Monday, September 01, 2025

Brazil on Shortwave

 

Special thank you to Ray Robinson and Jeff White for sharing this week's edition of Wavescan.  Shortwave broadcasts continue to dwindle from South America; however, Brazil remains a favorite to monitor.

Jeff:  Our featured country this week is Brazil – the largest country in South America.  Back in 2021, we brought you a three-part series on the early history of wireless and medium wave radio in Brazil, but we’ve never covered the shortwave scene there before.  So here to rectify that is Ray Robinson, in Los Angeles.
Ray:  Thanks, Jeff.  And yes, Brazil is indeed a country of superlatives, larger than the continental United States.

The Amazon River is thought by many to be the world’s longest river, originating more than 4,000 miles inland from the Atlantic coast.  Large ocean-going vessels can ply the Amazon River for a thousand miles inland, and the river is navigable for smaller ships for another thousand miles further.  This huge river system disgorges fresh water at the rate of 18 million tons every minute, sending it out for a distance of 250 miles into the Atlantic Ocean.

Iguazu waterfalls (photo via Wikipedia)

The dramatic Iguazu waterfalls lie at the border between Brazil and Argentina.  The water at Iguazu plunges from a height of more than 200 feet, higher than the Niagara Falls.  These South American falls stretch across the landscape for more than a mile.  In season, the water tumbling over the edge of the cascading cliffs at Iguazu is greater in volume than that of all the other major water falls throughout the world combined, and the thunderous, tumultuous roar from Iguazu can be heard for miles.

Most of the major cities in Brazil lie along the Atlantic coast, with the largest being Sao Paulo (population 22 million) and the second largest Rio de Janeiro (population 12 million).  Only Brasilia, founded as the national capital in 1960 and now with a population of 3½ million, is located inland, some 1,000 miles from the ocean.

As we’ve told you previously, the medium wave scene in Brazil dates back to an experimental demonstration station that was set up in Rio de Janeiro in 1922.  In the early days when only a very few wealthy Brazilians owned receivers, radio clubs were formed in many areas which supported nonprofit radio stations through contributions from the members.  These were often called Radio Clube do and the name of the town or city, or sometimes Radio Sociedade do … wherever.  By the 1930’s, however, more Brazilians owned radio receivers, and commercial radio stations came on the air.  Gradually the radio clube and radio sociedade stations switched to private commercial ownership, although a few do still survive.



As the use of medium wave began to proliferate, so did the use of tropical band shortwave and even the higher shortwave bands, for domestic purposes.  Some stations solely used shortwave, while others simulcast their medium wave programming on one or more shortwave frequencies.  Some Radio Nacional stations were run by the government and carried less advertising, similar to the CBC in Canada or PBS in the USA.  Educational stations were also run by the Catholic Church.  But most stations were commercial, and with huge territory to cover, shortwave was the most efficient way of doing it.

By the early 1970’s, over 200 shortwave stations were listed in Brazil in the WRTH, all targeting domestic audiences, mostly in Portuguese, but also a few in indigenous Indian languages.  Transmitter powers were typically around 1-5 kW on the 90- and 60-meter tropical bands, but as much as 50 kW on the higher international shortwave bands, where some 2-3 dozen stations operated, all the way from 49 meters right up to the 16-meter band.  The only other countries to make such extensive use of shortwave for domestic purposes were Peru and Indonesia, although the transmitter powers in Brazil were generally higher.

The government of Brazil from 1964-1985 was a military dictatorship, and in the early 70’s, they became concerned at the amount of cold war propaganda that was being transmitted to Brazil in Portuguese by foreign countries, especially socialist or communist ones such as Cuba.  Foreign broadcasts in Portuguese were easily heard by Brazilians who were very used to using shortwave – it was part of their culture – and the government feared that such foreign broadcasts might start winning over hearts and minds.

The dictatorship already had a couple of very grandiose infrastructure projects under its belt – the 2,600-mile-long Trans-Amazonian Highway and the Rio-Niterói Bridge, which at over 8 miles long was, at the time of its construction, the second longest bridge in the world, second only to the Lake Pontchartrain Causeway in Louisiana.  So, in the early 70’s, they decided to undertake one more major infrastructure project – the “High Power Broadcasting System” – for Radio Nacional de Brasilia – a station which had been inaugurated in 1958, but which at that time only had transmitters in the major cities.



