.685.
2-7-23 from 1915 to at least 2200 UTC, I checked several times and there it was! 
2-8-23 I checked around 1700 UTC and it was there already, and I didn't document how long it was in.
I was listening on an IC7600, IC756proII, FT-100D, 3 element tri-band beam.  I don't have any proper antenna for 8 meters.
I'm unable to make the auto tuners in these radios to tune on 40 MHz because they won't transmit there. So it's possible the signal might have been much stronger than what I was getting.
John Lee K6YK

Report 2 from N7MWV: I was listening to the 8m band today (I decoded WM2XEJ in EM83 on FT8 at 18:24 UTC)
and found your beacon later today; Friday 2/10. I’m no longer hearing the beacon, but it was up to
a S3 to S4 at 20:49 UTC. My QTH is Rochester WA and I’m in grid square CN86lt. QRZ says we’re
2,432 miles away. My antenna is a 7 element 6m M2 at about 61ft AGL. My receiver is my ICOM 756 Pro III transceiver with the 1st RX preamp on.
John Price N7MWV"

George continues..."Like the two reception reports I received about two weeks ago from AZ and AB that I reported to you, this weeks CA and WA stations reception reports both over 2K miles away were receiving the 30 Watt beacon on the backside of the beacon's antenna (which I keep beaming towards Europe).  I believe the current SFI of over 200 and SSN at 190 is having a positive effect in the beacon being heard in the western part of US and Canada."

Addendum: In addition to the two reports above, I also found an additional report from K7RWT on the DX Cluster from the 11th of February 2023. 

K7RWT 40684 WM2XCS/B 17:53 11 Feb 23 FN30-CN85 539 United States

K7RWT is just to the south of N7MWV and the distance is again around the 4000km mark.

In conclusion: With the solar flux now up around the 200 mark, we are now seeing east-west trans-continental openings at 40 MHz across North America. The distance of about 4000kms is perfect for one F2 layer hop. 

The fact that the 8m opening is east-west as opposed to north-south just goes to show how good conditions are at the moment. Any serious 6m operators on the west coast of the USA should be looking for this 8m beacon in New Jersey as it may suggest that a trans-continental opening at 50 MHz is possible.

Link: For more information on the 8m band, look at my 40 MHz page.

Saturday, February 11, 2023

13,318km opening on the 40 MHz band from the Caribbean to New Zealand - 10th Feb 2023


10th Feb 2023: This was another good day on the 40 MHz (8m) band as shown from the map above showing the FT8 paths from Martin, PJ4MM on the island of Bonaire in the Caribbean.

The 8m signal from PJ4MM went well into Europe and reached as far as Poland and Greece. The one path that caught my attention was the opening across the Pacific to New Zealand. I believe this is the first time a 40 MHz signal from the Caribbean has been heard in New Zealand.

These are the FT8 reports for PJ4MM in order of distance.

 Txmtr Rcvr Band Mode Distance Time (UTC)
PJ4MM ZL1RS 8m FT8 13318 km 22:51:41
PJ4MM SV8CS 8m FT8 9094 km 15:43:44
PJ4MM SR4DON 8m FT8 8830 km 14:26:30
PJ4MM SP9TTG 8m FT8 8755 km 14:35:11
PJ4MM 9H1TX 8m FT8 8563 km 15:39:44
PJ4MM DG0OPK 8m FT8 8173 km 14:51:12
PJ4MM DK8NE 8m FT8 8136 km 14:50:14
PJ4MM G9PUV 8m FT8 7438 km 14:52:44
PJ4MM EI4GNB 8m FT8 7083 km 14:28:14
WM2XCC PJ4MM 8m FT8 5485 km 19:00:56
PJ4MM CE3SX 8m FT8 5080 km 20:24:43
PJ4MM WB0DBQ 8m FT8 4453 km 18:04:41
PJ4MM VO1SIX 8m FT8 4072 km 15:05:41
PJ4MM VE2BI 8m FT8 4025 km 15:59:11
PJ4MM XE2OR 8m FT8 3826 km 18:04:44
PJ4MM WW1L 8m FT8 3595 km 15:08:44
PJ4MM K5YT 8m FT8 3557 km 18:01:44
PJ4MM K2ZD 8m FT8 3348 km 14:51:11
PJ4MM N4WLO/3 8m FT8 2901 km 20:52:11
PJ4MM PJ4GR 8m FT8 10 km 22:43:41

Bob, ZL1RS mentions that his 8m Yagi is permanently fixed at about 70 degrees.  With just 3 elements, the -3dB beam width is about 70 degrees (+/-35 deg).  So it covers 040 to 110 degrees quite well. PJ4MM is at 96 degrees.

