Weekly Propagation Forecast Bulletins

 Product: Weekly Highlights and Forecasts

:Issued: 2025 Feb 24 0214 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 17 - 23 February 2025

Solar activity was at low levels on 18-20 and 22 Feb, moderate levels on 17 and 21 Feb, and reached high levels on 23 Feb. In total, seven M-class flares (R1-Minor) were observed, ranging from M1.0 to M4.9, and one X-class (R3-Strong) flare. Contributing regions were 3992 (S06, L=246, class/area Eai/090 on 17 Feb), 3998 (S14, L=114, class/area Ekc/290 on 23 Feb), 4000 (N17, L=105, class/area Dai/180 on 22 Feb), and 4001 (N24, L=176, class/area Dai/050 on 23 Feb). The sole X flare was an X2.0 from Region 4001 at 23/1927 UTC. 

No proton events were observed at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit reached high levels on 17-18 Feb due to persistent negative polarity CH influence, and was at normal to moderate levels on 19-23 Feb. 

Geomagnetic field activity reached G1 (Minor) storm levels on 18-19 Feb, and saw an isolated active period on 20 Feb, due to persistent negative polarity CH influence. Conditions were at quiet to unsettled levels 21-23 Feb as CH effects dissipated. 

Forecast of Solar and Geomagnetic Activity 24 February - 22 March 2025

Solar activity is expected to range from low to moderate levels throughout the period. R1-R2 (Minor-Moderate) activity is possible at different points throughout the period as active regions grow, evolve, return from the far-side of the Sun. There is a slight chance for R3 or greater events if any of the active regions develop additional complex magnetic structures. 

There is a slight chance for S1 (Minor) or greater proton events, pending the development and activity of the active regions. 

The greater than 2 MeV electron flux at geosynchronous orbit is expected to be at normal to moderate levels from 24 Feb-09 Mar and 19-22 Mar. From 10-18 Mar, high levels are likely as recurrent negative polarity coronal holes are expected to move into geoeffective positions. 

Geomagnetic field activity is expected to be at quiet to unsettled levels on 24 Feb-06 Mar with periodic, weak CH influences. Unsettled to active levels, with isolated G1 (Minor) storming conditions are likely from 07-18 Mar as recurrent negative polarity CHs are expected to be in a geoeffective position. A return to mostly quiet conditions is expected on 19-22 Mar as the CHs move out of a favorable position. 

:Product: 27-day Space Weather Outlook Table 27DO.txt

:Issued: 2025 Feb 24 0214 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 2025-02-24

#

#   UTC      Radio Flux   Planetary   Largest

#  Date       10.7 cm      A Index    Kp Index

2025 Feb 24     210           8          3

2025 Feb 25     210           8          3

2025 Feb 26     210           6          2

2025 Feb 27     200          10          3

2025 Feb 28     195          12          4

2025 Mar 01     195          10          3

2025 Mar 02     190           8          3

2025 Mar 03     190           5          2

2025 Mar 04     190           5          2

2025 Mar 05     190           5          2

2025 Mar 06     185           5          2

2025 Mar 07     180          10          3

2025 Mar 08     170          10          3

2025 Mar 09     160          25          5

2025 Mar 10     155          15          3

2025 Mar 11     160          15          3

2025 Mar 12     170          25          5

2025 Mar 13     180          30          5

2025 Mar 14     185          30          5

2025 Mar 15     185          20          4

2025 Mar 16     185          18          4

2025 Mar 17     180          15          3

2025 Mar 18     180          20          4

2025 Mar 19     185           8          3

2025 Mar 20     190           5          2

2025 Mar 21     195           5          2

2025 Mar 22     200           5          2

(NOAA)

NHK Japan is slated to end QSLing in March 2025

 

NHK Japan QSL featuring Mt Fiji

NHK World-Japan, has been issuing colorful verification cards to listeners for decades. The station's recent announcement on the future of QSLing announced,

"Please be advised that we have decided to stop issuing the Verification Cards. The cards will be sent for confirmation on broadcasts up to March 20, 2025.

