Programming update for FTIOM and UBMP

 The main feature will be special guest Kiki Valera with some of his new son cubano album Vacilón Santiaguero

From the Isle of Music

The main feature will be special guest Kiki Valera with some of his new son cubano album Vacilón Santiaguero

May 11: 0900-1000 UTC 9670 kHz 

1900-2000 UTC 3955 and 6070 kHz

Uncle Bill’s Melting Pot, May 18, 2024

The main feature will be special guest Eugene Pao, Hong Kong’s foremost jazz guitarist, with some of his new album Jazz at Lincoln Center recorded live during a tour of the United States. 

May 18 0900-1000 UTC 9670 kHz 

1900-2000 UTC 3955 and 6070 kHz

Both programs will feature additional music to round out the hour.

It’s great to be back on Channel 292!

(Bill Tilford/Tilford Productions)

DX Central Announces a New Summer-Long AM DX Challenge

 

 THE 2024 SUMMER OF DX!

DX Central and Loyd Van Horn are pleased to announce the latest challenge for MW DXers to test their skills against the temperament of the ionosphere with the 2024 Summer of DX challenge, open now through 2359 UTC on August 31, 2024.

"Who says that mediumwave season ends in May?  Definitely not us," says Van Horn.  "Some of my best MW DX catches ever have come through in the summer months.  While more difficult, the patient and determined DXer can reap fantastic results by braving the lightning crashes and summer static for MW DX!"

The Summer of DX challenge is open to any DXer, worldwide, for any station broadcasting between 530 and 1710 kHz.  There will be point values assessed for each entry and final point totals will be calculated after the conclusion of the challenge.  Results will be presented during the season premiere of Season 5 of the popular DX Central Live! DX-themed livestream in the fall of 2024.

"We made a conscience effort with our scoring setup for this challenge to try to level the playing field as much as we could to remove biases such as the use of SDRs or proximity to stations, that some DXers may see as discouraging for participation," says Van Horn.

"I wanted to make this something that any DXer around the world would want to actively be a part of!"

Those interested in participating can find a full list of rules, scoring information and other details at the challenge Web site:  dxchallenges.com.  Once registered, DXers can begin submitting their logs and accumulating points!

DX Central is a multimedia platform that specializes in mediumwave (AM) and FM DX and related topics.  The platform includes a web site with written educational material on MW and FM DX, propagation, equipment reviews and more; a popular weekly livestream during the peak of MW season in the Northern Hemisphere with live DX, discussions around DX-related topics and active participation from viewers; the DX Central YouTube channel with a large assortment of videos including instructional videos from the DX101 and Radio101 series as well as MW and FM identification airchecks to aid DXers in identifying their own DX catches; and the host of a series of weekly frequency challenges during the peak of MW DX season to motivate DXers to push their skills and help them hear more stations!

The DX Central Platform:

dxcentralonline.com

dxcentrallive.com

youtube.com/@DXCentral

dxchallenges.com

Voice of Indonesia to adjust frequency

 

Voice of Indonesia, the Overseas Service of Radio Republik Indonesia (VOI RRI) will carry out an adjustment on our shortwave frequency starting Monday, 13 May 2024 at 0000 UTC. We are moving from 4750 kHz to 4755 kHz. 

Meanwhile, our 3325 kHz will continue as usual. We are asking for your understanding. Please send your feedback to our email address voilisteners@gmail.com

Thank you. (Station Direct via WRTH Facebook)

(R D'Angelo/NASWA)

(edited or clarity)

Voice of Indoneaia website: https://voinews.id/ 

HAARP slated for research campaign

 

The High-frequency Active Auroral Research Program (HAARP) will be conducting a research campaign on May 8-10 UTC, with operating times specified below. Operating frequencies will vary, but all HAARP transmissions will be between 2.8 MHz and 10 MHz.

Actual transit days and times are highly variable based on real-time ionospheric and/or geomagnetic conditions. All information is subject to change.