Just for reference, the solar flux on the 10th of February was back over 200.

Bob confirms that there many decodes of PJ4MM on the day and he has kindly sent on a list of decodes to me. I have them listed below for reference.

Friday, February 10, 2023

Even more Trans-Pacific openings on the 40 MHz band - 6th to 9th Feb 2023

In previous posts, I reported on some impressive 40 MHz openings across the Pacific Ocean. On the 28th of December 2022, there was a 12,000km+ opening on the 40 MHz band from California to Australia. On the 25th of January 2023, there was a 10,470km opening on the 40 MHz band from California to New Zealand.

The common element in both posts was that the station in California was WM2XCC, the experimental 40 MHz station which is operated by Chris, N3IZN. Now we have reports of two other experimental stations being heard across the Pacific.


WM2XEJ: The first report is of Bob, ZL1RS in New Zealand receiving the WSPR signal from WM2XEJ in Georgia in the USA. This is interesting not only because of the 13,129km distance but WM2XEJ is a lot further east than the previous reception reports of WM2XCC in California.

These are the WSPR reports...

Local   (y-m-d) TX txGrid RX rxGrid MHz W SNR drift km
2023-02-08 23:34 WM2XEJ EM83ji ZL1RS RF64vs 40.68156 100 -18 0 13129
2023-02-08 23:40 WM2XEJ EM83ji ZL1RS RF64vs 40.681561 100 -1 0 13129
2023-02-08 23:46 WM2XEJ EM83ji ZL1RS RF64vs 40.681558 100 1 -1 13129
2023-02-08 23:54 WM2XEJ EM83ji ZL1RS RF64vs 40.68156 100 -1 0 13129
2023-02-09 00:08 WM2XEJ EM83ji ZL1RS RF64vs 40.681558 100 -9 0 13129
2023-02-09 00:14 WM2XEJ EM83ji ZL1RS RF64vs 40.681558 100 -17 0 13129

As you can see, the signal comes out of the noise and peaks at +1dB which is strong enough for say a good CW contact. After that, it fades away again. The opening possibly coincided with a sunset in Georgia. or a sunrise in New Zealand?

The other stations shown on the map above are from the last week and show plenty of F2 propagation on the 40 MHz (8m) band.


WM2XCW: The WM2XCW experimental 40 MHz station is located in the far north of Washington state and has now been received in New Zealand. This is significant because WM2XCW is the most northerly of the US experimental stations on the 40 MHz band.

ZL1RS... Again, most of the reports are from Bob, ZL1RS on the 6th and 8th of February 2023...

Local   (y-m-d) TX txGrid RX rxGrid MHz W SNR drift km
2023-02-06 21:48 WM2XCW CN88lx ZL1RS RF64vs 40.681533 10 3 0 11246
2023-02-06 21:58 WM2XCW CN88lx ZL1RS RF64vs 40.681533 10 -4 0 11246
2023-02-06 22:48 WM2XCW CN88lx ZL1RS RF64vs 40.681532 10 -7 0 11246
2023-02-06 22:38 WM2XCW CN88lx ZL1RS RF64vs 40.681534 10 -7 0 11246
2023-02-08 22:48 WM2XCW CN88lx ZL1RS RF64vs 40.681535 10 -10 0 11246
2023-02-08 22:58 WM2XCW CN88lx ZL1RS RF64vs 40.681535 10 -12 0 11246
2023-02-08 22:38 WM2XCW CN88lx ZL1RS RF64vs 40.681534 10 -12 0 11246
2023-02-08 22:18 WM2XCW CN88lx ZL1RS RF64vs 40.681532 10 -12 -1 11246

Note that while WM2XEJ in Georgia is listed as 100-watts, WM2XCW in Washington state is using a much lower 10-watts. The strong signal peaked at +3dB suggesting a weak SSB contact may have been possible.

ZL1RQ... There are several reports from Alan, ZL1RQ for WM2XCW but they are listed as being on 28 MHz. As WM2XCW only transmits on 40 MHz, it seems likely that ZL1RQ is listening on 40 MHz but his older version of WSJT-X software isn't configured for 40 MHz reports.