Thank you for your understanding and continued support. You can continue to submit your comments and requests to English language services through our website at: https://www3.nhk.or.jp/nhkworld/

Your feedback will be used to improve our broadcasts and services."

NHK Japan QSL featuring rice fields 

WRMI technical update

 

 

 

Important Notice: 

On Thursday, February 20, Florida Power and Light Company will be connecting new transformers for WRMI.  This is the end of a months-long process to replace the station's original transformers, which date from the late 1970's. 

The new transformers have been installed, and this should provide more reliable electrical power and fewer power outages.  However, on February 20 FP&L will have to remove the old transformers using a crane, and then connect the new transformers to us. 

This is a lengthy process requiring a lot of equipment and personnel, so they told us to expect to be without power from approximately 1300-2200 UTC.  During this time we will be off the air on all frequencies, except possibly 7730 kHz and our 9955 kHz live stream (www.wrmi.net). 

We will return to the air on all frequencies as soon as the work is finished.  Thanks for your understanding.

(WRMI FB)

 

Shortwave Radiogram, Program 390

 

Hello friends,

Here in northern Virginia, we have just endured two days of high temperatures below freezing. This is unusual for us, but typical for many of you living farther north. Tomorrow, our typical winter weather, reaching above freezing during the day, returns. And by Sunday, hints of spring.

Producing this week's Shortwave Radiogram has been much easier than last week. I am getting more used to the software that runs under Windows 11. The programs that I use primarily are Fldigi (of course), Audacity, UltraEdit, MS Paint, and Snipping Tool. 

I still have to find solutions for a few quirks in Windows 11. Firefox windows and even instances of Fldigi will disappear, not to be found in the Task Bar or anywhere else. I know the Firefox windows are running because if they have audio (eg a KiwiSDR), I can hear it. I can access some of the hidden Firefox pages by using Firefox History. Frequent trips to Task Manager are required to clean up all those hidden but running apps and pages. 

And Audacity will claim that there is insufficient memory to paste a small segment of audio. So I have to save the Audacity file to a wav file and build on to that.  Sorry to bore you with these details!

Please note that the Saturday 2300-2330 UTC transmission is now (or at least least week was) on three frequencies: 7570, 7780 and 9455 kHz, all from WRMI Florida.  The 9455 transmitter seems especially to offer DX opportunities.

A video of last week's Shortwave Radiogram (program 390) is provided by Scott in Ontario (Wednesday 1330 UTC). Mark maintains the audio archive in the UK.  @CadiereGerald contributes this IQ audio file of the Friday 0530 UTC show. The analysis is provided by Roger in Germany.

Here is the lineup for Shortwave Radiogram, program 390, 21-26 February 2025, in MFSK modes as noted:

 1:44  MFSK32: Program preview

 2:55  MFSK32: Why we think planet Theia existed

 6:31  MFSK64: Test of new geothermal technology in Germany*

12:56  MFSK64: This week's images*

28:23  MFSK32: Closing announcements

* with image(s)

Please send reception reports to radiogram@verizon.net

And visit http://swradiogram.net 

Twitter: @SWRadiogram or https://twitter.com/swradiogram 

(visit during the weekend to see listeners’ results)

Facebook group: https://www.facebook.com/groups/567099476753304

Shortwave Radiogram Gateway Wiki: https://wiki.radioreference.com/index.php/Shortwave_Radiogram_Gateway

THE SHORTWAVE RADIOGRAM TRANSMISSION SCHEDULE IS IN THE IMAGE IMMEDIATELY BELOW. IF THE IMAGE DOES NOT DISPLAY FULL WIDTH, CLICK ON IT. 

Other Shortwave broadcast programs that include digital text and images include The Mighty KBC, Pop Shop Radio and Radio North Europe International (RNEI). Links to these fine broadcasts, with schedules, are posted here.

 

Thanks for your reception reports!

Kim

Kim Andrew Elliott, KD9XB

Producer and Presenter

Shortwave Radiogram

Reporting on international broadcasting at https://twitter.com/kaedotcom

U.K. Propagation Update, February 21

 

RSGB

GB2RS News Team

February 21, 2025

It seems we were a little over-ambitious in suggesting that last week would be better for HF propagation. It looked like we would avoid coronal mass ejections and see the Kp index fall to lower levels.

