Monday, March 02, 2026

Coalition Maritime Forces – Radio One

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



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

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

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

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

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

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

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

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

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

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

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

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

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


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

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

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

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

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

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

CARN audio available for download

 

CARN audio available for download

In case you missed Sunday's program, Jen's Eclectic Views & Real Deal is up and ready for listening and downloading. 

Here's this week's Cast of Eclectic & Real Deal.


Short Link.


For your contact pleasure

Jen In The Rad.

Weekly Propagation Forecast Bulletins, March 2, 2026

 :Product: Weekly Highlights and Forecasts
:Issued: 2026 Mar 02 0144 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 23 February - 01 March 2026

Solar activity was reached moderate after an M2.3 flare at 25/1154 UTC from Region 4379 (S17, L=205, class/area=Bxo/050 on 26 Feb). A Type II radio sweep was also observed on 25 Feb, associated with a 5-degree filament eruption near S08W27 and a C2.6 flare at 25/0656 UTC. Modeling of the ejecta from the event suggested possible glancing influence at Earth on 28 Feb - 01 Mar. For the remainder of  the week, activity was observed between low and very low levels. 

No proton events were observed at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit was primarily at high levels through the past seven days. 

Geomagnetic field activity was reached G1 (Minor) geomagnetic storm levels on 23 Feb during the onset of a negative polarity CH HSS. Solar wind speeds increased from ~450 km/s to ~700 km/s. Total
magnetic field strength peaked around 7 nT, then fell to at or below 5 nT for the remainder of the outlook period. Active conditions were observed over 24-26 Feb and finally to unsettled levels over 27 Feb - 01 Mar as solar wind speeds from the coronal hole gradually waned. 

Forecast of Solar and Geomagnetic Activity 02 March - 28 March 2026

Solar activity is expected to be at low levels, with a change 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 on the visible disk as well as the potential from regions that are expected to return from the Sun's farside. 

No proton events are expected at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit is expected to reach high levels on 02-08 Mar, 11-12 Mar, 15-19 Mar, and 21-28 Mar due to anticipated influence from multiple, recurrent,
CH HSSs. The remainder of the outlook period is likely to be at
normal to moderate levels. 

Geomagnetic field activity is expected to range from quiet to G2 (Moderate) geomagnetic storm levels. G2 conditions are likely on 21 Mar; G1 (Minor) conditions are likely on 22 Mar; active conditions
are likely on 03 Mar, 10 Mar, 12 Mar, 14-15 Mar, 20 Mar, and 23-25 Mar; unsettled conditions are likely on 02 Mar, 04 Mar, 06 Mar, 08-09 Mar, 11 Mar, 13 Mar, 16-19 Mar, and 26-28 Mar. 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 02 0144 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 2026-03-02
#
#   UTC      Radio Flux   Planetary   Largest
#  Date       10.7 cm      A Index    Kp Index
2026 Mar 02     150          10          3
2026 Mar 03     150          12          4
2026 Mar 04     150           8          3
2026 Mar 05     155           5          2
2026 Mar 06     158           8          3
2026 Mar 07     156           5          2
2026 Mar 08     156           8          3
2026 Mar 09     150          10          3
2026 Mar 10     145          18          4
2026 Mar 11     140          10          3
2026 Mar 12     135          15          4
2026 Mar 13     128          10          3
2026 Mar 14     125          15          4
2026 Mar 15     120          15          4
2026 Mar 16     118          10          3
2026 Mar 17     115          10          3
2026 Mar 18     120          10          3
2026 Mar 19     120          12          3
2026 Mar 20     120          15          4
2026 Mar 21     122          35          6
2026 Mar 22     122          24          5
2026 Mar 23     125          15          4
2026 Mar 24     128          15          4
2026 Mar 25     128          18          4
2026 Mar 26     130          10          3
2026 Mar 27     135           8          3
2026 Mar 28     140           8          3
(NOAA)

Sunday, March 01, 2026

QSL Report 2.0-March 2026

 


                                  Bringing you the latest in QSLing from across the globe

Welcome to the March 2026 edition of QSL Report 2.0!  Thank you for your comments and contributions.

QSL Report 2.0 is a revival of my former QSL Report column in Monitoring Times magazine. Each issue brings you updates on QSLing trends—what worked (and what didn’t), along with special event QSLs and stations verified across amateur radio, mediumwave, pirate, shortwave, and utility bands. If you’ve received a QSL from any of these stations, share your results with the world!

Send your contributions to w4gvhla@gmail.com

Euro-Free Radio
Enterprise Radio, 6925 kHz. Full data e-QSL in one day for e-report to enterpriseradio@hotmail.com (Carlos Alberto Erdman, Brazil/FB QSL)

Radio Batavia, 6300 kHz. No-data email response in two hours, for e-report to radiobatavia@hotmail.com (Hashimoto Kenji, Japan/FB DX Fanzine).


