Monday, February 16, 2026

Israeli Army Radio

 
Thank you to the Wavescan staff for a closer look at Israel's Galei Tzahal,, also known as Army Radio.

Jeff:  It was recently announced in Israel that the national network known as Galei Tzahal, or Army Radio, will be closed down in two weeks’ time, on Sunday March 1st.  So, what exactly is Israeli Army Radio, and what is its history?  Ray Robinson in Los Angeles has been investigating.

Ray: Thanks, Jeff.  Many countries have, or have had, radio stations set up to provide news and entertainment from home for military personnel while they are serving overseas; you can think of AFRTS, AFN in Germany, AFKN in Korea and AFVN in Vietnam, the British Forces Broadcasting Service (BFBS), the Canadian Forces Network (CFN), German Army Radio which operated in Finland and Norway, the Radio Forces Françaises de Berlin which operated in the French Sector of West Berlin, and so on.  But, Israeli Army Radio is not like any of those.

Ever since the Israeli Declaration of Independence in 1948, fixed-term military service has been compulsory for all Jewish men and women in Israel – currently two years eight months for men, and two years for women.  Arab citizens of Israel may also serve in the IDF (Israeli Defense Forces) on a voluntary basis.  So to a large extent, almost the entire population of the country either is or has been a part of the IDF, serving within Israel for the defense of the country.

On September 24, 1950, the IDF opened a station named Galei Tzahal, which literally translates as “IDF Waves” but it’s familiarly known in English as Army Radio.  Transmissions began with a trumpet blast at 6:30 p.m. followed by HaTikva, the Israeli national anthem.  An improvised studio had been set up inside a former school building in Ramat Gan, a suburb of Tel Aviv, with army blankets hung on the walls to muffle background noise.  It was the first competition for the government station, Kol Israel, and programs produced for soldiers which had previously been aired on Kol Israel were then transferred to the new station.

The first listing for Galei Tzahal in the World Radio Handbook is in the 1952 edition, which lists it then with three 250 watt medium wave transmitters on 1304, 1336 and 1390 kHz, and one 1 kW shortwave transmitter on the out-of-band frequency of 6725 kHz.  Broadcast hours were limited to 5:30-9:00 PM local time daily, with mostly informational and educational content for soldiers and immigrants, all in Hebrew.

The station's legal status was formalized in 1956 under Israel Broadcasting Authority legislation, which embedded it within the national media framework while preserving its IDF affiliation and operational independence from civilian oversight.

By the early 1960’s, Galei Tzahal, Army Radio, began expanding its reach, gradually attracting a wider civilian audience through modest increases in programming diversity, though it remained predominantly military-oriented until later decades.

In the 1970’s, Army Radio expanded their broadcast hours following the Yom Kippur war, and listener popularity surged as programming evolved to include extended news updates and cultural segments, positioning the station as a key alternative to the state-run Kol Israel.  Remember, there was no private independent broadcasting allowed in Israel at that time – Abie Nathan’s Voice of Peace started off the coast of Tel Aviv in 1973, and George Otis’ Voice of Hope started just north of the Lebanese border fence in ‘Free Lebanon’ in 1979, but apart from those, Army Radio was the only station in Israel not directly run by the government and having at least a modicum of editorial independence.

Army Radio subsequently grew into a nationwide radio network, broadcasting on both medium wave and shortwave, and later on FM.  It has been partially funded by the state, and partially by advertising – another differentiator between Israeli Army Radio and the forces stations of other countries.  It has been a full-service network, running 24-hour programming in Hebrew, encompassing news, current affairs, cultural discussions, and music.  

The 1990’s marked a pivotal diversification.  With the demise of Abie Nathan’s Voice of Peace in 1993 and the licensing of private commercial FM stations, Army Radio launched a second channel on October 31, 1993, Galgalatz, dedicated to 24-hour pop music, traffic reports, and casual programming aimed at the youth demographic, leaving the main channel to focus on its core news/talk format.  Galgalatz quickly became one of Israel's top-rated stations, and by decade's end, the station had solidified its dual-channel model, balancing its usefulness to the military with widespread civilian appeal amid Israel's media liberalization.  By 2024, Galgalatz commanded approximately 28 percent of daily listenership, underscoring its role as the nation's leading pop music outlet.

