Thursday, March 19, 2026

Uncle Bill's Melting Pot, March 2026

 


Uncle Bill's Melting Pot March 2026 
We are going to feature music from Ghana, including a tribute to the memory of Ebo Taylor.  
Friday, March 20, 2026, :3955 kHz, 1700 CET (1600 UTC), repeat 2300 CET (2200 UTC) 
 
Our eQSL policy includes recognizing reports from remote SDRs as long as the entire program is reported and the location of both the remote SDR and the listener is included.  Shorter reports will get a short note of thanks instead. 
William "Bill" Tilford, Owner/Producer 
Tilford Productions, LLC

Tuesday, March 17, 2026

Radio in Antarctica-Part 1

 

Penguins and the remains of the wreck The Gratitude, Nuggets Beach, Macquarie Island, 1911, Frank Hurley

Part 1 – Macquarie Island & South Georgia

Thank you to the staff of Wavescan, for Part 1 of Part 3 in this series

Jeff:  This week, we begin a two-part look at radio broadcasting in a part of the world few of us will ever get to visit – Antarctica.  In part 1 this week, Ray Robinson looks at the history of broadcasting in two remote islands in the Antarctic region – Macquarie Island, governed by Australia, and South Georgia, governed by the British.

Ray: Thanks, Jeff.  Macquarie Island is a cold, windswept island located halfway between the South Island of New Zealand and the Antarctic land mass.  It is a long, thin island, 21 miles long and 3 miles wide, and is actually the exposed top of the Macquarie Ridge where the Australian and Pacific tectonic plates meet.  Consequently, the area is prone to earthquakes, and two very large ones have occurred there so far this century, up around 8 on the Richter Scale.  In spite of its remoteness and extreme climate, though, the island’s latitude is actually less than 55 degrees south – about the same latitude in the northern hemisphere as, say, Newcastle in England, or Copenhagen, Denmark.

The island has no permanent human population, but it has been governed as part of the Australian state of Tasmania since 1880.  It is also home to the entire Royal Penguin population during their annual nesting season. 

Macquarie Island has been noted as a place of shipwreck and as the temporary, unplanned home of shipwreck survivors.  It was named in honor of a governor of New South Wales, Governor Lachlan Macquarie.  The first known visitors to Macquarie Island were Polynesian sea travelers, most likely from New Zealand, although it’s not known when they initially encountered the island.

The first European to visit the island was Captain Frederick Hasselborough aboard the Perseverance who came across the island by chance on July 10, 1810.  Ten years later, a Russian explorer, Thaddeus von Bellinghausen, also visited Macquarie.  And then two years later again, Captain Douglass on the Mariner visited the island and pronounced it as unfit for human habitation.  But, in 1825, Macquarie Island was declared to be part of Van Diemen’s Land, or Tasmania as we know it today.

For about 100 years, the island was used as a base for commercial companies harvesting animal oils, furs and skins.  This commercial exploitation ended around 1920, by which time the animal populations had been hunted almost to extinction.

Since shortly before World War I, a total of four different communication stations have been established on Macquarie Island and its claim to fame is that the very first wireless station in the Antarctic region was installed on this forbidding island.  The story goes back to the year 1911.

It was in December of 1911 that a small convoy of sailing ships, led by the Aurora, left Hobart, Tasmania, bound for Macquarie Island.  A little over a week later, these venturing ships arrived off the coast of Macquarie, only to find several seafarers already on the island, survivors of a ship that had been wrecked there just the day before.

On board the Aurora was all of the apparatus intended for the new wireless station; a 1½ kW Telefunken spark transmitter & receiver, masts & wires, and a petrol generator.  All of this electrical equipment was installed in a newly built wooden hut at the northern end of the island, for operation by the commercial companies engaged in animal hunting and processing there.  Twin wooden masts were erected on top of a nearby hill which was 350 ft above sea level.

The first historic wireless contact with the outside world was made on the evening of February 13, 1912 when station MQI talked with shipping south of Australia and New Zealand in spark gap Morse Code.  Soon afterwards, Morse Code contact was made with wireless stations AAM in Melbourne, AAA in Sydney & WN in Wellington.  However, the Macquarie Island wireless station didn’t fare well.  The aerial system was damaged and destroyed by high winds on three or four occasions, and there was always difficulty in making adequate contact with the Antarctic mainland as well as with Australia and New Zealand.

Finally, at the end of nearly three years of difficult service, the station was dismantled and shipped back to Australia, but the ship carrying it was sunk in a naval skirmish soon after the commencement of World War I in 1914, and all of the equipment was lost.  Both New Guinea and Samoa were German colonies at that time, and naval engagement with Australia and New Zealand began as early as August 1914.

The second wireless station for Macquarie Island was planned after World War I, and was listed with the callsign VIQ in 1921.  However, available records indicate that it may only have been on the air for a short period of time, if indeed it was ever erected at all.

A third station, this time for voice communication, was planned for Macquarie Island in 1947.  This was to be a shortwave station with the callsign VJM, and it was finally installed by a contingent of amateur radio operators five years later in 1952.  This station, again using 1½ kW, was in intermittent usage, depending on the availability of personnel, until communication on shortwave was phased out in 1988 in favor of satellite communication.

However, the shortwave station on Macquarie was re-activated in 1992 under the same callsign, VJM, but with a batch of new equipment, including a 1 kW Racal transmitter.  Thus, Macquarie Island has been on the air with communication equipment during four widely separated eras under three different callsigns, MQI, VIQ & VJM.  Wireless and radio messages from Macquarie Island were mainly for the benefit of passing shipping and other isolated wireless stations, with the home base on the island of Tasmania.

It is understood that a few QSL’s do exist verifying the VJM callsign, and in addition, several amateur radio operators who served on the island also issued their own amateur QSL cards.

And then there’s another very remote island near the continent of Antarctica – South Georgia in the far South Atlantic Ocean.  Like Macquarie, this island is also less than 55 degrees south, but is often covered by snow, and famously was where Ernest Shackleton finally made landfall in 1916 following the disastrous Imperial Trans-Antarctic Expedition.

South Georgia is larger than Macquarie, being about 100 miles long and 25 miles wide, but it is equally as forbidding.  The first settlement on the island was established in 1904 by a colony of Norwegian seafarers, and it ultimately became the hub of the whaling industry with some 2,000 permanent residents.

In 1925, a shortwave wireless station with the call sign ZBH was established by the British administration to enable communication with the outside world.