Radio Cuckoo (Ireland) 6280 kHz. Full data QSL card by postal mail, for e-report to radiocuckoo@yahoo.com (Juan Carlos Pérez Montero, Spain/FB QSL)

Radio Jupiter, 1287 kHz. Pepared QSL returned as verified in three, for postal report to: Lindenlaan 71, 7975 AG Uffelte, Netherlands (van der Galien).

Radio Kleine Cowboy, 1539 kHz. Prepared QSL card returned as verified in 19 days for postal report to: GW VD Meulen, Rustenburgsweg 60, 

096 AC Olderbroek, Netherlands (Jouk van der Galien, Netherlands/BDXC). 

Radio Luka, 1920 kHz. Full data e-QSL in 39 days for e-report to radioluka@gmail.com (J?gen Waga, Germany/BDXC).

Radio Matrix, 1548 kHz. Partial data e-mail response with no-data QSL in 20 days, for e-report to radiostationmatrix@hotmail.com (Waga).

Radio Vonkentrekker, 1611 kHz. Prepared QSL card returned as verified in 16 days, for postal report to: Dordseddijk 475, 7891 NR Klazienaveen, Netherlands. (van der Galien).

Taxus Radio, 6290 kHz. Prepared QSL card returned as verified in 21 days, for postal report to: p/a Broekweg 23a, 7891RP Klazienaveen, Netherlands (van er Galien).

Mediumwave
Brazil
Radio 9 de Julho, 1600 kHz. No-data email response in a few days, for e-report to comercial@radio9dejulho,com.br (Jari Lehtinen, Finland/FB QSL)


Radio Terra, 760 kHz. Full data e-verification letter in 12 hours from Michele Oliveira Santos-Gerente, administrative, for e-report to michele@radioterraam.com.br (Ariel Osvaldo Torres, Argentina/DX Fanzine).

France
TWR Europe via Roumules 1467 kHz. Full data QSL, station sticker, and info sheet from Kalman Dobos, received via postal mail. E-report to kdobos@twr.org (Torres).

Paraguay
ZPI Radio Nacional de Paraguay 920 kHz. Partial data e-mail in 15 minutes from Carmen Beatriz Insurralde, Directora, for e-report to cinsaurralde@mitic.gov.py (Fischetto).

Shortwave

Armenia
Radio Andorra relay via Gavar, 7540. Full data e-QSL from Jean-Marc Printz, within the day, from second e-report follow-up reminder to printz@aquiradioandorra.com (Néstor Damián Fischetto, Argentina/DX Fanzine).

SM Dessau relay via Gavar, 12060. Full data e-QSL in a few hours, for e-report to maxberger@smradio-dessau.de (Waga).


Australia
TWR Asia via Kununurra, 11965 kHz. Full data e-QSL in 40 days for e-report to asiafeedback@twr.org (Christian Ghibaudo, France/BDXC).

Brazil
Rádio Nacional da Amazônia, 11780 kHz. Full data e-QSL in one day for e-reports to: centraloouvinite@ebc.com.br  ouvidoria@ebc.com (Dmitrij Zhavoronkov, Russia/FB QSL).

Germany
All Tribes Radio via Rohrbach Waal, 9670 kHz. Full data e-QSL in two days for e-report to alltribesradio@icloud.com (Waga).

India


Akashvani via Bengaluru, 15410 kHz. Full data QSL  card by postal mail in 32 days, for e-report to spectrum-manager@prasarbharati.gov.in (Waga).

Clandestine
Radio Dabanga 11640 kHz. Full data e-QSL in two days from Jared Wedge-Thomas, for e-report and MP3 audio file to info@dabangasudan.org (Roberto Taberna Torino, Italy/DX Fanzine).

Radio Zaman Bidari 9705 kHz via Issoudun, France. Full data e-QSL in five days for e-report to radiozamanbidari@proton.me (Jonathan Bailey, IL).

Colombia
La Voz de tu Conciencia 6010 kHz. Full data e-QSL and antenna photos in six hours from Rafael Rodriguez, QSL Manager at rafaelcoldx@yahoo.com (Rod Pearson, FL). 

Finland
RealMix Radio 6195 kHz. Full data color QSL in 50 days from Joakim Veckstrom, Station Director, for e-report to realmix,sw@gmail.com (Pearson).

Germany
Atlantic 2000 International, 9670 kHz via Channel 292, Rohrbach. Full data e-QSL in seven days for e-report to atlantic2000international@gmail.com (Ian Wilkenson, UK)/BDXC)

Jake FM, 9670 via Channel 292. Full data e-QSL in one hour for e-report to qsl@jake-fm.de (Pearson).



