Saturday, April 25, 2026

U.K. Propagation Update

 

RSGB
RadCom Assistant Editor | April 24, 2026
Compiled by G0KYA, G3YLA and G4BAO on 23 April, 2026
Last week’s HF propagation was dominated by the effects of a high-speed stream from a large coronal hole on the Sun.
This pushed the Kp index up to 4 and 5 at times with the result that maximum usable frequencies, or MUFs, were lowered. The ionosphere struggled and often the MUF over a 3,000km path was below 21MHz.
Yes, there were some openings up to 10m but they were generally weak. Checks showed that paths opened up to Brazil, Kenya and Chile on the 10m band using FT8, but the signals were well down in the noise and barely workable.


Get used to this as it could be the norm for the next few years!
Meanwhile, the solar flux index increased to 116 by Thursday, 16 April, no doubt aided by active sunspot group 4420.
Next week, NOAA forecasts that the solar flux index could rise to 125. It also predicts that the Kp index may remain low due to a lack of coronal hole activity. Fingers crossed that we don’t have any coronal mass ejections over the next week.
If this pans out as predicted, we could have some decent HF conditions over the next seven days. Yes, the MUFs may be lower, but 14, 18 and perhaps 21MHz could be usable, with very occasional openings on 24 and 28MHz.
DX to be worked this week includes TX9W from the Marquesas Islands; VP9KF in Bermuda; 7P8WR from Lesotho; C5B, C5C and C5D in The Gambia; D60DX in Comoros; and JD1BMH operating from Ogasawara.
VHF and up propagation news:
Compiled by G3YLA and G4BAO
The strong region of high pressure will remain with us for the next two weeks. So tropo should be considered a first-choice mode for a while.
The main criteria for the quality of any resulting tropo is moisture. This is because moisture is a component in the calculation of the refractive index of the air.
High pressure usually produces dry air above any temperature inversion but we may not always get the moisture below the inversion.
The end of last week was good with reports of beacons in Norway and Sweden into JO02 on 1.3GHz because of moisture present below the inversion.
However, if the dry easterly wind returns, it may not go so well.
Meteor scatter should continue to be uplifted by the declining Lyrids meteor stream, which peaked last week, and rain scatter is off the menu since the charts are dominated by high-pressure systems.
Aurora is showing as occasional weak alerts, but apart from the odd fluttery signals on the LF bands, nothing too interesting at the moment.
As usual, watch for the Kp index going up to 5.
Keeping the best until last, we are approaching the period when Sporadic-E usually becomes a mode of interest.
Work is well underway on a rewrite of the Propquest website, which should be ready soon. This will be the go-to place for the daily updates during the 2026 Sporadic-E season.
EME now, and the Moon is moving into a lower noise position. Declination is high but falling and path losses will increase as we move away from the Moon’s perigee, its closest point to Earth, which occurred on Friday, 17 April.
Apogee, the Moon’s furthest point from Earth and the point of highest path losses, occurs on Sunday, 17 May.
(Mike Terry/BDXC)

Thursday, April 23, 2026

Throwback Thursday - The Lonely Voice from Down Under!

This week's edition originally aired on March 5, 2000

Girls' High School, Sydney, Australia

The Lonely Voice from Down Under!

What happened to the original radio base that carried the shortwave programming from Radio Australia?

In the western suburbs of Sydney, there is a Girls' High School standing on a spacious and attractive property. Nearly 100 years ago, this location was in an isolated area, some 20 miles distant from old and faraway Sydneytown. Ask the students who are attending the high school today: "Do you know the important history of this property?" At a guess we would probably say no, most of them do not know the interesting background associated with this property. This school property was at one time the site for one of the world's largest radio stations.

It was here in Pennant Hills that the newly-formed federal government purchased the 40-acre property quite early in the last century for the purpose of establishing a large wireless station. Electrical engineers came out from Germany to install the newly developed Telefunken wireless apparatus, and finally, on August 19, 1912, wireless station POS was inaugurated. The original transmitter was a 25 kw spark unit and the antenna was an omnidirectional vertical radiator; in other words, just simply a tall steel mast.

Station POS was intended to become the key station in a nationwide network of wireless stations for the purpose of intercommunication throughout the Commonwealth of Australia and its territories. The callsign POS stood for "Post Office Sydney," and the counterpart near Perth in Western Australia, some 3,000 miles distant, was POP. However, the callsigns were soon changed to conform to the new international regulations, and POS and POP became VIS and VIP, as they are to this day.

A large number of radio transmitters were installed over the years at this Pennant Hills location, many for communication traffic and some for radio broadcasting. During the year 1927, a new building was erected on the Pennant Hills property, specifically to house a new 20 kw shortwave transmitter. This unit made its inaugural broadcast under the now nostalgic callsign VK2ME on October 27, 1927, with its famous first "Empire Broadcast."

Soon afterwards, two more shortwave transmitters were installed at Pennant Hills, and these were in use as VLK and VLM for international communication and as VK2ME for program broadcasting.

When the climactic events of 1939 finally broke out into open warfare, the Australian government hastily organised an international shortwave service under the designation "Australia Calling." At Pennant Hills, the two transmitters on the air previously as VK2ME and VLK-VLM became VLQ and VLQ2, and they went on the air with the inaugural broadcast of "Australia Calling" on December 20, 1939 with programming from the studios of the ABC in Sydney.

This shortwave station, "the lonely voice from down under," was on the air for six years as the main facility for Radio Australia. However, when the new shortwave station at Shepparton in Victoria was commissioned in 1944, the usage of Pennant Hills was terminated. The AWA radio station at Pennant Hills then reverted back to full time usage as a communication facility, though occasionally the 10 kw transmitter VLN was on the air with Radio Australia programming beamed across the Pacific.

The Pennant Hills radio station was finally and forever closed on October 31, 1955 when all services were transferred to a newly constructed facility located at another Sydney suburb, Doonside. The property was sold, and upon it was built the Carlingford High School.

The only reminders left in the radio world of this once powerful voice from down under are references in old radio magazines and QSL cards in old collections. The AWR historic collection in Indianapolis contains two original QSL cards from the old VK2ME, both in color, with a laughing Kookaburra superimposed on an outline map of Australia. One card is dated 1932 and the other 1937.
(Wavescan 271/3/5/2000)
(photo/FB-Old sydney Album)

Wednesday, April 22, 2026

Radio Comes to Australia

 Special thank you to the Wavescan staff for sharing this week's edition of nostalgic radio in Australia

Jeff: In the early 2000’s, our editor-in-chief, Dr. Adrian Peterson, wrote a series of articles under the strapline ‘Reminiscing with a Radio’, about his recollections of early radio listening in Australia.  Just over 20 years ago in March 2006, one of these articles was titled ‘Australia Gets Radio.’  Here’s Ray Robinson in Los Angeles with that story.