Many Israeli broadcasters first learnt their craft at Army Radio, which provided training in many media skills.  However, Army Radio’s military oversight has persistently sparked controversies, including accusations of left-leaning political bias, detachment from its soldier-oriented mandate, and undue influence on public opinion.  This has prompted governmental committees and legislative proposals in recent years to evaluate its structure.  At various times it was suggested that the network should be privatized, or at least separated from the IDF.

A reporter for Army Radio,  taken in 2019


Until December 2013, Army Radio broadcast 24 hours daily on 9235 and 15850 kHz shortwave to Europe, as well as on medium wave and FM.  The medium wave transmissions were ended in 2015, and since then, the two Army Radio channels have operated exclusively on FM networks within Israel.  However, in 2024 when the IDF were increasingly deployed in Gaza and along the northern borders with Lebanon and Syria, it was found there were many areas where the FM signals didn’t penetrate.  So, for the main Galei Tzahal channel, they went back to supplementing the FM network with powerful medium wave transmitters – on 945 kHz from Yavne south of Tel Aviv that gave good coverage throughout Gaza, and on 1287 kHz in the north that gave extended coverage along the length of the northern border.

However, in recent years, the ongoing controversies surrounding the station’s perceived editorial biases, often characterized as left-leaning or elitist, have fueled political pressures for change.  The parallels are very obvious with the way Federal funding in the USA has now been cut off from National Public Radio and of course, the Voice of America.

In December, Israeli Defense Minister Israel Katz asked the government to shut down the main Army Radio channel known as Galei Tzahal.  He framed the decision as a necessity for Israel’s security, saying that Army Radio was established by the Israeli government as a military station to serve as both a mouthpiece and an ear for IDF soldiers and their families — not as a platform for voicing opinions, many of which attack the IDF and the IDF soldiers themselves.  And that’s the crux of the matter.  It’s not really a financial issue – the station’s annual budget is only 
52 million shekels (US$14 million), and roughly 87% of that is funded by advertising and sponsorships.  So rather it’s about perceived editorial bias at what is tantamount to a public broadcaster, and the awkwardness of having young Army Radio reporters interviewing senior government and military officials, to whom they are subordinate.  The very existence of this station has been a paradox unique to Israel.

A few weeks ago in January, after a unanimous vote by the Israeli Cabinet, the Prime Minister’s office announced that the Defence Minister’s request had been approved.  There have been protests, petitions against the closure, and legal action from the Attorney General, but currently Israel Army Radio is still set to close by Sunday, March 1st.  Whether it will re-emerge as a private station or under some civilian oversight structure independent of the IDF remains to be seen.

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

USSR Radio History on the 'Woodpecker'

 


The Russian woodpecker that the whole world heard: how a Soviet antenna as tall as a 50-story building frightened the West and disappeared after Chernobyl.

Details: BC-DX 1644, 10 February 2026, Editor: Wolfgang Bueschel. Germany.

Audio available for Jen & GB's Valentine weekend specials

 


Did you miss the very special V-Day programming on February 14 or 15th? No problem! Program audio for listening and downloading is now available at the following links:

Sunday, February 15, 2026

Weekly Propagation Forecast Bulletins, February 16, 2026

 Product: Weekly Highlights and Forecasts
:Issued: 2026 Feb 16 0314 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 09 - 15 February 2026

Solar activity reached moderate levels on 09, 11, 12, and 13 Feb and was at low levels on 10, 14, and 15 Feb. Region 4366 (N14, L=203, class/area Fkc/950 on 09 Feb) continued to be the most prolific spot group, producing five out of the six M-class flares during the period. 

The largest flare was an M2.8 flare that occurred at 09/0227 UTC, followed by an M1.2 at 10/0009 UTC, an M1.1 at 11/0044 UTC, an M1.4 at 11/1312 UTC, and finally an M1.4 at 12/0240 UTC. Region 4373 (N09, L=110, class/area Hax/140 on 10 Feb) was the only other region to contribute to the M-flare activity, adding an M1.0/Sf flare at 13/0858 UTC. There were 35 C-class flares, with the largest being a C9.2/Sf at 09/2302 UTC from Region 4374. 