Pop Shop Radio, 3955/9670 kHz via Channel 292, Rohrback. Full data e-QSL received in two days for e-report to radiopopshop@gmail.com (Pearson).

Sunny Jim’s Trance Journey, 9670 kHz via Channel 292. Full data e-QSL in two days, for e-report to sitjradio@gmail.com (Bailey).

Luxembourg
Radio Nova International via Junglinster, 9530 kHz. Full data e-QSL in three days, for e-report to qslnova@gmail.com (Ghibaudo). 

Netherlands
SuperClan Radio via Putten, 5955 kHz. Full data e-QSL in 11 days for e-report to superclanradio@yahoo.com (Waga).

Romania
Radio Romania International, 11650 kHz. Full data e-QSL in 75 days for e-report to span@rri.ro (Sam Wright, MS).

South Korea
KBS World Radio 9740 kHz. Full data e-QSL in 36 days, for e-report to spanish@kbs.co.kr (Montero) 

United Arab Emirates
Gaweylon Tibetan Radio via Dhabbayah 15215 kHz. Full data e-QSL in one day from Anil R. Alfred, Director. E-report to gaweylon@gmail.com (Montero).

Uzbekistan
BVB Bible Voice Broadcasting, 9730 kHz. Full data e-QSL in 25 days, for e-report to mail@bvbroadcasting.org (Van Horn).

Vatican
Vatican Radio, 9710 kHz. Full data e-QSL in 100 days, for e-report to qsl.request@spc.va (Pearson).


Saturday, February 28, 2026

Calling All Radio Nutz, February 28th edition

 

It's time for the February edition of CARN; this time it's GB's mediumwave roundup plus GB's 40m antenna experiment. 

In addition to the usual DX tips and diary dates, we have our usual taped series for you, this time in a chunked-up format from David H, ORF Morse course, foreign language recognition course with Dr. Richard E Wood, and finally, radio waves and the ionosphere. Plus, last but not least, live tuning with Jen in CO and GB in Swinging England.

The bands are alive !!

19:00 - 22:00 UTC - Saturday, February 28, 2026

Live Stream. 

For your contact pleasure

Hope you can join us 

73s & Good DX for the end of Winter !!
From Jen & GB.

Blog Logs-March 2026

 


Welcome to the March 2026 issue of Blog Logs. Thank you for your emails, logging contributions and following my latest daily tweets on X at: Shortwave Central (Gayle Van Horn W4GVH@QSLRptMT

Have you subscribed to the Shortwave Central YouTube channel? You will find a vast selection 
of videos and audio airchecks, and the Playlist is growing! Join your fellow radio enthusiasts at: https://www.youtube.com/c/ShortwaveCentral 

The Shortwave Central blog brings you the latest from the ever-changing realm of radio. Additional radio information is covered in my Bits & Bytes monthly column in The Spectrum Monitor e-zine at: https://www.thespectrummonitor.com/ 

Languages as indicated
// denotes station heard on a parallel frequency
*Sign-on Sign-Off*/ frequencies in kHz
Monitoring  January 1-27, 2026   

UTC, frequencies kHz 

Mediumwave
Argentina
540, Radio Nacional, Sante Fe at 0418. Popular Argentine songs with the announcer’s commentary during the external period. (Rudolf Grimm, Brazil).
680, Radio AM680, Rosario. Spanish heard at 0426. Musical sequence with a similar format to Radio Nacional. No signal observed from Radio Copacabana/Rede Aleluia, Rio de Janeiro 680 kHz. (Grimm).

Brazil
1080, Rádio de Universidad Federal do Rio Grande do Sul, Porto Alegre. Monitored 0051-0100 with classical music on piano/guitar. Station ID. S-7 signal. (Grimm).


Bulgaria
576, 2159-2203 (270 kW). BNR Horizont Bulgarian music to the lady’s station ID, time tips, national anthem into announcer’s additional ID and national newscast. YT Video https://youtu.be/AfUiR63dX8Y (Van Horn).

Clandestine 
864, Radio Iran Azad 1655-1710. Persian programming, including a male’s text about Iran. Instrumental piano music to station ID, contact info and items on the internet. Fanfare introduces a news format. (Kiwi RU SDR) YT video https://youtu.be/Zc1R3AXQZW4 (Van Horn).


Hungary
540, Kossuth Rádió. 2000 kW. Evening broadcast in Hungarian with national news items, station info and website quote to 2130.* YT video at: https://youtu.be/Yc4rfuKMT68

Paraguay
730, ABC Cardinal, Asunción. Spanish police news about traffic incidents in Asunción, including the passing of a Brazilian citizen in one of the accidents. (Grimm).