In 1938, a solar eclipse occurred over South Georgia on Sunday morning, May 28. The British arranged for special broadcasts from the island for the occasion and two small portable transmitters were stationed at two different locations, one on South Georgia itself, and the other further south on South Orkney, much closer to the Antarctic landmass.  It is understood that these transmitters operated in the old Apex Hi-Fidelity Band, 30-40 MHz, feeding live transmissions to a more powerful relay station in Argentina, probably at Monte Grande.

Records also indicate that the communication station ZBH, located at King Edward Point on South Georgia Island, was also used to relay the live broadcasts from the two small portable transmitters.  At the time of the eclipse, ZBH was on the air with 1 kW, on 8205 kHz.

In 1947, ZBH was again noted on 8 MHz with an irregular schedule that included a relay of the BBC news at 6:00 am.  Station ZBH in South Georgia was later shown on a set of postage stamps, issued in 2006.

Reception reports for the special eclipse broadcasts from South Georgia were requested and these were to be addressed to the Colonial Secretary at Port Stanley in the Falklands.  However, it is unknown whether any QSL’s were ever issued for the event.  It is also unknown whether any QSL’s were issued for the relay of the BBC news via ZBH, or for any of its regular communications on shortwave.

Well, next week, I’ll be looking at the history of broadcasting on the Antarctic landmass itself, and there is quite a bit more to that than you might think.

Back to you, Jeff.
(Ray Robinson/Jeff White)

Monday, March 16, 2026

Audio available for Jen &GB's St. Patrick program from March 15

 


If you missed it .... no problem !

Jen & GB's St Patrick's Day Annual Cast On Unique audio for Sunday, March 15, is up and ready for listening and downloading.  Programming includes a variety of Irish tunes, reels, jigs, and other goodies from the Celtic world, plus an all-green edition of Real Deal.

Audio available at:

Tiny URL link: 
Contact at: 

Trump nominates new head of VOA's parent agency after court ruling against Kari Lake

 
President Donald Trump nominated a senior State Department official on Thursday for the top post at the U.S. Agency for Global Media after a federal judge ruled that Kari Lake's leadership violated federal law.

Trump nominated Sarah Rogers, the undersecretary of state for public diplomacy, less than a week after U.S. District Judge Royce Lamberth ordered that all actions Lake took as acting CEO from July 31 to Nov. 19 be considered void, including an Aug. 29 reduction-in-force that eliminated jobs for more than 500 employees at Voice of America and elsewhere within USAGM.

Additional story at: 

Weekly Propagation Forecast Bulletins

 Product: Weekly Highlights and Forecasts
:Issued: 2026 Mar 16 0302 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC cweb ontact www.swpc.noaa.gov/content/subscription-services
#
#                Weekly Highlights and Forecasts
#
Highlights of Solar and Geomagnetic Activity 09 - 15 March 2026


Solar activity was at low to moderate levels with a total of 37 C-class flares and 2 M-class flares observed. The largest flares of the period were an M1.2 flare on 13/0955 UTC from Region 4384 (N10, L=150, class/area Eho/300 on 03 Mar), a C8.9/1n flare on 13/2023  from Region 4392 (S15, L=017, class/area Cso/170 on 15 Mar), and an M1.0/Sf flare on 15/0939 UTC from Region 4392. The most active region of the period was Region 4381 (N08, L=173, class/area Eao/220 on 03 Mar), which produced a long-duration C8.0 flare on 13/1518 UTC in addition to 11 other weak C-class events. 

No proton events were observed at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit reached high levels on 09 - 13 Mar and 15 Mar with a peak flux of 2,940 pfu observed at 12/1545 UTC. Normal to moderate levels were observed on 14 Mar. 

Geomagnetic field activity ranged from quiet to G2 (Moderate) storm levels throughout the 09-15 Mar period. The week began at quiet to unsettled levels on 09 Mar, with active conditions observed on 10-11 Mar due to the influence of a negative polarity coronal hole high speed stream (CH HSS). Conditions returned to mostly quiet to unsettled levels by 12 Mar. Activity intensified midday on 13 Mar, reaching G1 (Minor) to G2 (Moderate) storm levels following the onset of a positive polarity CH HSS. These storming levels continued through the first half of 14 Mar before waning to unsettled and active levels later in the day. On 15 Mar, the field reached active levels early in the period, followed by a return to quiet and unsettled conditions as positive polarity CH HSS effects gradually diminished. 

Solar wind parameters reflected the influence of two distinct CH HSS regimes during the period. The week began under the influence of a negative polarity CH HSS, with solar wind speeds initially ranging between 450-500 km/s before gradually declining to ambient levels near 400 km/s by 12 Mar. Total magnetic field (Bt) remained mostly around 6 nT during this interval, while the North-South (Bz) component saw periodic southward deflections to -7 nT. A solar sector boundary crossing (SSBC) occurred early on 13 Mar, indicated by a shift in the phi angle from the towards to away sector. This was immediately followed by the onset of a more powerful positive polarity CH HSS. Solar wind speeds rose sharply from 400 km/s to a peak of 725 km/s on 14 Mar. During this period, Bt reached 13 nT and the Bz component reached a maximum southward deflection of -10 nT.
By 15 Mar, solar wind speeds began a slow decline but remained elevated near 600 km/s through the end of the period. 

Forecast of Solar and Geomagnetic Activity 16 March - 11 April 2026

Solar activity is expected to be at low levels, with a slight chance for M-class (R1-R2/Minor-Moderate) flares throughout the outlook period. Elevated probabilities are related to the flare potential of both currently observed spot groups as well as the potential from returning regions. 

No proton events are expected at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit is expected to be at high levels on 16-20, 22-30 Mar, 04-09, and 11 Apr due to the influence of multiple, recurrent, CH HSSs. The remainder of the outlook period is likely to be at normal to moderate levels. 

Geomagnetic field activity levels are likely to reach G1 (Minor) geomagnetic storm levels on 22 Mar, 04 Apr, 09 Apr, and 11 Apr due to CH HSS influences. G2 (Moderate) geomagnetic storm levels are likely on 11 Mar and 10 Apr due to CH HSS influences. Unsettled to active levels are likely on 16-18, 20, 23-27, 30-31 Mar, and 03 and 05-07 Apr. All elevated levels of geomagnetic activity are associated with the anticipated influence of multiple, recurrent, CH HSSs. The remainder of the outlook period is likely to be at mostly quiet levels. 

