Tracking the KJ7VBX-11 Pico-Balloon over Ireland & the UK - 8th May 2024

As we are now at the peak of the solar cycle, some radio amateurs are using WSPR on the 28 MHz band for their Pico-Balloons as they travel around the world.

Back in April of 2024, I had a post about reception of the KD9NGV pico-balloon as it made its way off the west coast of Ireland to the North Sea. See post HERE

I often see these pico-balloon on my receive list for 28 MHz WSPR but they're nearly all somewhere far away and the propagation mode is via the ionosphere. What I find interesting about the rare really close passes is that there is no propagation mode as such, the balloon is essentially line of sight to my location.

KJ7VBX-11... On the 8th of May 2024, I noticed that I was hearing the KJ7VBX-11 pico-balloon early in the morning just as it had woken up with the sun shining on it's solar panels. I was able to hear it pretty much all day from 07:40 UTC until 18:20 UTC.

During this time, it travelled from a spot off the west coast of Ireland, over the northern counties of Donegal, Derry and Antrim in Ireland, over the south-west of Scotland and then over Cumbria in England before falling silent for the night.

On the 9th of May, it woke up over the English Channel and then headed over the Netherlands.

The balloon is at an altitude of about 13,500 metres or 44,000 feet. The WSPR transmitter is supposed to be 20-milliwatts. As far as I know, it was launched on the 2nd of May 2024 but there seems to be very little information about it.

Format... Early on the morning of the 8th, I was the only person reporting it and it was the only signal I was hearing so I was able to do some tests without any confusion from other signals.

The WSPR transmitter on the balloon seems to have two formats. The first one is shown above. The transmitter turns on as a plain carrier for 30-seconds and then sends one WSPR transmission. I presume this carrier is to warm up the transmitter which is at or below 0 deg C and the 30 second carrier stops any drifting of the following WSPR signal.

The second format is shown below...

This time, there is a second WSPR transmission after the first one.

This is a sample of the decodes that I got in the space of about an hour...

0640    6  -1.6   28.126061   -2   KJ7VBX        IO33     13    361
0642    6  -1.6   28.126060    0   0O2MCY        GC73     53  13482
0650    7  -1.6   28.126060    0   KJ7VBX        IO33     13    361
0700    8  -1.7   28.126060    0   KJ7VBX        IO33     13    361
0702    8  -1.7   28.126061    0   0S2ZAQ        FR20     10   3937
0710    9  -1.6   28.126060    0   KJ7VBX        IO33     13    361
0712    8  -1.6   28.126061    0   0U2MNO        GJ72     10   6437
0720    9  -1.7   28.126060    0   KJ7VBX        IO33     13    361
0722    9  -1.7   28.126059    0   0X2LYI        II99     60   5842
0740    7  -0.3   28.126057    0   KJ7VBX        IO43     13    255
0750    9  -0.4   28.126057    0   KJ7VBX        IO44     13    343
0752    9  -0.4   28.126057    0   012OMZ        JP66     43   2019

The short format results in just a KJ7VBX decode.

The longer format results in an additional decode which are shown above in red.

At first sight, they look wrong. The callsign, locator and power levels seem to be nonsense. However note that the callsign field starts with a zero. This is a special data WSPR signal and contains the information about the location, altitude, temperature and battery voltage. It's just the WSJT-X receive software shows it in a format that doesn't seem to make any sense.

In conclusion... The balloon is currently heading over Europe so it's going to be line of sight to a lot of stations. Just listen on WSPR on 28 MHz and see if you can hear it.

Tracking a WSPR balloon on 28 MHz off the west coast of Ireland - Apr 2024

On the 28th of November 2023, Perri Moore KD9NGV launched a Pico-Balloon from Illinois in the United States with a solar powered payload that transmits a WSPR beacon on 28.1246 MHz.

Most of the Pico-Balloons launched from the USA tend to take a path closer to about 30 degrees north of the equator and cross areas like the north of Africa and south Asia. In contrast,  the KD9NGV balloon seems to have covered a much wider area and has been reported at more northerly latitudes as shown on the map above.

By the 16th of December 2023, it had gone around the world once! By the 19th of February, it had gone around the world three times. By mid April 2024, it has gone around the globe multiple times and the red dots on the map show where it was when I received some of the WSPR signals over the last few weeks.

What caught my interest was that back on the 7th of April 2024, the KD9NGV Pico-Balloon was off the west coast of Ireland. Most of the reception reports of the WSPR transmitter are via F2-layer propagation during the daytime. When it was off the west coast of Ireland, it was at about 40,000ft (12.2kms) altitude and line of sight to my location.