A 1,200-acre site was selected at the Parque do Rodeador, or Rodeo Park, about 30 km (18 miles) northeast of downtown Brasilia in the Brazilian Federal District.  It is well away from any other telecommunications services, and sits on the highest point in the district, 4,400 feet above sea level, surrounded by small farms.  Much of the property had to be cleared of tropical rain forest.

Initial construction was completed in 1974, at a cost, adjusted for inflation, of half a billion Brazilian Reals, equivalent to about US$90 million.  The High-Power Broadcasting System at the Parque do Rodeador was inaugurated on March 11, 1974 by then president Emilio Médici – who arrived by helicopter and in short order opened the station himself by turning on a medium wave transmitter, and the Minister of Communications who was with him turned on a shortwave one.

Radio Nacional 


A 1,200-acre site was selected at the Parque do Rodeador, or Rodeo Park, about 30 km (18 miles) northeast of downtown Brasilia in the Brazilian Federal District.  It is well away from any other telecommunications services, and sits on the highest point in the district, 4,400 feet above sea level, surrounded by small farms.  Much of the property had to be cleared of tropical rain forest.

Initial construction was completed in 1974, at a cost, adjusted for inflation, of half a billion Brazilian Reals, equivalent to about US$90 million.  The High-Power Broadcasting System at the Parque do Rodeador was inaugurated on March 11, 1974 by then president Emilio Médici – who arrived by helicopter and in short order opened the station himself by turning on a medium wave transmitter, and the Minister of Communications who was with him turned on a shortwave one.

By 1979 the site housed 6 x 250kW Brown Boveri shortwave transmitters from Switzerland, and also 2 x 300kW medium wave transmitters which could provide a combined output power of 600kW, sufficient to cover the entire country at night on 980 kHz.  The shortwave transmitters were used for both domestic and international coverage, the primary frequencies being 6180 and 11780 kHz.  They also had a high-power FM transmitter on 96.1 MHz for the city of Brasilia.  

For the international broadcasts they used five languages - English, German, French, Spanish & Portuguese.  Programs were produced first in Portuguese, and then translated into each of the other languages.  They mostly consisted of news, but also included politics, the economy, science and technology, culture and the arts, Brazilian music and listeners' letters.  Broadcasts ran seven days/week, with two hours in each language, scheduled to reach listeners during the evenings in their target areas.  In the days before web SDR's, Brazilian embassies around the world were used to monitor reception quality, and recordings were sometimes played back by telephone, so the technical staff in Brasilia could hear what the broadcasts sounded like.



Eventually, though, budget cutbacks and failing equipment meant the end of the international service.  Transmitter tubes failed, and replacements were no longer available.  So, they had to reduce the number of transmitters in service, and the Amazon became the priority for coverage instead of international audiences.  The name of the station was then changed to Radio Nacional do Amazonia, broadcasting exclusively in Portuguese.

In 2018, Parque do Rodeador was classified as a critical national infrastructure resource, because in the event of a major catastrophe (such as floods, blackouts, or natural disasters), it's the only place from where the government can broadcast to the entire country, without dependence on satellites or Internet infrastructure.

This station has always been a good verifier, with QSL cards featuring iconic Brazilian tourist scenes including the seven falls at Iguazu, Rio de Janeiro with the statue of Christ the Redeemer, the Amazon rain forest, and Brazilian beaches.

Today, Radio Nacional do Amazonia still operates on the same two frequencies as back in the 1970’s – 6180 and 11780 kHz, but now with 100 kW on each.

And on April 1st this year, they reintroduced some brief programming in English and Spanish in DRM mode at 0150 UTC daily – 5 minutes in each language.

