Friday 19 April 2024

Bernd Wilde, DL7APV, SK.

I learned via the EI7GL blog site (see link in sidebar) that Bernd, DL7APV, has become silent key.

Bernd was a fixture on 432MHz before he constructed his massive antenna in 2018, and after that he introduced many to the potential of the band. His behemoth array has 128 11 element antennas formed into a vast box with an overall gain of 33.7 dBd. Not only did I work him via Earth-Moon-Earth using this monster, I also worked him easily on tropo at a distance of over 1000km.

Bernd, DL7APV, now sadly SK, and his 70cm antenna

I will miss Bernd's gentle reminders about upcoming contests. He had a delightful way of expressing his wish for me to come on and give him a contact via moonbounce. He would send me an email and point out the date of the forthcoming event. He would then say that if it could be fun for me to have a contact with him, it would also be fun for him to have a contact with me during the contest. He did not say "come on and work me", but rather he correctly pointed out that I could if I would enjoy it. He was right: I did enjoy it.

Actually there was no need for a formal sked, I could hear him very clearly and reply to his CQ call. My antenna only has about 14 dBd gain, so he was doing all the work. No doubt he sent similar E mails to large group of operators who, like me, had enjoyed early EME success working Bernd on 70cm. 

I shall miss Bernd and I send his surviving family and friends my condolences.

Where will we ever find such an enthusiast again?

73 Jim 

GM4FVM

Monday 1 April 2024

Amateurs - don't do as I say !!!

Amateurs - don't do as I say ... do what you want to do!

Please, I implore you - find your own way. Do not follow anyone's insistence, but learn from the many voices out there. Also, I encourage you to learn from what you do, and to progress in your own path.

And I know, that is me telling people what to do.

Irony, eh? Who needs it?

I recently posted an encouragement to VHF+ amateurs to try Q65, a splendidly efficient data mode devised by Joe Taylor and his merry tribe of creators. I did not say "give up your old modes". 

Here is a screenshot taken by Phil, EI9KP of our 2m QSO on Q65. Not bad at all - 479km on a flat band. We went on using Q65 successfully on 70cm. Eventually we tried 23cm, and although we did not complete a QSO there no doubt we will in due course. Q65 is good for contacts like this as it benefits from scatter enhancement such as that from aircraft. 

I think that it is best to use the best mode for the purpose, so for meteor scatter I use MSK144, for HF I would use FT8, and so on. Those were a great set of QSOs with EI9KP. You do not have to follow suit, but you can see how it can be done. As usual, click on the images to enlarge if you wish.

144MHz Q65-30B contact between EI9KP and GM4FVM on 25 March 2024 (Screenshot EI9KP)

Then I went on the 2m/70cm KST chat room [that is where you went wrong, Jim]. 

On KST someone asked for a meteor scatter contact and I explained that I can use MSK144. He then told me that I was wasting my time with MSK144 and I should install MSHV and use the JTMS mode instead. He said that there is "scientific evidence" from many hams to prove that JTMS was more efficient. 

What is the difference between me encouraging people to use Q65, and him telling me to install MSHV and use JTMS not MSK144. Is it just that I cannot take instruction, or learn from scientific evidence?

Well, I think not. I sincerely hope that everybody who reads this blog takes my ideas as representing what works for me. You can read about what I do, go away to your own blogs, and say the opposite. Or go to the local club and say that that old codger GM4FVM is talking nonsense. Sometimes I do talk nonsense. I can be wrong and I often am (source of ionisation for Es, for example). I can learn as I go along, and so can everybody else. I can even admit to being wrong.

Returning to the recent KST barney. I simply said that I use MSK144 on meteor scatter. This seemed to make things worse. After a blast in return I said that I respected his choice of mode and I hoped that he would respect mine. And then things calmed down a bit. I had some support from others on KST which I appreciate.

As for the scientific evidence, he did not say what he was talking about. Data modes for meteor scatter work on the principle that the meteor pings are short duration, thus the data rate is set so that the message fits into a very short timeframe. It is then repeated over and over again for 30 seconds in the hope that some of it will be transmitted at the same moment as a meteorite provides a tiny moment of propagation between the two stations. Different modes use different periods but from what I recall MSK144 repeats the message every 72 milliseconds. That would suggest that your message is repeated more than 415 times in your 30 second period, and almost all of those repeats is not detected by anyone.

The argument has been put that because the pings are of shorter duration at higher frequencies, then the time of repeat needs to be shorter too. That is a fair enough argument except that MSK is also up to about 8dB more sensitive than some other modes, and that affects the timing issue too. When you increase the sensitivity the pings are received for longer. This is because as the ping proceeds the amplitude declines, and with more sensitivity you can receive it further down the "tail" as it tails off. This means that the decode can lasts longer. Thus MSK does not need such a short timeframe. This is a benefit which some people use to argue against MSK, even though it is actually a benefit.

MSK144 is tailored for the 2m band and is probably over-engineered for 4m and 6m (so of course it works even better there). Maybe it would not be quite so good on higher frequency bands. The WSJT-X notes say it is designed for VHF bands so it would not be my choice for 70cm.