Ray: Thanks, Jeff.  Adrian’s own personal memories of radio broadcasting in his hometown of Adelaide immediately after the end of World War II in 1945 prompted him to write about events 27 years earlier, immediately after the end of World War I.  He wrote:

The war was over, troops were returning home, families were reuniting, difficult restrictions were progressively lifted, and technological development for peaceful purposes was resumed.  This was the scene in Australia, and in many other countries also, at the beginning of the era when wireless became radio.

During the war, the annual Royal Perth Show, always held in the autumn, was temporarily discontinued, “for the duration”.  This popular event was reintroduced just before the end of the war and it attracted huge crowds of eager spectators.  On the occasion of this first (almost) post-war show, wireless experimenter Wally Coxon staged a public demonstration of radio broadcasting with a transmitter in one pavilion and a receiver in another.  The year was 1918, and this was the first public demonstration of radio broadcasting in Australia.

In the Eastern States, the first experimental radio broadcasting transmitter was constructed just four months after the first direct wireless communication from England to Australia.  The enterprising Ernest Fisk was the Managing Director of AWA, and Fisk invited William Bostock, a decorated war veteran who had recently returned to “civvy street”, to head up the project.  Work began to build a radio transmitter in early 1919, using the newly available Marconi “Q” valve imported from England.  Bench tests were made from this new transmitter during the month of March, and then it was ready for wider experimentation.

One of the main uses of wireless transmissions had been for ship-to-shore communications, and so it was decided to install the new radio transmitter on a ship.  There was a fourteen-year-old single-stack interstate passenger/cargo vessel plying the Australian coastline at that time called the “Riverina”, owned by Huddart Parker of Melbourne.

Arrangements were made for the “Riverina” to carry the new little “Q” transmitter during its regularly scheduled voyages for a three-week series of seaborne test transmissions.  These test broadcasts took place during the month of April, 1919.  The output power was around 10 watts, and the operating frequencies were in what are now designated as the longwave and medium wave bands.  These experimental broadcasts were successful, although of course, there were very few receivers capable of tuning in to the informal programming.

 At the same time, there was another single-stack steamer plying the Australian coastline – the fifteen-year-old “Bombala” owned by Howard Smith, also of Melbourne.  A second series of test transmissions using the same “Q” transmitter was carried out in July of 1919.  Clear signals were heard over the salt water pathway at a remarkable distance, even as far away as Gabo Island, more than 300 miles south of Sydney.

Having proven the concept, the next event needed was a genuine public demonstration, and that was soon in the making.  Ernest Fisk announced that he would address the Royal Society of New South Wales on Wednesday evening August 13 (1919) and that he would present a live radio program as a practical demonstration of the new radio medium.  This event, as a historic first in Australia, was staged in the Royal Society’s Hall at 7 Elizabeth Street in Sydney.  A series of some twenty locally-constructed loud speakers with tin horns were all connected to the same receiver and strung from the ceiling.  The “Q” transmitter was installed at AWA Wireless House (at 97 Clarence Street in those days) and the sixty foot long “T” type antenna was strung on the roof of the same building.  The programming for this first auspicious occasion consisted entirely of gramophone recordings played into a carbon microphone.  At the appropriate timing during the Fisk speech, the National Anthem came through suddenly and dramatically; a clear demonstration that radio without wires was indeed a reality.  The transmitted signal had traveled in the heart of old Sydneytown from one main street to another covering a distance of about half a mile.

Meanwhile, down in Melbourne, AWA was planning another series of dramatic radio events.  It should be remembered at this era, that Sydney was the larger city, but Melbourne was assuming political importance as the de facto capital of Australia due to the fact that the Federal Parliament was headquartered in this city.  (The Australian Capital Territory, ACT, and the city of Canberra had not yet been surveyed.)  Two Marconi speech transmitters were imported from England and one was installed in the Brighton home of the local AWA manager, Lionel Hooke, with a simple antenna in the family garden.  This unit came on air with a special broadcast to the Federal Parliament which was meeting in Queen’s Hall, Melbourne.  The date was Wednesday October 13, 1920; the receiving aerial was installed on the roof of Parliament House; and the loud speakers were the ones with tin horns from Sydney.

AWA conducted many promotional test broadcasts in the Melbourne area during this period.  The 500 watt transmitter was transferred from Hooke’s residence to another suburban residence, that of engineer Sydney Newman in Canterbury.  At this location, the familiar callsign 3ME was introduced.  In fact, AWA in Melbourne registered a series of callsigns ranging from 3MA – 3ME.  Station 3ME was installed at the permanent fixed location of Canterbury, but the others were apparently used at various temporary locations for demonstration test broadcasts using another 500 watt Marconi transmitter.  These two transmitters, twins from Chelmsford in England, were rated at less than one “horsepower”!

At this stage, the AWA callsigns in Melbourne became quite prominent, in fact more prominent than the similar series in Sydney, 2MA – 2ME.  In particular, the Melbourne callsign 3ME was soon afterwards transferred to Braybrook where it identified a shortwave transmitter co-sited with 3LO.  It was not until AWA began a series of international shortwave broadcasts from Pennant Hills near Sydney that the 2ME callsign became better known than the southern sister 3ME.

Throughout the five-year period from early 1919 to late 1923, the number of radio broadcast programs, and the number of radio broadcasting stations, all experimental and mostly amateur, began to proliferate, mainly in Sydney & Melbourne, though also in other cities as well.  In Sydney there were 2CM & 2MB; in Melbourne 3ME & 3DP; in Brisbane 4CM & 4CH; in Adelaide 5AH & 5BN; and in Perth 6AG; plus a host of others that came and went as well.  In fact, there were so many amateur broadcasters on the air in Sydney for example that the newly-launched “Wireless Weekly” established an evening rota for all amateur broadcasting stations in an effort to reduce interference.
As a result of all of this amateur broadcasting activity, it became evident that Australia needed a regular licensed broadcasting system.  In 1923, two organizations in Sydney applied for broadcast licenses, and construction work on both was carried out simultaneously.  The first on the air was 2SB, followed soon afterwards by 2FC.  Test broadcasts for 2SB began on October 19, 1923 with the use of another hurriedly constructed 10-watt transmitter.  This unit was installed in the Smith’s Weekly building in Phillip Street and the amateur callsign, 2HP, was transferred from William MacLardy’s suburban location to the new facility in the city.

This new radio broadcasting station was officially opened on November 23, 1923, with a new 500 watt transmitter operating at lower power under its official callsign, 2SB.  This call was changed early in 1924 to the more familiar 2BL.  Similar officially licensed radio broadcasting stations were soon afterwards inaugurated in each of the other state capitals throughout Australia.

Back to you, Jeff.