Local   (y-m-d) TX txGrid RX rxGrid MHz W SNR drift km version
2023-02-07 21:18 WM2XCW CN88lx ZL1RQ RF64 28.12616 10 -26 0 11318 2.5.2
2023-02-07 21:08 WM2XCW CN88lx ZL1RQ RF64 28.12616 10 -23 0 11318 2.5.2
2023-02-06 22:48 WM2XCW CN88lx ZL1RQ RF64 28.126157 10 -16 1 11318 2.5.2

There is also one report from ZLBEACON with the same frequency, short locater square and software version as ZL1RQ so I presume these were from Alan as well.

Local   (y-m-d) TX txGrid RX rxGrid MHz W SNR drift km version
2023-02-08 21:08 WM2XCW CN88lx ZLBEACON RF64 28.12616 10 -28 0 11318 2.5.2


WM2XCC: Unsurprisingly, most of the trans-Pacific 8m reception reports are for WM2XCC in California. Note that WM2XCC is using different power levels at different times.

VK4OTZ: There is one single report from VK4OTZ on the east coast of Australia on the 7th of February 2023.

Local   (y-m-d) TX txGrid RX rxGrid MHz W SNR drift km 
2023-02-07 23:38 WM2XCC DM13ji VK4OTZ QG62jo 40.681528 50 -24 1 11637 

ZL1RQ: There are several reports of WM2XCC from ZL1RQ but again, the frequency shown is 28 MHz rather than the correct 40 MHz one.

Local   (y-m-d) TX txGrid RX rxGrid MHz W SNR drift km version
2023-02-08 00:00 WM2XCC DM13ji ZL1RQ RF64 28.126111 50 -25 0 10550 2.5.2
2023-02-07 23:56 WM2XCC DM13ji ZL1RQ RF64 28.126111 50 -23 0 10550 2.5.2
2023-02-07 23:46 WM2XCC DM13ji ZL1RQ RF64 28.126111 50 -11 0 10550 2.5.2
2023-02-07 23:42 WM2XCC DM13ji ZL1RQ RF64 28.126112 50 -16 0 10550 2.5.2
2023-02-07 23:38 WM2XCC DM13ji ZL1RQ RF64 28.126113 50 -12 0 10550 2.5.2
2023-02-07 22:56 WM2XCC DM13ji ZL1RQ RF64 28.126113 2 -28 0 10550 2.5.2
2023-02-07 22:38 WM2XCC DM13ji ZL1RQ RF64 28.126113 2 -21 0 10550 2.5.2
2023-02-07 22:18 WM2XCC DM13ji ZL1RQ RF64 28.126113 2 -23 0 10550 2.5.2
2023-02-07 21:56 WM2XCC DM13ji ZL1RQ RF64 28.126113 2 -20 0 10550 2.5.2

ZL1RS: Bob has by far the most reception reports and these are shown below.

Thursday, February 9, 2023

Request for more reception reports on the 40 MHz band - Feb 2023

The 8th of February 2023 was another good day on the 40 MHz band with lots of reports. Both Robbie, EI2IP in Ireland and Paul, G9PUV are active almost daily on the band and their reports are shown below.

Both EI2IP and G9PUV are looking for more reception reports on 40.680 MHz. Just try listening on that frequency with FT8 and see if you can decode anything. Just make sure you have the correct frequency set on your FT8 software.

With WSJT-X, go to File - Settings - Frequencies and change one of the unused microwave bands to 40.680 000 MHz.

An antenna tuned for 28 MHz or 40 MHz should still give reasonable reports although of course, it would be best to have a dedicated antenna for the band.

Reports for the 8th of Feb 2023...


EI2IP: The map above shows the stations that heard the FT8 signals from Robbie on 40.680 MHz. Robbie writes... "The band has been on fire these last few months, and the SWL reports are extending to Mexico, Cuba, Ecuador and well into East Coast of North America."

Robbie reports that Osmany, CO2OQ  in Havana, Cuba was using a 6M Moxon antenna and an ICOM-7300 and 50 Watts. Signal reports of +4dB and -12dB were exchanged on FT8.


G9PUV: The map above for Paul shows a similar pattern with the 8m signals reaching Cuba, Mexico and Ecuador to the west.

F14700: The FT8 signal from CO2OQ was also received by SWL Jean Trenscène, F14700 in the north of France. Jean was using a SDR Play RSP1A receiver with a D3000 discone antenna.

Analysis... The signal paths that are now being reported on the 40 MHz are reminiscent of what the 50 MHz band would be like if only the solar flux and sunspot numbers were higher.