CME activity included a large filament (located near N15W25) that lifted off and disappeared from GONG H-alpha imagery at around 10/1910Z. Initial coronagraph imagery from LASCO C2 at 10/1948Z revealed the eruption likely coincided with a separate eruption from S22W80 (first visible in C2 at 10/1924Z). This event is thought to have passed near Earth late on 14 Feb, slightly enhancing the geomagnetic field. Additionally, a CME associated with the M1.0 on 13 Feb first became visible off the NW in LASCO C2 at 13/0924Z and first became visible in STEREO COR2 imagery at 13/0938Z. This event likely arrived at Earth on 15 Feb, possibly embedded in the CH HSS. 

No proton events were observed at geosynchronous orbit on 09-15 Feb.

The greater than 2 MeV electron flux at geosynchronous orbit was at high levels on 09, 10, 12, and 13 Feb, reaching a peak flux value of 1,764 pfu at 09/1500 UTC. Flux levels were at moderate levels on 11, 14, and 15 Feb. 

Geomagnetic field activity was at quiet to unsettled levels on 09 and 12 Feb, reached active levels on 10, 11, 13, and 14 Feb, and reached minor storm levels on 15 Feb. The elevated levels starting on 09 Feb and lasting through 14 Feb were likely associated with negative polarity coronal hole (CH) high speed stream (HSS) influences combined with intermittent transient effects. The increase in activity on 15 Feb is thought to be the result of a co-rotating interaction region ahead of a positive polarity CH HSS, possibly mixed with glancing effects from the CME that left the Sun
on 13 Feb. 

Forecast of Solar and Geomagnetic Activity 16 February - 14 March 2026

Solar activity is expected to continue at low levels, with a slight chance for M-class (R1-R2, Minor-Moderate) flares on 16-21 Feb. Activity is expected to increase to moderate levels with M-class (R1-R2, Minor-Moderate) flares expected and a chance for X-class (R3-Strong or greater) on 22 Feb through 07 Mar as Region 4366 returns to the visible disk. Activity should then decrease to low levels, with a chance for M-class (R1-R2, Minor-Moderate) flares on 08-09 Mar as Region 4366 transits the western limb. Low levels, with a chance for M-class flares, are expected to return on 10-14 Mar as old Region 4366 rotates to the far side once again. 

The greater than 10 MeV proton flux levels are likely to be below the S1 (Minor) level on 16-21 Feb and again on 08-14 Mar. There is a chance for the 10 MeV proton flux to reach S1-S2 (Minor-Moderate) storm levels from 22 Feb-07 Mar as old Region 4366 returns to the visible disk. 

The greater than 2 MeV electron flux at geosynchronous orbit is expected to be at high levels on 16 Feb through 03 Mar, 06-08 Mar, and 11-12 Mar as CH HSS influence sporadically continues. Moderate  levels are likely on 04-05, 09-10, and 13-14 Mar, outside of CH HSS influence. 

Geomagnetic field activity is expected to be at unsettled to active levels on 16-21 Feb, 24-25 Feb, 05-07 Mar, and 10 Mar due to recurrent negative polarity CH HSS effects. Active conditions are likely on 12 Mar following a solar sector boundary crossing, then again on 14 Mar with the onset of a positive polarity CH HSS. Barring the potential for CME activity, mostly quiet to unsettled levels are expected from 19-23 Feb, 26 Feb - 04 Mar, and 08, 09, 11, and 13 Mar. 

:Product: 27-day Space Weather Outlook Table 27DO.txt
:Issued: 2026 Feb 16 0314 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 2026-02-16
#
#   UTC      Radio Flux   Planetary   Largest
#  Date       10.7 cm      A Index    Kp Index
2026 Feb 16     115          20          5
2026 Feb 17     115          12          4
2026 Feb 18     110          10          3
2026 Feb 19     110           8          3
2026 Feb 20     110           5          2
2026 Feb 21     105           5          2
2026 Feb 22     120           5          2
2026 Feb 23     130           8          3
2026 Feb 24     135          20          5
2026 Feb 25     130          20          5
2026 Feb 26     130           8          3
2026 Feb 27     140           5          2
2026 Feb 28     160           5          2
2026 Mar 01     165           5          2
2026 Mar 02     170           5          2
2026 Mar 03     170           5          2
2026 Mar 04     170           5          2
2026 Mar 05     165          15          4
2026 Mar 06     165          15          4
2026 Mar 07     165           8          3
2026 Mar 08     145           5          2
2026 Mar 09     140           8          3
2026 Mar 10     130          18          5
2026 Mar 11     130           8          3
2026 Mar 12     120          12          3
2026 Mar 13     120           5          2
2026 Mar 14     120          20          5
(NOAA)

Friday, February 13, 2026

Special Valentine programming from Jen & GB's - February 14, 15

 


Don't miss the special Valentine programming from Jen & GB. 