Tuesday, April 21, 2026

Update on the future of Radio Seagull

 


Radio Seagull on Facebook
By Martin Wallis
14 April 2026
An article from our regional radio and TV station ‘Omrop Fryslan’ in the Frisian language:

It was such a great plan: the red lightship Jenni Baynton from Harlingen would go out to sea again, to make radio broadcasts from behind anchor. So the foundation behind the ship wanted to raise money for the maintenance, which is much needed. But it won’t continue. The diesel is too expensive.

The Jenni Baynton is the last ship that still broadcasts radio. It has a similar history to that of Radio Veronica. It started as a sailing lighthouse in 1949. After that, it was also a disco when it was located in Rotterdam.

In 2005, the Friends of the Lightship Foundation bought it, and the volunteers turned it into a functional ship again. Between 2005 and 2015, for example, Radio Waddenzee could be heard from the ship. The
ship would anchor in the Wadden Sea for five weeks. Not only to make radio, but also for other cultural events. And although the ship’s engines do not use much diesel when it is at anchor, electricity is needed. This is also generated on the old ship with diesel.

According to the board of the Friends of the Lightship foundation, the price of diesel has recently become so high that the cost of electricity on board can rise to 300 euros per day. Then the whole action would no longer generate any money, but money would have to be added.

The money would be used for a shipyard overhaul. The last shipyard overhaul the ship received was in 2009. The Friends of the Lightship Foundation, therefore, wants to make the ship look good again. Volunteers usually maintain the ship, but for a major overhaul, it has to go to a shipyard and the costs to do so are high.

 From June 1 to July 7, the ship will not be anchored at sea, but with its ropes on the shore in Harlingen. This also has an advantage, says the board: it will now be much easier for visitors to get on board.

It is possible that the ropes will still be loose for a while with the Tall Ships Races. These will be in Harlingen from July 3 to 6. The board is now investigating whether this is possible. “That beautiful red
Lightship as a gatekeeper at the entrance to the harbor to welcome the sailing ships does have some extras”, says the board.

Mike Terry to nordx iog (2026-04-15)
(Ydun's MW & LW Info)

Monday, April 20, 2026

Weekly Propagation Forecast Bulletins

 Product: Weekly Highlights and Forecasts
:Issued: 2026 Apr 20 0331 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC web contact https://www.swpc.noaa.gov/content/subscription-services
#
#                Weekly Highlights and Forecasts
#
Highlights of Solar and Geomagnetic Activity 13 - 19 April 2026


Solar activity was at very low to low levels during the period. Very low levels occurred on 14, 15 and 19 Apr, while low levels were observed on 13, 16, 17, and 18 April. 

Region 4419 (N14, L=314, class/area=Eki/360 on 17 Apr) was the most active region of the period, responsible for 5 out of the 7 C-class flares observed during the week, including the largest one: a C4.1/Sf at 17/0442 UTC. The remaining 2 C-class flares of the period were: a C1.1/Sf at 13/1137 UTC from Region 4414 (N15, L=026, class/area=Dro/030 on 08 Apr) and a C1.6 at 18/0704 UTC from Region 4416 (N19, L=047, class/area=Dai/140 on 12 Apr). Coronal activity was observed during the week with some filament eruptions and few CMEs without Earth-directed components. 

No proton events were observed at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit was at high levels on 13-17 Apr, followed by a day at moderate levels on 18 Apr and returning to high levels on 19 Apr, with a maximum flux of 3,250 pfu observed at 15/1800 UTC. 

Geomagnetic field activity was quiet to Moderate storm levels during the period. From 13 to 17 Apr, the geomagnetic activity remained at quiet levels. On 18 Apr, the arrival of a negative polarity CH HSS influence disturbed the Geospace, elevating the activity from unsettled to Moderate storm levels. On 19 Apr, Moderate storm levels were observed during an isolated synoptic period (0600-0900 UTC) and the geomagnetic activity returned to quiet level by the end of the day as the CH HSS effects waned. 

Forecast of Solar and Geomagnetic Activity 20 April - 16 May 2026

Solar activity is expected to be at low levels, with a varying chance for M-class (R1-R2/Minor-Moderate) flares and a slight chance for X-class (R3/Strong or greater) flares through 16 May. 

No proton events are expected at geosynchronous orbit, barring any significant, non-recurrent solar activity. 

The greater than 2 MeV electron flux at geosynchronous orbit is expected to reach high levels on 20-22 Apr, 27-28 Apr, 30 Apr-05 May, and 08-14 May. Normal to moderate electron flux levels are expected on 23-26 Apr, 29 Apr, 06-07 May, and 15-16 May. 

Geomagnetic field activity is expected to remain at quiet to active levels during most of the outlook period, with the exception of 5 days when G1 (Minor) storm levels are anticipated due to the recurrent influence of CH HSS: 29-30 Apr (-CH HSS), 07 May (+CH HSS) and 15-16 May (-CH HSS). 

Product: 27-day Space Weather Outlook Table 27DO.txt
:Issued: 2026 Apr 20 0331 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
#
#      27-day Space Weather Outlook Table
#                Issued 2026-04-20
#
#   UTC      Radio Flux   Planetary   Largest
#  Date       10.7 cm      A Index    Kp Index
2026 Apr 20     105          18          4
2026 Apr 21     110          15          4
2026 Apr 22     120           8          3
2026 Apr 23     125           5          2
2026 Apr 24     120           8          3
2026 Apr 25     115           8          3
2026 Apr 26     120           5          2
2026 Apr 27     125           5          2
2026 Apr 28     125           5          2
2026 Apr 29     125          20          5
2026 Apr 30     125          18          5
2026 May 01     125          12          4
2026 May 02     125          10          4
2026 May 03     115           8          3
2026 May 04     108           8          3
2026 May 05     105           5          2
2026 May 06     100           5          2
2026 May 07      95          20          5
2026 May 08      90          15          4
2026 May 09      90           8          3
2026 May 10      95           5          2
2026 May 11     100           5          2
2026 May 12     105           5          2
2026 May 13     110           5          2
2026 May 14     110           5          2
2026 May 15     105          25          5
2026 May 16     105          20          5
(NOAA)

Thursday, April 16, 2026

Saturday broadcast for Radio Voxtup International

 
Germany
Radio Voxtup International - "The Children's and Youth Program": Talkmusic on Shortwave (Talkmusik auf Kurzwelle), is produced by 12-year-old "radio freaks". 

This programme will be heard via Shortwave Radio Gold on Saturday 18 April at 1800 UT on 3975 & 6160 kHz. Probably in German language, but I think worth a listen and good to encourage younger people into the hobby.   

They can be contacted via WhatsApp: https://whatsapp.com/channel/0029Vb6CBrWA2pLBb66G9L07; WhatsApp Nr: +0049 (0) 5419987825; email: talkmusic@outlook.de; Web site: https://www.voxtrupwelle.de/startseite
Alan Roe, Teddington, UK

1500 Meters Longwave Part 2 – After World War II

This week, Wavescan continued their feature on longwave - thank you to the staff for sharing 


Part 2 -   1500 Meters Longwave Part 2 – After World War II

Jeff:  Today we continue with part 2 of our feature on the history of AM longwave broadcasting in the UK, picking up the 1500 meters story just as World War II has come to a close.  Here’s Ray Robinson again in Los Angeles.