The problem in the past was that the 28 MHz band was too far away from the 50 MHz band to warn of imminent openings. Now with the 40 MHz band, 6m operators know that the maximum usable frequency is just 10 MHz below and there is some potential of an opening.

It would be good to have more stations providing reception reports on FT8 and WSPR. 40.680 MHz in the middle of the ISM band seems to have become the default frequency in terms of activity.

Both EI2IP and G9PUV are looking for more reports from Asia, Africa, South America and the western half of the USA.

Link... For more info on the 8m band, see my 40 MHz page

Heard lists... These are the stations that heard both G9PUV and EI2IP in order of distance...

Wednesday, February 8, 2023

Good conditions on the 40 MHz band - Mon 6th Feb 2023

Several stations have reported good conditions on the 40 MHz band on the 6th of February 2023.


These are the FT8 paths for Paul, G9PUV / G7PUV in the SE of England.


Robbie, EI2IP in the SW of Ireland experienced similar conditions.


Martin, PJ4MM was heard by quite a number of stations across the Atlantic on the 40 MHz band. This makes a pleasant change from just a year or two ago when the number of stations listening on the band was a lot lower.

PJ4MM writes... "Today's reports 8m, everybody thanks for the reports! All ft8 except 9a5cw

Sunday, February 5, 2023

4853km TEP opening at 432 MHz reported from Curacao to Argentina - 5th Feb 2023


Brett, PJ2BR in Curacao in the Caribbean reports that on the 5th of February 2023 (01:18 UTC), his 432 MHz signal were heard by Javi, LU5FF in Argentina by Trans-Equatorial Propagation (TEP). The distance was 4853 kms!

This really is ground breaking news (*). It was only on the 4th of February that I put up a post about what was up to then the only 432 MHz reception report via TEP in South America and that was from 1978. I tagged PJ2BR on Twitter about the post and a few hours later, we have a second 70cms TEP report!


The Green exchange is for 144 MHz while the Yellow is for 432 MHz (*).

Proof of Concept (*)... For this TEP opening on 432 MHz, PJ2BR was using the Q65b weak signal mode. This is significant because it means that modern digital weak signal modes can be used for TEP openings at 70cms. It's not a case of there being too much doppler or spreading of the signal that only CW can be used. This would likely require a much stronger signal for a contact to be made.

For the record, here is a screen grab off the PSK Reporter website before it disappears.


Let's hope that this news will encourage more stations in the Caribbean and in South America to try to make a TEP contact on the 432 MHz.

(*) = Caveat... Someone raised the question if the reports on 432 MHz are genuine? They do after all follow some Q65 reports on 144 MHz and they wonder if it's the software generating these 70cms reports?

It's a bit like conducting a science experiment and we have one data point, not exactly the five-sigma required for a definitive conclusion. What we need are more stations in South America and the Caribbean to test the TEP path on 432 MHz. If there are no more reception reports then it raises some question mark over this new report. If there are more reports then it means this report was probably ok.

Addendum: 6th February 2023... There was another TEP 'reception report' on 432 MHz on the 6th of February 2023. This time it was from WP4KJJ in Puerto Rico to LU9FVS in Argentina.


I believe the stations involved have concerns about the software generating incorrect reports after the band has been changed.

I suspect what is required is the reception of a good old fashioned CW signal to eliminate any software issues.

Saturday, February 4, 2023

5100km TEP opening on 432 MHz from Argentina to Venezuela - February 1978

While openings via TEP (Trans-Equatorial Propagation) on the 144 MHz band seem to be relatively common in South America, it's a different story on the higher frequencies.

While there have been verified TEP openings at 432 MHz in Africa in the past, any reports of TEP openings on the 70cms band seem to be extremely rare.

Back on the 13th of February 1978, YV5ZZ in Venezuela reported hearing LU3AAT in Argentina on '432.1 MHz'. The distance was approximately 5,100kms.

I'm not sure of the exact locations of either stations but Buenos Aires to Caracas is about 5,100kms and seems to be the right distance.

I found two accounts about this remarkable reception reports.

Article 1) The first one appeared in the Amateur Communications column, Electronics Today International from May 1978.

"Evening-type TEP extended to 432 MHz?

Recent record-breakng contacts on the 144 MHz band apparently supported by evening-type (or Class II) trans-equatorial propagation between Australia and Japan, Puerto Rico and South America, have been hot news in amateur circles amongst those who are keen on VHF/UHF DX.