As can be seen from the map above and the reports below, my first reception report on the 7th of April was at 14:10 UTC when it was about 400kms to the west. A few others reported it via F2 layer propagation but I was the main one reporting it as it tracked its way up off the west coast of Ireland.

After 17:50 UTC, I lost it but it then came into the range of GM0HBF in the Western Isles of Scotland.

It then went silent as darkness fell. Once daylight broke again on the 8th of April, it was over the North Sea and GM4WJA started to report it.

At the time of the screen grab, LA3FY/2 in Norway was hearing it and it continued then over Scandinavia. It has since crossed over Russia and at the time of writing is up over the far north of Canada.

KD9NGV Payload... The actual payload pre-launch is shown below.

The 28 MHz WSPR signal is generated by a Si5351 clock generator and the power output is just 9 milliwatts... 0.009 watts!

The antenna is a vertical half-wave dipole made of #36 enamelled wire.  The top half is from the balloon to the U4B tracker (QRP Labs) and the lower half hangs below the tracker.  Three Powerfilm MPT 3.6-75  in a vertical triangle provide the power.  The complete payload weighs 12 grams.

The balloon is described as a "silver SAG Balloon with Helium.".

In conclusion... I have noticed these WSPR pico-balloons many times on the 28 MHz band before but they are nearly always flying over some exotic location. It was just unusual to have one pass so close and be line of sight.

Reception reports for the Arctic VY0ERC 28 MHz beacon - March 2024

VY0ERC is an amateur radio station located at a weather station on Ellesmere Island at 80 degrees north in the Canadian Arctic. They operate a WSPR beacon on several HF band including one on 10m on 26.1246 MHz.

I noticed that this was one of the unusual stations that I had heard on the WSPR mode on 28 MHz recently so I checked to see what stations reported hearing this Arctic beacon on 10m over the last 5-weeks. The results are shown above.

Some observations...

1) Over the 5-week period, just 101 stations reported hearing VY0ERC on 28 MHz. In the same time period, I heard 1224 stations here on the south coast of Ireland. G0PKT near London runs a similar power (0.2w) but was reported by 1224 stations.

2) The closest reporting station to VY0ERC was TF3HZ in Iceland at 2583kms. My location is 4134kms. The best DX was EA8BFK in the Canary Islands at 6545kms.

3) From what I could tell, VY0ERC was reported somewhere on nearly every day during the 5-week period. 

4) These are my decodes of VY0ERC and I would have been listening nearly every day for the 5-weeks on 10m.

  local   y-m-d txCall txGrid rxCall rxGrid MHz W SNR drift kms
2024-03-11 15:38 VY0ERC ER60tb EI7GL IO51tu 28.126173 0.2 -18 0 4134 
2024-03-11 15:18 VY0ERC ER60tb EI7GL IO51tu 28.126109 0.2 -13 -1 4134 
2024-03-11 14:58 VY0ERC ER60tb EI7GL IO51tu 28.126160 0.2 -17 -1 4134 
2024-03-11 14:38 VY0ERC ER60tb EI7GL IO51tu 28.126168 0.2 -24 0 4134 
2024-03-11 13:58 VY0ERC ER60tb EI7GL IO51tu 28.126088 0.2 -18 0 4134 

All of my decodes were on the 11th of March and were between 13:58 and 15:38 UTC. The signal strength ranged from -13dB to -24dB so it was really buried in the noise.

In conclusion... I included this report of VY0ERC because it's a good example of how different propagation is just 10 degrees from the North Pole. While we're all enjoying worldwide propagation on 28 MHz at more southerly latitudes, it's a very different story in the Arctic region.

The two primary reasons for the lack of signals are a) the maximum usable frequency (MUF) drops are you head towards the polar regions and b) VY0ERC is in the auroral zone and this can severely distort digital signals like FT8 & WSPR.

The lack of signals coming from VY0ERC might also suggest that some of those long distance paths we see on 10m going over the polar regions are in fact not direct at all and might be skewed further south?

Opening from Hawaii to Europe on 28 MHz - March 2024

Over the last few weeks, I have been listening on the WSPR frequency of 28.1246 MHz and feeding the decoded WSPR signals to the WSPRnet website. As we're near the peak of the sunspot cycle, I was  hearing stations all over the world on the 10m band. I know when I see east-west paths open to the west coast of the USA and to Japan then conditions must be good.