There are still six other regular private broadcasters left who transmit on shortwave, plus a handful of occasional come-and-go reactivations.  The ones you may still be able to hear are:

Radio Brasil Central from Goiânia with 10 kW on 4985 and 11815 kHz,
Radio Clube do Para from Belém with 2 kW on 4885 kHz,
Radio Clube Riberão Preto from the town of Riberão Preto on 15415 kHz,
Radio Inconfidencia from Belo Horizonte with 5 kW on 6010 & 15190 kHz,
Radio Nove de Julho from São Paulo with 10 kW on the off-channel frequency of 9819 kHz, and
Voz Missionaría from Camboriú with 10 kW on 5940, 9665 and 11750 kHz.

Back to you, Jeff.
(NWS 862/Ray Robinson)

Jen's Labor Day End of Summer Special audio available

 


Jen's Labor Day End of Summer Special - which includes GB's All That Jazz Show for August 31- is now up and ready for downloading or listening.


Link for Sunday, August 31, 2025




Next week's regular program, Jen's Eclectic Views & Real Deal  will be on September 7 at 1800-2100 UTC, but for different time zones, we may begin the program earlier...stay tuned for additional information.


For your contact pleasure

Jen In The Rad.

Weekly Propagation Forecast Bulletins

Product: Weekly Highlights and Forecasts
:Issued: 2025 Sep 01 0133 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 - 25 - 31 August 2025

Solar activity was at low levels on 27 and 31 Aug. Activity reached moderate levels on 25, 26, and 28-30 Aug. Region 4197 (S17, L=131, class/area-Eki/720 on 27 Aug) produced six M-class flares, the largest being an M4.5/1n at 26/0525 UTC. Region 4199 (N04, L=115, class/area-Cao/200 on 26 Aug) produced five M-class flares, with its largest being an M4.5 flare as well, reaching a peak at 25/0524 UTC. This region was also responsible for a long-duration M2.7 flare at 30/1911 UTC. The associated full halo CME is forecast to arrive at Earth sometime late on 01 Sep into early on 02 Sep. 

The greater than 10 MeV proton flux at geosynchronous orbit reached S1 (Minor) storm levels at 25/1355 UTC, observed a peak of 13 pfu at 27/0740 UTC, and decreased below threshold at 27/1510 UTC. Levels remained enhanced, but below the 10 pfu threshold, for the remainder of the period. 

The greater then 2 MeV electron flux at geosynchronous orbit was at high levels on 25 Aug, but returned to normal to moderate levels from 26-31 Aug. 

Geomagnetic field activity reached unsettled levels on 25-28 Aug and again on 31 Aug. Field activity was at low levels on 29-30 Aug. 

Forecast of Solar and Geomagnetic Activity - 01 September - 27 September 2025


Solar activity is expected to be at low levels, with varying chances for M-class flares (R1-R2/Minor-Moderate events) through 27 Sep. 

The greater than 10 MeV proton flux levels are expected to be slightly enhanced, but below the 10 pfu level for 01-03 Sep. There is a chance levels could exceed the 10 pfu threshold on 01-02 Sep as the halo CME from 30 Aug passes Earth. Conditions are then likely to return to near background levels after 04 Sep, barring any additional strong flare events. 

The greater than 2 MeV electron flux at geosynchronous orbit is expected to be at moderate levels on 01-02 Sep, 15-19 Sep, and 22-27 Sep. Flux levels are expected to reach high levels on 03-14 Sep and 20-21 Sep in association with coronal hole (CH) high speed stream (HSS) influence. 

Geomagnetic field activity is expected to reach G2 (Moderate) geomagnetic storm levels on 01 Sep, G3 (Strong) levels on 02 Sep, and active conditions on 03 Sep following the arrival of the halo CME from 30 Aug. Active conditions are likely on 06-10 Sep, and 15-19 Sep with CH HSS influence. Quiet to unsettled levels are
expected on 04-05 Sep, 11-14 Sep, and 20-27 Sep. 