However, no sooner was the upper frequency limit of Class II TEP extended to 144 MHz, previously established as being in the 100 MHz region, than evidence of the possible extension of this ionospheric propagation mode even higher in frequency - to 432 MHz - has come to hand.

YV5ZZ, located in Venezuala, is reported to have heard an Argentinian station, LU3AAT on 432.1 MHz in February during an opening when Argentinian stations were heard working Caribbean stations and stations in the northern countries of South America.

However, two way contact was not established, but this seems only a matter of time."


Article 2) The second one appeared in an article titled 'A Newly Discovered Mode of VHF Propagation [1978]' from the QST magazine dated October 1978.

"On February 13, 1978, YV5ZZ heard weak but identifiable signals from LU3AAT, on 432.1 MHz. Two-meter and 432 propagation far exceeds the capability of the TE mode YV5ZZ was using his satellite antenna system, which is steerable in azimuth and elevation. In the direction of LU3AAT, his horizon is obstructed by a range of mountains. The lowest elevation angle which allows for clearance of the mountain range is 8 degrees. 

On February 16, 1978, YV6ASU heard LU3AAT on 432 MHz, with his antenna at about the same angle of elevation. On yet another occasion, KV4FZ heard LU3AAT on 145.1 MHz. He reported that a peak in signal strength occurred when the antenna elevation angle was 8-10 degrees. This geometry suggests that single-hop F-layer reflection isn’t involved. The angle also seems high for the tilt associated with TE."

Analysis... In preparing this post, I did a search for the first 432 MHz contact with Trans-Equatorial Propagation (TEP) in South America and much to my surprise, I couldn't find anything. Despite the 1978 article saying that a 70cms contact would only be a 'matter of time', it looks as if it never happened and has yet to happen.

This raises the point that I have made in previous TEP related posts... Is there anyone in South America trying to make TEP contacts on 432 MHz??

I see many reports of TEP contacts at 144 MHz made by LU, PY, CX & ZP stations in South America and that's fine. But I think radio amateurs should also be experimenting to see what is possible, to try something new and to push the limits.


The chart about shows the progression of sunspot numbers since 1965. In 1978, the levels aren't that much higher than they are now in the Spring of 2023 and 1978 was also about two years before the peak of solar cycle 21.

Doppler... TEP propagation is well known for it's distortion of the signal due to some spreading. The higher the frequency, the higher the distortion.

I'm assuming that the distortion at 432 MHz will mean that modes like FT8, FT4 and Q65b cannot be used? But is that a correct assumption?

If nothing else, the use of modern weak signal modes will allow a weak signal to be seen on a screen even if it can't be decoded. A sign that a CW contact might be possible if only the signal was a bit stronger.

In conclusion... If anyone has any information about previous TEP contacts on 432 MHz from South America then  please let me know. If not, perhaps someone would like to try for the first 432 MHz TEP contact from South America?

Acknowledgement... Thanks to Carlos, LU7MC for sending on the Electronics Today International article. If your first language is Spanish and you're reading this post via Google Translate then send your information to LU7FC if it's easier.

Link...
1) For examples of TEP contacts on 2m, see my 144 MHz page.
2) For examples of other long distance contacts on 70cms, see my 432 MHz page.

Friday, February 3, 2023

LH4C - The 1962 expedition to Bouvet Island by W4BPD


In response to a recent post on the blog about the predicted 28 MHz propagation for the 3Y0J expedition on Bouvet Island, someone left a comment about a previous expedition from the 1960's.

In November 1962, Gus Browning W4BPD landed on Bouvet island with a guide and operated for four and half days. He recounted his exploits in the October and November 1967 issues of 73 Magazine.

It's an interesting account of what the conditions were like and it was certainly a very different time with less environmental concerns about wildlife disturbance.

It is reproduced below if anyone wants to read it. 

Bouvet Island - Gus Browning W4BPD Cordova, South Carolina 

Thursday, February 2, 2023

Prediction for 28 MHz propagation for 3Y0J on Bouvet Island - Feb 2023


First a disclaimer! I really don't have much interest in DX on the HF bands, DX-peditions or the HF bands in general but I have seen a lot of 'chatter' about predictions for propagation for the 3Y0J expedition on Bouvet Island during February 2023. I decided to have a look at what propagation on 28 MHz might be like and I will concentrate on Europe and North America.

If you want to see a video about general HF propagation then have a look at this previous post with a video from OH6BG.


Bouvet Island is a small island in the South Atlantic. The 3Y0J team plan to operate from a location 80m above sea level at Cape Fie at the south-east tip of the island.