Ray:  Thanks, Jeff.  As we stated last week, the new BBC Light Programme, as it was called, was inaugurated on July 29, 1945.  The other BBC channel, the ‘Home Service’ continued on medium wave, and was primarily a ‘spoken word’ network with news, commentary, discussion programmes, documentaries, drama and comedy.  Short regional opt-outs for more local news were programmed in some areas.  The Home Service very much continued the tradition and vision set by Lord Reith before the war of providing serious, thoughtful and non-frivolous content intended to educate and inspire listeners to a higher level of culture.  One of the comedies that ran on the Home Service, though, was ‘It’s That Man Again’, commonly referred to by its initials as ITMA.  In the late 1930’s, one of the London daily newspapers, the Daily Express, had used the expression ‘It’s That Man Again’ anytime Adolph Hitler had been in the news, so the show decided to use the phrase to try to make light of the situation.  The first pilot episodes were in 1939 and it continued weekly until its star Tommy Handley’s untimely death in 1949.  Interestingly, the initial setting for the show was on board a pirate commercial radio ship from which Tommy broadcast, and one of the regular features was Radio Fakenburg, a send up of Radio Luxembourg.  But I digress.

The ‘Light Programme’ was given a different ethos to the ‘Home Service’.  The Light was a truly national station broadcasting primarily on 1500 metres, 200 kHz with the 150 kW 5XX transmitter, and also on a few medium wave transmitters on 247 metres, 1214 kHz.  The Copenhagen Plan of 1948 permitted an increase of power, so a previous wartime 400 kW medium wave transmitter at Droitwich was converted to longwave, and this went into service on March 15, 1950 when the Copenhagen Plan came into effect.

Here’s a clip of the station opening up for the day at 6:30am in 1950:

< Audio Clip - 1950 00 00 - BBC Light Pgm 0630 Start of Day (29 secs) >

The Light Programme’s content was primarily music-oriented, although it also carried most of the BBC’s early comedy shows, such as:
Much Binding in the Marsh, which ran from 1947-1950,
Take it from Here, from 1948-1960
Up the Pole, also in 1948,
‘Ray’s a Laugh’ in 1949,
Variety Bandbox in 1950,
Educating Archie (with Archie Andrews and Tony Hancock), which ran from 1950-1957,
Life with the Lyons from 1950-1961
the much-loved Goon Show from 1952 to 1960
Hancock’s Half-Hour from 1954-1959, and
The Floggits in 1956, with Doris and Elsie Waters

These shows were designed to appeal to ‘the common man’, and in the climate of post-war austerity (remember food rationing with coupons continued in the UK until July 1954!), it was designed to lift morale in the sense of ‘we’re all in this together’.  The comedy shows often poked fun at the British themselves.

Interestingly, ‘Much Binding in the Marsh’ was actually picked up by Radio Luxembourg in 1951 for a fifth series after it had been cancelled by the BBC, although it did return to the BBC for series seven, two years later.

But, the main diet on the Light was music, and this presented a special challenge for the BBC.  As far back as the 1920’s, the British musicians' union had negotiated an agreement with the BBC which restricted the amount of commercially recorded music that could be transmitted during any 24 hour period.  This was known as ‘needletime’, and in the 1950’s amounted to only about 4 hours per day, or less than 30 hours per week.  This was increased to 5 hours per day in the 1960’s, but it continued to affect both BBC and independent stations in the UK right up until 1988.

To get around this, the BBC formed a number of in-house orchestras such as the BBC Symphony Orchestra and the Northern Dance Orchestra which they could record themselves playing instrumental versions of the hits of the day.  Also in the BBC studios, they recorded cover versions of popular songs by groups such as Shane Fenton and the Fentones.

Some of the iconic weekday programmes were Housewives’ Choice at 9am

To hear the audio clips, go to the Wavescan podcast page 

 Audio Clip – Housewives’ Choice theme 
Music While You Work at 10:30am

Audio Clip – Music While You Work theme

Audio Clip – Listen with Mother 

Listen with Mother, at 1:45pm, which was a 15-minute programme where a story would be read.  It would always begin with a xylophone tune followed by “Are you sitting comfortably?  Then we’ll begin.”

Yes!  Just like that.  I remember in the mid-50’s before I first went to school, settling down with my mother in front of the wireless after lunch, turning it on a few minutes early to allow time for the valves to warm up, and hearing the sound slowly fade in.  We rarely missed it.  And then there was the magazine programme ‘Womens’ Hour’ from 2-3pm, and more ‘Music While You Work’ at 3:45pm.

Pop stars of the day were invited to come to the BBC studios on Saturday mornings for ‘Saturday Club’, where they were interviewed and then played live performances of their songs.  A few programmes were allowed to play the original hits of the day, such as ‘Two-Way Family Favourites’ on Sunday mornings, Jack Jackson’s Record Roundabout, and ‘Pick of the Pops’ which started in 1955 on Friday nights and later moved to Sunday afternoons.

But by the early 1960’s, the vibrancy of the pop music scene and the fact that there was very little of it on the Light Programme was one of the direct causes of the explosion in British offshore broadcasting that began in 1964.

In September 1967, the BBC restructured its services, and the Light Programme on 1500 metres became BBC Radio 2, which really was just a change in name only.  And so it continued on 200 kilohertz, 1,500 metres, until November 23, 1978 when a new frequency plan for Europe (the ‘Geneva Plan’) came into effect.  At that time, the former ‘Home Service, now BBC Radio 4, took over the longwave frequency, and Radio 2 moved to medium wave instead.

 As previously, the Droitwich longwave transmitter continued to give good national coverage for Radio 4, except it was found that in Scotland there were some significant coverage gaps due to the topology, and the fact that Radio 2 had previously had some medium wave transmitters for fill-in purposes.  If you’re not familiar with Scottish geography, there are basically three main areas – the Highlands in the north, the Southern Uplands, and a central valley between the two which runs from Glasgow in the west to Edinburgh in the east.  And it’s in the central valley where most of the population lives.  Because the Radio 4 longwave signal from Droitwich was effectively being blocked by the Southern Uplands, it was decided to add a second longwave transmitter at a place called Westerglen, midway between Glasgow and Edinburgh, and a third on the northeast coast at Burghead for coverage of the Highlands.  Both of these operated on the same 200 kHz frequency with a power of 50 kW each, and went into service in 1982.

 In 1985, two new 250 kW longwave transmitters manufactured by the Marconi Company were installed at Droitwich, and these were used in parallel to generate 500 kW output power.  And these are the same transmitters that are still in use today.  On February 1, 1988, the operating frequency was adjusted from 200 kHz to 198 kHz (1515 metres) – the last remaining requirement of the Geneva Plan.