Specials: Saturday February 14, 20:00-0000 UTC, and Sunday, February 15th, 1900-2200 UTC with Valtine Melodies

Plenty to hear from Jen's V-day show with Lovey Dovey/Diss the Diss Love can be messy. 
Programs will include all forms of musical persuasion. 

So Join us on our Unique live digital stream.

Plus, our live chat room is open for you at

Click on connect, then web chat, and insert the following:
For nick: name or like me radionutresss
Then next line channel, that's the following:
#eyeradiojd
And you are in the room !!

Enjoy Jen & GB's dipping into Cupids Arrow ... musically speaking.
Jen & GB
88's

February 13 programming from Sender Waldheim

 

Sender Waldheim is back on air with Digital Radio Mondiale (DRM) shortwave broadcasting on 6195 kHz. The transmissions are authorised for ITU Zones 27 and 28. The intended coverage area is Europe, around Germany. The authorisation is not programme-specific, allowing Sender Waldheim to relay a variety of programs and special broadcasts from different partners.
 
Broadcasts are scheduled at 09:00 and 15:00 UTC. Program relays will be repeated within this time window in various configurations, modes, and robustness settings.

6195 kHz 

Friday, 13 February 2026 – Special programme for UNESCO World Radio Day
(Mike Barroclough/BDXC)

More information on Sender Wallheim and those broadcasting on it at the link
(Mike Barroclough/BDXC)

Atlantic 2000 slated for Feb 14th broadcast

 


Atlantic 2000 will be on the air this Saturday, 14th of February from 0900 to 1000 UTC (1000 to 1100 CET) on 6070 and 9670 kHz via Channel 292.

Streams will be available simultaneously on our website.

Before that, you can listen to our 24/7 webstream or our podcasts on our website.
Good listening!

Visit our website and listen to Atlantic 2000, 24 hours a day: http://radioatlantic2000.free.fr   
And follow us on Mixcloud and YouTube 
(BDXC)

Thursday, February 12, 2026

Vatican Radio to celebrate World Radio Day on Feb 13

 

This World Radio Day, Vatican Radio celebrates 95 years with seven multilingual programs dedicated to the future of radio and the day's theme that 'AI is a tool, not a voice.'

On 13 February 2026, on the occasion of World Radio Day (WRD), Radio Vaticana – Vatican News promotes a special initiative in seven languages with seven radio programs that will become thematic podcasts dedicated to the future of radio, public service, innovation, and the relationship between media, society, and artificial intelligence.

The initiative comes the day after the 95th birthday of the Radio of the
Popes: 12 February 2026. Founded in 1931 at the behest of Pope Pius XI and created by the father of radio, Guglielmo Marconi, the Pope’s broadcaster represents one of the oldest radio experiences in the world, born to connect the Holy See with every part of the planet and to speak to people, cultures, and languages that are different.

At the heart of the programs will be the theme chosen for WRD 2026: “AI is a tool, not a voice”. A statement that becomes a starting point for reflection and dialogue also in light of the Message of the Holy Father for the World Day of Social Communications 2026, which recalls the value of human responsibility, discernment, and the authentic voice in communication in the age of artificial intelligence.

The seven programs will involve international experts, broadcasting executives, scholars, innovators, and professionals from the radio and media sector, called to reflect on how radio, a profoundly human medium, made of voice, relationship, and closeness, can inhabit the time of AI without losing its own identity.

Article continues here: 
(Mike Barraclough, UK/BDXC)

From the Isle of Music's February programming

 



From the Isle of Music, February 2026 

We are going to go "retro" this month and feature some lesser-known but excellent Cuban fusion and dance bands from the 1970s and 1980s. Some listeners who only know the North American narrative about Cuban music  will be surprised at what was being recorded, performed, and broadcast then.  