This campaign is being conducted in support of research proposals from the University of Alaska Fairbanks and is a study of mechanisms for the detection of orbiting space debris. Space debris poses a major risk to all space operations, including manned spacecraft and communications satellites. 

These experiments are being performed at HAARP will help identify ways to improve collision detection on satellites.

For more information on space debris, see the NASA Orbital Debris Program Office's FAQ at: https://orbitaldebris.jsc.nasa.gov/faq. For more information research at HAARP, see the online HAARP FAQ at: https://haarp.gi.alaska.edu/faq 

Date (UTC) May 8 May 9 May 10

Time (UTC) 2000-0200 2000-0200 2000-0230

Frequencies (MHz) 3.25, f0F2 3.25, f0F2 3.25, f0F2

For updates on ionospheric cconditions in Gakona, please consult ionograms from the HAARP

Diagnostic Suite: https://haarp.gi.alaska.edu/diagnostic-suite

Weekly Propagation Forecast Bulletins

 Product: Weekly Highlights and Forecasts

:Issued: 2024 May 06 0628 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 29 April - 05 May 2024

Solar activity was at moderate to high levels. Moderate levels were observed on 29 Apr and 01-02 May. High levels were reached on 30 Apr, due in part to an M9.5/2b flare at 30/2346 UTC from Region 3654 (S07, L=134, class/area Fkc/550 on 30 Apr). Region 3654 was the largest and most complex spot group on 28 Apr-01 May, however it was in decay as it approached the SW limb on 01 May. The region produced a total of 11 M-class flares. On 30 Apr, Region 3663 (N26, L=037, class/area Fkc/580 on 05 May) emerged in the NE quadrant, followed by Region 3664 (S19, L=352, class/area Ekc/580 on 05 May) on 01 May. Both regions grew steadily over the following days. Region 3663 produced 17 M-class flares and 3 X-class flares while Region 3664 produced only 5 M-class flares. The three X-class flares included an X1.6/1b at 03/0222 UTC, an X1.3/1b at 05/0601 UTC, and an X1.2/1b at 05/1154 UTC. The X1.6 flare had associated Type II (959 km/s) and IV radio sweeps, a 550 sfu Tenflare and an associated CME first observed in SOHO/LASCO C2 imagery at 03/0248 UTC. Modelling of the event showed a potential glancing blow arriving around 05/1800 UTC.

There were two further CME runs of note. Those included an eruption near N13W09 at 29/0909 UTC that displayed a westward flow across GOES 16 SUVI imagery. C2 imagery showed a CME off the NW limb at 29/1248 UTC that was modelled as a potential glancing blow on 03 May around 1500 UTC. Lastly, a CME that was associated with a C3.9 flare at 03/2037 UTC from a plage area in the NE quadrant. The flare had associated Type II (392 km/s) and Type IV radio emissions and a CME first observed in C3 imagery at 03/2218 UTC. Analysis showed a potential glancing blow on 09 May. Other eruptive events associated with radio signatures were observed, but did not produce ejecta determined to be on the Sun-Earth line. 

No proton events were observed at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit was at normal to moderate levels throughout. 

Solar wind parameters began the period under mild positive polarity CH HSS influence solar wind speed was mostly in the 450-500 km/s range and total field around 2-4 nT. Solar wind speed began to diminish to nominal levels on 30 Apr. After 30/1130 UTC, the first of three CMEs were observed. Total field increased to near 14 nT while the Bz component rotated from -9 nT to +13 nT. Solar wind speed continued to decrease to near 350 km/s. The geomagnetic field responded with quiet levels on 29 Apr, followed by quiet to active levels on 30 Apr-01 May. On 02 May, a shock arrival was observed at 02/1317 UTC, indicating the arrival of the second CME. This CME was possibly the one that left the Sun on 29 Apr. The IMF increased to approximately 21 nT and the Bz component shifted southward to -19 nT. Solar wind speed increased initially to near 450 km/s and later to near 510 km/s on 03 May. The geomagnetic field responded with unsettled to G3 (Strong) storm levels on 02 May and quiet to active levels on 03 May. By early on 03 May, the IMF had decreased to nominal levels with solar wind speed slowly returning to background conditions. Nominal conditions returned on 04 May and through the midday on 05 May. Around 05/1500 UTC, another enhancement was observed in the IMF, likely the arrival of the 03 May CME. 