One unusual signal though was the club station KH6EJ in Hawaii. The power output is just 0.2 watts into a MFJ 1982-LP antenna and it transmits on 80m, 40m, 30m, 20m, 17m, 15m, 12m & 10m. The 28MHz transmissions are at 18, 38 & 58 minutes past the hour. 

The received signals were in the range of -23dB to -29dB which means they were buried in the noise. These are the four decodes...

 local   y-m-d txCall txGrid rxCall rxGrid MHz W SNR drift km
2024-03-20 18:58 KH6EJ BK29 EI7GL IO51tu 28.126175 0.2 -23 0 11449
2024-03-20 18:38 KH6EJ BK29 EI7GL IO51tu 28.12617     0.2 -29 -1 11449
2024-03-14 18:38 KH6EJ BK29 EI7GL IO51tu 28.12614         0.2 -25 0 11449
2024-03-11 18:58 KH6EJ BK29 EI7GL IO51tu 28.126062 0.2 -23 0 11449

Why is it unusual?

1) I was the only station in Europe to decode the KH6EJ 10m WSPR signal over a 4-week period. Obviously my location in the north-west of Europe helps but I'm only using a simple vertical half-wave antenna for receive. Why didn't other stations in Europe decode the signal?

2) The short time window. I got just four decodes over the space of three days and they are all in the 18:38 to 18:58 UTC time window. This is close to the sunset times for my location.

3) The northerly path. The auroral zone in the Arctic can and does distort signals. If the signals are on  SSB or CW then they can sound a bit rough but for digital signals like WSPR or FT8, it can often mean that the signals are not decoded at all. 

In conclusion... I've worked Hawaii on 28 MHz a long time ago but if I was looking for it now as a new country on 10m then I'd be checking the band at sunset in March.

Australian stations heard on 28 MHz WSPR over a 4-week period - Jan & Feb 2024

Conditions on the 28 MHz band have been really good for the last few weeks as can be seen from the map above which shows all of the WSPR stations that I heard from the 23rd of January to the 19th of February 2024.

In total, there are 1334 individual stations which is a lot for a mode like WSPR which after all is just a beacon mode and not designed to make two way contacts. There are a lot of interesting paths in the map but the one I will focus on here are the ones to Australia.

My location in north-west Europe is in the region of 15,000 to 17,500 kms from Australia. While it's not exactly the 'other side of the planet' i.e. 20,000kms, it's still a long way for a 28 MHz signal to travel.

In total, I heard 28 stations from Australia over the 4-week period on 28 MHz. The list is shown below...

local   y-m-d txCall txGrid rxCall rxGrid MHz                 W SNR drift kms
2024-02-15 13:58 VK6TQ OF76of EI7GL IO51tu 28.126101 20 -16 0 15139
2024-02-01 13:22 VK6MJV OF77 EI7GL IO51tu 28.126135 10 -27 0 15028
2024-01-31 12:56 VK6LDL OF77vx EI7GL IO51tu 28.126201 5 -20 1 15047
2024-02-13 12:34 VK6HQ OF87av EI7GL IO51tu 28.126028 0.2 -26 0 15071
2024-02-06 12:26 VK6CRO OG65ud EI7GL IO51tu 28.126137 0.2 -24 -2 14335
2024-02-13 12:22 VK6BMT OF78ve EI7GL IO51tu 28.126038 0.2 -25 0 15031
2024-02-03 07:58 VK5ZBI PF95ga EI7GL IO51tu 28.12613     10 -27 0 16794
2024-02-09 07:54 VK5ADE PF94hj EI7GL IO51tu 28.126084 20 -22 0 16849
2024-02-01 08:54 VK4TMT QG62 EI7GL IO51tu 28.126097 0.1 -18 0 16894
2024-02-01 08:56 VK4SA QG62 EI7GL IO51tu 28.12615     0.2 -26 0 16894
2024-02-19 08:58 VK4PK QG62qi EI7GL IO51tu 28.126134 0.2 -19 0 16923
2024-02-14 08:42 VK4NE QG62nj EI7GL IO51tu 28.126133 0.1 -26 -1 16909
2024-02-19 09:00 VK4LA QG62 EI7GL IO51tu 28.125991 0.2 -26 0 16894
2024-02-01 08:42 VK4JBY QH30jq EI7GL IO51tu 28.126168 0.2 -28 -3 15801
2024-02-19 08:42 VK4EKA QG62ap EI7GL IO51tu 28.126177 1 -7 0 16838
2024-02-19 08:58 VK4BA QG62 EI7GL IO51tu 28.126196 0.2 -20 0 16894
2024-02-03 09:10 VK4AGR QG53wg EI7GL IO51tu 28.126187 0.2 -27 0 16768
2024-02-04 09:18 VK3VJP QF12 EI7GL IO51tu 28.126022 0.2 -20 0 17273
2024-02-16 08:06 VK3KCX/1 QF22qd EI7GL IO51tu 28.12603  5 2 -14 0 17449
2024-02-18 09:46 VK3CWF QF22ke EI7GL IO51tu 28.12606 5 -25 0 17415
2024-02-01 08:18 VK3AMW QF22ir EI7GL IO51tu 28.12607  5 5 -16 0 17362
2024-01-30 08:52 VK2XSM QF56og EI7GL IO51tu 28.12605     1 -19 -1 17419
2024-02-06 08:12 VK2VJ QF57vb EI7GL IO51tu 28.12604     1 -21 1 17373
2024-02-01 08:22 VK2QQ QF55gt EI7GL IO51tu 28.126209 5 -23 -2 17427
2024-02-12 09:20 VK2KYB QF56lf EI7GL IO51tu 28.126085 5 -27 0 17410
2024-02-19 09:52 VK2HL QG56 EI7GL IO51tu 28.126156 0.2 -25 0 16406
2024-02-16 08:06 VK2GDF QF67ch EI7GL IO51tu 28.126142 0.2 -14 4 17369
2024-02-01 07:56 VK1KF QF44mr EI7GL IO51tu 28.126049 5 -22 -3 17445