Product: 27-day Space Weather Outlook Table 27DO.txt
:Issued: 2026 Mar 16 0302 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 2026-03-16
#
#   UTC      Radio Flux   Planetary   Largest
#  Date       10.7 cm      A Index    Kp Index
2026 Mar 16     108          15          4
2026 Mar 17     108          10          3
2026 Mar 18     105           8          3
2026 Mar 19     105           5          2
2026 Mar 20     105          10          3
2026 Mar 21     100          35          5
2026 Mar 22     102          25          5
2026 Mar 23     105          15          4
2026 Mar 24     110          15          4
2026 Mar 25     100          18          5
2026 Mar 26     110          10          3
2026 Mar 27     120           8          3
2026 Mar 28     125           5          2
2026 Mar 29     125           5          2
2026 Mar 30     125          15          4
2026 Mar 31     125          10          3
2026 Apr 01     130           5          2
2026 Apr 02     135           5          2
2026 Apr 03     140          18          5
2026 Apr 04     135          20          5
2026 Apr 05     135           8          3
2026 Apr 06     130          15          4
2026 Apr 07     135           8          3
2026 Apr 08     130           5          2
2026 Apr 09     125          25          5
2026 Apr 10     120          40          6
2026 Apr 11     115          20          5
(NOAA)

Sunday, March 15, 2026

Info on WEWN website update

 


USA.  The WEWN/ETWN website has updated (after 2 years) its frequency schedule page at https://www.ewtn.com/radio/frequency-guide and is now showing the schedule for 28 March to 24 October 2026, as follows:  12050 from 1400-0600 UT and 15610 from 1900-0600 UT.  No languages listed, but 12050 is Spanish, and 15610 would be English but is still, I think, currently off-air.
)Alan Roe, Teddington UK/BDXC)

Saturday, March 14, 2026

Jen' & GB's Annual St. Patrick's Day program

(designs by Gayle Van Horn)

Get your green on !! Jen and GB's St. Patrick's Day Annual Cast On Unique, Sun March 15th  at 18:00 -23:00 UTC and beyond! 


First intro to 18:15 UTC
Then GB takes over with his Irish Variety Selection to around 1930 UTC, then I finish up to past 2300 UTC with reels, jigs,and other goodies from the Celtic world, plus my all-green edition of the Real Deal
.

Live Stream:

Join us in our "Green" chat room


Click on connect, then web chat
Please put in the following:
For Nick: name or like me radionutresss
Then the next line channel, that's the following:
#eyeradiojd
and you are in the room.

Slaint !

Jen & GB

For contact pleasure.

Jen In The Rad.
73'' & 33''


Friday, March 13, 2026

Radio Six International slated for Saturday broadcast on 1467 kHz

 

Radio Six International info

Thanks to everyone who sent us reception reports after Saturday night's test broadcast on medium wave. 122 reports from 24 countries, almost all of which report excellent reception. 

We were being heard as far away as Canada, and we had a plethora of reports from Scotland, England, Italy, Germany, France, Spain, the Netherlands, Iceland, and Finland. 

We are now launching a weekly show on medium wave with 1,000,000 watts of power, starting on Saturday, 14th March, from 23:00 -00:00 UTC. 

Midnight Rendezvous will be heard on 1,467kHz (204m)on mediumwave, right across Europe. Most listeners will be able to tune in on an ordinary portable radio or car radio wherever they are in the UK, Ireland, or on the Continent.

https://www.radiosix.com/

DXer Ivo Ivanov, Radio Bulgaria ...and more

 
A nostalgic QSL collage from Radio Bulgaria

DX legend Ivo Ivanov: Even on the Internet, tell about Bulgaria!


Regular shortwave broadcasts of Radio Sofia's program to foreign countries—now Radio Bulgaria—began in April 1936. The number of languages broadcast varied, the frequencies shifted, radio exchanges with other radio stations began and ended, broadcasts to foreign countries were interrupted and then resumed, but the voices of the best translators and announcers continued to reach the most remote corners of the world, telling stories about our small but beautiful Bulgaria.

Since 1974, they have been reaching listeners via the Pydarsko Radio Transmitting Center near Plovdiv, which by the late 1980s was operating with a transmitting power of over 175,000 kilowatts, becoming the most powerful radio transmitting station in Bulgaria. It also featured a PA A30-31 rotating antenna system, unique in our country, with the ability to select the direction of the radiation.

Additional story available at: 
(article courtesy R Peason)

U.K. Propagation Update

 


RSGB
RadCom Assistant Editor | March 13, 2026

There has been plenty to work on the HF bands this past week.
3Y0K on Bouvet Island is still attracting a lot of radio amateurs, but there is also 8Q7ZW on the Maldives and German group J51A on Guinea-Bissau to get your attention.

DXpeditions to look out for next week include TX5EU from the Austral Islands, YJ1JXZ in Vanuatu, the tail-end of operations at T80K in Palau and VP2EAD, VP2ELX and VP2EWE on Anguilla.
HF propagation has been reasonable, rather than outstanding, with a solar flux index in the 140s, declining to the 120s as the week progressed. There have been a few C-class solar flares but nothing stronger.

Geomagnetic conditions have also been reasonable with the Kp index mostly in the twos and threes. There was one excursion where the planetary Kp index hit 4 around 7-8 March but otherwise it has been relatively calm.

The maximum useable frequency (MUF) over a 3,000km path has exceeded 28MHz on most days. 14MHz was open to the Maldives via FT8 as late as 2200UTC on Tuesday, 10 March.
Next week, the stand-out item is a large, but relatively thin, coronal hole on the Sun, and the high-speed solar wind stream from this reached the Earth on Friday, 13 March. Expect the Kp index to rise and HF propagation, especially on northerly paths, to suffer.

The Space Weather Prediction Centre forecasts that the solar flux index will decline further to be around 110 in the coming week. After this weekend’s geomagnetic disturbance due to the coronal hole, the Kp index is forecast to be more settled with a predicted maximum Kp of 3.

Things may heat up later in the week with a predicted Kp of 4, rising to 6 on Saturday,  21 March. Expect reduced maximum usable frequencies and poorer HF propagation, particularly on polar paths.
VHF and up propagation news from G3YLA and G4BAO:

The current spell of changeable weather is likely to stay with us through the bulk of the coming week but there is a glimmer of hope for better conditions after midweek, with a suggestion of high pressure over northern Britain.

To begin with, this means that rain scatter, including snow in places, will be worth checking out on the GHz bands, but strong winds may test antennas at times.

The transition to high pressure should lift conditions a little but since it’s forming in a cold polar air mass, it may not be as good as it could be.

The 1.3GHz UK Activity Contest on Tuesday, 17 March will probably still be in the wet and windy period so there may be a rainscatter bonus if the rain is heavy enough to affect such a low GHz band.