Total field strength increased gradually to 14 nT while the Bz component reached a southward deflection of -12 nT. Solar wind speed increased to near 380 km/s. The geomagnetic field responded with unsettled to active levels late on 05 May. 

Forecast of Solar and Geomagnetic Activity 06 May - 01 June 2024

Solar activity is expected to be at moderate to high levels (R1-R3/Minor-Strong) through 12 May as Regions 3663 and 3664 rotate across the visible disk. Low to moderate levels are expected on 12 May-01 Jun. 

There is a chance for S1-S2 (Minor-Moderate) solar radiation storm levels on 06-13 May due to the flare potential of Regions 3663 and 3664. 

The greater than 2 MeV electron flux at geosynchronous orbit is expected to be at normal to moderate levels on 06 May-01 Jun. 

Geomagnetic field activity is expected to be at unsettled to G2 (Moderate) storm levels on 06 May due to persistent CME influence. The geomagnetic field is expected to reach unsettled to active levels on 07-09 May, 12-14 May, 23-25 May, 27-28 May, and 31 May-01

Jun due to recurrent CH HSS activity. 

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

:Issued: 2024 May 06 0628 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 2024-05-06

#

#   UTC      Radio Flux   Planetary   Largest

#  Date       10.7 cm      A Index    Kp Index

2024 May 06     180          35          6

2024 May 07     185          12          4

2024 May 08     190           8          3

2024 May 09     185          10          3

2024 May 10     175           5          2

2024 May 11     175           5          2

2024 May 12     175           8          3

2024 May 13     175          15          4

2024 May 14     180          10          3

2024 May 15     205           5          2

2024 May 16     205           5          2

2024 May 17     200           5          2

2024 May 18     195           5          2

2024 May 19     190           5          2

2024 May 20     185           5          2

2024 May 21     180           5          2

2024 May 22     175           5          2

2024 May 23     170           8          3

2024 May 24     165          12          4

2024 May 25     170           8          3

2024 May 26     175           5          2

2024 May 27     175          12          4

2024 May 28     170           8          3

2024 May 29     165           5          2

2024 May 30     165           5          2

2024 May 31     165           8          3

2024 Jun 01     175          12          4

(NOAA)

Propagation news update from the U.K.

 

RSGB

May 3, 2024

What a strange week we had; with the solar flux index in the 167 range, falling to 130, conditions should have been reasonable, but the Kp index hit 4 and even 5.33 on the evening of Friday 26 April, which meant propagation on Saturday the 27th was truly dire.

Stations taking part in International Marconi Day on the 27th found the 40m band only open to long skip in the morning. This was due to the critical frequency being below 5MHz. The predicted MUF over a 3,000km path fluctuated between 15MHz and 19MHz for the whole day, which meant only 14MHz was open reliably. As a result, QSOs were hard to come by and many stations reported that it was slow going with virtually no signals from outside of Europe.

So what happened? Well, it was a combination of factors. The increased Kp index—due to a fast solar wind—took its toll; and we are now moving to a summer ionosphere, where chemical changes make it harder to ionize. This will mean we should see MUFs dropping as the season progresses, at least during the day. Nighttime MUFs will be higher than in winter.

So it may be that the glory days of 28MHz F2-layer propagation are on hold until autumn, with only short-skip sporadic E on the 10m band to keep us entertained.

F2-layer propagation is still available on the higher HF bands, but it may be patchy.

International Marconi Day station GB0CMS in Caister, Norfolk, reported that its 20m signals were picked up by a reverse beacon network skimmer in Utah, despite not working anyone outside of Europe. 

Meanwhile, on the morning of the 2nd, Laurie, G3UML was quite surprised to work YJ0CA on Vanuatu on the 15m band using SSB. He also worked 3D2CCC on Conway Reef on the 20m band using CW, and JD1BMH in Japan on the 15m band, also using CW.