Product: 27-day Space Weather Outlook Table 27DO.txt
:Issued: 2025 Sep 01 0133 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC webcontact www.swpc.noaa.gov/content/subscription-services
#      27-day Space Weather Outlook Table
#                Issued 2025-09-01
#
#   UTC      Radio Flux   Planetary   Largest
#  Date       10.7 cm      A Index    Kp Index
2025 Sep 01     215          20          6
2025 Sep 02     210          55          7
2025 Sep 03     200          10          4
2025 Sep 04     195           5          2
2025 Sep 05     185           5          2
2025 Sep 06     175           8          3
2025 Sep 07     160          12          4
2025 Sep 08     140          12          4
2025 Sep 09     130          12          4
2025 Sep 10     125          10          4
2025 Sep 11     125           5          2
2025 Sep 12     120           5          2
2025 Sep 13     120           5          2
2025 Sep 14     120           5          2
2025 Sep 15     120          20          5
2025 Sep 16     125          15          4
2025 Sep 17     125           8          3
2025 Sep 18     130          10          4
2025 Sep 19     140           8          3
2025 Sep 20     150           8          3
2025 Sep 21     175           8          3
2025 Sep 22     180           8          3
2025 Sep 23     180           8          3
2025 Sep 24     180           5          2
2025 Sep 25     180           5          2
2025 Sep 26     180           5          2
2025 Sep 27     170           5          2
(NOAA)

Sunday, August 31, 2025

Blog Logs-September 2025


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

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

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

Languages as indicated
// denotes station heard on a parallel frequency
*Sign-on Sign-Off*/ frequencies in kHz
Monitoring  July 1-30, 2025   

UTC, frequencies kHz 

Mediumwave
Argentina
710, Radio Diez, Buenos Aires. Spanish at 2329. Regional items to time check as “Radio Diez…veinte horas y treinta minutos…Noticias Radio Diez.” SINPO 25432. (Rudolf Grimm,  SP Brazil). 

750, Radio Salta. Spanish ads “Tienda San Juan to station promo as, “Radio Salta, la mayor potencia de radio del norte Argentino.” SINPO 25442 (Grimm).

900, Radio Provincia de Corrientes. Typical Argentine songs and Spanish items by male announcer. SINPO 24542 (Grimm). 
990, Radio 990 AM, Formosa. Spanish soccer commentary at 0100. (Grimm).


Brazil
670, Rádio Gazeta, Carazinho at 2312. Station relay of  Rádio Gre-Nal, Porto Alegre, with sports news updates and interviews. SINPO 25432 (Grimm).
690, Rádio Difusora, Londrina at 0156. Christian music format and ID as “Difusora…to ads. SINPO 34433 (Grimm).
750, Rádio Jovem Pan News, Brasilia at 0022. Political comments to interview and ID as, “Jovem Pan News” SINPO 25432 (Grimm).
890, Rádio Ubá, Ivaiporá at 2340. Commercial ads and regional time check. SINPO 24542 (Grimm).
920, Rádio Cultura, Visconde do Rio Branco at 2138. Brazilian music vocals to station ID and location (Grimm).
920 Rádio Novo Tempo, Salvador at 2150. Christian music program to station ID (Grimm).
930, Rádio Cultura, Curitiba at 2208. Station ID “ZYJ92…programa Mente Aberta.” SINPO 35543 (Grimm).

Iraq
792, Iraqi Media Network-Republic of Iraqi Radio  1610-1625. Arabic service from 1610 tune-in. Recitations to male/female comment exchanges, SIO 322 (G Van Horn, LA/Kiwi Kuwait). 

Paraguay
650, Radio Uno, Asuncion. Spanish at 2306 with sports news and soccer commentary, SINPO 35543 (Grimm).

Uruguay
1280, Radio Tacuarembo. Spanish text to Uruguayan music and announcer’s chat and reference to “Tacuarembo.” SINPO 25432 (Grimm).
1340, Radio La Voz de Melo, Spanish text to romantic 
ballads. Announcer’s “siga con nosotros…La Voz de Melo.” SINPO 25342 (Grimm).

Shortwave
Ascension Island
21660, Follow the Bible Ministries relay at 1700-1710. Swahili programming in addition to biblical themes. SINPO 45544 (Jose Ronaldo Xavier/HCDX)

Bolivia
3310, Radio Mosoj Chaqui, Cotapachi, 0040-0055. Quechua ads and comments to Andean music vocals. (Rod Pearson, FL)

Belarus
3940, Music Wave Radio 2003-2024. Russian vocals to comments. SINPO 25422. Also heard 1946-2015 in Russian (Manuel Méndez, Spain/BDXC).