 In 2011, as a result of budget cuts, the BBC announced that there would be no re-investment in longwave transmissions.  The same year, The Guardian newspaper reported that the Droitwich longwave transmitters each rely upon a pair of glass valves (or tubes) for their final power amplification stage, of which at that stage they reported there were less than 10 left in the world.  The BBC stated it was unsafe to manufacture more, because "slightly faulty" replacements could cause catastrophic failure.  And so, it was finally announced that BBC Radio 4 will end its longwave broadcasts from Droitwich, Westerglen and Burghead on September 26 this year, 2026, and then remaining on FM and digital only.  1515 meters, 198 kHz will then be silent forever.

 

Back to you, Jeff.

 For schedule information of BBC Radio 4, covering news/talk format of BBC Radio 4 on 198 LW, FM, DAB and streaming, go to: https://www.bbc.com/audio/schedules/bbc_radio_fourfm



Wednesday, April 15, 2026

Texas Radio Shortwave, April 16, 19

 
A sample QSL from TRSW

UTC/ relays via Germany


April   16  at 1900 on  3975/6160 kHz, via Shortwave Radio Gold to Europe. Featuring the Music of  The Sons of the Pioneers



April   19  at 1000 on 6070 kHz via Channel 292 to Europe. Featuring the music of Lightin' Hopkins
(TRSW)

This schedule is subject to change based on listener requests for specific Texas artists or music genres, propagation conditions, and other things beyond our control.
Texas Radio Shortwave is an independent producer of musical and topical shows, usually about Texas.
Unless otherwise shown, programs are one hour long.

Programs for Europe and beyond on 3975 and 6160 kHz over Shortwave Radio Gold in Winsen, Germany, are transmitted with 1 kW into crossed dipole antennas.

Programs for Europe and beyond on 6070 and 9670 kHz over Channel 292 in Rohrbach, Germany, are transmitted with 10 kiloWatts into an inverted V antenna.

Programs for North America and beyond on 9670 kHz over Channel 292 are transmitted with 10 kW into a 10.5 dB gain beam antenna.

Texas Radio Shortwave uses a version of The Yellow Rose of Texas as its Interval Signal/Signature Song.

Texas Radio Shortwave verifies correct, detailed reception reports by electronic QSL. This includes reports from listeners using remote receivers (SDRs). Texas Radio
Many TRSW programs are archived at www.mixcloud.com/texasradiosw.
Texas Radio Shortwave's Facebook page is www.facebook.com/texasradiosw.
Texas Radio Shortwave's Listeners' Group Facebook page is www.facebook.com/groups/580199276066655/.
(TRSW) 
(Photos-Texas State Historical Assoc)

Monday, April 13, 2026

WRMI Summer Schedule Update

 


The current color grid program schedule, dated April 3, 2026, is available at: 

Previous schedule post on March 3, 2026

All times UTC
Programming in English, French, Italian, Japanese, Portuguese, Russian, Slovak, Spanish

0000-0100   5010ca  5850na  5950na  7730na  9455na  15770eu  17790af
0100-0200   5050la  5800la  5950na  7730na  7780ca   17790af  15770eu
0200-0300   5010ca  5050la  5950na  7780na  9955sa  15770eu
0300-0400   5050la  9955sa  15770eu
0400-0500   7570na  7730na  7780ca  15770eu
0500-0600   7570na  7730na  7780ca  9395na  15770eu
0600-0700   5850na  7570na  7730na  7780ca  9395na  15770eu
0700-0800   5850na  7570na  7730na  7780ca  9395na  15770eu  
1800-0900   7730na  7780ca  9395na  15770eu
0900-1000   5850na  7730na  9395na  15770eu
1000-1100   7570na  7730na  7780ca  9395na  15770eu
1100-1200   5850na  7730na  9395na
1200-1300   7730na  9395na  15770eu
1300-1400   7730na  9395na  
1400-1500   7730na  9395na  15770eu  17780af
1500-1600   7730na  9395na  17790af
1600-1700  7730na  9395na   17790af
1700-1800   7730na  9395na  15770eu  17790af
1800-1900   7730na  9395na  15770eu  17790af
1900-2000   7730na  9395na  17790af
2000-2100   9395na  17790af
2100-2200   7730na  17790af
2200-2300   5850na  7730na  15770eu  17790af
2300-0000   5010ca   5850na  7730na  9455na  17790af

Target Areas:
ca  Central America
eu  Europe
la  Latin America
na North America
sa  South America
va  Africa/South America

WRMI website:  http://wrmi.net/
Reception Reports: info@wrmi.net 
Rapid E-QSL: Send a reception report and receive an immediate e-QSL to: wrmiqsl@gmail.com
(GVH/Teak Publishing)

Jen's Eclectic Views & Real Deal audio available for April 12 program

 


Did you miss it?  No problem... audio for the April 12 program is available for YOU !! 

Weekly Propagation Forecast Bulletins

 :Product: Weekly Highlights and Forecasts
:Issued: 2026 Apr 13 0104 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC web contact  www.swpc.noaa.gov/content/subscription-services
#
#                Weekly Highlights and Forecasts
#
Highlights of Solar and Geomagnetic Activity 06 - 12 April 2026



Solar activity was at very low to moderate levels during the period. Moderate levels were reached on 09 Apr, with low levels observed on 06-08 Apr and 11-12 Apr. Very low levels occurred on 10 Apr. 

Region 4409 (N02, L=158, class/area=Eai/190 on 07 Apr) was the most active region of the period, producing 11 C-class flares and the only M-class flare of the period, an impulsive M1.0/Sf at 09/0845
UTC. Region 4417 (S08, L=123, class/area=Dao/30 on 12 Apr) also contributed notable activity with 7 C-class flares after appearing quickly on 11 Apr near the West limb. Other activity included a
C8.7/Sf flare from Region 4414 (N15, L=26, class/area Dro/30 on 08 Apr) at 08/1543 UTC, which was associated with Type III radio emissions and a weak CME without any Earth-directed components. 

No proton events were observed at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit was at high levels throughout the reporting period. Flux levels reached a peak value of 10,679 pfu at 09/1605 UTC. 

Geomagnetic field activity ranged from quiet to active levels during the period. The beginning of the period (06-07 Apr) saw quiet to unsettled conditions as the influence of a negative polarity coronal
hole high speed stream (-CH HSS) continued to wane. From 10-12 Apr, quiet to active levels were observed under the onset and influence of a positive polarity CH HSS (+CH HSS). Quiet conditions prevailed
during all other days of the period under a nominal solar wind regime. 

Forecast of Solar and Geomagnetic Activity 13 April - 09 May 2026

Solar activity is expected to be at low levels, with a varying chance for M-class (R1-R2/Minor-Moderate) flares and a slight chance for X-class (R3/Strong or greater) flares through 09 May. 