Anyway, I use MSK144 for another reason too. MSK144 has powerful error correction which other modes used for meteor scatter lack. I think that the reason why some people prefer other modes is because they produce less well corrected results which they interpret their own way. I do not criticise this, but I choose not to do it myself. I used older modes for years and I have had enough of looking at screens full of gibberish. Back then I quickly saw that I could interpret the results they produced in hundreds of different ways. To me that means anyone can interpret them in ways that suit them.

If you need some low-down on this you might find this from K5ND interesting:-

https://k5nd.net/2020/10/msk144-vs-fsk441-meteor-scatter-modes-my-scattered-compilation-of-data-points/

Before MSK, most modes used much weaker error correction, leaving operators to make sense of bits and pieces of decodes. The temptation to find evidence of success blinded quite a few to the fact that they were actually piecing together bits of decode provided by random noise.

70MHz FSK441 screen from 4 January 2016 showing partial decodes.

The example shown above is actually from a fairly long and successful period of reception on  4m - a band where results are better than on 2m. It looked like EA2BCJ was calling me, and this eventually proved to be the case. Maybe he was calling GM4F6M, which was also a possibility. Despite all the favourable factors, no single ping contained both correct callsigns together. In many cases there were screens full of garbage from which amateurs of the time would piece together the evidence they thought constituted a contact. Bill Somerville, G4WJS, is quoted in the K5ND piece in the link above commenting on those operators "who prefer to pick out a few relevant characters from a jumbled stream of uncorrected errors and decide that a QSO has been completed." Of course they can do that, but I do not want to.

Sadly Bill is now silent key and we miss his wisdom.

My simple decision was to use only MSK144 on meteor scatter. I think that I am free to decide that. Others seem happy to only use CW on Top Band, some only use 20 metres to have chats around Europe, still others just solder together circuits they never use. Fine business old men. You have that choice. I am not wasting my time doing what I want to do just because you do something else. I might say here that Q65 is going begging, but I don't tell people that they are wasting their time doing anything else. It is up to them.

We all think that our own set-up is the best. The only better one is the one we plan to buy when we can afford it. Most of us think that everybody else is barking up the wrong tree. Fine, but please don't preach to me.

I did not have the heart to tell this guy on KST that I already have MSHV installed here. I could run JTMS if I wanted to. I choose not to. As I said, mode is my choice, just as much as it is his. I could run some other meteor scatter mode, but give me proper error correction and lots of sensitivity every time.

Here is some advice from someone with years of experience - do not accept advice from people with years of experience. By all means listen to them, but form your own ideas yourself and go your own way.

Even if you go the wrong way, it is still your way. And, you can always learn some more and change later.

Finally, an 11 minute QSO from the good old days before strong error correction. Is this complete?

70MHz FSK441 contact between GM4FVM and SQ85PZK on 6 April 2015

Who decided that GM5JVM was wrongly decoded but GM4FVM was correctly decoded? Is this my QSO at all? I would rather leave decisions like that to the algorithms in WSJT-X.

73

Jim GM4FVM

Monday 25 March 2024

Q65 on aurora, plus the arrival of the Es season.

Not long after Jeremy, M0XVF posted here that he had used Q65 effectively on aurora than up popped another aurora.

Stereo Ahead spacecraft image of CME on 23 March 2024.

A coronal mass ejection early on 23 March reached Earth later on 24 March. Although the speed of the arrival suggested a strong effect, the field quickly turned northwards and had smaller radio outcome than had been predicted.

At GM4FVM this was an early opportunity to see how Q65 might work on 50MHz during an aurora. At first I could hear OH6KTL and then even stronger DK8NE. This was once I had worked out that people were using Q65-30C submode. I worked G3YDY on 50.305, but OH6KTL was on 50.265. I decided to look for a clear frequency to call CQ, and I found 50.268. Eventually five other stations arrived on 50.268.

This map shows the QSOs I had on 6m Q65. All of them were auroral with no tone.

Contacts on 50MHz Q65 at GM4FVM, 24 March 2025.
 
I saw on KST someone calling those people anticipating a huge event "aurora maniacs". In the event the predictions of the "aurora maniacs" proved to be too optimistic. Auroras are notoriously hard to predict. Even if the identification of the material streaming from the Sun prove to be right, the polarity can swing to the north as it did during this event. Still, it quickly changed from being a widespread event into being a "Scottish aurora". More limited, but fine in my book.
 
The term "Scottish aurora" comes from the excellent book "Radio Auroras" by Charlie Newton G2FKZ. The type of thing he describes means a limited aurora opening with contacts possible with at least one station being in Scotland. Of course, radio does not observe boundaries and stations in the North of England and Ireland at one end are also often involved. However, Charlie's the term has stuck.

I might have hoped for more, but a Scottish aurora will do for me. Six contacts with the best DX being EI2IP at 579km. Another EI station was worked by several other stations but I could not hear it at all - which just shows how localised auroral propagation can be. I heard nothing on any mode on 70 or 144MHz.
 
Anyway, whatever you call it, this was an interesting event for me. I had also thought it might have been a bigger event than it was. However it still allowed me to prove to myself that Q65 could be a big help to me. I have always struggled to hear either SSB or CW during auroras. I am not sure why that should be, but being able to use a data mode would be a great advantage to me.

When I found that people were using 30C submode I followed suit. I guess that somebody knows that the other submodes do not work so well. It is a pity that we cannot use either B or A submode as those would allow us to fit several QSOs into one 3kHz filter's width. I am not complaining - if we can organise ourselves around a central point (I guess 50.275) then that would be fine.