Brazil (Portuguese)
5035, Rádio Educacao Rural de Coari at 1020-1026. Announcer reading messages to listeners, “bozo precisa far urgente com voce…estara te esperando para falar com…atencao rapaziada do no Urucu…bom dia bom dia.” Station sign-off at 1006. (Lucio Otavio Bobrowiec, Brazil/HCDX).

15190, Rádio Inconfidencia, Belo Horizonte, 2005-2025. Station ID/ifo to regional ads and announcer’s evening comments. (Pearson).




Cuba
4765, Radio Progreso, Bejucal 0310-0401.* Cuban salsa to Spanish service, including announcer’s comments and ID as “Radio Progreso Cadena Nacional, la onda de la Alegria, transmitiendo desde Cuba, territorio libre en  América. Cuban national anthem to 0401 closedown. (Pearson).

Egypt
9890, Radio Cairo 1915. Tentative as this station in Russian with a very poor signal.  SINPO 14222 (Sam Wright, MS)

Eswatini
9500, TWR Africa 1645-1700. Fair signal quality for Christian text and programming to an instrumental tune. (Wright).

Ethiopia
6110, Radio Fana 1720-1745. Presumed Amharic programming and mentions of Addis Ababa. Selection of Afro pop vocals with China’s Xizang station underneath. (Van Horn/Qatar Kiwi)
6030, Radio Oromiya, Addis Ababa, 1818-1836. Vernacular program comments. SINPO 15422 (Méndez).
6090, Amhara Radio 1740-1755. Lady announcer’s news script in presumed Amharic to conversation with male announcer. (Van Horn/Qatar Kiwi)


Finland
6195, RealMix Radio, Raasepori, 1951-2026. English pop songs to Spanish at 2026 “la major musica de onda corta en RadioMix Radio.” Additional pop songs. SINPO 24322. Also heard station 0443-0554 with English pop vocals (Méndez).

Germany
9670, Channel 292 via Rohrbach. German programming at 2110. Romantic ballads to announcer’s comments. Target area to Europe. SINPO 15321. (Grimm)

Japan
6055, Radio Nikkei 1 at 1200. Japanese service promoting the station’s YouTube channel. Top of the hour ID, partially in English. Cyndi Lauper's classic tune amid good signal (Tony Pavick, Canada/NASWA).

Mali
5995, Radio Mali via Bamako, 1940-2000. French service of Afro pops to announcer’s presumed soccer scores and accompanying interview (Frank Hillton, SC).

México
6185, Radio Educación de México, 0510-0700. Spanish programming of regional items and classic Mexican-themed music. (Wright).

New Zealand
7425, RNZ Pacific, Rangitaki. English at 1138, including male/female chat about New Zealand. Target to West Oceania. SINPO 15421 (Grimm).

Peru
4820, Radio Senda Cristiana, Cotahuasi (tentative)  0135-0200. Spanish comments via a very weak and fading signal. (Wright).



Philippines
9400, FEBC Radio Liangyou 1, Iba. Mandarin service at 1143. Items of interest from a female announcer. Target Area to the Far East. SINPO 25422. FEBC Manila on 9920 via Iba at 1220. Christian messages, SINPO 15321 to Southeast Asia (Grimm).

Taiwan
9490, Radio Taiwan International, Tamsui. Russian service with announcer’s comments. Target area to the Russian Siberian region. SINPO 25432 (Grimm),

United States
7730, Supreme Masters TV via WRMI. Sign on at 2059 with ID and Ian McFarland station promo. QSL info, station website info, and address. Additional programming on living the Vegan lifestyle, followed by salsa music and travelogue info on San Juan, Puerto Rico (Van Horn/SW Central Kiwi/ LA)


7730, Radio for Peace International via WRMI, 2043-2059. Lady’s interview on presumed Dari or Pashto to English ID “You are listening to Radio for Peace International.” Multilingual IDs to text about Ukraine. (Van Horn/SW Central Kiwi/LA).

9265, WINB Red Lion, PA at 0115. Christian programming to “this is WINB Red Lion, Pennsylvania, United States of America.” Followed by Spanish programming. SINPO 34433 (Wright).