No proton events are expected at geosynchronous orbit, barring any significant, non-recurrent solar activity. 

The greater than 2 MeV electron flux at geosynchronous orbit is expected to reach high levels on 13-17 Apr, 19-24 Apr, 26-28 Apr, 30 Apr-05 May, and 08-09 May. Normal to moderate flux levels are
expected on 18 Apr, 25 Apr, 29 Apr, and 06-07 May. 

Geomagnetic field activity is anticipated to reach G1-G2 (Minor-Moderate) storm levels on 19 Apr and 29 Apr due to -CH HSS influences, and on 07 May due to +CH HSS influences. Active
conditions are expected on 18 Apr, 20 Apr, and 30 Apr-01 May in response to -CH HSS effects, and on 15 Apr, 25 Apr, and 08 May due to +CH HSS effects. Mostly quiet to unsettled conditions are
expected for all other days of the period. 

Product: 27-day Space Weather Outlook Table 27DO.txt
:Issued: 2026 Apr 13 0104 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC web contact www.swpc.noaa.gov/content/subscription-services
#
#      27-day Space Weather Outlook Table
#                Issued 2026-04-13
#
#   UTC      Radio Flux   Planetary   Largest
#  Date       10.7 cm      A Index    Kp Index
2026 Apr 13      95           8          3
2026 Apr 14      90           8          3
2026 Apr 15     100          12          3
2026 Apr 16     105           8          3
2026 Apr 17     110           5          2
2026 Apr 18     110          15          3
2026 Apr 19     110          20          4
2026 Apr 20     120          12          4
2026 Apr 21     130          10          3
2026 Apr 22     140           8          3
2026 Apr 23     145           5          2
2026 Apr 24     145           8          3
2026 Apr 25     140          12          4
2026 Apr 26     140          10          3
2026 Apr 27     140           5          2
2026 Apr 28     140           5          2
2026 Apr 29     135          20          5
2026 Apr 30     130          18          5
2026 May 01     125          12          4
2026 May 02     125          10          3
2026 May 03     115           8          3
2026 May 04     108           8          3
2026 May 05     105           5          2
2026 May 06     100           5          2
2026 May 07      95          20          4
2026 May 08      90          15          3
2026 May 09      90           8          3
(NOAA)

Saturday, April 11, 2026

Sunday programming from Jen's Eclectic View & Real Deal

 


Don't miss it -

Aanother jammed-packed program from Jen's Eclectic Views & Real Deal R & R

Sunday, April 12, 2026, at 1700 UTC

Live Stream:  

For contact pleasure.

Thanks.

Jen In The RAD.

Friday, April 10, 2026

U.K. Propagation Update

 


RSGB
RadCom Assistant Editor | April 10, 2026
Compiled by G0KYA, G3YLA and G4BAO on 9 April, 2026.
After a pretty stormy run-up to Easter, from a geomagnetic disturbance point of view, the Sun has been quieter. In fact, the Kp index has been below 3 all week. Unfortunately, the solar flux index has also declined, standing at 108 on Thursday, 9 April.
The only advantage has been a lack of solar flares. There have only been 12 minor C-class flares over the past three days compared with 29 C-class flares and six M-class flares on 4-5 April.
We always look for a low Kp index over a higher solar flux index for better HF conditions.
So how does this all affect HF propagation? The maximum useable frequency, or MUF, over a 3,000km path has been struggling to get up to 28MHz on most days. This leaves only 21MHz and 24MHz open after the initial post-dawn ionospheric build-up.
This doesn’t mean that 10m is dead but it may be that the band is only open to DX and not open to Europe.

This may change once the Sporadic-E season starts but we are still a month away from that.
DX being worked, according to the CDXC Slack group, includes 5W1SA in Samoa on 17m FT8, F0/F6BCW from French Polynesia on 12m CW and 3DA0TM in Eswatini on 20m USB. T31TTT on Kanton Island, Central Kiribati, has also been spotted on the 20 and 30m bands using FT4 and FT8.
The DXpedition is focusing on FT modes, although the team is also operating some CW.
Next week, NOAA predicts that the solar flux index will start around 105 but will increase a little over the week to reach the low 120s.

Geomagnetic conditions are forecast to be quiet, with a maximum Kp index of 3 once we get over this weekend’s predicted disruption, which has a forecast Kp index of 5.
Then we are in for a rough ride next weekend, with a predicted Kp index of 6 on 19 April and disrupted conditions for three days. This is likely due to the return of active region 4392, which produced a coronal mass ejection that hit the Earth and caused the Kp index to rise to 7 on its last rotation.
VHF and up propagation news from G3YLA and G4BAO:
The warm, dry weather of the middle of last week has left us with ideas of spring but it has now been replaced by cooler, unsettled weather with rain or showers.
In fact, the next week or two will be generally unsettled, not atypical of April. This will be a good period for rain scatter on the upper GHz bands since April showers can be heavy and present good scatter opportunities.
This unsettled weather means tropo retreats into the background for this period.
Meteor scatter is still under the influence of random activity and best in the early morning hours. Aurora is currently looking more promising with solar conditions offering coronal holes and possible auroras as a result.

Sporadic-E will start to make an appearance soon, especially on the 10m band, but realistically, we probably need to wait until we are into May before chances are more rewarding for the 6m band.
It is often a feature of the early part of the Sporadic-E season that the traditional two periods of activity of the high season, morning and afternoon, start off as one broad period around the middle of the day.
For EME operators, Moon declination is starting to climb again, going positive on Wednesday, 15 April. Earth-Moon-Earth path losses are past maximum now and continue to fall all week.
144MHz sky noise is high today, 12 April, and will fall to low for the rest of the week. Friday, 17 April will be an exception as the Moon and Sun will be close in the sky.
(Mike Terry/BDXC) 

Thursday, April 09, 2026

April programming from Tilford Productions

 


THE FOLLOWING TIMES ARE TENTATIVE AND SUBJECT TO CHANGE - VISIT THE 
FACEBOOK PAGES OF EACH PROGRAM PRIOR TO BROADCAST FOR CONFIRMATION 
 
From the Isle of Music, Friday, April 10, 2026, 3955 kHz, 1600 UTC, repeats 2200 UTC 
This month, we present a surprise package of selections from several decades.  

Uncle Bill's Melting Pot, Friday, April 17, 2016: 3955 kHz at 1600 UTC, repeats 2200 UTC 
This month, we recognize the passage of Nuyorquino salsa artist Willie Colon with selections from some of his earliest recordings.  

In addition to direct radio reception, we do honor reception reports using remote SDRs as long as the whole program is described, and which SDR is specified. All QSLs are e-QSLs only.

