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. 

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.