Friday, August 29, 2025

UK Propagation Update

 
August 29, 2025
This week saw a change in HF propagation with a perceptible move towards more autumnal conditions.

The 10 and 12m bands have started opening up to the USA, at least on FT8. As we move into 



September this will improve further. Also, as we head towards the autumnal equinox, we can expect better conditions on north-south paths, such as the UK to South Africa.

The week saw the solar flux index climb to 226 on Thursday, the 28th, thanks to a host of sunspots, mainly in the Sun’s southern hemisphere.

Over the last seven days the Sun also provided us with 12 M-class solar flares. Any associated coronal mass ejections (CMEs) were not Earth-directed, so these had little effect and the Kp index stayed firmly at 3 or below. The latest updates suggest that there is only a 10 percent chance for a strong X-class solar flare.

FT8 continues to be the preferred HF mode, or so it seems, with stations in China, Japan, Indonesia and Cameroon making their way into UK logs on the 12m band.

The 10m band has also been humming, with South America rolling in during late afternoon and early evening. This can only get better as we move into September and October.

NOAA predicts that the coming week will start with a solar flux index of 155 on Monday, 1 September. This may be a little pessimistic, but we’ll see. It also predicts that the solar flux index will drop off as the week progresses, ending the week at 125.

Geomagnetic conditions are forecast to be good for the first half of the week, but then decline from 4 September. Batten down the hatches as a Kp index of 6 is forecast for 5 September, with unsettled conditions lasting until 10 September. Check for auroral HF signals on 5 September, or even the possibility of visible aurora from the UK.

We recommend you get your HF DXing in early next week!

VHF and up propagation news from G3YLA and G4BAO:
Last week saw some lovely late season sporadic E on the 6 and 4m bands, including Spain, Italy, and east into Ukraine. There was an opening to Brazil on the 24th that reached as far as East Anglia but, as usual, stations on the south coast and west of the country had the best of the transatlantic QSOs.

This is the last bulletin in the nominal 2025 sporadic E season, which lasts from May to August. However, last week was a good reminder not to give up too soon as there were several CW and SSB paths showing up, particularly on the 10 and 6m bands. There were also a few reports on the 4m band.

The daily sporadic E blogs on propquest.co.uk come to an end Sunday, 31 August, but the site will continue to provide the maps as usual. To help you, notes on how to interpret the maps are available on the website. Thanks to all the sporadic E operators who have submitted logs to the various clusters this year.

The change over to unsettled weather is now complete and we will see rain and thunderstorms in most areas from time to time. It’s a good period to check out rain scatter propagation if you are set up for the gigahertz bands.

The heavier rain is well-captured by the many online rain radar displays to help you track the most active scattering volumes, which move with the stronger winds quite high up in the atmosphere. Speeds of 30 to 60 miles per hour are common.

There is one note of contrast with the model evolution after midweek. One branch sticks with low pressure to the following weekend, while another outcome tries to bring in a ridge of high pressure and a chance of tropo propagation. If the latter turns out to be the actual evolution, it may prove useful for the 144MHz Trophy and Backpackers Contest next weekend. However, it may not have arrived in time for the 144MHz UK Activity Contest on Tuesday.

The solar conditions are still providing some interest for auroral propagation, but with a Kp index less than 3, nothing of use radio-wise. Look for a Kp index increase beyond 7 for that. Meteor activity is currently between major showers so expect random activity, which suggests early mornings for checking out meteor scatter prospects.

Moon declination is negative, reaching a minimum on Monday, 1 September. So, it’s a week to check out your equipment rather than to operate. With the Sun still high in the sky, it’s easy to check system performance with Sun noise. Path losses started to fall after apogee on Friday, 29 August. 144MHz sky noise is close to 3,000 Kelvin on Monday, dropping back to moderate on Wednesday.
 
(Mike Terry/BDXC)

Radio Blacksmith Knoll set for weekend broadcasts

 


Finland

Radio Blacksmith Knoll, a low-powered station airing from Finland, will broadcast on the following schedule

6120 kHz 

Please note that although our license allows 24-hour broadcasting, we may not always be on air continuously on the listed days.