Unfortunately, the Sun had other ideas and a fast-moving solar stream, often moving faster than 500 km/s, had a south-pointing Bz, which coupled more easily with Earth and sent the Kp index up to four or more.

So even by Wednesday 19 February the Kp index was hitting five.

But it seems that the geomagnetic disturbance merely lowered the MUF from around 40-45MHz to 31-32MHz, so it barely affected HF propagation.

At the time of writing there had only been one M-class solar flare in the past five days, but more than 50 minor C-class events. There were no Earth-directed CMEs.

Nevertheless, there was DX to be had with the standout stations being the V73WW DXpedition to Majuro Atoll on the Marshall Islands, TI1RRC Costa Rica, and 5N9DTG in Nigeria. Upcoming DX next week includes OX3LX (Greenland), Dave G4BUO as 5W0UO (Samoa), TO3Z (Guadeloupe), 4S7SPG (Sri

Lanka) and FS/VA3QSL (St Martin).

Next week, NOAA predicts that the week commencing the 23 February could see the solar flux index starting at 170, but then rising to 195-200 as the week progresses. Geomagnetic conditions are predicted to start quietly, with a Kp index of two, but then become unsettled by the 27 to

29 February, with a maximum predicted Kp index of five.

If this scenario does pan out then we may expect the best HF conditions to occur at the beginning of next week, from the 23 to 26 February.

As always, keep an eye on solarham.com for day-to-day solar news, and perhaps monitor PSKreporter, the Reverse Beacon Network and DX Clusters for digital, CW and SSB HF propagation updates.

VHF and up :

The current spell of unsettled weather seems likely to continue through to the end of next week. There will also be significant windy weather at times. It is therefore not a particularly good period for Tropo, or big antennas for that matter.

This leaves us with rain scatter on the GHz bands and some of these scattering regions will be large areas affecting the whole of the country as active weather fronts pass by, rather than more isolated and harder-to-follow showers which often provide our rain scatter.

Meteor scatter is still within its quieter period with no major showers and better chances coming from random meteor activity, which tends to peak in the hours before dawn.

Recent solar activity has provided some weak auroral conditions on many days.  As usual, check for high values of the Kp index as a good indicator, or even listen for a watery tone on the LF bands. Ultimately you will need to see the Kp index going to at least five to make it worth checking for auroral signals on VHF.

We are still in the dormant period for Sporadic-E propagation, which is a shame in view of the powerful jet streams likely during this stormy weather. These would produce good Es prospects in the main summer season, but weaker Es at low VHF are still a possibility despite being out of season.

Moon declination is at minimum today, Sunday 23 February, and path losses are decreasing as the Moon moves closer to Earth as it heads to perigee on Saturday 1 March. 144MHz sky noise goes high this weekend, beginning Saturday 22 February.

https://rsgb.org/main/blog/news/gb2rs/propagation-news/2025/02/21/propagation-news-23-february-2025/

(Mike Terry, UK/BDXC)

Encore classical music from Radio Tumbril

 

Dear Listener,

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 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.

ENCORE IS A ONE-MAN OPERATION -  PLEASE MAKE A PAYPAL DONATION AND HELP KEEP ENCORE ON THE AIR - Go to - www.tumbril.co.uk

WRMI and Channel 292 are very generous with their air-time but Encore still costs around 100 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 this FRIDAY 21st February by WRMI at 0200 UTC on 5850, and 2000 UTC on 15770 and then Channel 292 on SATURDAY 22nd February at 11:00 UTC on 9670 kHz:

Starts with part of a trumpet concerto by Johann Hummel, some of Mendelssohn's String Octet, and a wind band piece from contemporary US composer David Holsinger.

After that - The Woman with the Alabaster Box, a piece for voices by Arvo Pärt, and the chamber piece, Siegfried Idyll by Richard Wagner.

The programme ends with part of La Mer by Debussy.

(This bulletin is sent by Bcc to the many hundreds of listeners who have been in contact with Encore over the last nearly six years of broadcasting Encore.)