The ones I find of special interest are the low power stations which are in bold running output powers of 100 to 200 milliwatts. On my side, I'm just using a simple cheap half wave vertical CB type vertical to hear all of these stations.

It's just an example of how good conditions are now on 28 MHz at the peak of the sunspot cycle and is in marked contrast to the minimum a few years ago.

New WSPR receiver from RemoteQTH

RemoteQTH is a small company in the Czech Republic and they have just announced the release of a new receiver for WSPR. 

It can be used from 0.1 to 28 MHz and is described as follows..."The openWSPR receiver is a stand-alone HF receiver for WSPR. Just connect an antenna, internet and a DC power supply and you're ready to go! With this tiny receiver you can decode and relay WSPR messages to WSPRnet.org. 

Since the entire project is open source, receivers can be easily reprogrammed to receive signals other than WSPR. The nanoPi board inside runs Raspbian OS and several user programs, which are automated by custom scripts, making the receiver completely maintenance-free."

It is selling for €125 which at first glance sounds expensive but I guess one of the main features of this WSPR receiver is that it doesn't require an external PC or computer to run. All of the decoding is done inside the unit. All you need to do is connect the various cables, configure it, connect an Ethernet cable and it uploads the spots to WSPRnet.

Looking at the size of the box relative to the SMA or Ethernet connector then it's really small and just a few cms across.

Future products... They are also developing a separate transmitter module.

They have no information on this in terms of power output but 200 milliwatts seems to be the norm.

It's also interesting to see that they are developing a series of band pass filters...

I think these will be attractive to users of other WSPR products as well as all you need are the connecting SMA patch leads.... no construction, soldering or winding of torroids. 

The photo above shows the surface mount components inside the filter.

Nearly all of these low power WSPR transmitters have a square wave output and require some sort of filter to remove the higher harmonics. This is usually done with a low-pass filter rather than a bandpass filter which tends to have slightly more loss.

Where bandpass filters shine is with the receiver module as they keep all of the potentially large signals on the lower bands out of the front end of the receiver. I think these standalone filter modules may be of interest to anyone with a SDR receiver and who want to concentrate on one band.

Link... More info on the RemoteQTH website

Disclaimer: Just to clarify, no-one paid for this post or sent any product to me for review. These are new products that I think people will be interested in.

Addendum: Since putting up this post, someone hs asked about whether the receiver can hop between bands? Does it run WSJT-X? And what is the performance of the receiver?

I looked at the files section of the site and found a circuit diagram. The receiver schematic shows the input RF going straight into an IC without any preceding RF stage amplification. This might be ok on the bands on the lower bands like 40m or 80m but is it going to be sensitive enough on bands like 10m / 28 MHz?

The input has a single LC parallel circuit which suggests that it is intended for single band use. If these components are left out then an external band pass filter is required for each band.