William "Bill" Tilford, Owner/Producer 
Tilford Productions, LLC 
Lafayette, IN 

Tuesday, April 07, 2026

Wavescan radio history features 1500 Meters Longwave

1500 Meters Longwave
Part 1 – Before and During World War II

The Wavescan staff does it again .... a new and fascinating feature in radio history. on longwave. Thanks once again to our friends.

Jeff: Unique to Europe, North Africa, and parts of Asia is the use of longwave for AM radio broadcasting.  These days, many former longwave transmitters have been closed down, and the few that remain probably won’t do so for much longer.  But there is still a famous one that’s active in the British Isles, on 


198 kHz.  Ray Robinson has been looking into its history, which will be covered in two parts, this week and next.  Here’s Ray. ...

Ray: Thanks, Jeff.  When I was growing up in London as a young teenager in the 1960’s, one of my prized possessions was a small pocket radio I had been given for my 13th birthday.  I carried it everywhere, and I made good use of the single-piece earphones that came with it.  It was a 6-transistor, two-band model, but the two bands were not AM and FM as you might expect today.  They were medium wave and longwave, as was common in Europe at that time.

Today, the BBC still broadcasts their Radio 4 programming on 198 kHz longwave (as well as on FM and digital), and in fact, since the 1930’s, the BBC has used a high-power transmitter on longwave to achieve near national coverage.  But with the announcement that this will finally be shut down on September 26 this year, I thought it might be interesting to review the British use of longwave for radio broadcasting.

From 1922-1924, the BBC opened no less than nine medium wave stations in cities around the UK, beginning with 2LO in London.  These were all relatively low power – 1.5 kW each – and coverage in many parts of the country was poor to non-existent.

In October 1926, a 25 kW longwave transmitter was inaugurated at Daventry in the English Midlands on 1600 metres, 187.5 kHz, and this filled in a lot of the coverage gaps in central and southern England.  Then on March 9, 1930, a new ‘National Programme’ was launched by the BBC, using the longwave transmitter at Daventry and a new medium wave one at Brookmans Park in Hertfordshire, on the northern outskirts of London.  The National Programme was further extended to the north of England on July 12, 1931, again on medium wave, from a new transmission site high atop the Pennine Mountains, midway between Manchester and Leeds.  Other transmitters were added in central Scotland and Somerset in 1932 and 1933.

But by that time, it was planned that much of the medium wave network could be freed up for regional programming by instead utilizing a single high-power longwave transmitter for the National Programme.  Commercial stations were already heard with good signal strength in central and southern England from both Paris and Luxembourg, and so based on that evidence, it was hoped that a high-powered longwave transmitter somewhere in the heartland of the English Midlands would be able to provide near-nationwide coverage of the UK for the BBC.

The attraction of longwave, and specifically the part of the spectrum from about 150-300 kHz, was that signals could reach long distances by ground wave – up to 700 miles or more – with stable reception unaffected by ionospheric conditions, more or less around the clock.  Longwave was therefore of great interest to national broadcasters, especially in Europe and North Africa, which had large domestic territories to cover.  Unlike shortwave, longwave doesn’t rely on skywave propagation, and so doesn’t have a skip zone, fading, or any other atmospheric challenges.  It behaves much more like medium wave does during the daytime, but it has a much greater range, provided a high-power transmitter is used.  And in the 1930’s with 10 kHz bandwidth, the audio quality was pretty good for the monaural phonograph records of the day.

And so it was that in March 1933, a decision was made to purchase a site three miles northeast of Droitwich in Worcestershire, and the foundations for a transmitter hall there were laid in May.  By November 1933, the plans called for a 150 kW longwave transmitter to be constructed – the maximum power level allowed under the new Lucerne Plan, which was to take effect on January 15, 1934.  The Lucerne Plan was also the first international agreement that assigned frequencies to countries rather than to individual transmitters, and the frequency assigned to Great Britain was 200 kHz, exactly 1500 metres.  On the date the Lucerne Plan went into effect, January 15, 1934, the 150 kW transmitter at Droitwich was still under construction, so the existing 25 kW transmitter at Daventry was moved to the new frequency.  

The callsign 5XX which previously had been used at both Chelmsford and Daventry was also assigned to the new 150 kW longwave transmitter, which began testing on Monday, July 30, 1934, from midnight to 3am, daily except Sundays, after the Daventry transmitter had closed down for the night.  To radiate on the new longwave frequency of 200 kHz, a T-aerial was used, suspended between two 700-foot-high guyed steel lattice masts, standing 590 feet apart.

There was a soft launch of the new transmitter for some programming in the September, but the final cutover with an opening ceremony featuring an overture by the BBC Symphony Orchestra was on Sunday, October 7, 1934.  It’s interesting that this came a full 18 months after the opening of Radio Luxembourg’s all-day longwave broadcasts in English to the UK, which began in March 1933.




On Sunday morning September 3, 1939, the Prime Minister spoke to the nation in a broadcast to inform the people that Britain was now at war with Germany.  However, two days earlier, at 6:55pm on the evening of Friday, September 1, 1939, a message had been received by the B.B.C. from the government ordering all transmitters, including Droitwich, to be closed down and changed over to a pre-arranged wartime broadcasting system.  This involved wavelength changes for all medium wave transmitters so that they could operate in two synchronised groups, to avoid the possibility of them being used for direction finding.  At 8.15 that same evening, the medium wave transmitters returned to service with the Regional and National services now replaced by a single ‘Home Service’.  The medium wave transmitter at Droitwich, 5GB, was now broadcasting on 391 metres instead of 296 metres, and the longwave transmitter there, 5XX, had been closed down indefinitely.

By late 1939, many complaints were being received about the lack of choice and lighter entertainment for people serving in the British Armed Forces, both in the UK and that point, in northern France and the Low Countries.  In response to this, a new channel was formed called the BBC Forces Programme, which was launched on January 7, 1940, initially only from 6-11pm, although it was later extended to an all-day schedule.

The BBC Forces Programme was launched to appeal directly to those members of the armed services during the Phoney War who were mainly sat in barracks with little to do.  Its mixture of drama, comedy, popular music, features, quiz shows and variety was richer and more varied than the former National Programme, although it continued to supply lengthy news bulletins, informational programming and talk shows.

Use of the longwave transmitter, 5XX, resumed on November 16, 1941 with the European Service on 1500 metres, and from then on, coded messages were often sent to the French Resistance via that transmitter.  These were read during normal programmed broadcasts, usually at the end of news bulletins.

However, when American servicemen arrived en masse in 1943 and 1944 in preparation for Operation Overlord – “D-Day” – they found even the BBC Forces Programme to be staid and slow compared with the output of the American networks they were used to.

So, in response to appeals from General Dwight Eisenhower, the BBC abolished their Forces Programme and established the General Forces Programme instead, designed to provide a mixture of content suitable for both American and British servicemen, and also to appeal to the "Home Front", which research had shown wished to listen to the same type of output as the forces, once fighting had broken out.  The General Forces Programme replaced the BBC Forces Programme on February 27, 1944, and the main difference was that now a large number of American network and Canadian Broadcasting Corporation programmes were also included, alongside British programming such as the ‘Forces Favourites’ request show and comedies such as ‘Much Binding in the Marsh’ set in a fictional RAF station.