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

GMØTLY

Radio Öömrang slated for February 21 broadcast

 

Radio Öömrang in 2025

Every year on February 21, since 2006, Amrum amateur radio operator Arjan Koelzow, has aired an annual broadcast of Radio Öömrang (Radio Amrum) from the North Frisian Island on the German North Sea coast. The special broadcast is aired on the island’s holiday of Bikebrånen and targeted to the descendants of North Frisian immigrants in North America.

Programming is in the local Frisian dialect, Standard German, and English, and tentatively scheduled in 2025 on 15215 (500 kW) at 1600-1700 UTC, relayed from Issoudun, Franc,  brokered by Media Broadcast in Cologne, Germany, and confirmed from sources. 

Radio Öömrang does not verify reception reports, but you can direct programming details to qsl@shortwave@media-broadcast.com or to: Media Broadcast GmbH, Order Management & Backoffice, Erna-Scheffler, Strasse 1, 51103 Cologne, Germany. 

For a sampling of archived audio and video airchecks, consult the Shortwave Central YouTube channel. 

(Gayle Van Horn/TSM-Feb. 2025)

YouTube videos at Shortwave Central YouTube channel: 

 https://youtu.be/sAKqQrxGdFA

https://youtu.be/xGqIG4iRXSg

https://youtu.be/Sd2Tlf2i1Sk

 

World Radio TV Handbook Review-2025

 

The following review, is included in the February 2025 issue of The Spectrum Monitor e-zine

World Radio TV Handbook 2025 Review

By Gayle Van Horn W4GVH 

The 2025 edition of World Radio TV Handbook has recently been released, this being the third edition of WRTH and Volume 79, in the long and distinguished history of this highly anticipated release. 

After opening editorials and personal stories from handbook contributors, Günter Lorenz reviews the SDRplay RSPdx-R2. The new release is an improved version of the popular RSPdx from SDRplay, and noted as a reasonably priced and a high-quality SDR, with good overall performance, wide band coverage, all mode reception, powerful free software and is a “great little receiver.” Oliver Schmidt covers the SDR software and hardware section with an overview of HDSDR, SDRConsole, SDR++, SDRangel, GQRX, QIRX, Linrad and OpenWebRX+. The review continues with a look at Remote DX with NXP TEF 6686 Based Receivers, that can be controlled via the Internet and used for audio playback. This amazing tune-based receiver would be a good option for operating remote DX.

From the FMDX.org Project, we learn of two well-known DXers. Marek Farkaš, living in Czechia, and one of the creators of FMDX,org, a global community of DXers. Sjef Verhoeven, amateur radio operator (PE5PVB) is active in electronics and related software that led him to join the expanding community of FMDX enthusiasts.

Two additional reviews focus on a preselector and an antenna. Stampfl Wave Block Preselector, is a device that has a built-in bandpass filter for low-pass and high pass, and considered a top-notch preselector, which can improve the reception of any receiver. The NTI ALLMORPRAN (All Mode Passive Receiving Antenna) was reviewed as a perfect all-rounder, with rapid conversion between setup modes and ease of operation.

Manfred Rippich, known for his previous coverage on elusive radio stations, travels first to the island of Barbados, to focus on the early days of radio, to their role in the 21st century. The West African country, Liberia is widely known as home to the mission station, ELWA, however Liberia’s radio presence far exceeds shortwave to  AM and FM. 

Radio Polls by Mohazzab Abdullah discusses the East African nation of Uganda. Silent on shortwave, however the country’s focus on developments in the digital world is ongoing to reach a wide audience. 

If you thought DRM was a passing experiment in digital radio, Big Strides in Connecting All Through Innovation will convince you that DRM is a complete and global system on shortwave, mediumwave and FM.

The annual update of HF Broadcasting Reception Conditions Expected During 2025, predicts a year of “very good shortwave reception across the entire frequency range from 3 to 30 MHz.”

Twelve pages of colored maps, plus the World Timetable is a helpful introduction to the National Radio section. The section includes domestic radio stations on mediumwave, shortwave, FM and DAB. Listings are grouped by country to include frequencies, transmitter power, locations, contact and website information. The International Radio section lists the same information from international broadcasters. Clandestine and other Target Broadcast cover stations broadcasting politically motivated programming, or stations targeted at zones of local conflicts, followed by a two-page Winter 2025 DRM schedule. 