Will Q65 work under more difficult conditions with more distortion? Will it work on 144MHz, or even the highly distorted events on 432MHz? Who knows, but let us find out.

Next, my first contact of the Es season also seems to have happened on 24 March 2024.
Contact via Sporadic E at GM4FVM, 24 March 2024

24 March is actually quite late this year. I have been looking into the length of the Es season from this location and I may write more about this on this blog. But anyway, it usually starts with a single QSO like this. Often there are a few short openings until around the end of April it really gets going. We shall see if this year is an average year.

So many of my contacts on 50, 70 and 144MHz depend on Es propagation. This is not only Es directly, but also through linking to TEP and the like. It is always good to get the first contact out of the way. That map my not look like a big deal, but 1620km to OH7XM on FT8 was a really good QSO for me.
 
Each one of the contacts mentioned on this page was much appreciated by me. It may not be 14MHz where you turn on at any time and work somebody. There are the days when nothing happens at GM4FVM. Yesterday lots of things happened. Keep up the good work lads!

73 
 
Jim GM4FVM

Tuesday 19 March 2024

Why all the fuss about Q65 on VHF and above?

First, there is no fuss about Q65. There should be.

Time for a question and answer session.

What is Q65? It is a data protocol in the WSJT-X suit, amongst others like FT8, MSK144 and JT65.

What does it do best? It allows radio amateurs to communicate in difficult situations by exploiting scatter and coping well with Doppler effects.

What is it designed for? According to the WSJ-X users guide "Q65 is designed for fast-fading signals: tropospheric scatter, rain scatter, ionospheric scatter, trans-equatorial propagation (TEP), EME, and the like."

Which bands is it best for? According to the WSJT-X website -  "it is highly recommended for EME, ionospheric scatter, and other weak signal work on VHF, UHF, and microwave bands." I find that it can be helpful by bringing iono-scatter into play for 50 and 70MHz, using aircraft scatter on 144 and 432MHz, and various assistive scatter modes on 1296MHz (and probably higher).

Are amateurs using it? In general, no. The EME community are using it above 432MHz, but most EME on 2m is still using the outdated JT65. For other purposes such as scatter or other weak signal work you hardly ever hear it.

Have you seen the benefits? Yes. Switching to Q65 on 1296MHz during a tropo contact brings a huge benefit. However, this works for me simply because stations on 1296 are often in contact via email or KST. This allows me to ask to switch mode. On tropo on other bands I am not in contact with other stations so much.

How does it work? The WSJT-X model allows you to choose the most suitable submode for data rate and period length. So if you use Q65 submode B with a 30 second period you would call that Q65-30B.

How difficult is it to use? On WSJT-X you simply click the button Q65. Then you select the period and the submode. It does not seem to difficult to me.

Which submode should you use? That is up to you and you QSO partner. Perhaps 30A for 50MHz where you have time to exploit iono- or tropo-scatter, perhaps 15B for higher bands where you want to capitalise on short aircraft scatter events. I used 30C to complete a QSO with DJ8MS on 1296MHz on 12 January 2024. That was after trying FT8 and failing so we went for the most sensitive combination we could.

Anything else to look for? Just like other scatter modes, it is as well to turn up FTol. The default is 20. You can turn it up to as much as your computer can take - max is 1000. Once you have made contact with the other station you can turn it down again if you wish to narrow the receiver pass band. 20 is fine if you are on exactly the same frequency, but on the higher bands this is not always the case.

What is the problem with using it? I dunno.

Why are people sticking to FT8 and JT65 on VHF? I dunno that either. 

Can you show a QSO where Q65 worked? Yes, for example this 432MHz QSO between GM4FVM and G0MJI. A 265km path over the Pennines which would not have been possible without some assistance from aircraft scatter. If you look at the traces you can see steep Doppler inclination. This contact simply would not have been possible using FT8 due to Doppler shift which disrupts FT8. It was easy on Q65-15B. From what I recall, Bri was running 35W.

Q65 QSO between GM4FVM and G0MJI on 29 January 2024

Q65 is a powerful aid for VHF, UHF and microwave amateurs. VHF QSOs are being missed needlessly. We are not learning how scatter modes can help us. We are not dealing effectively with fading. This is us scoring an own goal.

I have remarked before about a long lived trend in amateur radio to stick with the old ways. If that worked we would still be using spark to transmit plus cats whiskers and coherers to receive. If progress is to mean anything we need to be ready to try new ideas.

Q65 has been around for some years now. Joe Taylor and his band of helpers have created something very useful in Q65. And yet many VHF DX-ers hardly use it.

Anyone who wants to try Q65 on a marginal path between 50MHz and 1296MHz can feel free to contact me.

73 

Jim GM4FVM

Monday 4 March 2024

Scientific explanations for how Sporadic E happens, and how amateur literature differs (long).

I have not been posting much lately. [What have you been doing Jim?] Well, at this time of year there is not much on the radio so I have been watching Ski Sunday. Isn't  Clément Noël amazing? Why is the Ski Sunday season so much shorter than the ski season?

And now Paris-Nice and the start of the cycling season. Very distracting. Remco Evenepoel, Cian Uijtdebroeks, and all those people.