August 30, 2025 
2100 UTC  (24 hour scheduled)  with chill vibes and dreamy night tunes to snooze like a pro!
Freeform, unscripted programming

August 31  Freeform, unscripted programming





Music Programs on Shortwave update available

An updated version (Version 4) of my Music Programmes on Shortwave PDF file for the current A-25 broadcast season is now available to download from the permanent link at:



Note that you will also find here my at-a-glance programme grids for BBC WS*, VO Turkey*, CGTN R, R Romania Int and R Taiwan Int* (* have been recently updated).
I hope that you find these of interest.
As always, I appreciate any updates or corrections. 
(Alan Roe, UK/BDXC) 

Thursday, August 28, 2025

Active Brazilian Stations on Mediumwave

 


Active Brazilian Stations on Mediumwave
The following list represents Brazilian stations on mediumwave that are actively being heard. As the shift from AM to FM for various Brazilian stations, this list may be adjusted frequently. Your additional information and observations are welcome at: w4gvhla@gmail.co

Broadcast in Portuguese

Brazil
570         Rádio Eldorado, Criciuma, SC
580         Rádio América, Uberlândia, MG
580         Rádio Relógio Federal, São Goncalo, SP
590         Rádio 79, Ribeirão Preto, SP
610         Rádio Itatiaia, Belo Horizonte, MG
620         Rádio Assunção Cearense, Fortaleza, CE
620         Rádio Jandaia, jandaia do Sul, PR
640         Rádio Deus é Amour, Londrina, PR
650         Rádio Difusora, Piracicaba, SP
670         Rádio Gazeta, Carazinho, RS
690         Rádio Difusora, Londrina PR
720         Rádio Difusora, Casa Branca, SP
730         Rádio Cidade, Jundiai, SP
750         Rádio América, Belo Horizonte, MG
750         Rádio CBN Vale, São José do Campos, SP
750         Rádio Jovem Pan News, Brasilia, DF
760         Rádio Manchete, Rio de Janeiro, RJ
810         Rádio Cancão Nova, São José de Rio Preto, SP
820         Rádio Jauense, Jauú, SP
830         Rádio Tropical, Nova Iguacu, RJ
840         Rádio Bandeirantes, Sáo Paulo, SP
850         Rádio Difusora, Campos de Goytacazes, RJ
870         Rádio Central, Campinas, SP
870         Rádio São Francisco do Sul, SC
880         Rádio Inconfidencia, Belo Horizonte, MG
890         Rádio Difusora, Bento Goncalves, RS
890         Rádio Ubá, Ivaiporã, PR
910         Rádio Venãcio Aires, Venãncio Aires, RS
920         Rádio Cultura, Visconde do Rio Branco, MG
920         Rádio Novo Tempo, Salvador, BA
930         Rádio Cidade, Caxias do Sul, RS
930         Rádio Cultura Curitibe, PR
950         Rádio Aleluia, Belo Horizonte, MG
960         Rádio Deus é Amor, Aparecida de Goiania, GO
970         Rádio Difusora, Marechal Candido Rondon, PR
970         Rádio Piratininga, São da Boa Vista, SP
990         Rádio Contemporánea, Rio Janeiro, RJ
990         Rádio Cultura Regional, Dois Córregos, SP
1010 Rádio Difusora, Lencois Paulista, SP
1020 Rádio Educacao, Limeira, SP
1030 Rádio Difusora, Franca, SP
1030 Rádio Emissora da Barra, Barra Bonita, SP
1050 Rádio Deus é Amour, Vitoria, ES
1060 Rádio Educadora, Piracicaba, SP
1080 Rádio Deus é Amor, Juiz de Fora, MG   
1080 Rádio Monumental, Aparecida, SP
1090 Rádio Metropolitana, Rio de Janeiro, JP
1120 Rádio Clube, São José dos Campos, SP
1130 Rádio Princesa do Oeste, Xanxerê, SC
1140 Rádio Bandeirantes, Rio Claro, SP
1160 Rádio Cacique, Taubaté, SP
1160 Rádio Luz e Alegria, Frederico Westphalen, RS
1170 Rádio Vanguarda, Ipatinga, MG
1180 Rádio Cultura, Alfenas, MG
1190 Rádio Regional, Taquarituba, SP
1210 Super Rádio, Brasilia, DF
1250 Nossa Rádio, Veapasiano, MG
1270 Rádio Brasil Central, Goiania, GO
1290 Rádio Novo Tempo, São José do Rio Preto, SP
1310 Rádio Coronados, São Fidélis, RJ
1320 Rádio Tropical Gospel, Curitiba, PR
1320 Rádio Vitória, Videira, SC
1340 Rádio Jornal da Manhã, Ijui, RS
1350 Super Rádio Boa Vontade, via Rádio Cristal, Salvador, BA
1360 Rádio Bandeirantes, Rio de Janeiro, RJ
1370 Rádio Cancão Nova, Curitiba, PR
1380 Rádio Cidade, Brasópolis, MG
1410 Rádio Santa Rosa, Santa Rosa, RS
1420 Rádio Guarujá, Florianópolis, SC
1430 Rádio Estacão Portão, Portão , RS
1430 Rádio Serra Negra, Serra Negra, SP
1430 Rádio Campinas, Campinas do Sul, RS
1460 Rádio Campinas, Campinas do Sul, RS
1470 Rádio Absoluta, Campos dos Goytacazes, RJ
1470 Rádio Mensagem, Jacarei, SP
1480 Rádio Boituva, Boituva, SP
1500 Rádio Aparecida do Sul, Ilicínea, MG
1510 Rádio Teresópolis, Teresópolis,, RJ
1520 Rádio da Cidade, Mogi das Cruzes, SP
1530 Rádio Sulina, Dom Pedro, RS
1540 Rádio Cultura, Leme, SP
1540 Rádio Deus é Amor, Sertãozinho, SP
1550 Rádio Cacique, Capnivari, SP
1550 Rádio Imperial, Petrópolis, RJ
1560 Rádio Jornal, Leopoldina, MG
1590 Rádio Cultura, Andirá, PR