Next week NOAA predicts the solar flux index will be in the 125 range, rising to 175 as the week progresses. Geomagnetic conditions are dependent on coronal mass ejections. We have had eight M-class solar flares in the past three days, and a Kp index of 5 on Thursday, the 2nd, which doesn’t bode well for next week. So, keep an eye on solarham.com for current conditions, and look for the best HF propagation if the Kp index is low for a day or two.

VHF and up propagation news from G3YLA and G4BAO:

The weather pattern remains very unsettled for the whole period, with areas of low pressure edging north across the UK from the continent.

There will be a risk of thundery weather at times, with locally heavy rainfall, which will be good for rain scatter on the Gigahertz bands. Tropo looks to be hard to find as we end the current week dominated by low-pressure systems, but there are signs of high pressure returning after mid-week, but only temporarily.

This could produce some tropo paths, especially across surrounding waters such as the Irish Sea, English Channel, and North Sea.

The nominal summer season of sporadic E propagation is upon us and—from May to early September—daily blogs will be provided on the propquest.co.uk website, highlighting the possible sporadic E

It’s well worthwhile getting into the habit of regularly checking the DX clusters and activity maps since the early season is usually characterized by a complex jet stream pattern with multiple potential locations for sporadic E propagation.

Timewise, it eventually settles into a more traditional behavior with activity often in two phases, one in the morning and the second in late afternoon and early evening.

As you listen to this report, the Eta Aquariids meteor shower should be peaking. Unfortunately, the best viewing for the shower—which is part of the debris from Halley’s comet—will be in the southern hemisphere.

Nevertheless, this is expected to be one of the best showers this century. For those viewing the shower, a waning Moon means that light levels should be low, making for ideal visual sighting.

For EME, the Moon will be waning all week with the New Moon around 8 May. The Moon will be rising in the sky throughout the week, with zero declination on 5 May and peaking at its highest in the sky on Saturday, 11 May.

The lowest additional path loss occurs Sunday and Monday, the 5th and 6th, but high Sun noise–with the Moon close to the Sun at New Moon—occurs shortly afterward. Later in the week, as the Sun ‘leaves’ the Moon behind, noise levels, at least on the higher bands will fall to around normal.

https://rsgb.org/main/blog/news/gb2rs/propagation-news/2024/05/03/propagation-news-5-may-2024/

(Mike Terry/BDXC)

FastRadioBurst 23 to air on May 5

 

FastRadioBurst 23 will air on Sunday, May 5 at 0900 and 1300 UTC on 6160 kHz and at 2000 UTC on 6160 kHz & 3975 kHz. The program will be on  Test Cards on Radio. This program is beamed to Europe via Shortwave Gold. Don't miss it !!

Finland's RealMix Radio plans weekend broadcast

 

RealMix Radio is an exciting new radio project based in Raasepori, Finland. This is their studio building!

Recently granted an official broadcasting license, plans are for a broadcast on the first weekend in May 2024. 

The station is using a modest 15-watt transmitter, with future plans for 250 watts. Plans are also underway to expand RealMix’s broadcasting capabilities to include a medium wave frequency. 

Due to the very low power, a Scandinavian Kiwi SDR is recommended. 

The driving force behind this venture is Joakim Weckström who may be contacted at:  realmix.sw@gmail.com.

6185 kHz

Broadcast times UTC

Saturday May 4, 2024 

07:00 music program 

09:00 Delta Mike On Air 

Sunday May 5, 2024 

07:00 Delta Mike On Air 

08:00 Listener's Requests 

Reception reports to realmix.sw@gmail.com 

Interesting nostalgic story on Radio Afghanistan

 

AFGHANISTAN  

 I would like to remember one more broadcaster heard on the air - Radio Afghanistan. Broadcasting in Russian by the international service Radio Afghanistan began in January 1961. The station had low-quality transmitting equipment and was unlucky with the choice of frequencies. Therefore, there were often problems with receiving the station.

