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