I just wrote a VERY long piece quoting all the research papers about Sporadic E which I have also been reading. I have been reading research papers because most amateur books and websites say things about Es which are either just plain wrong or full of imaginings about thunderstorms, jet streams, upwards pointing plasma bursts and other fanciful tales.

Mike GM3PPE sent me a good scientific paper and then I turned up another one which together seem to explain the process. Further reading amongst amateur tales made me turn up a third one. So now, rather than using all that material in detail, I will try to set out what I understand. What I understood before was wrong. I can see that now.

I learn that the ionised layer does appear to come from material ionised during entry into the Earth's atmosphere. The E-layer ions last for a remarkably long time before recombining, thanks to being organised by the magnetic field and due their mass being greater than gaseous ions in other layers. The daily pattern of daytime Es during the Summer is driven by solar influenced wind shear. The Es layers descend towards the Earth on a twice-daily air current. There is a wealth of new information in these papers, plus some useful maps.

Here is one of my diagrams. It is an attempt to precis what comes later in the boring text.

Probable Sporadic Es process. Definitely not to scale. (GM4FVM after Arras)

This is a diagram you will need to click on to enlarge, if you want to see the detail. It covers a slice across the ionosphere between about 150km and 80km above ground. The magnetic field would run vertically into the page from above.

What follows replaces the VERY LONG piece with a LONG piece. Sorry, but it isn't easy to summarise.

I will put in the details of the papers at the end. Anything I have taken up wrongly in this piece is my fault.

For this purpose I will try to explain a timeline through the process.

Firstly the iron which will make up the metallic component of the E-layer arrives in the Earth's atmosphere. This is material from meteorites and similar bodies. Most comes from other parts of our solar system but a small amount may come from cosmic dust.

We amateurs are familiar with some of this stuff through meteor scatter propagation. However, many amateurs concentrate their activity on certain meteor showers during the year. These showers allow 5 or 6 days activity per annum. This tends to deflect attention from the fact that the majority of this material arrives at all other times, 365 days per year, 24 hours per day. These are the "random" meteors which hardly souls like GM4FVM and OZ1JXY used to make over 130 contacts entirely outside the meteor shower season.

There have been suggestions that if meteors are involved then the Es season should be influenced by the meteor shower timetable. This only affects Es to a limited extent. The showers produce only a short lived peak in the material arriving and anyway the peak period for arrival of meteors does not coincide with the shower season. Meteor showers are just the short but energetic ones we see and the vast majority are much smaller. In fact these small meteors, called micrometeors, are about the size of a grain of sand. 

Estimates vary but but overall about 25 million objects arrive on Earth each year weighing in total about 15,000,000 kg. The larger of these break up in to small grains. Amounts vary during the year, with a minimum in February and a maximum during Autumn. The amount and energy levels of the arriving particles varies during the day due to the orientation of the observer to the plane of the ecliptic as the Earth circles around the Sun. Amateurs can exploit these variations in meteor scatter propagation but none of it aligns with Es peaks.

These meteors arrive travelling at huge speeds relative to Earth. As they get closer the atmosphere becomes dense enough for friction and chemical action cause them to be heated to huge temperatures. Some are ionised. The ones we are interested in are made up of, or contain, metallic elements - principally iron. In addition to iron, some meteors contain smaller amounts of magnesium, sodium and calcium which also may become ionised. The density of the atmosphere is about right at around 100 to 150km above the Earth for meteors to be heated to the required temperatures. This region thus become a relatively dense layer of ions and we call it the E-layer.

We now have the iron ions (Fe+) and electrons in the right area. What you would expect from something as heavy as a metal is that it would fall to Earth. Even these tiny specks of matter will descend under gravity, though perhaps slowly as the density of the atmosphere increases. 

You would also expect that they would recombine with electrons to convert from Fe+ to Fe. We are familiar with the gaseous ions in the D- and F-layers recombining once the influence of the Sun is deminished at night or during the winter. However, in the E-layer they remain as ions and electrons for long periods. The Earth's magnetic field will exert an influence and tend to organise the two sets of + and - charges along the magnetic field lines. The Fe+ ions are a lot heavier than the gaseous plasma ions in the D- and F-layers and are therefore less likely to wizz around and find electrons. The combination of these processes give enough time for this mass of ioinised matter to come under further influences. The papers reckon it takes between 27 hours and 3 days for the Fe+ ions to recombine.

One of the surprising things to me about this is that the papers suggest that this ionisation takes place by the process of micrometeors arriving on Earth and not from the Sun's energy as in the other layers. I say suggest, as they do not mention solar energy at all as part of the ionisation process. I was wedded to the idea that ionisation in all three layers would be caused by the energy from the Sun. This would explain why Es occurs during the day and mostly during the summer. But apparently not. It matters little though, because the Sun still has a major effect as we shall see shortly. I cling to the idea that the Sun may play a part in keeping the energy level high enough for this story to continue.

The ionised material descends in a particular pattern. What is called "diurnal tides" result in a twice a day air current bringing the layer downwards at a specific rate. Amateurs report a twice a day peak in Es, presumably as the layer passes through the right region for propagation. Other patterns are superimposed on this, including daily- and trice-daily tides, so the picture is not simple.