Spain
9690, Radio Exterior de España, Noblejas. Spanish programming to North America 2341-2347. Commentary on cinema, films, Almodovar, and film history. Additional audio excerpts of dialogue from certain films. S-5 signal (Grimm).


United Kingdom
693, BBC Radio Five Live, 2150-2205-Bexhill-on-Sea. BBC Sports with the 2026 Olympic event results. YT video at: https://youtu.be/nNXN0IwlbHk (Van Horn).

1026, BBC Radio Jersey - 2200-2210, Trinity. Evening news and promos to music program for the 1 kW station, scheduled to close on 31 March 2026. YT video available at: 

1116, BBC Guernsey-BBC Radio 5 Live 2045-2105, Saint Peter Port. Full station ID into national and world news. Local time check and Guernsey promo. YT video available at: https://youtu.be/2fnPljuBwZQ (Van Horn).

Uruguay
1430, Radio Durazno in Spanish. Noted at 0448 with rhythmic music, suitable for dancing. Chat from announcer and mentions of “Durazno.” S-5 signal (Grimm).

Shortwave
Algeria
13855 Ifrikya FM, Ourgla 1938-2004. Arabic service for regional music. French comments and news // 13640. SINPO 25422; 17600 – 0709-0744 with French programming  (Manuel Mendez, Spain/BDXC).


Australia
17650, Reach Beyond, Kununurra. Japanese service to Japan 2227-2236. Possible interval signal to “This is Reach Beyond Australia,” to station comments. S-7 signal. (Grimm).

Bolivia
3310, Radio Mosoj Chaski, Cotapachi 0015-0045. Fair signal Quechua religious text programming. SINPO 24333 (Rod Pearson, FL).

Brazil (Portuguese)
6180, Rádio Nacional da Amazônia, Brasília 2047-2116.Announcer’s talk and intro to  Brazilian music and comments // 11780. SINPO 25422 (Méndez).
9818.5 Rádio 9 de Julho São Paulo, 0652-0727. Religious programming and songs. SINPO 35433 (Méndez).
11780, Rádio da Amazônia,  Brasília 2038-2111. Brazilian songs and comments, followed by “Sintonia da Nacional musical Brasileira.” SINPO 35433 (Méndez).

Bulgaria
6005, Radio Taiwan International, Kostinbrod 1921-1930.* French comments to the male announcer’s “Radio Taiwan International.: SINPO 35433 (Méndez).


Canada
6070 CFRX Toronto 0802-0816. English newscast and comments. SINPO 13421 (Méndez).

China
5925, CNR-5 Cross-Strait Radio, Beijing. Mandarin service to Taiwan 2059-2104. Announcer’s talk to text. Additional station from China noted as: 7210 PBS Yunna via Kunming-in Lahu to China. Monitored as 0102-0108; 7225 PBS Sichuan 2 via Chengdu in Tibetan to China at 0109-0114. (Grimm).

9665, CNR-5 Cross Strait Radio, Beijing, in Chinese to Southern China and Taiwan. Monitored 2332-2340 with announcer’s talk and typical rhythmic music. S-4 signal, no signal from 9665 kHz from Tadio Voz Missionaria (Grimm).

Colombia
6010, La Voz de tu Conciencia, Puerto Lleras 050-0105. Spanish religious program to vocal hymn for a fair signal. SINPO 23333 (Pearson). 


Cuba
11760, Radio Habana Cuba 1615-1735.* Station IDs and promotional. Spanish national news, // 11880 // 15140 kHz. Sam Wright, MS). Cuba’s Radio Rebelde, Bauta 0542-0633. Spanish news and comments about Cuba. Station ID “Radio Rebelde,” “Portada Rebelde,” Cuban music to program “Nosotros. SINPO 35333 (Méndez).

Ethiopia
6030, Radio Oromiya, Addis Ababa 1811-1827. African vernacular service covering comments. SINPO 15422 (Méndez). 6110 Radio Fana, Addis Ababa 1816-1829 in Vernacular text and East African music. SINPO 25422. (Méndez).

Guam
15400, Adventist World Radio via Agat in Karen service. Programming targeted to Southeast Asia and Myanmar. Monitored 1438-1444 with music and a Christian message. 15505, AWR in China to Southeast Asia 1420-1428. Christian message to music and 1428.* (Grimm). (Grimm).


India
15280, AIR Akashvani External Service via Bangalore in Chinese 0043-0049. Announcer’s talk with background music, continuous instrumental pop music. S-7 (Grimm).

Kuwait
5860, Radio Farda via Kuwait City in Persian to Iran 2042-2050. Conversations from two male announcer’s, including an interview. S-4 signal (Grimm).