The General Forces Programme was on the air daily from 6:30am to 11pm, and in addition to the medium wave transmissions, it was also broadcast on the shortwave frequencies of the BBC’s Overseas Service, so it could be heard in North Africa, Italy, the Middle East and the Far East.  But the war in Europe ended on May 8, 1945, and so far as the British home audience was concerned, it was decided to replace the General Forces Programme with a new channel called the BBC Light Programme, and this was inaugurated on July 29, 1945, on 1500 metres longwave.  The General Forces Programme continued to be aired on shortwave only, primarily for forces stationed in the Far East, until December 31, 1946.

And we’ll pick up the story again with the new post-war BBC Light Programme on 1500 metres next week.
(Ray Robinson/Wavescan)


Music programs on Shortwave-Version 1, now available

 

The first version of my "Music Programs on Shortwave" PDF file for the new A-26 broadcast season is now available to download from the permanent link at 



You will also find here my "at-a-glance" single-page PDF programme grids for the English language programs on shortwave of BBC World Service, CGTN Radio, Voice of Turkiye, Radio Romania International, and Radio Taiwan International - all updated for the new A-26 broadcast season.
I hope that you find these of interest.
As always, I appreciate any updates or corrections.
(Alan Roe, Teddington, UK/BDXC)

Audio now available for Jen's Eclectic Views & Real Deal

 

No problem if you missed Sunday's program of  Jen's Eclectic Views & Real Deal.  The audio is now available for listening and downloading.

Jen's Eclectic Views & Real Deal. 



For contact pleasure.

Jen In The RAD.

Monday, April 06, 2026

Weekly Propagation Forecast Bulletins

 Product: Weekly Highlights and Forecasts
:Issued: 2026 Apr 06 0211 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC web contact www.swpc.noaa.gov/content/subscription-services
#
#                Weekly Highlights and Forecasts
#
Highlights of Solar and Geomagnetic Activity 30 March - 05 April 2026



Solar activity reached high levels on 30 Mar and 04 Apr, moderate levels on 02-03 Apr, with low levels observed on 31 Mar, 01 Apr, and 5 Apr. 

Region 4409 (N02, L=156, class/area=Eai/170 on 04 Apr) was the most active of the period, producing 50 C-class flares and six M-class flares. Region 4405 (S27, L=220, class/area=Eai/220 on 02 Apr) added the strongest flare of the period, an X1.4/Sf flare, on 30 Mar at
0319 UTC. Accompanying the flare was a Type II radio sweep (estimated velocity 1872 km/s) and a partial halo CME first seen in LASCO C2 imagery at 30/0312 UTC. Expected impacts from this CME were on 01 Apr. Region 4409 also produced a C8.1 flare at 01/1958 UTC.
Accompanying this flare was a filament eruption and subsequent CME that had a likely Earth-directed trajectory with impacts likely felt on 03-04 Apr. 

Slightly elevated proton levels were observed from 01-05 Apr, but conditions remained below alert thresholds throughout the period.   The greater than 2 MeV electron flux at geosynchronous orbit reached high levels throughout most of the period of 30 Mar - 05 Apr, with a
peak flux value of 6,000 pfu observed at 05/1645 UTC. The only exception was on 02 Apr when conditions dropped to moderate levels for that 24-hour reporting period. 

Geomagnetic field activity ranged from quiet to G3 (Strong) storm levels during the 30 Mar - 05 Apr period. Quiet to unsettled levels were observed on 30 Mar - 01 Apr, and most of 05 Apr (aside from an isolated active period at the beginning of the UT day). Conditions
increased to active to G2 (Moderate) levels on 02 Apr following the onset of a negative polarity coronal hole high speed stream (CH HSS). Conditions remained at active to G1 (Minor) levels through midday on 03 Apr, when they increased to G3 (Strong) levels with the
arrival of the anticipated CME from 01 Apr (C8.1 flare and filament eruption). Conditions then decreased to G1 levels to start 04 Apr, before decreasing to quiet to active conditions lasting through 05 Apr. 

Forecast of Solar and Geomagnetic Activity 06 April - 02 May 2026

Solar activity is expected to be at low levels, with a varying chance for M-class (R1-R2/Minor-Moderate) flares, and a slight chance for X-Class (R3/Strong) flares from 06 Apr through 02 May. 

No proton events are expected at geosynchronous orbit, barring any significant, non-recurrent solar activity. 

The greater than 2 MeV electron flux at geosynchronous orbit is expected to reach high levels on 06-09 Apr, 11-16 Apr, and 18 Apr-02 May. Normal to moderate flux levels are expected on 10 and 17 Apr. 

Geomagnetic field activity is anticipated to reach G1/G2 (Minor/Moderate) geomagnetic storm levels on 18-19, and 29 Apr due to the influence of negative polarity CH HSS (-CH HSS). Periods of G1 (Minor) storming are likely on 04 April in response to a negative
polarity CH HSS (-CH HSS). Unsettled to Active levels are expected on 06-07 Apr, 20-22 Apr, and 30 Apr, as well as 01-02 May associated with negative polarity CH HSS effects. On 10-13 and 25-26 April, positive polarity CH HSS influences are expected to bump geomagnetic
conditions to unsettled to active levels. Mostly quiet levels are expected during all other days of the period. 

Product: 27-day Space Weather Outlook Table 27DO.txt
:Issued: 2026 Apr 06 0211 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC web contact www.swpc.noaa.gov/content/subscription-services
#
#      27-day Space Weather Outlook Table
#                Issued 2026-04-06
#
#   UTC      Radio Flux   Planetary   Largest
#  Date       10.7 cm      A Index    Kp Index
2026 Apr 06     118          10          3
2026 Apr 07     115           8          3
2026 Apr 08     113           5          2
2026 Apr 09     111           5          2
2026 Apr 10     108          12          4
2026 Apr 11     106          18          5
2026 Apr 12     105          10          4
2026 Apr 13     108           8          3
2026 Apr 14     110           7          2
2026 Apr 15     115           5          2
2026 Apr 16     115           4          2
2026 Apr 17     120           7          2
2026 Apr 18     122          48          6
2026 Apr 19     124          22          5
2026 Apr 20     130          12          4
2026 Apr 21     140          12          4
2026 Apr 22     150           8          3
2026 Apr 23     155           5          2
2026 Apr 24     160           8          3
2026 Apr 25     155          12          4
2026 Apr 26     150          10          3
2026 Apr 27     145           5          2
2026 Apr 28     140           5          2
2026 Apr 29     140          20          5
2026 Apr 30     135          18          5
2026 May 01     130          12          4
2026 May 02     120           8          3
(NOAA)