Aircraft scatter will always be the best option for this band when tropo is poor. The 70MHz UK Activity Contest on Thursday, 19 March, may fare better for tropo in Scotland and Northern Ireland.
Meteor scatter will offer up meagre rations as we remain between major showers. The April Lyrids are still a long way away. Aurora is still in the frame around the spring equinox so as usual, check for the Kp index moving up to 5 or higher.

Sporadic-E is not usually part of the story at this time of the year in these latitudes and, if anything is triggered, look to explore the path on digital modes first to see which directions are being favoured.
For EME, the conditions are poor for the coming week with the Moon declination negative but rising, not going positive until next Thursday. We continue with short Moon windows and low peak elevation, but with falling path losses.

While 144MHz sky noise is moderate to low in the coming week, Wednesday and Thursday see the Sun and Moon close in the sky, meaning high noise on the lower bands due to wider antenna beamwidths.
 
(Mike Terry, UK/BDXC)

Thursday, March 12, 2026

BBC adds extra mediumwave frequency to Iran

 


Cris Greenway from the U.K. reports the following:

Alongside the existing 702 (from Oman) and 1395 (from Armenia), the BBC has now added 720 (from Cyprus) and 1296 (from Tajikistan) for its Persian broadcasts. 

From the Isle of Music, March 2026

 

This month will feature some exciting new and recent releases by Cuban bands.  
Friday, March 13, 2026,  3955 kHz, 1800 CET (1700 UTC), repeat 2300 CET (2200 UTC) 

Our eQSL policy includes recognizing reports from remote SDRs as long as the entire program is reported and the location of both the remote SDR and the listener is included.  Shorter reports will get a short note of thanks instead. 

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

Wednesday, March 11, 2026

Texas Radio Shortwave, March 12, 14, 15

 


UTC/Station/Frequency/Station/Target Area/Program Feature

March 12, 2026
2000   3975   Shortwave Radio Gold   Europe  The Music of Janis Joplin 



March 14, 2026
1300 6160 Shortwave Radio Gold  Europe  The Music of Texas Mariachis (Rebroadcast)           
1900 3975 Shortwave Radio Gold  Europe  The Music of Texas Mariachis (Rebroadcast)

March 15, 2026
1100   6070 Channel 292  Europe   Michael Strah on Texas Radio, The Music of Texas Sidemen 

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 (Eur) 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 (Eur) 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 (NAm) 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) 

Tuesday, March 10, 2026

News from World Music Radio

 


DENMARK
World Music Radio posted this today on their Facebook page:
World Music Radio will be off the air for a few hours today, March 10th, from around 12 UTC.  
15700 from north of Randers was switched off yesterday. It will hopefully soon return from another transmitter site. 

The 5930 frequency has had no modulation for some weeks. I am trying to resolve it within a week.  A new 5G router has been purchased. 

The New mailing address (for snail mail) will be announced shortly. Please don't use the old address in Randers anymore.
(Alan Roe, Teddington, UK/BDXC)

Monday, March 09, 2026

The Story of Radio Diego-Suarez

Thank you to the staff of Wavescan - for another nostalgic look at radio history

Jeff: This week, we have a story about a shortwave station that was setup during World War II in a French Overseas Territory controlled by Vichy France.  And once again we thank Dr. Martin van der Ven for contributing to this item.

Ray: Thanks, Jeff.  Following the Nazi invasion of France that began in May 1940, the French capital, Paris, was occupied without a fight on June 14.  The remnants of the French government had left Paris four days earlier, and by agreement with the occupiers with whom they collaborated, they moved about 220 miles south to the central southern French town of Vichy, from where the southeastern part of the country was administered until August 1944.  What is not widely appreciated is that all of the French overseas territories were also administered from Vichy during the war, not from Paris by the Germans.

Much of the French overseas territory in the Far East was quickly occupied by the Japanese, but elsewhere, the Vichy-controlled territories were viewed with much suspicion by the Allied Forces.  For instance, the British were concerned that both the French island of St. Pierre off the south coast of Newfoundland and the French island of Martinique in the Caribbean might be used as refueling bases for the U-boats that were attacking merchant and allied shipping in the North Atlantic.

But, further afield off the east coast of Africa lay the much larger island of Madagascar, which from 1896 to 1958 was a French colony.  The British had concerns in the early 1940’s that Madagascar could be used as both a refuge and a refueling base for Japanese submarines that were operating all over the Indian Ocean.  And so, it was decided in London to initiate “Operation Ironclad,” to occupy the island of Madagascar.  This operation began on May 5, 1942.

The primary objective was to neutralize the French naval base of Diego-Suarez (which is shown on maps these days as Antsiranana) at the very northern tip of Madagascar.  The operation was launched from a small flotilla of ships – primarily the HMS Winchester Castle, accompanied by four smaller ships, Keren, Karanja, Llandaff Castle, and Sobieski, all escorted by the battleship HMS Ramilles.

The 20,000-ton HMS Winchester Castle had been constructed as a passenger ship in 1926, and before the war had been operated by the British Union-Castle Line for passenger and mail services between Great Britain and South Africa.  Earlier in the war, she had been equipped with sonar and wireless direction-finding equipment, after which she was used as a training ship, and then as a troop transporter.

After the successful landings, the port of Diego-Suarez was in the hands of the British within two days, and on May 7, 1942, the Winchester Castle anchored in the bay.



700 miles to the south in the capital, Tananarive, the Vichy radio station then launched propaganda broadcasts to discredit the British and hinder their progress in occupying the southern part of the island.  They claimed that Diego-Suarez had been destroyed by bombs and that there were many civilian casualties.

So to counter this, a British officer who spoke French decided to use a powerful transmitter on board the HMS Winchester Castle.  A studio was set up in cabin 136, and a signals sergeant assisted with the technology.  The ship’s transmitter was tuned to the frequency of Radio Tananarive, which operated on 6063 kHz, in the 49 meter band, with 5kW.  As soon as the French station ended its broadcasts in the evening, the officer powered up the Winchester Castle transmitter and opened the microphone, saying in French:  “Hello, hello, this is Radio Diego-Suarez, stay tuned.  A British officer is speaking to you.”  He then informed the residents of Madagascar that the situation in Diego-Suarez was normal, and that there were no civilian casualties.  He even read 25 reports from civilians to reassure their families.  This information was subsequently gratefully accepted and repeated by Radio Tananarive.