The Frequency List covers by-frequency listings of worldwide mediumwave stations, Shortwave Station of the World, is a by-frequency listing of stations, followed by National TV. The closing section is Reference, an extensive listing of country indexes and codes, transmitter sites, target area codes, radio clubs, Standard Time and Frequency stations, International Organizations, and Selected Resources. 

The new edition has improved formatting and labeling, with an improved font size and clearer reference listings, which makes finding the information far easier than in former editions. There are improved DRM schedule listings which are a great assist in your digital radio quest. There is also expanded details on regional program schedules and station identifications, including an advanced listing of Latin American callsigns for identifying stations. 

This is the third edition published by the new publisher, Radio Data Center GmbH, which began with WRTH 2023. Coupled with a global resource staff, this new edition continues to set the standard for radio and television information. It remains the most comprehensive exemplary reference book, crafted for the casual or seasoned radio hobbyists. WRTH 2025 should be in every listening post as a companion to your global listening. It remains the gold-standard, and the most authoritative source. This is the gem of the industry.

World Radio TV Handbook 2025, is available from the following sources:

WRTH https://wrth.info/ 

Universal Radio http://www.universal-radio.com/

Amazon http://www.amazon.com 

The Amazing Story of Three Early Wireless Stations in China

 

Thank you to Ray Robinson and Jeff White for sharing this week's script of Wavescan, for our readers.

Jeff: In the field of shortwave broadcasting, there are many heroic stories of how stations were established in far-flung corners of the globe.  I think of Alaska, Madagascar, Guam, Palau, the Northern Territory of Australia, Zambia, etc. and we just heard in our program immediately before Christmas that it took chief engineer Doug Garlinger no less than 37 trips to the Big Island of Hawaii to establish KHBN in the 1990’s.  But, none of those situations come close to the challenges that were experienced in setting up wireless stations across China in the years immediately following World War I.  Here’s Ray Robinson in Los Angeles with the story.

Ray: Thanks, Jeff.  Telegraphy first entered China in 1871 when a newly laid cable between Shanghai and Hong Kong linked Qing-era China to the British-dominated international telegraph system.  But by the 19-teens, there were still significant gaps in the telegraph network in the interior of China.  The Marconi Company in England agreed to extend the network wirelessly, and as soon as the hostilities of World War I ended in November 1918, they signed a contract to erect three wireless stations in remote but important commercial centers in northern and western China.  These three stations were planned for installation at Urga, Urumchi and Kashgar.  As an additional part of the contract, Marconi would provide 600 portable wireless stations for local and regional communication in the areas between these three main stations.

• Urga means "Residence" in the Mongolian language and it was the old name for Ulaan Baatar, the modern capital of what is now Mongolia.

• Urumchi is located in north west China; the name means "Beautiful Pasture" in the Mongolian language and it was a major hub along the famous ancient trade route between Asia and Europe, the Silk Road.

• Kashgar means "Mount Kash" in the old Persian language and it is located in the far west of China close to the borders of Kyrgystan and Tajikistan; it was an oasis along the same famous Silk Road.

In 1919, Major S. T. Dockray was commissioned by the Marconi company to install the three wireless stations, each with a power of 25 kW, in the three remote locations.  The first station was intended for installation at Urga (Ulaan Baatar).  The immediate challenge was how to get the equipment there, which included three steel towers each 100 ft. long and weighing more than 300 tons.  The Trans-Siberian Railway had just been completed in 1916, but then in 1917 the Russian Revolution occurred, and it was considered too dangerous and unreliable to try to transport the equipment via that route.  So instead, it was sent by ship from England to Shanghai on the coast of China.

The huge consignment of wireless equipment was then taken by rail to Kalgan (which means "Frontier Gate") in Chinese Inner Mongolia and then by camel and bullock cart across the Gobi Desert to Outer Mongolia, a distance of 800 miles.  Ultimately, this new wireless station was installed, tested and taken into regular service, and Dockray journeyed back into China, to Peking, or Beijing as it is known today.