Madagascar
11610, MWV The Light of Life via Mahajanga. Mandarin programming to Europe, 2125-2131. Conversations, possibly a religious sermon. Beautiful Mandarin music. S-6 signal (Grimm).


Mali
5995, Radio Mali/ORT via Bamako. 1900-1915. French ID to new script. African pop/rap to African vernacular text and announcer’s comments (Pearson).

Mexico
6185 Radio Educacóon. 0600-0735. Cultural programming includes various classical selections. Station ID and promos. (Pearson).

Netherlands
6130, Radio Europe 1740-1750. English DJ format with U.S./Euro techno-pop vocals. (Ben Clement, TX)


North Korea
9650, Voice of Korea, Kujang in Japanese; 2131-2137. Orchestral music to talk and announcements (Grimm).

Peru
4775, Radio Tarma 0030-0045. Spanish ID, text and comments. Better signal quality than previous attemps (Wright).

4810, Radio Logos, Chazta. Spanish to Peru 0128-0135 with commentaries from the announcer. QRM from utility station (Grimm).
4820, Radio Sena Cristiana, Cotahuasi, Arequipa in Spanish. Noted 1Kw by WRTH at 0004-0022 to Christian message and hymns. (Grimm).

United States
15380 Radio Marti. 1805 tune in to stations promotional ID. News and commentary on Cuba. Excellent signal. (Van Horn/Airspy LA).

Friday, February 27, 2026

U.K. Propagation Update

 

RSGB
RadCom Assistant Editor | February 27, 2026
We have just had a period of zero sunspots – the first time since June 2022. However, don’t worry. This may be a sign of things to come, but this zero-spot period was short-lived.
There are now signs of sunspots appearing over the Sun’s eastern limb with old region 4366, last seen on 11 February, making its return. It is now renamed Active Region 4378.
This is helping to boost the solar flux index, which stood at 125 on Thursday, 26 February. This is a long way off the usual solar flux index lows we experience at sunspot minimum when it can be as low as 66-70.

As we are now entering March and, with the hours of daylight increasing, we are seeing a change in HF propagation. The Spring equinox is a time for good north-south propagation, especially on the higher HF bands, although we may see the 10m band tailing off a little as we head towards summer.
For the best overall DX HF propagation, head to 21MHz or higher where you may get maximum global coverage.

Propagation has been reasonable, but a high-speed solar wind stream from a coronal hole pushed the Kp index to 4 for long periods. This has not helped HF propagation, although its effects are not as bad as a Kp index of 6 or higher.
DXpeditions to be worked this week include Bouvet Island, 3Y0K; Guinea Bissau, J51A and the final days of Desecheo Island, KP5/NP3VI, which is due to end around 3 March.
Lubo, OM5ZW and Laco, OM4WM, will also be active from Thulusdhoo Island in the Maldives as 8Q7ZW until 12 March.
Next week, the Space Weather Prediction Center predicts that the solar flux index will remain in the 120 to 130 range.

The solar wind model predicts that a cloud of plasma may hit Earth today, 1 March, so watch out for an increased Kp index. Otherwise, the first half of the coming week may be quiet, geomagnetically. However, the Kp index is predicted to rise to 4 on 5-6 March.
 VHF and up propagation news from G3YLA and G4BAO:
The early part of last week saw brief 50MHz FT8 spots of the J51A DXpedition to Guinea-Bissau in the southern part of the UK. As with TZ1CE last week, stations much further south benefited from the best propagation.

As of 26 February, Clublog showed no UK stations in its log yet. Earlier in the week the station was an easy catch using FT8 on all the lower bands.
The current spell of very unsettled weather will last into the early part of the coming week. Thereafter, it seems likely that high pressure will start to build over the country, possibly with another weak front after mid-week. This may soon be followed by another high before the end of the week.
In terms of radio propagation, although some further rain scatter is probable at first, as we head into the coming week, there is every chance of tropo becoming a mode of choice.

It’s important to remember that not all highs are equal and, although they all tend to produce a strong temperature inversion, they may not be good for tropo if the air near the surface is too dry.
Ideally, we need to see some misty low cloud or early morning fog trapped under the inversion for the better-quality lifts. This is because a change in moisture across the top of the inversion produces the biggest change to the refractive index.

Other modes to consider, though not too seriously, are aurora after the recent coronal hole stream. The indication you are looking for is a high value Kp index, say 5 or greater, up to the maximum of 9.
With meteor scatter, we are in a long gap in shower activity until the Lyrids in late April so relying on random meteor activity is the best we can expect.