The one thing to take away from this image is that there are mountains that are about 600-700m high about 4-5 kms from the 3Y0J site and these will impact the signal on the 10m band. It might be fine for the lower HF bands like 40-17m where there may be much higher level angles of radiation involved for propagation but the mountains will block some of the low angle signals required for 28 MHz. This is especially true for North America. More on that later.


This is the Great Circle map for Bouvet Island. Starting from the west... 270 degrees...and going clockwise.

North and South America are to the north-west and in the direction of the mountains... not great.

Europe to the north is blocked somewhat but is much better than North America. Japan has a sea path. Australia also has a sea path and it's likely that VK6's in Perth will fare better than their VK2,3 & 4 colleagues. The required path for some place like Sydney requires the signal to travel further south and there may be no propagation on the higher HF bands. New Zealand is at the other side of the Antarctic so that will be a challenge.


3Y0J Horizon... I put together a very rough horizon plot for the 3Y0J site on Bouvet Island and it's shown above. Note that the vertical scale is exaggerated for clarity.

A - 268 deg - This is the direction of Los Angeles and Buenos Aires. For low angle signals on 28 MHz, they fare better than the rest of the Americas. Los Angeles is a challenge from a distance point of view whereas stations in South America have a lot fewer hops to contend with

B - 282 deg - Houston. The mountains will block anything below 6.5 degrees on 28 MHz which is significant.

C- 291 deg - Florida and Sao Paulo. A 6 degree obstruction.

D - 305 deg - New York. About 6.5 degrees.

E - 323 deg - Newfoundland. Starting to get a bit easier but still a 5 degree obstruction.

F - 350 deg - Lisbon. Now down to just under 4 degrees. Better but still not great.

G - 357 deg - London. About 3.5 degrees. I have a local hill here which is about this level. I can hear stations on 28 MHz coming in from that direction but the performance is a lot worse compared to  someone who doesn't have this obstruction 

H - 6 deg - Berlin. Just below 3 degrees.

I - 11 deg - Warsaw. Down to 2 degrees. Getting down to a level where I'd start considering it being not too much of an obstruction on 28 MHz.

28 MHz Predictions - Feb 2023... For the 10m predictions, I used 100-watts from a CW station ...a typical signal for an average station and not someone with beams, towers and amplifiers. 3Y0J will of course be using much more than this but these are the kind of signals they will be listening for. 


10:00 UTC : Band is just getting going with a modest signal into Europe. The first F2 hop puts a big signal into South Africa. You can see the second F2 hop over the centre of Africa. Note that places like Greece and Sicily are in a bit of a skip zone.


12:00 UTC : The propagation moves further west. The 4th F2 hop improves signals across the centre of Europe. Note again that skip zone between the 3rd and 4th hops in the south of Europe. The path just opens to the the east coast of the USA.


16:00 UTC: The one thing to note here is the sun setting in the east of Europe. This creates a peak in signals at 28 MHz as it passes. It's a bit like a surfer waiting to catch that big wave. What's good about this is that it is confined to a relatively small geographic area.

For example, a station in Warsaw at sunset should see a peak in signals and is competing in the pile up with stations in the east of Europe as opposed to all of Europe.

There are signals in the south of Europe but it's still in a bit of a skip zone. Most of the USA is now covered.


18:00 UTC : The sunset peak reaches western Europe. It's also the best time for stations in southern Europe but there's plenty of competition from stations to the north. Signals are improving in North America.


20:00 UTC : The propagation reaches North America but the sun also starts setting in Bouvet. The one thing to notice here is that there will be skip zones. The signal could be reasonable in New York and weak in Chicago.

Caveats... It should also be noted that this is just a prediction! 

The 3Y0J team is there for most of February and the sunrise and sunset times will change a good bit over that period.

The predictions above are based on a station on a flat site with a flat horizon. The mountains and hills will block the low angle signals in certain directions and the more northern parts of where the peaks are shown are likely to be missing.

Top Tip!... Regardless of what band you're on, look for sunrise and sunset times for Bouvet and your own location, This is especially true for stations in Europe and North America. 

As the sun sets, the layers in the ionosphere can get tilted and a high angle signal going over those obstructions on the horizon can get turned into a low angle signal to be propagated forward.

Bottom Line... If you're in North America and on any of the bands from 30m to 10m then look at the sunset time in Bouvet.