Originally, Radio Diego-Suarez was supposed to broadcast only a few times, but due to its success, it was decided to extend the experiment.  The officer’s prepared texts were reviewed and refined linguistically by the French cook on board.  Radio Diego-Suarez could eventually broadcast regularly.  In the evening, Radio Tananarive concluded its programs with the French national anthem, La Marseillaise, and shortly thereafter, Radio Diego-Suarez started its program with La Marseillaise as well.  Personal messages for the population were disseminated, along with useful information and a program called “Paroles de Churchill,” (or, Words of Churchill) aiming to correct the propaganda of the Vichy regime.

A land-based studio for the new Radio Diego-Suarez was set up in a former cinema, and three weeks after the landing, the HMS Winchester Castle left the port.  She sailed first to Mombasa, Kenya and then on to New York.  Radio Diego-Suarez continued to broadcast in French and Malagasy, and the music programs became more diverse.  On November 5, 1942, six months after the operation had started, the British troops captured Tananarive and took over the main radio station there.  Radio Diego-Suarez then ceased broadcasting, and three days later, on November 8th, the last fighting French forces in the south of the island surrendered.

Sadly, no recordings are known to exist of Radio Diego-Suarez, and it’s unlikely that any QSL cards would have been issued for reception reports from shortwave listeners to this temporary wartime station.

Back to you, Jeff.
(Ray Robinson/Jeff White-Wavescan)


Encore classical music from Radio Tumbrill

 

Dear Listener

Regular Broadcast times of Encore By WRMI and Channel 292 are:
02:00 - 03:00 UTC Friday 5850 kHz WRMI to US
20:00 - 21:00 UTC Friday 15770 kHz WRMI to Europe
11:00 - 12:00 UTC Saturday 9670 kHz Channel 292 to Europe
01:00 - 02:00 UTC Sunday 5850 kHz WRMI to US and Canada
18:00 - 19:00 UTC Sunday 3955 kHz Channel 292 to Europe
02:00 - 03:00 UTC Monday 5950 kHz WRMI to the US and Canada
13:00 - 14:00 UTC Tuesday 15770 kHz WRMI to Europe, east coast of US, and Iceland. (Sometimes RTTY on the lower sideband. Suggest notch out or use USB.)

Some Things to see on The Encore Website:
The Encore website is www.tumbril.co.uk, where you will find:
Important information about the funding of Encore - Radio Tumbril.
Up-to-date transmission times and frequencies.
The playlists for the most recent programmes.
An email link.
Informal reception reports as well as those requesting eQSL cards are welcome.

PLEASE MAKE A PAYPAL DONATION AND HELP KEEP ENCORE ON THE AIR - Go to - www.tumbril.co.uk

WRMI and Channel 292 are very generous with their air-time but Encore still costs around 130 Dollars/Euros a month to broadcast.
If you can - please send a small contribution to help Encore keep going.

THE DONATION BUTTON is on the homepage of the website - www.tumbril.co.uk - which folks can use if they would like to support Encore.

(Please don't be put off by the POWR security wall when using the PAYPAL button - it is a harmless requirement of WIX the website hosting service.)

THIS FORTNIGHT'S PROGRAMME - First broadcast on FRIDAY 6th March by WRMI at 0200 UTC on 5850, and 2000 UTC on 15770 and then Channel 292 on SATURDAY 7th March at 11:00 UTC on 9670 kHz:
Starts with the overture from The Barber of Seville by Rossini. After that part of a cello sonata by Martinü and a piano piece from contemporary composer Caroline Shaw.
A mass for five voices by Byrd, Part of a Haydn symphony- No. 84 in E-Flat Major - and a Bach partita are next.
The Programme ends with the third movement from the Octet in C Major by Romanian composer Enescu.

(This bulletin is sent by Bcc to the many hundreds of listeners who have been in contact with Encore over the last six years of broadcasting Encore.)

Brice Avery - Encore - Radio Tumbril - www.tumbril.co.uk
GMØTLY



Jen's 'It's All About Time & Change', audio available from March 8th

 


The Sunday, March 8th edition of  Jen's Tic- Toc of a show, which aired from 18:00-21:00 UTC, plus on Unique is up and ready for listening and downloading

Jen's Tic -Toc of a show Link.


Short Link.

Weekly Propagation Forecast Bulletins

 Product: Weekly Highlights and Forecasts
:Issued: 2026 Mar 09 0207 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 02 - 08 March 2026

Solar activity was at low levels with a total of 24 C-class flares observed. The largest flares of the period were observed early on 02 March; a C6.1 flare at 02/0206 UTC from Region 4380 (S20, L=195,
class/area Dao/140 on 26 Feb) and a C5.2 at 02/0615 UTC and a C 5.9 at 02/ 0749 UTC, both from Region 4381 (N08, L=173, class/area Eao/220 on 03 Mar). Region 4384 (N10, L=150, class/area Eho/300 on
03 Mar) was the most active, producing 10 weak C-class events. No Earth-directed CMEs were observed in available LASCO imagery. 

No proton events were observed at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit reached high levels on 02, 03 and 08 Mar with a peak flux of 10,450 pfu observed at 02/1810 UTC. Normal to moderate levels were observed on
04-07 Mar. 

Geomagnetic field activity reached quiet to G1 (Minor) geomagnetic storm levels during the period. Quiet levels were observed on 02 Mar through midday on 03 Mar. Unsettled to G1 (Minor) storm levels were
observed on the last half of 03 Mar into early 04 Mar due to effects from a positive polarity CH HSS. Quiet to isolated unsettled levels were observed on a majority of 04 Mar through 06 Mar. Negative
polarity CH HSS effects influenced 07-08 Mar with quiet to active levels observed on the 7th and quiet to G1 (minor) storms observed on 08 Mar. 

Solar wind parameters observed a peak wind speed of about 675 km/s late on 07 Mar. Total field reached peaks of 11 nT on 03 Mar and 12 nT midday on 07 Mar, while Bz was southward to -10 nT late on 03 Mar
and -9 nT late on 06 Mar. Phi angle was in a mostly positive orientation on 02 Mar through midday on 06 Mar and in a negative orientation from midday on 06 Mar through 08 Mar. 

Forecast of Solar and Geomagnetic Activity 09 March - 04 April 2026

Solar activity is expected to be at low levels, with a slight chance for M-class (R1-R2/Minor-Moderate) flares throughout the outlook period. Elevated probabilities are related to the flare potential of
both the currently observed spot groups and the potential from returning regions. 

No proton events are expected at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit is expected to be at high levels on 09-11, 16-19, 23-30 Mar and 04 Apr due to the influence of multiple, recurrent, CH HSSs. The
remainder of the outlook period is likely to be at normal to moderate levels. 