Next thing in the story is "wind shear". As I understand it, wind shear is a type of turbulence created when a mass of air meets a more or less static object. As a callow youth I looked out the window of my lofty office in Dundonald House, a strangely curved multi-story edifice, and saw the snow falling upwards past the window. Everywhere else it did what you would expect, but here right beside the building it rose and swirled in eddys as if trying to polish the window glass. Not that the air is as dense in the E-layer as it was inside or outside the DHSS office in which I toiled.

The theory here is that the wind shear effect, when present, helps to shape and compress the metallic ion layer into a thin (about 1.3km thick) shaped mass of relatively dense molecules, atoms and electrons. Key to all this is that the wind shear effect is driven by the Sun - which makes Es a largely daytime and summer event. Crucial to it all is that at certain regions the mass of ions becomes sandwiched between eastwards (below) and westwards (above) winds. Although similar conditions occur in both hemispheres, the wind directions in the Southern Hemisphere are reversed in relation to the Northern Hemisphere.

So, many variables are coming into this. Although the quantity and mass of meteors is large it will vary to some extent, the ions are descending and will need to pass through the height we need them to be, they need to stay ionised long enough to create the layer, the diurnal tides need to draw them to the right place and the wind shear needs to be in the right aspect (the papers suggest generally eastwards winds in the Northern Hemisphere, and with an upwards component) to create the layer we need, and reversed winds above. It is surprising it happens at all.

None of this explains the effect we amateurs know as "Winter Es". This is not mentioned in any of the papers I have seen. It may be caused by one of the alternative Es mechanism which create other minor effects. Or it could be explained by the "spillover" theory. Possibly it could just be an aspect of the effect, mentioned in the papers, that Es tends to trail the annual seasonal cycle to some degree. Whatever the explanation, I think that it is important to keep in mind that I find Winter Es is responsible for about 1% of my activity and none of my DX whereas regular Es accounts for the other 99% of the activity and all of the interesting contacts.Winter Es is an odd quirk, but also a very small quirk.

How does the research method used differ from the methods we as amateur use?

The method used in the scientific papers was GPS Radio Occultation (GPS RO or just RO). This involves observing scintillations in GPS radio signals passing through the Es cloud. GPS satellites orbit at about 20200km. For this purpose the GPS signals are not received directly on Earth but are detected by low Earth orbiting (LEO) satellites which orbit at about 2000km above Earth.

Both transmitting (GPS) and receiving (LEO) satellites are outside the E-layer and are, in effect, watching the E-layer from "above" in relation to ground level. Actually they are on either side of the E-layer. As they travel at different speeds to maintain different orbits there are regular windows of about 5 minutes when the GPS signal can be scanned for the presence of an ionised E-layer between them. Any phase changes or multipath interference can be attributed to the E-layers This is not simple though, as other variables in other layers have to be eliminated from the results. However this appears to have been possible.

By using the RO method the researchers are able to observe the Sporadic E layers themselves. We as radio amateurs are only able to observe the results of Es in our log book. Beyond that we can use sites like DX Maps and PSK Reporter (PSKr) to look for patterns and interesting events.

PSKr works by receiving reports from amateurs over the internet and presenting them as lines on maps and other formats. It therefore shows only contacts made, not paths available. It mainly shows data contacts and rarely records beacon reception. Whilst some amateurs can click the box on their software to pass reports on to PSKr, not all do. Many amateurs use directional antennas which limit the possible paths. The results are therefore partial.

DX Maps and similar sites collect data from the DX Cluster and present it in the form of maps and various tables. This information is limited to anything reported to the Cluster, though it includes more reports of CW and SSB contacts plus selected reception reports. DX Cluster has a very helpful map showing the locator squares in which Es layers must be located plus the MUF at that point. This uses a mid point between the path between the reported two stations. This is useful but it a rough estimate, it is historic and it relies on reports - it does not plot the layers themselves.

I use both PSKr and DX Maps extensively. They help me chase DX, but they do not give any clue as to how the E-layer is made up, nor any predictions about how or when the propagation might appear next.

In my view the methods used by amateurs tends to give a distorted view of Es, as of course we rely on other stations being around to receive our transmissions - and for example there are not many in Africa and vanishingly few in the middle of the Atlantic Ocean. The Es map in DXMaps then estimates that the refraction happens mid-way between the stations and shows this as one locator square. This is very helpful but not really scientific.

How does the scientific literature differ from what we read in amateur literature?

The scientific view is that the presence of Fe+ ions and wind shear are the crucial factors in forming a dense thin layer which makes Sporadic E propagation possible. Solar driven winds in the E-layer and the effects of the Earth's magnetic field are also crucial.

Reputable amateur publications give details of the scientific data but steer clear of going further.

Other amateurs have often taken the results from DX Maps, PSKr and other sites and laid them onto weather maps. From this they have come up with the idea that somehow weather systems close to ground play a part in Es formation. As there seems to be no direct relationship between our weather and conditions 100km or so up in the atmosphere they often postulate all sorts of mechanisms without any scientific basis. They then publish this on the Internet as is their right, just as I am doing now. Sometimes their ideas appear in books, society publications and magazines.

The amateur approach creates huge variables because of the indirect and variable nature of the data collection. This is in addition to their often cranky ideas about the influence of Earth weather on the upper atmosphere.