I remember the only period when audibility was unusually good for three years from 1974 to the end of 1976. The broadcast was carried out during the day at a frequency of 15195 kHz from 13.30 to 15.00 Moscow time for half an hour consecutively in Russian, German and English. True, the time for listening was inconvenient, but I sometimes adapted to listen at work in a special laboratory, where I first did my internship, and then worked for a short time before the army. There was some kind of service radio in the laboratory, which I used.

Over the years,the content of Russian Radio Afghanistan broadcasts has remained approximately the same. This was the case in 1974: news, Russian music, commentary, Afghan music, conversation (about Afghanistan), Afghan music.The broadcasts covered the changes taking place in Afghanistan since the recent overthrow of the monarchy in July 1973 and the activities of President Mohammed Daoud Khan,the cousin of the former king Mohammed Zahir Shah, whom he overthrew. These were the last years of relative stability,

after which, from April 1978, a period of revolutions and civil wars began in Afghanistan.

In the early 80s,and perhaps earlier, some periodicals sold in Soyuzpechat kiosks in other countries published schedules of foreign, including Russian-language broadcasting in these countries:

Radio Afghanistan - in the newspaper "Kabul new times"

Radio Damascus - in the newspaper "Syria times"

Radio Ulaanbaatar - in the newspaper "News of Mongolia"

BBC - in the magazine "England".

(Vladimir, Rybinsk, Yaroslavlskaya oblast-RUS) 

RUSdx #1287 via wwdxc BC-DX TopNews April 28)

Now called IEA - Islamic Emirate of Afghanistan.

(WWDXC Top News 1579/02 May 2024)

Texas Radio Shortwave on Channel 292 on May 5

 

On Sunday, May 5, Channel 292, Rohrbach, Germany, will air TRSW’s monthly program at 1000 UTC on 9670 kHz and 2100 UTC on 3955 kHz.

These changes are based on three test transmissions in mid-April.

TRSW welcomes detailed reception reports emailed to texasradioshortwave@protonmail.com.  This includes reports from listeners using remote SDRs.

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

10:00 - 11:00 UTC Saturday 9670 kHz Channel 292 to Europe

01:00 - 02:00 UTC Sunday 5850 kHz WRMI to US and Canada

19:00 - 20:00 UTC Sunday 3955 kHz Channel 292 to Europe

02:00 - 03:00 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 OR 'BUY ME A COFFEE' AND HELP PAY THE  BROADCASTERS AND 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 AND 'BUY ME A COFFEE' BUTTON are 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 3rd May) by WRMI at 0200 UTC on 5850, (and 2000 UTC on 15770) and then Channel 292 on SATURDAY (4th May) at 10:00 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.

A very good site for online SDR receivers all over the world is: http://kiwisdr.com/public/  Click the 'Map' button in the top left of the screen.

 

Thank you for spreading the word about Encore - Classical Music on Shortwave on Radio Tumbril - and thank you for your support.

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

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

GMØTLY

Shortwave Radiogram, Program 352

 

Hello friends,

In last week's email, I wrote "It will be hot enough, soon enough." Well, as I type this, it is 90°F/32°C in Arlington, Virginia. And we obstinately have not turned on our house's air conditioning. The AC is for when it really gets hot. Which will be soon enough.

Our front yard is green, thanks to a variety of weeds, enough to support a botany thesis. Mixed in among these are occasional blades of grass. And not, I suspect, the most desirable species of grass. Ah, summer.

Dramatic events in space weather continue, but generally, we were lucky last week with propagation during the Shortwave Radiogram transmission times. Our surprise mode DominoEX 22 usually showed some errors, a reminder of why we don't use this mode more often.

A video of last week's Shortwave Radiogram (program 351) is provided by Scott in Ontario (Wednesday 1330 UTC). The audio archive is maintained by Mark in the UK. An analysis is provided by Roger in Germany.