Geomagnetic field activity is expected to reach G1 (Minor) geomagnetic storm levels on 14 Mar, 22 Mar, 25 Mar and 03-04 Apr during the onset CH HSS. G2 (Moderate) geomagnetic storm levels are
likely on 21 Mar due to negative polarity CH HSS effects. Unsettled to active levels are likely on 09-11, 15-20, 23-24, 26-28, 30 Mar and 02 Apr. All elevated levels of geomagnetic activity are
associated with the anticipated influence of multiple, recurrent, CH HSSs. The remainder of the outlook period is likely to be at mostly quiet levels. 

Product: 27-day Space Weather Outlook Table 27DO.txt
:Issued: 2026 Mar 09 0207 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC contact  www.swpc.noaa.gov/content/subscription-services
#
#      27-day Space Weather Outlook Table
#                Issued 2026-03-09
#
#   UTC      Radio Flux   Planetary   Largest
#  Date       10.7 cm      A Index    Kp Index
2026 Mar 09     135          12          4
2026 Mar 10     130          10          3
2026 Mar 11     125           8          3
2026 Mar 12     120           5          2
2026 Mar 13     115           5          2
2026 Mar 14     110          20          5
2026 Mar 15     110          15          4
2026 Mar 16     110          10          3
2026 Mar 17     110          10          3
2026 Mar 18     110          10          3
2026 Mar 19     105          12          4
2026 Mar 20     110          15          4
2026 Mar 21     110          35          6
2026 Mar 22     110          24          5
2026 Mar 23     115          15          4
2026 Mar 24     115          15          4
2026 Mar 25     120          18          5
2026 Mar 26     125          10          3
2026 Mar 27     130           8          3
2026 Mar 28     130           8          3
2026 Mar 29     130           5          2
2026 Mar 30     130          14          3
2026 Mar 31     130           6          2
2026 Apr 01     135           5          2
2026 Apr 02     130          10          3
2026 Apr 03     130          20          5
2026 Apr 04     130          25          5
(NOAA)

Friday, March 06, 2026

U.K. Propagation Forecast

 

RSGB
RadCom Assistant Editor | March 6, 2026
What a difference a week makes…
In our last report, we mentioned that there were zero sunspots and a solar flux index of 130. This week has seen a turnaround with five active sunspot regions and a solar flux index of 144.
HF propagation has been reasonable with openings up to 10m to various parts of the world. We have only seen M-class solar flares, although there have been around 40 of them in the past five days.
We had a brief excursion in the Kp index when it went to 5 during one three-hour period, late on 3 March. However, it soon recovered and has been at 2 or lower for the past two days at the time of writing.

The effects of a small Earth-facing coronal hole started coming past the Earth on 6 March and is expected to be the source of a solar wind stream. According to NOAA and the Space Weather Prediction Centre, Active to Minor G1 geomagnetic storming will be possible today, 8 March.
We have now seen the start of the 3Y0K Bouvet Island DXpedition, which is due to run until around 17 March. It has already been worked from the UK on bands from 40 to 12m.
Bouvet is virtually due south from the UK and the higher bands should be open from around 0700 to around 1900UTC. The 40 and 30m bands should open from around 2000 to 0400UTC. So, there are plenty of opportunities to work the station.

Next week, the Space Weather Prediction Centre in the US forecasts that the solar flux index may be around 156 today, 8 March, but will then decline to be in the 120s or even 110s later in the week.
We may have slightly unsettled geomagnetic conditions around 10-12 March and again on 14-15 March, with an estimated Kp index of 4.

In summary, HF conditions are not bad. Keep an eye on solarham.com  for daily updates.
VHF and up propagation news from G3YLA and G4BAO:
The recent change of weather to introduce high pressure onto the scene provided some welcome enhanced tropo conditions in the last week.

The March RSGB 144MHz and 432MHz Championship should still be able to benefit, except perhaps for the northwestern fringe of the UK where the next Atlantic fronts will be making an intervention.
It looks a little more problematic for the 432MHz UK Activity Contest on Tuesday, 10 March. The same is true for the RSGB 50MHz UK Activity Contest on Thursday, 12 March as the low-pressure pattern returns and offers a chance of rain scatter for the microwave bands.

The meteor scatter prospects are still driven by random activity, so as usual a preference for the early hours of the morning are called for on this mode.
It has been mentioned before that the Spring and Autumn are periods when auroras are more likely. This is known as the Russell-McPherron effect when the Earth’s magnetic field is better coupled to the solar wind.
So, keep monitoring the Kp index for signs of it going above 5. Then check the bands for fluttery signals, even on the LF bands. CW can be used as an early ‘heads up’ for potential activity on the VHF bands.

Thoughts about Sporadic-E should be kept in check for a while yet since we are still very far away from the usual start of the season.
For EME, Moon declination is negative and falling to a minimum next Thursday, meaning shortening Moon windows and lower peak elevation until then.

Path losses are falling until apogee on Tuesday, 10 March. 144MHz Sky noise is moderate, rising to a high of more than 3000 Kelvin on Thursday and falling back by next weekend.
(Mike Terry, UK/BDXC)

Radio Six International program update

 


The Radio Six International programme scheduled for 7th March at 2300 UTC on 1467 kHz is Tony Currie's "Midnight Rendezvous" "with music from and to the continent.

Radio Six's full schedule for March is here: https://syndication.radiosix.com/Radio_News_702MW.pdf  (cover of this schedule magazine does mention Radio Six launching weekly transmissions on 1467 from Roumoules, but it is only listed inside on one Saturday in the March schedule, tomorrow's test, on the 7th).

Here in southern England, the sky wave signal from Radio Paradijs, local Dutch LPAM for Utrecht is usually in the clear and fair strength on 1467 after TWR has closed. Plus a het from Radio Qom, Iran, off channel on around 1467.4. But I guess they will be blocked tomorrow 2300-0000!)
(Alan Pennington, UK/BDXC)

Additional posting: 
After many years on shortwave, Radio Six International will be conducting a test transmission on Saturday 7th March on 1,467kHz medium wave.

This will run from 23:00 - 00:00 GMT, using the transmitter at Roumoules, France with a power of 1,000kW and a beam of 325 degrees.

If this is successful, we will provide a weekly programme at this time and help to prove that medium Wave is still alive!  Reception reports for this test transmission are crucial - please send to: 
letters@radiosix.com  Reports will be acknowledged with an eQSL.