WSPR activty report for the 28 MHz band - Nov 2023

Every day for the last few months, I have left the radio listening on the WSPR frequency of 28.1246 MHz and I feed the spots up to WSPRnet. Most days, I don't even check what the radio heard, I just leave the radio on so that others can see how far their 10m WSPR transmitters are reaching.

I had a look today at what I heard for the last 5-weeks which is from the 26th of October to the 29th of November 2023. Considering that we're near the peak of the sunspot cycle, this post gives an idea of what what the band was like.

Totals & Distribution... In total, I heard about 1200 individual stations on 28 MHz during the 5-week period. This is a huge change from a few years ago when I would hear relatively few. It's not that conditions just got good but I think a lot of WSPR users came up to 28 MHz from the lower bands. 

There are a few false reports in the 1200 from strange callsigns out in the middle of nowhere but the vast majority of them are genuine.

The map above shows the distribution and it's obvious most of the WSPR activity is centred on North America and Europe. South America is surprising low and there is almost nothing from Africa outside of South Africa. There is however a good amount of activity from Australia.

DP0GVN... I heard the German Antarctic research station DP0GVN a total of 47 times during the 5-weeks. The best times seem to be in the afternoon but I heard it as early as 07:48 UTC and as late as 18:48 UTC.

Japan???... Where is everyone? I know there have been paths from Ireland to Japan on 28 MHz for people using FT8 but I heard nothing on WSPR. I checked some of the reports for some of the Australian stations and these seem to confirm that there seems to very little interest in WSPR in Japan.

North America... This is the distribution of stations in North America. For the USA, this pretty much mirrors the level of activity and population in the country. You can draw a line north from Houston, Texas and a lot of the radio amateurs are to the east of that.

From Ireland, it's pretty easy to hear the eastern half of the USA so it's nice to see all of those more difficult northerly paths to the west coast. This is especially true when I start seeing those VE6's and VE7's in the north-west.

I do have one report of hearing KL2OF in Alaska but I think it was bogus. I only heard it once, QRZ says the call has expired and the signal was only sent for one 2-minute period. 

I'm not even sure if a WSPR path is likely to Alaska from Europe considering the polar flutter on the signal at 28 MHz?

The UK on Backscatter... There are quite a number of stations in England using WSPR on 28 MHz and most of these stations shown above are about 400-700kms from my location. This is too short for single hop F2 layer and they are in my 'skip zone' according to usual propagation textbooks.

There might be some Sporadic-E in there but it's likely the vast majority are F2 layer backscatter. The 10m signal is being reflected off distant objects like mountains and ocean waves 1000's of kms away. It's certainly not aircraft scatter.

France - Où êtes-vous???... The map above shows the distribution of signals from western Europe. WSPR is popular in the Netherlands and Germany but where is all the WSPR activity from France???

It doesn't seem to be just a lack of transmitters either. There seems to be a equal shortage of people in France listening on the band and reporting.

Australia on 10m... It's always nice to see the 28 MHz WSPR signals from Australia coming through and I heard 29 VK stations in the 5-week period. For whatever reason, I didn't hear any VK7 stations from Tasmania.

As can be seen from the chart below, most of these stations are about 15,000 to 17,500 kms from my location.

Note the Signal to Noise reports (SNR). Most are these signals are buried in the noise and below what can be heard by the human ear. That's the magic of the WSPR mode.

WSPR seems to have a niche following in Australia and those guys are doing some interesting work investigating propagation paths on the 50 MHz and 144 MHz VHF bands.

Polar Stern... Nearly all of the WSPR signals are from stationary stations but a few are on the move. The map above shows my reception reports of the German polar research ship Polar Stern which uses the call DP0POL. It went through the English Channel a few weeks ago and made it's way down to South Africa.

Some days, propagation is good and I get a string of reception reports resulting in a blurred line. Some days, I heard it only a few times if t all.

Path of pico-balloon AF6IM

Pico-Balloon AF6IM... The very small balloon AF6IM was launched from California a number of weeks ago and it has gone around the world at least once. See my previous post.

The map above shows where I heard it over the last few weeks.

In summary... As a beacon mode, WSPR won't be of interest to everyone but it's nice to see a good level of interest in the mode especially on the 28 MHz band.

Just for reference, I was using a simple CB type half-wave antenna for this test so nothing special on my side.

Link...
1) The best website to check WSPR reports is http://wspr.rocks/

Tracking the AF6IM Pico-Balloon on 28 MHz from the USA to China - Oct 2023

For the last 12-months or so, I have been being monitoring the WSPR beacon frequency of 28.1246 MHz nearly every day and uploading the reception reports to the WSPRNet site.