The prospects for Sporadic-E are not necessarily zero but are unlikely to be too exciting in this part of the year. The main summer season is normally considered to run from late April to mid-September. In the interim, the occasional burst of activity is possible but probably limited to the 10 or 6m bands.
For EME, Moon declination has started to fall again, going negative on Wednesday, 4 March. This means shortening Moon windows and lower peak elevation. Path losses are rising again after perigee. 144MHz sky noise is low throughout the coming week.
And that’s all from the propagation team this week.
(Mike Terry/BDXC)

Monday, February 23, 2026

Three Perth Stations Shift to FM-Last Day of Service Videos

 



You heard about it from Jeff White on the February 22 episode of Wavescan - Perth Australian mediumwave stations shifting to FM.

The #Last Day of Service of February 23, 2026 - videos for the three Perth stations are available at the Shortwave Central YouTube channel at: https://www.youtube.com/c/ShortwaveCentral. 

Don't forget to subscribe to the channel. Stay tuned... as more videos are in YOUR future. 

Videos:
ABC Radio National https://youtu.be/EjWsfYm0NCs

Weekly Propagation Forecast Bulletin, February 23, 2026

 

Weekly Propagation Forecast Bulletin, February 23, 2026

Product: Weekly Highlights and Forecasts
:Issued: 2026 Feb 23 0204 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 16 - 22 February 2026

Solar activity ranged from very low to moderate levels. The largest event was an M2.5 flare (R1-Minor) at 16/0435 UTC from a location beyond the east limb. A Type II radio sweep (est. 310 km/s) was observed on 18 Feb and associated with a large eruption just beyond the southeast limb. Only low-levels C-class activity was observed over 17-23 Feb. The sun ended the summary period free of sunspots on the visible disk for the first time since 2022. 

No proton events were observed at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit reached high levels over 16-20 Feb following sustained higher wind speeds from a positive polarity coronal hole. Normal to moderate levels were observed over 21-22 Feb. 

Geomagnetic field activity reached a peak of G2 (Moderate) levels on 16 Feb due to influence from a positive polarity CH HSS. Quiet to unsettled levels were observed over 17-19 Feb. Active levels over 20-21 Feb were likely associated with transient passage. By 22 Feb,a CIR ahead of a negative polarity CH HSS increased geomagnetic conditions up to G1 (Minor) geomagnetic storm levels. Wind speeds were observed between 600-700 km/s on 22 Feb as the high speed stream set in. 

Forecast of Solar and Geomagnetic Activity 23 February - 21 March 2026

Solar activity is expected to be at very low, with a good change for C-class flares and a slight change for M-class flare (R1/R2-Minor/Moderate) throughout the outlook period. 

No proton events are expected at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit is expected to reach high levels on 23 Feb - 03 Mar, 06-08 Mar, 11-12 Mar, 15-19 Mar, and 21 Mar due to anticipated influence of multiple recurrent coronal holes. The remainder of the outlook period is likely to be at normal to moderate levels. 

Geomagnetic field activity is expected to reach G2 (Moderate) levels on 21 Mar.;G1 (Minor) geomagnetic storm levels are likely on 23 Feb, 10 Mar, 14 Mar, and 20 Mar; active levels are likely on 24 Feb, 05-06 Mar, 12-13 Mar, 15-16 Mar, and 19 Mar; unsettled levels are likely over 25 Feb, 07 Mar, 09 Mar, 11 Mar, and 17-18 Mar. All increases in geomagnetic activity are anticipated due to expected influence from multiple, recurrent coronal hole 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 Feb 23 0204 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 2026-02-23
#
#   UTC      Radio Flux   Planetary   Largest
#  Date       10.7 cm      A Index    Kp Index
2026 Feb 23     112          20          5
2026 Feb 24     115          12          4
2026 Feb 25     118          10          3
2026 Feb 26     120           5          2
2026 Feb 27     122           5          2
2026 Feb 28     122           5          2
2026 Mar 01     122           5          2
2026 Mar 02     125           5          2
2026 Mar 03     125           5          2
2026 Mar 04     125           5          2
2026 Mar 05     125          15          4
2026 Mar 06     130          15          4
2026 Mar 07     130           8          3
2026 Mar 08     130           5          2
2026 Mar 09     125           8          3
2026 Mar 10     122          18          5
2026 Mar 11     120           8          3
2026 Mar 12     118          12          4
2026 Mar 13     116          12          4
2026 Mar 14     116          20          5
2026 Mar 15     116          18          4
2026 Mar 16     115          12          4
2026 Mar 17     115          10          3
2026 Mar 18     115          10          3
2026 Mar 19     112          12          4
2026 Mar 20     110          18          5
2026 Mar 21     110          38          6
(NOAA)

NBC Use of Shortwave

 

Thank you to the Wavescan staff for this week's nostalgic look at NBC.