Friday, February 13, 2026,  3955 kHz, 1800 CET (1700 UTC), repeat 2300 CET (2200 UTC) 



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

Be advised that in January, our programs started several minutes late during the first transmission, but they did then air in full.  Hopefully that won't recur in February, but if it does, don't touch that dial!  
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. 



Wednesday, February 11, 2026

Encore classical music from Radio Tumbril

 

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 (Transmitter under repair - see above.)
03:00 - 04:00 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 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.

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 Feb by WRMI at 0200 UTC on 5850, and 2000 UTC on 15770 and then Channel 292 on SATURDAY 7th Feb at 11:00 UTC (and 0800 UTC) on 9670 kHz
Begins with some of a sonata by C P E Bach - one of J S Bach's sons - for Viola da Gamba, the piano trio by Ravel, and a three-voice Agnus Dei by Firminus Caron - Renaissance composer.
After that the Elegy for Horn and Piano written by Poulenc and dedicated to the horn player's horn player - Dennis Brain, and some of Mozart's concerto for flute and harp.
The program finishes with part of a late Beethoven string quartet.

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

Listening in to Radio Mali

 



A great feature on one of the few African stations to log and QSL ... Mali. Thank you to the staff of Wavescan.

Jeff: A few weeks ago, we received an email from Professor Dr. Hansjörg Biener in Nuremburg, Germany, who said:  “I would still like to extend my New Year's greetings to you and the team of Wavescan.  Maybe I can help start the new year with the following article which I hope proves to be a useful contribution to Wavescan.  So, here’s Ray Robinson in Los Angeles with Dr. Biener’s article.

Ray: Thanks, Jeff.  Dr. Biener writes:

Radio (Nationale du) Mali is one of the stations you could still listen to on shortwave to ring in the New Year.  But the original reason for this listening project was the second summit of the leaders of Burkina Faso, Mali, and Niger, scheduled for 22 and 23 December 2025, in Bamako, Mali.  Speeches in African French, or speeches with simultaneous translation, could indeed be heard during those days, but the reception quality (in Germany) and my French skills were insufficient for detailed comprehension.  The Alliance of Sahel States (Alliance des États du Sahel) was founded in 2023.  It emerged after military coups in the three states mentioned and relies on Russia as its international partner.  Among the most important outcomes of the summit were the establishment of a 5,000-strong military force for counter-terrorism, the founding of a joint bank, various infrastructure projects to connect the capital cities, and the introduction of a common passport and identity card.  But overall, there was only meager press release-style reporting on Radio Mali’s website, www.ortm.ml.

The traditional broadcast schedule remains in effect:


From 0600-0800 UTC on 5995 kHz there’s the morning program "Au Chant du Coq" (or in English, ‘At the Rooster’s Crow’).  These broadcasts on shortwave sometimes begin well before 0600, and sometimes considerably later.

Then at 0800 they switch to the 31 meter band and transmit
from 0800-1800 UTC on 9635 kHz.



Then for the evenings they switch back again to 49 meters, and from 1800-2400 UTC are heard on 5995 kHz, the same as in the early mornings.
  
In December 2025, reception (in Germany) on 5995 kHz was already so good in the early evening that one could enjoy the long, sometimes very complex, African music.  The morning program "Au Chant du Coq" could also be followed with a medium-quality reception.  The frequent crowing of a rooster was very unusual for urban European ears.  Apparently, one of the presenters once imitated it so well that a recording was also played several times.  Reception was possible on the daytime frequency of 9635 kHz up to two hours before the end of the broadcast, although it was affected by Chinese National Radio 17 on 9630 kHz.  There is also a weekly English-language segment, broadcast on Saturdays from approximately 1850–1905 UTC on 5995 kHz (which was heard on 13 December, but not on 20 December). 

Looking at the station’s website, www.ortm.ml, there are some current articles, but many outdated news items can also be seen.  This was noteworthy not only with regard to the AES summit, but also with regard to the African Football Championships, which were held from 21 December 2025 – 18 January 2026.  For a long time, nothing in the broadcasts sounded like football or football results.  This would be understandable if ORTM (the Office de Radio et Télévision du Mali) had broadcasting rights only for Mali's matches.  But then, on 3 January 2026, after the group stage, the round of 16 match between Mali and Tunisia at 1900 UTC was heard live on 5995 kHz, at least for a while, because reception was poor that evening.  