Texas Radio Shortwave, March 7,8

 

UTC/Station/Frequency/Station/Target Area/Program Feature

March 7, 2026
1500   6160   Shortwave Radio Gold   Europe  The Music of Texas Mariachis
1900   3975  Shortwave  Radio Gold   Europe   The Music of Texas Mariachis

March 8, 2026
1300   9670   Channel 292  Europe   The Music of Texas Mariachis
2300   9670   Channel 292  North America  The Music of Texas Mariachis

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

Thursday, March 05, 2026

Radio Caroline slated for March 7-8 broadcast

 
Ross Revenge


Our next Radio Caroline North broadcast is between 7th – 8th March, live from our radio ship Ross Revenge.

You'll hear some great music from the 60s to 90s – plus you could win a superb KLIM retro boombox in this month's competition draw.

Listen on 648 AM across England, The Netherlands, Belgium and beyond, on
1368 AM in the North/North-West courtesy of our friends at Manx Radio, worldwide online here via our Caroline North Player, on smart speakers and the Radio Caroline app.

We'd love to hear from you during the broadcast via north@radiocaroline.co.uk, and remember, it's the only email address that gets you straight through to our 'North' broadcasters.

https://www.radiocaroline.co.uk/#home.html
(Mike Terry, UK/BDXC)

NHK World Japan, broadcasting 24-hour service to the Middle East

 
Press Release
March 1, 2026, Tokyo – In light of recent developments in the situation in Iran, NHK has begun temporary shortwave transmissions of its Japanese-language international radio service, NHK World Japam Radio, starting on March 1, 2026, 
This measure is based on NHK’s mission as an international public service media to provide essential information to Japanese nationals residing in or traveling in the region.
Due to the attacks on Iran by the United States and Israel, internet connectivity and international telephone services in the region have become unstable, resulting in limited access to information in Japanese. In response, NHK has begun temporary shortwave transmissions of its Japanese-language international radio service, NHK World-Japan Radio, to provide essential information to Japanese nationals staying in the area. These broadcasts started at 11:30 a.m. (Japan Standard Time) on Sunday, March 1.
NHK normally broadcasts six hours of shortwave programming per day to the Middle East. However, in view of the current situation, the broadcast schedule has been expanded to provide continuous 24-hour service. In addition to content from NHK Radio 1, the broadcasts will include timely safety and security information for those in the region.
For those in neighboring countries or other areas where internet access remains available, NHK also provides Japanese-language news on the NHK WORLD-JAPAN website, along with simultaneous and on-demand streaming of its television and radio programs. We encourage people to use these trusted sources to help ensure their safety.
NHK World Japan in Japanese 

(This service is not accessible from within Japan and is available only overseas.)
Details of the Temporary Transmission
During the temporary transmission period, NHK will provide simultaneous broadcasts of NHK Radio 1, along with NHK WORLD-JAPAN’s own Japanese-language international news and “Overseas Safety Information,” which focuses on travel advisories issued by Japan’s Ministry of Foreign Affairs, including updates related to the situation in Iran. Because shortwave broadcasts can be transmitted directly from Japan, they are considered less susceptible to restrictions by local authorities.
The broadcast frequencies will change as needed. Information on the frequencies and other details of the temporary transmissions will be announced on the Japanese-language website of NHK World Japan. 

NHK orld Japan Radio 
Emergency Shortwave Transmissions to the Middle East
Broadcast Schedule and Frequency List
NHK is providing 24-hour temporary shortwave transmissions of Japanese-language news and programming to the Middle East from the KDDI Yamata Transmitting Station in Koga City, Ibaraki Prefecture, and other relay sites.
(All times are shown in Japan Standard Time.)
Transmissions from the Yamata Transmitting Station
Time (JST) Frequency
01:00–02:00 11915 
02:00–04:00 11670 
04:00–06:00 9665 
06:00–08:00 11675  (regular slot)
08:00–10:00 11660 
10:00–14:00 17560 
14:00–18:00 9700 
18:00–22:00 9740 
22:00–23:00 11685 
23:00–01:00 9450 

Transmissions from the France Relay Station
Time (JST) Frequency
02:00–04:00 11800  (regular slot)
12:00–14:00 6150 (regular slot)

Due to the characteristics of shortwave broadcasting, listeners may need to switch receiving frequencies every few hours.

NHK (Japan Broadcasting Corporation) is Japan’s sole public service media organization. Funded by receiving fees from Japanese households, it has a reputation for impartial, high-quality news and programs, including documentaries, children’s and educational programs, music, entertainment, culture, animation, and drama.
Comment 
(NHK)




Tuesday, March 03, 2026

WRMI Winter Schedule Update- 03 March 2026

 

The current color grid program schedule,  effective to 29 March 2026, is available at: 

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

0000-0100  5010ca  5850na  7730na  9455na  15770eu  17790va
0100-0200  5050la  5800la  5950na  7730na  7780ca  9455na  15770eu  17780va
0200-0300  5010ca  5050la 5950na  7780ca  15770eu
0300-0400  5050la  5950na  9955sa  15770eu
0400-0500  5050la  7570na  7730eu  7780ca  9955sa  15770eu
0500-0600  7570na  7730na  7780ca  15770eu
0600-0700  5850na  7570na  7730na  7780ca  9395na  15770eu
0700-0800  5850na  7570na  7730na  7780ca  9395na  15770eu
0800-0900  7730na  7780ca  9395na  15770eu
0900-1000  5850na  7730na  9395na  15770eu
1000-1100  7530na  7730na 7780ca   9395va  15770eu
1100-1200  5850na  7570na  7730na  7780ca  9395na
1200-1300  7730na  9395na  15770eu
1300-1400  7730na  9395na
1400-1500   7730na  9395na  15770eu
1500-1600   7730na  9395na  17790va
1600-1700  7730na  9395na  17790va
1700-1800  7730na  9395na  15770eu  17790va
1800-1900  7730na  9395na  15770eu  17790va
1900-2000  7730na  9395na  17790va
2000-2100  9395na  17790va
2100-2200  5850na  7730na  9395na
2200-2300  5850na  7730na  15770eu  17790va
2300-0000  5010ca  5850na  7730na  9455eu  17790va

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)

Monday, March 02, 2026

Coalition Maritime Forces – Radio One

Thank you to the Wavescan staff for this nostalic story on the Global War on Terror. 



Jeff: Just over 20 years ago, shortwave radio regained strategic importance in 2004 and 2005 during the so-called “Global War on Terror.”  Here’s Ray Robinson in Los Angeles to remind us of what happened.

Ray: Thanks, Jeff.  This is a story that I must admit passed me by at the time, but Dr.  Martin van der Ven in Germany recently drew my attention to it, and I found it had been written about quite extensively at the time on the DXing.info website, in Radio World, Monitoring Times and in other radio journals.  So, what happened?