Many amateurs have looked for "triggers" for Es. Unlike the scientists they cannot see the E-layer except where it creates reported propagation for amateurs. I doubt very much if there is a "trigger" involved. The ham literature I have read says that the authors are looking for something they think needs to cause the ionisation in some direction or at a certain time. The scientific papers say that tons of ionised particles arrive every day without any other input and variables in the ionsphere explain the variability. If ionisation is already present, why look for a trigger?

One particular internet piece written by an amateur seems to go right off the path beaten by the scientists. He claims that tools like DX Maps and PSKr give amateurs a reliable way of spotting and tracking Es formation. In my view they only provide a method of tracking the contacts. He reckons that storms and lightning from Earth weather trigger Es. Having looked at the scientific evidence I feel that he is mistaken. All that DX Maps and PSK reporter do is to record some of the outcome of Es filtered through a skewed fabric of random influences.

PSKr often shows just single receptions due to transient effects which are not Es related. DX Maps also shows contacts after they have happened, and only the ones reported to the DX cluster. They cannot show paths which are not reported for all sorts of reasons. They never show potential paths which have not been exploited nor ones that don't exist. Only scientific approaches which, like the ones summarised here, can actually image the existence or not of Sporadic E layers and their location. This is the best way to try to find an explanation for what is happening. This research can show the process involved in creating the propagation in real time as scanned by the satellites.

When well meaning amateurs take charts from PSK Reporter or DX Maps and use them to try to plot Es activity it is almost inevitable that they are using unreliable data. When they go further and try to align this with weather, storm or lightning maps, they are likely to find doubtful patterns. If they go further again and try to predict future Es based on already unreliable information then the outcome is likely to be pretty wide of the mark.

Finally.

Right. Where have we got after all this waffle? There is plenty of scientific evidence as to what causes Es. We as amateurs can use the excellent tools available to us (including PSKr and DXMaps) to exploit this and have lots of interesting fun. By understanding the process by which Es is formed we can develop our learning. As for trying to out-think the professionals - you can try but you might be wasting your time. 

A basic human freedom is that everybody is authorised to waste their time as they think fit. Even me.

Sources.

These are the working links as I write this. Contact me if they do not work and I will try to help if I can.

1) A Global Survey of Sporadic E Layers based on GPS Radio Occultations by CHAMP, GRACE
and FORMOSAT–3 / COSMIC. Christina Arras. 2010 GroForschungsZentrum Helmholtz-Zentrum Postdam. Scientific Technical Report STR10/09

https://gfzpublic.gfz-potsdam.de/pubman/faces/ViewItemOverviewPage.jsp?itemId=item_23022

You can download the entire paper by clicking "full text".

This is a very full (~100 pages) paper, one of the first using the RO method. There is some very good information on how RO works.

2) Examining the Wind Shear Theory of Sporadic E With ICON/MIGHTI Winds and COSMIC-2 Radio Occultation Data. Y. Yamazaki. 2011 Geophysical Research Letters Vol 49 Issue 1.

https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2021GL096202

 As the wind shear theory was not well proven at this stage this paper concentrated on that matter. These are some interesting maps and diagrams.

3) Morphology of sporadic E layer retrieved from COSMIC GPS radio occultation measurements: Wind
shear theory examination. Y H Chu et al. 2014 Journal of Geophysical Research: Space Physics. Research Article 10.1001/2013JA019437.

https://pdfs.semanticscholar.org › c9a0 › 3c2ab977b9507b019e661904c5a4ebdf6fa2.pdf

A further verification of the wind shear theory. This paper includes many more E-layer maps and diagrams which will be of interest to the amateur.


Sunday 14 January 2024

At last a decent tropo opening plus 40MHz awakes.

Firstly I should mention that after a long lull during December and early January, some F layer activity has returned to 40MHz. As I start writing this on 13 January I have been receiving ZF1EJ at up to -4dB on the second day of good propagation this year. Let us hope this is a good start to the year, and maybe DX will reach 50MHz too before long.

My last posting was a whinge to complain about pretty flat conditions lasting 69 days. Well, eventually, after 86 days in total a reasonable lift started at last on 10 January.

It had been well signposted in advance. Both of the tropo predictors from Hepburn and F5LEN (see sidebar for links) predicted good conditions for 11 and 12 January 2024.

Hepburn Tropo Index for 18:00 on 11 January 2024

F5LEN Tropo map for 18:00 on 12 January 2024

Click to enlarge images if you need to, as usual. I like F5LEN's view of a misty field to represent high pressure.

Based on the maps I expected things to open mainly towards Sweden and perhaps into the Baltic. It started that way but most of the activity was to the South East.

Anyway, along with my FM warning system bringing in the Norwegian coastguard, I worked OZ1BEF on 2m at 14:24 on the 10th. This was followed by LA6GKA, but after that things generally moved away from that direction.

Over all, between those first QSOs and 10:00 on Saturday 13 January I made 98 contacts on four bands, reaching 38 squares and 11 countries. Best DX was on 2m to Olli DH8BQA thanks to his remote station in JO73, a distance of 1093km.

2 Metres

On 144MHz this was the result:-

144MHz contacts at GM4FVM 10 to 13 January 2024
This was the result of 43 QSOs to 10 countries. During events like this I tend to migrate to higher frequencies and simply keep a watch on 2m for anything interesting. In pure DX terms there was nothing very surprising with most QSOs around 800km. Notably absent were contacts to Central Europe, but I am not complaining. Not much anyway.