Link...
1) Try out the Proppy prediction page HERE

Wednesday, February 1, 2023

5,800 km TEP opening on 144 MHz between the Dominican Republic and the west of Argentina - 29th Jan 2023


Very long distance contacts in the region of 5000-6000 kms on 144 MHz from the Caribbean to the south of Brazil, Uruguay and the area near Buenos Aires in Argentina are reasonably common via TEP (Trans-Equatorial Propagation). 

The geometry is just right for these contacts ...a) Population centres at each end of the path with active amateur radio stations ...and b) At right angles to the Geomagnetic Equator.

This map from the 2nd of February 2022 shows a typical opening...


All the paths tend to be parallel to each other as they cross the Geomagnetic Equator at 90 degrees. However even in the example above, you can see a few paths that are not exactly parallel.

LU7MC... Carlos, LU7MC is in the west of Argentina and active on 144 MHz for many years. His location is shown on the map at the top of the post in the far west of Argentina. For Carlos, the other end of his usual TEP path falls in areas further west in the Caribbean around Jamaica and Cuba, areas where there is very little 144 MHz activity.

Carlos writes..."I always wondered the same thing, why no TEP? Many years ago my interest in VHF DX awoke and I began to investigate. I believe that one of the main obstacles is the small number of operators who, are unaware of TEP and miss out on the opportunity to experiment with the different types of propagation at 144 MHz and higher.

After a long time of trying (13 years) it finally happened!! A TEP contact from the west of South America on 144 MHz :  LU7MC - HI3I Q65B 5827Km, Very atypical conditions where the strict Trans Equatorial propagation theory seems not to apply. It was always thought that it would occur with stations further west in the Caribbean."

As Carlos writes, it does seem to have been an unusual TEP opening where the path was not quite a right angles to the Geomagnetic Equator. 

It also shows that location is everything for TEP... someone near Buenos Aires can almost make daily 144 MHz contacts on TEP with the Caribbean at certain times of year and someone in the west of Argentina has to wait 13 years!


Carlos sent on a few images. This one shows the predicted map of the critical frequency of the ionosphere around the time of the TEP opening. Notice the less intense zone over the Geomagnetic Equator in South America and the more intense region either side which sets up the perfect conditions for a TEP opening.


This screenshot from Carlos shows that the contact was made on 144.180 MHz using the Q65B weak signal mode. Signals are in the region of -12 to -14dB which is just about detectable to the human ear. A CW contact would be very difficult at this signal level.

Note that the time is in UTC. Evening time TEP usually peaks around 8pm local time.


This final image shows the solar conditions on the left with the Solar Flux at 138 and the K index at 1.7. The right hand side of the image shows the confirmation of the contact via LOTW (Logbook of the World).

Chile (CE) ??? ...Now that there has been a successful TEP contact on 144 MHz from the west of Argentina, what about Chile? Is TEP possible from Santiago? Are there any stations in the west of the Caribbean interested in 144 MHz?

220 MHz and 432 MHz??? ...I would be interested to hear of any TEP openings at 220 MHz or 432 MHz. Will the distortion make digital weak signals modes unusable at the higher frequencies?

Thanks for Carlos, LU7MC for the above information and congratulations on your FB TEP QSO.

Link...
1) For more TEP contacts, check out my 144 MHz page HERE

Tuesday, January 31, 2023

Successful low power tests on the 40 MHz band in Australia - 29th Jan 2023


In Australia and New Zealand, anyone can use up to 1-watt ERP on a non-interference basis without a license on the 40 MHz ISM band. Hilary, VK2AZ has taken advantage of this and has been experimenting with a WSPR beacon on 40.680 MHz since the end of December 2022. 

On the 29th of January 2023, several stations heard the WSPR beacon from X/VK2AZ on 40.680 MHz. What's really amazing is that the power output was just 0.005 watts or 5-milliwatts!

VK2AZ writes... "At the end of December 2022 I decided to place a WSPR beacon on 40.680 MHz.
My beacon is an RFZero loaded with the WSPR transmitter code and a LPF (low pass filter) for 40MHz on its output. Currently it puts out about 5 milliwatts WSPR every 10 mins on 40.680 MHz using the call X/VK2AZ.

A local friend and Amateur, Michael, VK2TMC who is 8 km from me in the Blue Mountains, set up a Flex SDR and WSJT-X on 40.680 which allowed me to tune and test my setup.