I noticed recently an unusual signal out in the Mid-Atlantic.. AF6IM. I thought at first it was a bogus WSPR report but then I noticed that I had heard the signal several times and it was moving!

After some checking, I discovered that the signal was actually from a Pico-Balloon with a 13-milliwatt WSPR transmitter underneath it. It was launched by Mark, AF6IM in California at the end of Sept 2023 and it has been slowly drifting eastwards since. At the time of writing on the 26th of October, it is over China.

The map above shows my reception reports of the 13mW beacon. It only operates for a few hours every day as it is solar powered and has no battery. That's why the signal is shown as small batches of signal locations in a row.

The pictured is further complicated by the fact that Mark actually had two 28 MHz Pico-Balloons in the air over the last few weeks.

The design of the WSPR transmitter is shown above and you can find more information about it HERE

The antenna for this 28-MHz transmitter is a very thin wire which is 2.54 metres long which is a quarter wave on 10m.

This photo by AF6IM shows the pico-balloon at launch. As the balloon gains altitude and the pressure reduces, the size of the balloon will get larger.

The solar cells are not shown.

Even though the original balloon looks very small, it's still able to keep a very small payload aloft at a high altitude. The chart above shows the launch of the balloon and floating along at an altitude of about 12,500m or 40,000ft. This is well into the Jet Stream and this is what is now carrying it  around the world.

The temperatures at this altitude are well below zero as can be seen in this image above. One obvious advantage in not carrying a battery other than additional weight is that there are no problems with a battery trying to survive at these low temperatures.

In conclusion... There have been plenty of other pico-balloons operating on lower frequencies in the past like on 14 MHz but I really don't have much interest in those bands. This is the first time I recall seeing one operating on 28 MHz.

What I find fascinating is that I have heard the little 13-milliwatt 28 MHz transmitter over 450 times over the last few weeks while it was hanging below a little balloon up in the Jet-Stream.

If you want to track it, you can follow it HERE

Opening on the 40 MHz band from Ireland to Australia - Oct 2023

I noticed in the last few days that there has been a path open on the 40 MHz (8m) band from Europe to Western Australia in the morning hours.

Here are the WSPR spots from the Irish beacon EI1KNH which is just south of Dublin.

 y-m-d txCall txGrid rxCall rxGrid MHz W SNR drift km
2023-10-18 09:44 EI1KNH IO63ve VK6JR OF76mi 40.014505 20 -29 0 14969

2023-10-16 09:44 EI1KNH IO63ve VK6JR OF76mi 40.014511 20 -21 0 14969
2023-10-16 09:34 EI1KNH IO63ve VK6JR OF76mi 40.01451 20 -21 0 14969
2023-10-16 09:14 EI1KNH IO63ve VK6JR OF76mi 40.01451 20 -20 0 14969
2023-10-16 08:54 EI1KNH IO63ve VK6JR OF76mi 40.01451 20 -26 0 14969

2023-10-15 10:34 EI1KNH IO63ve VK6JR OF76mi 40.014509 20 -33 0 14969

2023-10-09 11:34 EI1KNH IO63ve VK6JR OF76mi 40.014499 20 -29 0 14969
2023-10-09 11:14 EI1KNH IO63ve VK6JR OF76mi 40.014498 20 -22 0 14969
2023-10-09 10:54 EI1KNH IO63ve VK6JR OF76mi 40.014498 20 -23 0 14969
2023-10-09 10:44 EI1KNH IO63ve VK6JR OF76mi 40.014499 20 -25 0 14969

2023-10-08 10:44 EI1KNH IO63ve VK6JR OF76mi 40.014498 20 -24 0 14969

EI1KNH transmits four times every hour using the WSPR mode and the power is about 20-watts into a vertical half-wave antenna. The receiving station was Wayne, VK6JR to the south of Perth in Western Australia. The distance was 14,969kms.

The signals are very weak and they are in the range of -20dB to -33dB. This would mean that they are inaudible to the human ear.

The path seems to have been open on five days from the 8th to the 18th of October 2023. The times range from 08:54 to 11:34 UTC.

Sunset in Perth is about 10:30UTC so it's likely there was some enhancement due to some tilting of the ionosphere. With the solar flux at about 140, the propagation mode may have been multi-hop F2 layer with perhaps some chordal hop as well.