The game ended 3-2 for the underdog Mali, after extra time and a penalty shootout.  Mali wasn't the favourite team in the quarter-final on 9 January 2026 either.  They were then eliminated 0-1 by Senegal.  Reception of that match was possible on 9635 kHz.  However, the commentators, a man and a woman, could barely be heard over the shouting and occasional vuvuzela sounds.  The signal-to-noise ratio was poor for reasons other than those typically associated with shortwave radio, as the music during breaks in the broadcast was fine (so one would suspect a poor-quality audio feed from the outside broadcast).  During extra time, the frequency switchover time of 1800 UTC approached, but Radio Mali remained on the air on 9635 kHz, but not a moment longer than the final whistle blew, sealing Mali’s defeat.  On 5995 kHz, however, the first thing heard was classic rock (Go Your Own Way by Fleetwood Mac, and Sunday Bloody Sunday by U2), before snatches of West African balafon music became audible around 1812 UTC.


Live streams, which would allow verification of shortwave reception or research of the broadcast content in more detail, have been unavailable for some years.  Many years ago, before the TV rights were acquired by a pan-African pay-TV provider, the African Championships were also broadcast on ORTM's regular television stream with no geoblocking.

And, we thank Professor Dr. Hansjörg Biener in Nuremburg, Germany for that very interesting article.  Now, Jeff – you’re just back from your travels – how was the HFCC conference in Kuala Lumpur?
(Ray Robinson/NWS Wavescan)

Vatican Radio special programming on Feb. 12

 

On the anniversary of its inauguration, February 12, 2026, Vatican Radio – Vatican News is renewing one of the most recognizable elements of its identity: the sound ident that has always accompanied listeners of the Pope's station, a modern reworking of the original "Christus Vincit" theme.

The project includes four main idents, all based on the Christus Vincit theme, each designed to accompany a different moment of the radio
broadcast: one dedicated to waking up, one for the morning, one for the afternoon, and one for the night. Two short idents are also included: the first uses the theme's opening, the second uses its ending, creating an immediate and recognizable connection with the original sound identity.

The programming schedule will be as follows:
Christian G. (Nice, France/BDXC)

Texas Radio Shortwave programming, Feb 12, 15

 
(graphic by Gayle Van Horn)
All times UTC

February 12, 2026 - featuring The Music of Amanda Shires 
(requested by Alan Roe, United Kingdom)
2000-2100 3975 via Germany's Shortwave Radio to Europe

February 15, 2026 - featuring Michael Strah on Texas Radio Shortwave: The Music of Chris Whitley
1100-1200 6070 via Germany's Channel 292 to Europe
1200-1300 6070 via Germany's Channel 292 to Europe featuring Texas Radio Shortwave: Legends of Tejano Music

This schedule is subject to change based on propagation conditions, listener requests for specific Texas artists or music genres, and things beyond our control.

Texas Radio Shortwave is an independent producer of musical and topical shows, primarily focusing on Texas.

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

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 Shortwave's email is texasradioshortwave@protonmail.com.

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)

Monday, February 09, 2026

Audio available for Jen's Eclectic Views & Real Deal, February 8

 


Jen's Eclectic Views & Real Deal for February 8 on Unique Radio is now up and ready for YOUR listening and downloading. 

Weekly Propagation Forecast Bulletins

 :Product: Weekly Highlights and Forecasts
:Issued: 2026 Feb 09 0534 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC web contactt www.swpc.noaa.gov/content/subscription-services
#
#                Weekly Highlights and Forecasts
#
Highlights of Solar and Geomagnetic Activity 02 - 08 February 2026

Solar activity reached high levels on 02-04 Feb, moderate levels on 05 and 08 Feb, and low levels on 06-07 Feb. The flare activity was dominated by Region 4366 (N14, L=204, class/area Fkc/1100 on 03
Feb). This region produced 31 C-class flares, 38 M-class (R1/R2-Minor/Moderate), and four X-class (R3-Strong) flares. The X-class flares included: an X2.8 at 02/0036 UTC, an X1.6 at 02/0814
UTC, an X1.5 at 03/1408 UTC, and an X4.2 at 04/1213 UTC. Region 4366 also added four M-class flares that were greater than the M5 level.