Here is the lineup for Shortwave Radiogram, program 352, 2-8 May 2024, in MFSK modes as noted:

 1:45  MFSK32: Program preview

 2:52  MFSK32: New lily species is first in 110 years*

 7:52  MFSK64: Bacteria-spore-loaded plastic eats itself*

12:14  MFSK64: This week's images*

27:56  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

Radio Carolina North slated for weekend broadcast

 

Our next Radio Caroline North broadcast is between 4th and 5th May, live from our radio ship 

Ross Revenge.

You'll hear some great music from the 60s to early 90s – plus a chance to win some goodies from our Web Shop, courtesy of Clive Ironmonger from Spilsby, Lincolnshire.

Listen on 648 AM across England, The Netherlands, Belgium and beyond, on 1368 AM in the North/North-West courtesy of our friends at Manx Radio, worldwide online here via our Caroline North Player, on smart speakers and the Radio Caroline app.

We'd love to hear from you during the broadcast via memories@... and remember, it's the only email address that gets you straight through to our 'North' broadcasters.

https://www.radiocaroline.co.uk/#home.html

Radio Free Asia,summer schedule

 USAGM- Radio Free Asia - A24 Summer schedule

All times UTC, programming daily and targeted to Asia 

31 March - 26 October 2024

Burmese

0030-0100 15245  15700  17530

0100-0130 15245  15700  17530

0200-0300 15245

1230-1300 9370  9990

1300-1330 9370  9990

1330-1400 9990  12140

1400-1430 9990

Khmer

1230-1300 9330 11885  12150

1300-1330 9330  11885  12150

1430-1500 9355  12140

2230-2300 12140  13715

2300-2330 12140  13715

Korean

1000-1100 1566

1200-1300 9900

1300-1400 9900

1500-1600 1188  9910  9990  11985

1600-1700 1188  9910  9990  11985

1700-1800 1188  9990  11985

1800-1900 1188  9990  11985

2100-2200 9540  11945  11985

Lao

0000-0100 15210

1100-1200  1 5195

Mandarin

0300-0400 11570  11895  12065  17800

0400-0500 11895  13750  17800  21570

0500-0600 11895  17800  21690

0600-0700 11895  13790  17800  17855

1500-1600 9940  11675  13810

1600-1700 7540  11610  13570  13810

1700-1800 9360  9970

1800-1900 9360  9970  12110

1900-2000 9360  9720

2000-2100 6080  9360  9535

2100-2200 7435  9685

2300-0000 9535  9720  15265

Tibetan

0100-0200 9370  9410  9705  17670

0200-0300 9865  11745  11965  

0600-0700 15610

1000-1100 13740

1100-1200 13580  15265  15490  17640

1200-1300 12055  13580  15490  17690  17860

1300-1400 11995  13720  15275  15490  17860

1500-1600 9355

2200-2300 7485

2300-0000 5950   9545  11700

Uyghur

0100-0200 9350  9780  9800

1600-1700 9355  9560  11675  

(USAGM/RFA)

European, Private Shortwave Stations-May 2024

 

The May 2024 edition of  Stig Hartvig Nielsen's monthly edition of  European, Private Shortwave Stations

is available at: 

https://s3-us-west-1.amazonaws.com/groupsioattachments/9411/105845499/157103/0?AWSAccessKeyId=AKIAJECNKOVMCCU3ATNQ&Expires=1714587705&Signature=0WuZM5edV4H9yrOgxedUwdPEas8%3D&response-content-disposition=inline%3B+filename%3D%22European%2520private%2520SW%2520stations%2520-%25201%2520May%25202024.pdf%22

Tiny URL: 

https://tinyurl.com/y4pjkvnk

SM Radio Dessau slated for May Day broadcast

 

On Wednesday, May 1, 2024, SM Radio Dessau will broadcast three one-hour broadcasts, to observe the May Day Parade 2024.

The broadcast will air from the following relays: 

All times UTC

0800  6070 kHz (10 kW) via Channel 292, Rohrbach-Waal, Germany

1200  6095 kHz (100 kW) via Media Broadcast, Nauen, Germany (repeat)

1900  3955 kHz (125 kW) via Encompass, Woofferton, UK (repeat)

Additional station information: http:///www.smradio-dessau.de