Greece to Australia on 40 MHz... VK6JR also heard the WSPR beacon of Costas, SV1DH in Greece.

y-m-d txCall txGrid rxCall rxGrid MHz W SNR drift km
2023-10-09 08:02 SV1DH KM18 VK6JR OF76mi 40.681494 10 -24 -2 12412
2023-10-09 07:38 SV1DH KM18 VK6JR OF76mi 40.681492 0.01 -28 -1 12412
2023-10-09 07:30 SV1DH KM18 VK6JR OF76mi 40.681492 0.01 -25 -2 12412
2023-10-09 07:26 SV1DH KM18 VK6JR OF76mi 40.681492 0.01 -23 -2 12412
2023-10-09 07:16 SV1DH KM18 VK6JR OF76mi 40.68149 0.01 -21 -1 12412
2023-10-09 07:10 SV1DH KM18 VK6JR OF76mi 40.681491 0.01 -19 -3 12412
2023-10-09 06:58 SV1DH KM18 VK6JR OF76mi 40.681491 0.01 -22 -1 12412

According to the data above, SV1DH was using around 0.01 watts or 10-milliwatts for the majority of his transmissions! The last one was at 10-watts. The distance was 12,412kms. 

In general, the path from the south-east of Europe to Australia is easier as the path is shorter and the signals stay closer to the equator.

In summary... We have seen plenty of other openings on the 40 MHz band between Europe and Australia over the last 12-months. I have details of these in previous posts which are linked from my 40 MHz page.

It's very likely that we will see more openings like this over the next few months. Serious 50 MHz operators should take note of these 40 MHz openings as they suggest that an opening on the 6m band may be possible.

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 ...

Canadian Arctic Research Station VY0ERC heard on 28 MHz - 19th March 2022

Saturday 19th March 2022: I was checking my 28 MHz log for WSPR when I noticed that I had heard the Canadian Arctic Research Station VY0ERC.

What is unusual about this is that the station is located on Ellesmere Island at 80 degrees north in the Canadian Arctic and this was on 28 MHz, not one of the lower HF bands.

In the last 5 weeks, it has only been heard on 28 MHz by 3 stations in the direction of Europe.

Local   (y-m-d) TX txGrid RX rxGrid MHz W SNR drift km
2022-03-19 15:58 VY0ERC ER60tb GM4VAC IO77xm 28.126127 0.2 -25 -3 3615
2022-03-19 15:38 VY0ERC ER60tb GM4VAC IO77xm 28.126062 0.2 -18 -3 3615
2022-03-19 15:18 VY0ERC ER60tb GM4VAC IO77xm 28.126089 0.2 -18 -3 3615
2022-03-19 14:58 VY0ERC ER60tb EA8BFK IL38bo 28.126176 0.2 -3 0 6545
2022-03-19 14:38 VY0ERC ER60tb EA8BFK IL38bo 28.1261 0.2 -3 -3 6545
2022-03-19 13:58 VY0ERC ER60tb EI7GL IO51tu 28.12604 0.2 -22 -3 4134

Station details... Eureka, Ellesmere Island, Nunavut, Canada. VY0ERC is currently operating out of the Polar Environment Atmospheric Research Laboratory (PEARL) Ridge Laboratory (RidgeLab) located on top of the hill at 80 degrees 3 minutes N and 86 degrees 25 minutes W at 600 m.a.s.l. 

The WSPR station was running just 200 milliwatts which makes it even more remarkable.

There are a few things that make this reception report unusual.

1) It was on 28 MHz and it's not usual to hear signals from so far north. The solar flux on the day was only 94 and most propagation paths are much closer to the equator.

2) The distance for me was 4,134 kms which suggests perhaps it was F2 propagation? If it was due to other propagation modes closer to the E layer than multiple hops would be required.

3) No distortion. Signals going across the polar regions tend to have an auroral flutter, something that is not conducive to WSPR.

4) Why the lack of stations hearing the signal in Europe? Why only two in the UK and Ireland?

Good opening from Europe to Australia on 28 MHz - 31st Jan 2022

Monday 31st January 2022: There was a nice opening on 28 MHz on the 31st with some strong signals between Australia and Europe.

The map above shows what I heard on WSPR on 28 MHz on the 31st. While conditions were poor to the west, it was good to the south and the east. It's worth noting that this is WSPR where there is a limited number of stations transmitting. If I had been listening on FT8 then the map would have a lot more dots.