These included: an M5.2 at 02/0251 UTC, an M6.7 at 02/1124 UTC, an M7.2/1n at 03/0701 UTC, and an M7.2 at 03/1456 UTC. The remaining 34 M-class flares produced by Region 4366 were at the R1/R2 levels,
ranging from M1.1 to M4.9. Surprisingly, very few radio emissions were observed in association with the increased flare activity.  There were only three F10.7 cm radio bursts recorded during the
week. The first was a burst of 140 sfu associated with the X1.5 flare at 03/1408 UTC, second was a 110 sfu burst that accompanied the M2.2 flare at 05/1934 UTC, and last, a 440 sfu burst that
coincided with the M2.7 flare at 08/1353 UTC. The only other radio signature of note was a Type II radio sweep that was detected by USAF observatories starting at about 02/0000 UTC, with an estimated
velocity of 955 km/s. No other radio signatures were noted. Other activity included a large, slow-moving filament eruption centered near N18W30 that began at 03/0400 UTC as seen in SUVI 304 imagery.

An associated CME was observed off the NW limb at 03/1836 UTC. There was another narrow eruption noted off the NE, first visible in SOHO/LASCO C2 imagery at 04/1426 UTC. This event was likely a
sympathetic eruption triggered by the X4.2, starting at approximately 04/1350 UTC near N15W22 between Regions 4366 and 4367 (N09, L=174, class/area Cao/50 on 03 Feb). There is a slight
potential of minor glancing blows from these eruptions early on 09 Feb. A coronal mass ejection was observed off the south/southwest limb in SOHO/LASCO C2 imagery at 05/1548 UTC. The source is likely
associated with an M1.8/1N flare from Region 4362 (S17, L=207,  class/area Dao/50 on 07 Feb) that peaked at 05/1513 UTC. Surface signatures in SUVI 284 imagery showed a faint southerly deflected
EUV wave. Model output suggests a glancing effect late on 08 Feb to early on 09 Feb. 

No proton events were observed at geosynchronous orbit on 02-08 Feb.

The greater than 2 MeV electron flux at geosynchronous orbit reached high levels on 02, 03, 04, and 08 Feb, with a peak flux value of 13,970 pfu at 04/1605 UTC. 

Geomagnetic field activity reached G1 (Minor) storm levels on 05 Feb following the arrival of a CME from an X8.1 flare that originated from Region 4366 at 01/2357 UTC. Conditions were at quiet to
unsettled levels on 02-03 Feb and for the first half of 04 Feb before increasing to active levels following the onset of a negative polarity coronal hole (CH) high speed stream (HSS). Quiet to active
conditions were observed on 06-07 Feb with combined influence from a negative polarity CH HSS and a possible passing transient. Quiet to unsettled levels returned by 08 Feb as -CH HSS effects lingered. 

Forecast of Solar and Geomagnetic Activity 09 February - 07 March 2026

Solar activity is expected to continue at moderate levels with further M-class (R1-R2, Minor-Moderate) flares expected and a chance for X-class (R3-Strong or greater) on 09-10 Feb as Region 4366
transits the western limb. Low levels, with a chance for M-class flares, are expected on 11-22 Feb. An increase to moderate to high levels is once again likely on 23-28 Feb as Region 4366 returns to
the visible disk. Conditions should again return to low to moderate levels on 01-07 Mar as old Region 4366 rotates to the far side once again. 

There is a chance for the 10 MeV proton flux to reach S1-S2 (Minor-Moderate) storm levels through 12 Feb as Region 4366 transits the visible disk and beyond. Levels are likely to be below the S1
(Minor) level on 12-22 Feb. An increase to above the S1 (Minor) storm levels 23-28 Feb is possible as Region 4366 returns to the visible disk. Chances decrease on 01-07 Mar as old Region 4366
rotates to the far side once again. 

The greater than 2 MeV electron flux at geosynchronous orbit is expected to be at high levels on 09-10 Feb, 16-21 Feb, 24-25 Feb, and 05-07 Mar as CH HSS influence sporadically continue. 

Geomagnetic field activity is expected to be at unsettled to active levels on 09-10 Feb as CH HSS influence decreases. Barring the potential for CME activity, mostly quiet to unsettled levels are
expected from 11-15 Feb, 22-23 Feb, and 26 Feb - 04 Mar. Unsettled to active levels are likely on 16-21 Feb, 24-25 Feb, and 05-07 Mar due to recurrent negative polarity CH HSS effects. 