The RFZero is also GPS locked. https://rfzero.net/examples/wspr-transmitter/

To my surprise, my 5 milliwatt beacon has been spotted at considerable distance. 
On 29 Jan 2023 my beacon was spotted by Peter, VK5PJ in South Australia at a distance of 1076 km and Warwick, E51WL in the North Cook Islands at a distance of 5902 km.

Just goes to show that you don't need a lot of power on these "Magic Bands". 
In an email to Bob, ZL1RS, Warwick, E51WL described it as "nice wspr frames from that VK with his flea"

***

For his 40 MHz propagation tests, VK2AZ is using a horizontal dipole for 40 MHz and it's broadside to Central America.

WSPR Spots from E51WL in the Cook Islands (5902kms) and VK5PJ near Adelaide...

 Local   (y-m-d) TX txGrid RX rxGrid MHz W SNR drift km
2023-01-29 00:30 X/VK2AZ QF56if E51WL BI01xa 40.663511 0.005 -26 1 5902
2023-01-29 00:20 X/VK2AZ QF56if E51WL BI01xa 40.681511 0.005 -26 0 5902
2023-01-29 00:00 X/VK2AZ QF56if E51WL BI01xa 40.681513 0.005 -24 1 5902

2023-01-29 10:50 X/VK2AZ QF56if X/VK5PJ PF95 40.681565 0.005 -20 0 1084
2023-01-29 10:20 X/VK2AZ QF56if X/VK5PJ PF95 40.681559 0.005 -18 1 1084
2023-01-29 10:00 X/VK2AZ QF56if X/VK5PJ PF95 40.681539 0.005 -20 4 1084
2023-01-29 09:50 X/VK2AZ QF56if X/VK5PJ PF95 40.681514 0.005 -15 4 1084
2023-01-29 10:50 X/VK2AZ QF56if VK5PJ PF95mk 40.681513 0.005 -22 1 1076
2023-01-29 10:20 X/VK2AZ QF56if VK5PJ PF95mk 40.681515 0.005 -20 0 1076
2023-01-29 10:00 X/VK2AZ QF56if VK5PJ PF95mk 40.681513 0.005 -25 0 1076
2023-01-29 09:50 X/VK2AZ QF56if VK5PJ PF95mk 40.681514 0.005 -24 1 1076
2023-01-29 09:40 X/VK2AZ QF56if VK5PJ PF95mk 40.681515 0.005 -24 0 1076
2023-01-29 09:30 X/VK2AZ QF56if VK5PJ PF95mk 40.681515 0.005 -33 0 1076
2023-01-29 09:10 X/VK2AZ QF56if VK5PJ PF95mk 40.681513 0.005 -25 1 1076
2023-01-29 09:00 X/VK2AZ QF56if VK5PJ PF95mk 40.681513 0.005 -23 1 1076
2023-01-29 03:10 X/VK2AZ QF56if VK5PJ PF95mk 40.681515 0.005 -26 0 1076


RF Zero board


VK2AZ has been monitoring 40MHz for about a year and a half now, hoping to see some activity from around the world using an ICOM IC-7100 and a horizontal dipole for 40MHz.

As reported in this previous post, VK2AZ managed to receive the WSPR signals from WM2XCC in California on the 28th of December 2022.

Analysis... First of all... WOW! What amazing reception reports for just 5-milliwatts and at 40 MHz as well! But what about the propagation mode?

VK5PJ at 1076 kms was probably via Sporadic-E and the strongest report was -15dB which is buried in the noise. As it's the Summer Sporadic-E season in the Southern Hemisphere then that's easy to explain.

As for E51WL at 5902 kms??? If it was Sporadic-E then we have to believe that it was something like 3 x 2000km hops. I suspect F2 propagation was involved and it was something like 2 x 3000km hops.

Whichever one you want to believe, it's still amazing for just 0.005 watts.

The way forward... I have no doubt that we need more people using the WSPR beacon mode on 40.680 MHz. A lot of countries seem to allow people to transmit very low power on the 40 MHz ISM band without any special sort of licence or permit.

Wouldn't it be great to have a load of low power WSPR stations all over Europe for the Sporadic-E season? Check your local regulations.

Links... As always, there is loads of 8m information on my 40 MHz page.

Monday, January 30, 2023

40 MHz Facebook Group reaches 600 members


Over the weekend, the 600th person joined the 40 MHz and 60 MHz Group on Facebook.

While there are many platforms for sharing information, a group on Facebook works well for sharing photos, screenshots and commenting on other peoples posts.

There are plenty of posts on this group now with lots of news about the various openings and tests in the low VHF part of the spectrum. You can find the group HERE