Well, one of the more unusual and historically significant examples of the revival of shortwave radio during that period was the establishment of Coalition Maritime Forces – Radio One (or CMF Radio One), a low-power shortwave broadcasting service operated by the United States Navy through its Maritime Liaison Office (MARLO), headquartered in Bahrain.  Beginning in April 2004, this operation combined elements of psychological operations (or ‘psyops’), maritime security communications, and traditional radio broadcasting, targeting seafarers across the Persian Gulf, Gulf of Oman, Arabian Sea, and beyond.  And the interesting thing was that the broadcasts came from ships.

Origins and Official Disclosure (April 2004)
The existence of the broadcasts first came to public attention through a navigational warning rather than a conventional media announcement.  On April 20, 2004, the U.S. National Geospatial-Intelligence Agency (the ‘NGA’) published a notice, intended for mariners operating in the Persian Gulf, explicitly announcing that “Coalition Maritime Broadcasts” had commenced on shortwave radio as of April 15, 2004.

According to the official text, the broadcasts were initiated “in response to all mariners that have helped Coalition Maritime Forces in the Global War on Terror” and as a means to build broader engagement with regional audiences.

Programming consisted primarily of popular regional and international music, interspersed with informational segments in Arabic, Farsi, Hindi, Pashto, Urdu, and English.  The purpose of the broadcasts was to urge seafarers to report terrorist activity conducted at sea.

At first, two daily transmission windows were specified: a morning broadcast from 0300 to 0800 UTC on 6125 kHz, and an early evening broadcast from 1400 to 1900 UTC on 15500 kHz.  Although the original web page hosting the warning was subsequently deleted, cached versions preserved by Internet archive sites and reports from DX enthusiasts confirmed the authenticity of the announcement.

MARLO and the Strategic Context
The broadcasts were coordinated by the Maritime Liaison Office (MARLO), an organization established to facilitate information exchange between the United States Navy and the commercial shipping community within the U.S. Central Command (CENTCOM) area of responsibility.  MARLO’s stated mission emphasized maritime safety, situational awareness, and cooperation with civilian seafarers – an especially critical concern in the post-9/11 security environment, where fears of maritime terrorism, attacks on oil terminals, and the use of shipping lanes by non-state actors were prominent.

Radio Netherlands and later BBC Monitoring independently confirmed MARLO’s role, noting that the broadcasts were part of a broader effort to encourage voluntary intelligence sharing from seafarers.  The informational segments also promoted the U.S. “Rewards for Justice” program, which offered financial incentives for information preventing or resolving terrorist acts.

Technical Characteristics and Early Monitoring
The transmissions originated from coalition naval vessels operating in the Gulf of Oman and the northern Arabian Sea, using single-sideband transmitters with a power output of only about 250 watts.  Such low power, combined with shortwave propagation characteristics and skip zones, meant reception was variable, and the broadcasts were difficult for the international DX community to monitor.

Nevertheless, by early May 2004, reception reports did begin to emerge from Europe.  On May 4, 2004, Finnish DXer Jari Savolainen reported hearing an upper sideband (USB) transmission on 15500 kHz featuring continuous Middle Eastern and South Asian music, with intermittent announcements in Urdu or Hindi and English, including a U.S. toll-free telephone number associated with the Rewards for Justice program.  This was an especially difficult catch, not only because of the low power being used, but also because Radio Kuwait was broadcasting at the time on the two split-channels 5 kHz above and below 15500 – 15495 and 15505 kHz.  

But, all the evidence suggested that the broadcasts were not merely informational but constituted a form of psychological operations (‘psyops’), in a similar manner to the earlier ‘Information Radio’ broadcast by US forces from airborne medium wave and FM ‘Commando Solo’ transmitters over Iraq the previous year.

In 2005, a significant operational change occurred with the introduction of a new frequency:  9133 kHz (USB).  This frequency offered improved reception in Europe and the eastern Mediterranean, as confirmed by numerous DX reports from Sweden, Austria, and Finland.  BBC Monitoring formally documented broadcasts on 9133 kHz on May 1, 2005, noting Afghan and Arabic music interspersed with appeals for information related to terrorist activities, including specific references to Iraqi oil terminals.  Here’s an audio clip of one such announcement in English, providing instructions on how listeners could assist coalition forces by identifying and reporting terrorist activity at sea.  The speaker has a heavy Middle Eastern accent:


“Thank you for listening to Coalition Maritime Forces Radio One.  This broadcast is conducted continuously throughout the term of the violence around the world.  Tune to CMF Radio One anytime on 6125 kHz, 9133 kHz or 15500 kHz.  If you have any information regarding terrorist or illegal activities, please contact any coalition forces or coalition embassy, or by telephone to 001-800-877-3927, or email at mail@rewardsforjustice.net.  Your identity will be protected.”

Under the ‘Rewards for Justice’ program, the U.S.A.  offered financial rewards for information that prevented or favorably resolved acts of terrorism against the United States.  It is known that one unnamed Iraqi received US$1 million through the program for information that led to the arrest of Khamis Sirhan al-Muhammad, a Baath Party regional chairman and Iraqi insurgent leader.

Interaction with the DX Community and QSL Confirmations
Unusually for a military-linked broadcaster, CMF Radio One demonstrated a degree of openness toward the DX community.  In April 2005, Chief Warrant Officer Matthew Wilson of the U.S. Navy responded to listeners directly, thanking them for reception reports and soliciting further feedback on signal quality.  This correspondence confirmed active use at that time of 6125 kHz and 9133 kHz, with plans to return to 15500 kHz.

Several DXers received official QSL confirmations, including written replies from U.S. Naval Forces Central Command and the U.S. Fifth Fleet.  These confirmations, often signed by senior officers, conclusively established CMF Radio One as an official U.S. Navy operation rather than an ad hoc or clandestine broadcaster.

Historical Significance
Coalition Maritime Forces Radio One, which continued well into 2005, represented a rare modern example of ship-based shortwave broadcasting used for strategic communication rather than entertainment or public diplomacy alone.  It stands at the intersection of naval operations, intelligence gathering, psychological operations, and the long tradition of broadcasting from International Waters.  Its technical scale was modest, of course, and we could ask the questions, given the low power, odd choice of frequencies and use of single sideband – were they really serious about reaching an audience, and was anyone actually listening (besides a few DXers)?  But, the mere existence of this station does underscore how legacy technology such as shortwave radio can continue to play a role in twenty-first-century security operations – particularly in environments such as present-day Iran and North Korea, where internet and satellite communications cannot be assumed.

Back to you, Jeff.
(Ray Robinson/Jeff white/Wavescan