Jeff: Back in November last year, we told you about a CBS shortwave station in Philadelphia in the 1930’s.  The main competitor to CBS at that time was the National Broadcasting Company, NBC, and this week we can bring you a story about NBC’s involvement with shortwave radio, in that same pre-war era.  From Los Angeles, here’s Ray Robinson.

Ray: Thanks, Jeff.  Well strangely, the story begins with a large yacht on the U.S. West Coast.  One of the actors in an NBC radio drama, Phillips Lord, bought the 200’ yacht, and renamed it the Seth Parker after the character he played.  He extensively refurbished it, sailed it through the Panama Canal to New York City, and prepared it for a sponsored round-the-world voyage.

NBC provided a 1 kW shortwave transmitter valued at $12,000 and an engineer to operate it, so that progress reports from the voyage could be fed back to the NBC medium wave radio network in the United States.  The Seth Parker then set sail from New York Harbor on November 20, 1933, with twenty-seven people on board – Phillips Lord plus the crew, staff, and radio personnel.  The shortwave transmitter had been licensed with the callsign KNRA, and an additional low power experimental transmitter onboard was also licensed as W10XG.

The first port of call was at Portland, Maine, followed by several other ports down the eastern seaboard.  Radio transmissions from the yacht started nearly three months later beginning on February 13, 1934, from Wilmington, Delaware.  After that, special shortwave broadcasts were made each Tuesday evening from progressive locations down the east coast, then out in the Bahamas, and also from Haiti in the Caribbean.

However, NBC then ended their contract with Phillips Lord, and although the reasons were never officially stated, rumors persisted that many blatantly scandalous events were taking place on board.  NBC in New York even took steps to send staff down to Jamaica to remove their radio transmitter from the ship, but the ship eluded them.

It moved on, back through the Panama Canal, and out into the Pacific.  A shortwave broadcast was made from the Galapagos Islands; and the last known shortwave broadcast from the Seth Parker was made in February 1935 when it was some three hundred miles from Tahiti.

Then the story becomes even more controversial.  The Seth Parker supposedly encountered two storms in the Pacific, off the coast of Tahiti, badly damaging the vessel.  The onboard transmitter KNRA was heard sending an urgent SOS message in April 1935 that was picked up by the maritime station WCC at Chatham, Massachusetts.  The British Royal Navy had a vessel, the HMAS Australia, in the vicinity, and they were asked to assist, which they did.

The Australia reported that they had picked up all nine people who were then onboard the Seth Parker, but they also stated that they had not encountered any storms in the area. The Seth Parker was then towed by a tug boat into Pago Pago harbor in American Samoa, where it was eventually sold.

During its more than a year of spasmodic transmissions, KNRA on board the Seth Parker was logged by multitudes of international radio monitors in North America and Australasia, even though it was only intended for relay on the NBC medium wave network in the USA.  The transmissions were heard directly on shortwave from many exotic island locations.  Several different shortwave channels were used, and the corresponding land-based stations heard in two-way contact with KNRA were the RCA communication stations:
at Rocky Point on Long Island, NY,
at Bolinas, CA, and
at Kahuku, HI.

Additionally, KNRA was also heard on occasions in contact with station LSX in Argentina.

So, what happened to the 1 kW shortwave transmitter KNRA?  Well, that wasn’t the end of the story.  Before the Seth Parker was sold, the transmitter was rescued by NBC personnel and taken to Honolulu where it was installed on a small naval ship called the Avocet, which was used as a tender for servicing larger vessels.  The purpose this time was to relay reports from the Pacific back to the United States during a major eclipse of the sun in 1937.  The transmitter was assigned a new call –  WMEF – and the Avocet took up a position near Canton Island in what is now the nation of Kiribati, about 1,000 miles southwest of Hawaii.  From there, the ship’s transmissions were relayed first by the RCA station in Hawaii, and then onward to the RCA station at Bolinas in California.  Once again, the main purpose of the little transmitter was to feed news reports and commentaries back to NBC, New York for relay on medium wave across the United States.  However, as was quite common in those days, a secondary purpose was for direct reception on shortwave by any listener who might be interested.

But even that’s not the end of the story.  After the solar eclipse in the Pacific, the transmitter was taken back to the continental United States, and placed in storage.  Then five years later in 1942 after America had joined World War II, NBC took the transmitter out of storage, renovated it, and shipped it over to North Africa.

Immediately following the Allied invasion of Sicily in July and August 1943, the transmitter was transported to the island and set up and placed on the air in the city of Syracuse.  Shortly afterwards, following the troops, it was re-loaded onto a ship and taken to Bari on the west coast of Italy, where it was then taken overland by road north to the city of Naples and again placed on the air for reports back to NBC.

Finally, the transmitter was taken to the city of Rome, where it was placed on the air as a temporary shortwave relay station for the Voice of America.  By this time, the much-battered transmitter had been nicknamed the Relic, due to its age and size.