However, when he got to Peking, Dockray discovered that the Mongolian station was silent, so he made an arduous return journey back to Urga, only to discover that the area was in the midst of a local war.  He re-activated the wireless station, which was then badly damaged by artillery fire.  He was arrested as an English spy, he escaped, was subsequently quarantined during a raging epidemic of Bubonic Plague, and ultimately returned to Peking.

When the local war in Mongolia ended and the area was taken over again by the central government, Dockray returned to Urga for a third time and re-activated the station once more.  However, there were still two more stations to be installed, one at Urumchi and the other at Kashgar.

Dockray journeyed to inland Fengchen where he arranged an enormous caravan to convey the massive pile of wireless equipment to distant Urumchi.  This caravan, considered to be the world's largest ever, was made up of 1,200 camels, 468 horses and 117 bullock carts.

When everything arrived at Urumchi, the local army general at first resisted the installation of the station.  However, when all obstacles were finally overcome, this new station was activated in August 1922.

It took another journey of two months’ duration to continue on from Urumchi to Kashgar, across rugged mountain ranges and swift flowing rivers.  This station, the third in the Marconi wireless network in China, was completed and activated in May 1923, five years since the beginning of the project way back in 1918.

The project director, Major S. T. Dockray, returned to Peking from Kashgar, via the Mintaka Pass in the high Himalaya south into Kashmir, then to Calcutta, and finally by ship once again back to coastal China.  When he finally arrived in Peking, he discovered to his delight that all three stations, in Urga, Urumchi and Kashgar, were still active and on the air, and communicating successfully with many of the portable stations that had been distributed throughout the country.

Back to you, Jeff.

Jeff: Thanks, Ray.  Next week’s feature will also have a Chinese feel, as Ray looks at the shortwave broadcast scene in Shanghai during the period from the mid-1930’s up until the Communist Revolution in 1949.

(Wavescan)

Weekly Propagation Forecast Bulletins

 Product: Weekly Highlights and Forecasts

:Issued: 2025 Feb 17 0126 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 10 - 16 February 2025

Solar activity reached moderate levels on 10-11 and 13-14 Feb, with low levels of activity observed on 12 and 15-16 Feb. In total, six M1 flares (R1-Minor) were observed throughout the week from Regions 3981 (N07, L=341, class/area=Esi/190 on 10 Feb), 3990 (S10, L=191, class/area=Dki/310 on 14 Feb), and 3992 (S06, L=243, class/area=Dai/210 on 13 Feb). 

No proton events were observed at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit was at normal to moderate levels on 10 Feb, with high levels observed on 11-16 Feb. 

Geomagnetic field activity reached G1 (Minor) levels on 10 and 14-15 Feb, and active levels on 11-13 and 16 Feb, due to negative polarity CH HSS influences. 

Forecast of Solar and Geomagnetic Activity 17 February - 15 March 2025

Solar activity is expected to range from low to moderate levels throughout the period. There is a varying chance for R1-R2 (Minor-Moderate) events and a slight chance for R3 or greater events. 

No proton events are expected at geosynchronous orbit, barring significant flare activity. 

The greater than 2 MeV electron flux at geosynchronous orbit is likely to reach high levels on 18-19 and 23 Feb, and 10-15 Mar. Normal to moderate levels are likely to prevail throughout the remainder of the period. 

Geomagnetic field activity is likely to reach G1 (Minor) levels on 28 Feb, 09 and 12-14 Mar, with active levels likely on 17-18 Feb, and on 01 and 15 Mar, due primarily to CH HSS influences. Quiet and quiet to unsettled conditions are expected to prevail throughout the remainder of the period. 