70cm

Spending my time on 70cm produced a few more contacts there than on 2m.

432MHz contacts at GM4FVM 10 to 13 January 2024
46 contacts to 25 squares in 10 countries with the best DX being to F1RJ in JN18 at 888km. The fact that there were more contacts on 70cm justifies my policy of concentrating on 432Mhz, or at least it does to me. OK the peak DX is not as far, but the average is not very different. 70cm produced a new country for me - Faeroes. I had heard OY9JD on 2m but I did not try a contact, after all I have worked him before and all of Europe wanted to contact him. So when he came up on 70cm I had to try for a new DXCC. Not only was IP62 a new square on 432MHz, but so was IO62 which was gifted to me by Roger, EI8KN. So pretty good on 70cm.

23cm

On 23cm things worked out rather well.

1296MHz contacts at GM4FVM 10 to 13 January 2024

Although this does not look very dramatic, it is a good performance for a microwave band. 8 QSOs in 4 countries with 6 squares. However, each QSO took some organising. I logged on to the Microwave KST chatroom. Although I rarely ever use the other rooms, the microwave one works quite well. There is time to set up a QSO and work your way through it with your companion amateur. 

I had worked Roger, EI8KN on 70cm and asked him to join me on 23cm. This was something we had discussed at the GMDX Convention in Stirling last year. I had explained to Roger that I had not yet worked EI on 1296 and he offered to help. At first we tried aircraft scatter but that failed. At a distance of 527km that should be possible but the window into which the aircraft have to fly is very narrow at that range. In the end we had to give up and this was the next attempt 3 months later. And it worked this time, so thanks to Roger for QSYing and waiting for me.

One 23cm contact stood out as odd, simply because it was "normal", or perhaps "random".  I sometimes call CQ at various beam headings, though this almost never works on 1296MHz. Still, you never know. Three minutes after I stopped calling, up popped DK1VC in JO31 also calling CQ. I decoded him at -03db and he gave me +01dB. What a splendid thing to stumble across a QSO on 23cm. It does happen, but not often at 811km. I was still hearing him 40 minutes later, but he only seemed to work one more station.

My other 23cm contacts were more normal, having been arranged via KST. I had tried to work Walter, DK3RV, on previous occasions but kept failing to make a QSO at 771km. This time I could see a faint trace on the FT8 waterfall. Often during a tropo opening the QSB can be very severe, so we kept at it and eventually after about 5 minutes I decoded Walter's CQ at -18dB. He responded next period with -19, then my RRR took another five and a half minutes to get confirmed, but the QSO was then complete and I sent 73. JO31 would have been a new square for me had DK1VC not provided it for me the previous day.

After my contact with Walter, it was the turn of Maurice F6DKW in JN18 to suggest a contact. Maurice suggested CW, and he agreed to try even after I told him that my CW is dire in the extreme. He was wise enough to QRS and once I had got the beam pointing the right was the contact was easy, 559 copy at  840km.

Later, after completing with EI8KN, David G4YTL from IO92 asked me for a QSO. M0CTP joined in and we completed using Q65 as FT8 was not up to the job. M0CTP and I were able to complete via aircraft scatter. Currently I cannot get planes to display on Airscout, which makes it pretty useless. Gary confirmed that it is the same with him, which was helpful information. I can stop trying to find a solution in the settings here. There may be some other problem with Airscout.   

It was a similar thing with DJ8MS at 903km in JO54. I posted that I was about to go QRT and anybody who wanted to try for a contact should reply. Tor let me know he would like to try and after struggling with FT8 once again we switched to Q65 to complete the QSO. I had also tried to work Tor using FT8 on previous occasions. Once we were on Q65 the QSO was easy.

So what are the learning points from all this for 23cm operation? 1) KST is not always essential but it certainly helps. 2) FT8 is not great on this band, but CW and Q65 can get you out of a hole. 3) It is worth asking people to QSY from another band. 4) CW has a place on microwaves, even if it is slow.

4m

Tropo also helps on 70MHz. I was pleased to work Henning OZ1JXY with good signal reports. This is a series of QSOs which goes back a long way with well over 100 contacts via a variety of propagation methods.

Finally

After the end of my activity on 11 and 12 January I expected it all to be over but there was one more DX contact to be made. On 13 January at 09:30 I worked F5RZC in JO10 on 144MHz, a handy enough contact at 642km. After that the DX faded and the stations in IO82 and so forth reappeared after two days absence. It is funny how during a tropo lift you lose the nearer stations as well as hearing the distant ones. At the end I could also hear stations in IO90 etc who would have been nice for me to work, but they were all beaming south to work into F and EA. And that was the end of that.

If we neglect the one-off contact on 13 January, all the activity was between 14:24 on the 10th and 19:35 on the 12th. I only worked seven stations on the 10th, and at that stage it was looking very much like the Scandinavian opening which the maps had predicted. There were no distant DX stations (though I heard an HB9 a couple of times), none of the OE, OK, or EA stations I have worked during previous events. I am happy enough though. Once I could switch between 2m and 23cm using my IC-9700, working one and listening on the other, and at the same time use my IC-7100 for 70cm, there were stations on all bands and I was a happy camper.