So, what was the end for this historic transmitter?  Well, we don’t know for sure, but we presume it was simply abandoned after the war, there in the city of Rome.

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

Friday, February 20, 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
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 the funding of Encore - Radio Tumbril.
Up-to-date transmission times and frequencies.
The playlists for the most recent programs. .
An email link.
Informal reception reports as well as those requesting eQSL cards, are welcome.

WRMI and Channel 292 are very generous with their airtime, but Encore still costs around 130 Dollars/Euros a month to broadcast.

THIS FORTNIGHT'S PROGRAM - First broadcast on FRIDAY 20th Feb by WRMI at 0200 UTC on 5850, and 2000 UTC on 15770, and then Channel 292 on SATURDAY 21st Feb at 11:00 UTC on 9670 kHz:
Starts with Spring Morning by Lili Boulanger, some Corelli, and part of a wind Quintet By Carl Nielsen.
After that, two movements from Schubert's String Quartet No. 14 - Death and the Maiden, and a poem by Edmund Waller arranged for voices by Eric Whitacre.
The programme ends with The Carnival of Venice by Paganini - violin soloist Joshua Bell.

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

U.K. Propagation Update

 

RSGB
February 20, 2026

We had a week of relatively low solar flux indices and mostly settled geomagnetic conditions.

While the solar flux index fell to be in the 117 to 129 range, the Kp index was mostly in the twos and threes. This was after the weekend’s geomagnetic disturbance due to a large coronal hole that expelled solar plasma in a stream that moved past Earth at nearly 700km per second.

As a result, HF conditions have been quite good with plenty of DX being worked.

The KP5/NP3VI Desecheo Island DXpedition near Puerto Rico has been a struggle for many, due to its popularity and use of solar-powered batteries and low power.

One quick hint: try FT8 on the 40m band around 7am to 7.30am. You get a greyline enhancement at sunrise but for much of Europe the band is closing, which means there is little competition.

Let us know how you get on.

Other DX this week includes 8R1WA in Guyana. This is an Italian team operating until Friday, 27 February. Chuck will be active as VP2MCV on Montserrat and will be active in the ARRL DX CW Contest and until the end of the month.

A German team will be operating as J51A in Guinea-Bissau until mid-March.

Another large solar coronal hole became Earth-facing on Friday, 20 February, so we may expect unsettled geomagnetic conditions from today,
22 February.

Next week, the Space Weather Prediction Centre forecast a low solar flux index of 105 for yesterday, 21 February, before rising again to potentially reach 165 by the end of this month.

Unsettled geomagnetic conditions are forecast for 24-25 February with an estimated Kp index of 5.

VHF and up propagation news from G3YLA and G4BAO:

Friday, 13 February and Saturday, 14 February, saw afternoon openings on 50MHz to TZ1CE in Mali to generate DX interest.

However, as expected, it was stations much further south that benefited from the best propagation, with just a few stations in the southern areas of the UK making QSOs on FT8.

The present spell of unsettled weather remains the main theme for the period up to the end of the coming week.

The pattern is controlled by a strong Atlantic jet stream so ‘changeable’ is the watchword with periods of heavy rain alternating with brighter showery interludes and, of course, quite strong winds at times.

In terms of propagation, rain scatter is a clear favourite, although in one cloudy period in mild air around Tuesday, 24 February, some possible tropo may show up for the southern areas of UK.

The meteor scatter options are again subject to random activity since we are still some way off the next important shower, the Lyrids, in late April.

The auroral prospects have, at best, been gently simmering at low values of the Kp index, mostly less than 5. Stay tuned though, because we may see an uptick around Tuesday, 24 February.

So watch for signs of fluttery signals on the LF bands and then check for auroral tones on 10m and up through the 6m to 2m bands.

These events are always a bit of a long shot but should be worth checking this time.

The sporadic-E season is still some way off, although a strong jet stream pattern is always a positive.

For EME, Moon declination is positive and rising, meaning longer Moon windows and higher peak elevation. Path loss continues to fall as we approach perigee on Tuesday, 24 February. 144MHz sky noise starts the coming week low, rising to moderate towards the end.

And that’s all from the propagation team this week.

(Mike Terry, UK/BDXC)

Thursday, February 19, 2026

Uncle Bill's Melting Pot, February 2026

 


We are going to feature folk/folkloric music from Denmark.  Expect a surprise or three. Note that the hours are slightly different than for From the Isle of Music programming.  


Friday, February 20, 2026:3955 kHz, 1700 CET (1600 UTC), repeat 2300 CET (2200 UTC) 

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

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

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 are included.  Shorter reports will get a short note of thanks instead.