:Product: 27-day Space Weather Outlook Table 27DO.txt

:Issued: 2025 Feb 17 0126 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 2025-02-17

#

#   UTC      Radio Flux   Planetary   Largest

#  Date       10.7 cm      A Index    Kp Index

2025 Feb 17     185          10          3

2025 Feb 18     185          10          3

2025 Feb 19     180          10          3

2025 Feb 20     180           5          2

2025 Feb 21     175           5          2

2025 Feb 22     170           5          2

2025 Feb 23     170           5          2

2025 Feb 24     190           5          2

2025 Feb 25     195           5          2

2025 Feb 26     200           5          2

2025 Feb 27     195          10          3

2025 Feb 28     195          25          5

2025 Mar 01     190          20          4

2025 Mar 02     195           5          2

2025 Mar 03     200           5          2

2025 Mar 04     205           5          2

2025 Mar 05     205           5          2

2025 Mar 06     200           5          2

2025 Mar 07     200          10          3

2025 Mar 08     200          10          3

2025 Mar 09     195          25          5

2025 Mar 10     195          15          3

2025 Mar 11     195          15          3

2025 Mar 12     195          25          5

2025 Mar 13     200          25          5

2025 Mar 14     200          30          5

2025 Mar 15     200          20          4

(NOAA)

DOGE Targeting VOA And Radio Free Europe

 

Voice of America (VOA) and Radio Free Europe/Radio Liberty (RFE/RL) are in the sights of Elon Musk, the billionaire entrepreneur appointed by President Donald Trump to oversee the House Subcommittee on Delivering on Government Efficiency (DOGE).

Musk commented on a social media post by Richard Grenell, the U.S. Special Envoy for Special Missions, who said the radio networks are “state-owned media” and “are a relic of the past.”

“Yes, shut them down,” Musk wrote in his reply to the post. “Europe is free now (not counting stifling bureaucracy). Nobody listens to them anymore. It’s just radical left crazy people talking to themselves while torching $1B/year of US taxpayer money."

As previously reported by Inside Radio, DOGE wants to defund National Public Radio (NPR). DOGE Chair Marjorie Taylor Greene (R-GA) has asked the leaders of NPR and PBS, to testify to the subcommittee in the coming weeks. DOGE says it is looking into the “systemically biased news coverage” of the two public media outlets.

Additionally, a bill has been introduced in Congress that would specifically prohibit federal funding for National Public Radio. The proposed No More Funding for NPR Act of 2025 would not only cut off future funding of NPR but also require that any money that had earlier been allocated but not yet been spent be permanently rescinded.

(Inside Radio)

Special V-Day program from Jen & GB

 

Jen & GB's V day Special, will broadcast on Sunday, February 16, at 1900-2400 UTC, plus on Unique Radio, Australia

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

Join me & GB for our V-day show at 1900 UT Sunday.

GB's Valentines Day Show 2025 starts at 1915 until 2115 UT; 

then it's My Lovey Dovey & Diss show until 2400 plus UT.

So Join us on our Unique live digital stream.

http://uk4-vn.mixstream.net:8104/index.html

Plus our live chat room is open for you at

https://web.libera.chat

click on Connect, then Web chat

Please put in the following:

For nick: name or like me radionutresss

Then next line channel, that's the following:

#eyeradiojd

and you are in the room

See you then.

JenUR@proton.me

Jen & GB

73" 33" & V day 88's

Arctic 252, status update

 

February 2025

The 1kW longwave transmitter is now ready and a matching unit is currently being built.

The antenna has been a big problem and due to the winter conditions it's unrealistic to expect any station startup before the summer now. The 300kW transmitter that was offered was withdrawn and an extremely high price tag was put on the dismantling and engineering oversight by the communications company. The costs were vastly inflated in order to deter the project from acquiring this transmitter. In fact the costs were double that of a TRAM LW transmitter shipped complete!

Other high-power transmitters may become available in time as decisions have not yet been made about them. The stations interest in these has been conveyed to the companies. In all the amount of communication alone spent on this project is immense. The station is still getting emails from well-wishers and pleas from people to succeed so it drives the project on knowing at least some people will be happy to hear the station on air. 

We would still really need a higher power transmitter so any leads are very welcome no matter how old the transmitter is. MW, LW or SW! We have been offered a 1kW MW transmitter so this will be used for a project that will be announced in a few months. 

Interest in Shortwave broadcasting has also been expressed so if we can find a shortwave transmitter or even a good broadband linear amplifier SW can start very easily. 

https://arcticradio.net/news