I called CQ a lot of 23cm SSB, but almost all contacts were on FT8, with three on Q65 and one on CW.

You do not appreciate the good times without living through the bad times, as I often say.

2m now = 45 DXCC and 247 squares

70cm now = 20 DXCC and 99 squares

23cm now = 11 DXCC and 32 squares

I enjoyed those good times.

Thanks everybody for making the contacts with me.

Let the good times roll.

73 Jim

GM4FVM

Sunday 24 December 2023

Longer days and Winter doldrums

I write this on 24 December, and I am really looking forward to longer days.

Today at GM4FVM sunset is scheduled for 15:37. That makes for a day length of 6 hours and 59 minutes. I should grateful for the two seconds we have gained since 22 December, but I prefer to think about the hours we will gain in future months.

Why does this matter to amateur radio? Well, the energy which causes ionisation comes from the Sun. The longer the Sun shines each day the more ionisation. Some features we rely on need a lot of energy, so F- and E- layer propagation usually occurs at times of longer day length. Cross Equatorial propagation modes benefit from balanced day length on each side of the equator and thus they tend to happen mostly at the equinoxes, whereas DX within the northern or southern hemisphere usually occur at times of longer day length nearer the summer solstice.

And not much happens in the winter.

Of course these are generalisations. Today on 50MHz there has been a short burst of "Winter Es", sporadic E propagation which often occurs around the Winter Solstice, i.e. roughly around Christmas.

50MHz contacts at GM4FVM on 24 December 2023

Not bad for just over an hour and a half of work. 10 QSOs to 9 squares, best DX 9A2DI in JN95 at 1870km. The trick is to watch out for this type of propagation sometime during December and January, so an hour and a half is not quite correct. I have been waiting for a few weeks now.

Then, later on 24 December, there was a Trans-Atlantic opening on 6m which missed GM4FVM almost entirely. I heard K9RX and that was it, apart from seeing weighty amateurs further west working a stream of stations along the Eastern coast of USA and into the Caribbean. You win some and you lose some.

Of course there are VHF propagation modes which are not affected by the season. Usually on 144MHz and above we have a series of passing high pressure systems which produce tropospheric propagation, plus the odd aurora for the lower bands.

Here is my 144MHz map since 12 October 2023. As usual click to enlarge images if necessary.

144MHz contacts at GM4FVM, 13 October to 24 December 2023

This does not look too bad for 2m, until you consider that it took 69 days to achieve it. In fact, it looked a lot worse until in one day I worked two French stations and EA1U in IN83 at 1389km who was the best DX. The other 68 days were very uneventful save for 5 November. On that day an aurora brought M5AGY, G4ILI, G0JDL, G4MCU and (best DX) G4XDZ in JO01 at 544km. All five contacts were over 400km. 

That aurora brought me on to SSB, a mode I seem to have lost the knack to operate. Although those 5 were on 2m, I also worked Gerry GI4OWA on 6m. I failed entirely to recognise him. It is now so unusual for me to hear callsigns spoken that the old familiar ones no longer trigger my memories. Ah, the joys of data modes.

Perhaps I should add that my hearing is not great. I gave up on the aurora after a station called me repeatedly and I simply could not decipher their callsign. I could blame this on my advanced old age, but to be honest I have never been good at decoding distorted SSB or even CW during an aurora.

Anyway, if you subtract those two days, the one tropo opening and the one aurora, 2m activity has been pretty woeful. The usual passage of weather systems has just brought a variety of low pressures, followed by lower pressure systems. The one extended period of high pressure (when I worked EA1U) was accompanied by strong winds which pretty well cancelled out the whole enhanced propagation. High pressure and strong winds - frustrating.

70cm was worse.

432MHz contacts at GM4FVM, 13 October to 24 December 2023

7 QSOs in 69 days. Best DX was to F4FET in JO00 at 627km. Although I have worked Gil on 2m, that was a new callsign for me on 70cm, also worked during the one high pressure period, despite the wind.

Now I have to make this point clear. All the contacts, even the local ones, are welcome. However, rarely have I experienced such dire conditions on the higher VHF bands. Usually I can rely on a nice stable (and not windy) high pressure to settle over the North Sea during this period of the year. My usually reliable contacts into Denmark have not happened so far this Winter. 

23cms was even worse again. I was away during the November activity contest but I came on for the December one. And during that 23cm contest I heard nothing. Even the NGI beacon could not be decoded. I did hear the Central Scotland beacon in Kilsyth, but could not decode it. Conditions were absolutely dire.

There seems to be another issue. I suspect that the novelty of FT8 on 2m has passed, and now only DX-ers turn it on. That means that there is only activity when conditions are good, and that was at no time during those 69 days. Quite a few of the contacts I did have were on SSB during activity contests. Sad to relate, many GM stations seem to have given up on UK Activity contests as they tell me that they have no hope of winning or even doing well.

So there you have it. I hope that we have reached the bottom of a long decline on the higher VHF/UHF bands, and hopefully longer days will bring better conditions on the lower VHF bands. I cannot be sure of a high pressure system coming along soon, but I can be reasonably sure that the day length will steadily increase, for a six months or so anyway.

Have a Merry Christmas and see you all soon.

73 Jim

GM4FVM