Product: 27-day Space Weather Outlook Table 27DO.txt
:Issued: 2026 Feb 09 0534 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 2026-02-09
#
#   UTC      Radio Flux   Planetary   Largest
#  Date       10.7 cm      A Index    Kp Index
2026 Feb 09     165          15          4
2026 Feb 10     160           8          3
2026 Feb 11     155           5          2
2026 Feb 12     150           5          2
2026 Feb 13     145           5          2
2026 Feb 14     140           5          2
2026 Feb 15     150           5          2
2026 Feb 16     160          15          4
2026 Feb 17     170          15          4
2026 Feb 18     180          15          4
2026 Feb 19     175          15          4
2026 Feb 20     170          15          4
2026 Feb 21     160          15          4
2026 Feb 22     150           8          3
2026 Feb 23     140           8          3
2026 Feb 24     135          20          5
2026 Feb 25     130          20          5
2026 Feb 26     130           8          3
2026 Feb 27     140           5          2
2026 Feb 28     160           5          2
2026 Mar 01     165           5          2
2026 Mar 02     170           5          2
2026 Mar 03     170           5          2
2026 Mar 04     170           5          2
2026 Mar 05     165          15          4
2026 Mar 06     165          15          4
2026 Mar 07     165           8          3
(NOAA)

Friday, February 06, 2026

SWL Digest 2025 podcast, now vailable

 

If you’ve been a shortwave listener for a long time, you probably remember Ian McFarland’s popular SWL Digest program on Radio Canada International. Well, I’m happy to report that Ian is alive and well and living on the west coast of Canada, where he has recently released a series of podcasts called SWL Digest 2025, produced in cooperation with well-known DXer Colin Newell and available on Colin’s website, DXer.ca. 


On episode 1 of SWL Digest 2025, the program returns to its roots with an introductory walk down memory lane with Ian, Colin and Bob Zanotti, formerly of Swiss Radio International’s Two Bobs DX program. In episode 2, the journey continues with Ian McFarland and Larry Magne of Passport to World Band Radio. And on episode 3, the dialogue carries on with Ian, Bob, and Larry speaking with Colin Newell. 

I’m also happy to report that the first three editions of the new SWL Digest will be re-aired on WRMI shortwave on Tuesday, Wednesday, and Thursday, February 10, 11, and 12. Those are UTC days, and the times for those broadcasts on each of those days will be 0300 UTC on 9455 kHz, 0400 UTC on 5950 kHz, and 0500 UTC on 5850 kHz.

Jeff White, General Manager
WRMI Radio Miami International
10400 NW 240th Street
Okeechobee, Florida 34972 USA

Sunny Jim's Trance Journey update

 


It's 'Multiple Choice' day this Saturday, Feb. 7th,

with four opportunities to hear our latest program
 
RealMix Radio - 6005kHz - 11:00 UTC + 17:00 UTC
 
Channel292 - 9670kHz - 09:00 UTC + 14:00 UTC
 
Not sure if the ionosphere is going to be able to handle all this good new music - prepare for multiple solar flares & a spectacular aurora borealis at the above times...
(Jim Salmon/BDXC)

Texas Radio Shortwave, Feb. 7-8 programming

 

All times UTC

February 7, 2026 - featuring Texas Music Mix # 1
1500-1600  6160 via Germany's Shortwave Radio to Europe
1900-2000 3975 via Germany's Shortwave Radio to Europe

February 8 - featuring Texas Music Mix # 1
1300-1400 9670 via Germany's Channel 292 to Europe
2300-0000 9670 via Germany's Channel 292 to North America

This schedule is subject to change based on propagation conditions, listener requests for specific Texas artists or music genres, and things beyond our control.

Texas Radio Shortwave is an independent producer of musical and topical shows, usually about Texas.

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

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 Shortwave's email is texasradioshortwave@protonmail.com.

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)

Jen & GB's CARN audio available from Jan 31

 


For the HF Enthusiast in you, Jen & GB's CARN for Saturday, January 31 is up and ready for you


January 31, 2026 - CARN Show Link.


Short Link.


For your contact pleasure


The Bands Are Alive !!

73's & 33's
Jen & GB