Local   (y-m-d) TX txGrid RX rxGrid MHz W SNR drift km 
2022-01-31 09:20 VK3KCX/1 QF22qd EI7GL IO51tu 28.126017 50 8 0 17449
2022-01-31 12:10 VK3KTT QF22gg EI7GL IO51tu 28.126102 50 -18 0 17388
2022-01-31 10:54 VK3QD QF22ik EI7GL IO51tu 28.12601 2 -23 1 17385
2022-01-31 09:58 VK6XT OF86td EI7GL IO51tu 28.12618 5 -11 0 15311

I heard four VK stations on WSPR with all three of the VK3 stations near the city of Melbourne. 

The 50 watt signal of VK3KCX/1 had a signal to noise ratio of +8dB which is up at the level where a SSB contact would be possible. It was nice to see the 2 watt signal from VK3QD also making it through with a signal of -23dB.

I also heard the VK8VF beacon near Darwin on 28.268 MHz which was just above the noise. There's something magic about actually hear a CW signal from the other side of the world on 28 MHz. 

The video clip below from G8DX shows how strong the signals were on SSB...

Amazing conditions on 28MHz today - here’s a short clip of VK3KJ from this morning with my aerial at just 25ft due to strong winds #hamradio pic.twitter.com/RFsS2acrnN

— Jack G8DX (@jackg8dx) January 31, 2022

The solar flux was up at 130 so it seems the sun is well up on the 100 or so of late.

3155 km opening on 144 MHz between Australia & New Zealand - 28th Jan 2022

28th January 2021: There was another 3000km+ opening on 144 MHz between Australia and New Zealand when Peter, VK5PJ in Adelaide received the WSPR signal from Bob, ZL1SIX.

The two WSPR decodes are shown below and the signals were pretty weak at -19 and -20dB.

 UTC (y-m-d) TX txGrid RX rxGrid MHz W SNR drift km
2022-01-28 01:06 ZL1SIX RF64vt VK5PJ PF95mk 144.490537 10 -21 0 3155
2022-01-28 01:12 ZL1SIX RF64vt VK5PJ PF95mk 144.490537 10 -19 0 3155

The map above shows the WSPR signals heard on 144 MHz by VK5PJ over a 24 hour period. Most of the Australian signals are tropo but the 3155km distance was really something else.

Remember, 3155kms is the distance between Ireland and Newfoundland across the North Atlantic.

Propagation??... It's important to note that VK5PJ was the only station in Australia to hear ZL1SIX on 144 MHz that that. i.e. none of the closer stations near the south-east coast heard him. This does suggest that Sporadic-E was the main propagation mechanism.

One single Sporadic-E hop might account for a maximum of say 2300kms but not 3155kms. What makes up the difference?

The map above shows the tropo prediction from Pascal, F5LEN and it suggests that there might have been some tropo ducting over the Tasman Sea.

It's possible that the western path of the 3155km path was due to Sporadic-E and that coupled into a maritime duct for the remainder of the circuit to New Zealand.

A second option was that it was due to chordal hop Sporadic-E with the signal going between two Sporadic-E 'clouds'. This does happen at 144 MHz but it is relatively rare.

It's impossible to know for sure what the propagation mechanism was but the probability of a combined Sp-E / tropo duct opening is higher.

Link...
1) More examples of long distance paths can be found on my 144 MHz page.

12,000km opening between Australia & California - 27th Dec 2021

Monday 27th December 2021: It was interesting to see that there was a recent opening on the 50 MHz band between the SE of Australia and southern California. Unlike openings from Australia to South America, this one crossed the equator and went to North America.

There is a very active group in Australia & New Zealand using the WSPR beacon mode and on the 27th of December, VK2IJM and VK2EFM in New South Wales heard N3IZN in California.

 UTC (y-m-d) TX txGrid RX rxGrid                         MHz         W SNR drift km 
2021-12-27 01:16 N3IZN DM13ji VK2IJM QF56ni 50.294549 100 -24 0 12115 
2021-12-27 00:52 N3IZN DM13ji VK2EFM QF56oq 50.294554 100 -18 0 12091 

The distance was just over 12,000kms.

Propagation Mode?? The first most obvious answer is that it was multi-hop Sporadic-E but I suspect the reality is more complex that that. The signal path crosses the TEP zone around the equator so that may have had some impact. The solar flux is up around 120 and the MUF is now above 30 MHz most days. Is it reaching 50 MHz near the equatorial region?

Western Australia to Europe?? The example above was just over 12,000kms, that is the same distance from the west coast of Australia to the south-east of Europe. Are there openings between Europe and Australia on 50 MHz at the moment?