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)