Brazilian States
AC: Acre
AL: Alagoas
AM: Amazonas
AP: Amapá
BA: Bahia
CE: Ceará
DF: Distrito Federal
ES: Espírito Santo
GO: Goiás
MA: Maranhão
MG: Minas Gerais
MS: Mato Grosso do Sul
MT: Mato Grosso
PA: Pará
PB: Paraíba
PE: Pernambuco
PI: Piauí
PR: Paraná
RJ: Rio de Janeiro
RN: Rio Grande do Norte
RO: Rondônia
RR: Roraima
RS: Rio Grande do Sul
SC: Santa Catarina
SE: Sergipe
SP: São Paulo
TO: Tocantins   
(Rudolf Grimm/Gayle Van Horn via Teak Publishing)
(copyright 2025-2026/Teak Publishing)

Monday, August 25, 2025

Audio for Jen's Eclectic Views & Real Deal for August 24, now available

 


 Jen's Eclectic Views & Real Deal for August 24 is now up and ready for you! 

 Jen's Cast Link


 Live Stream for next week will be on Sunday, August 31, from 1800 to past 2200 UTC. There will be additional information as we move closer to programming..

 GB's All That World Jazz Show, and then I go on with my Labor Day End of Summer Special.


 For your contact's pleasure

 Jen In The Rad

The Transatlantic Race to Create Television

 A special thank you to Ray Robinson and Jeff White for sharing this week's Wavescan - with an interesting tie-in to radio !

Partially sourced from:
https://theconversation.com/the-transatlantic-race-to-create-the-television-258726
Published June 12, 2025


Jeff: We don’t often talk about television on Wavescan, but there’s a very interesting story of how it was first developed back in the 1920’s and 30’s, and it does include radio.  Various countries lay claim to the invention, but what was the reality?  Here’s Ray Robinson in Los Angeles, who has been uncovering the truth.

Ray: Thanks, Jeff.  Yes, when I was growing up in England, we were always taught that Scotsman John Logie Baird had been the inventor of television.  I was quite surprised when, in my 20’s at work, I met a Russian co-worker who insisted it had been a Russian.  And then when we came to the States in the 1980’s, I found that people here thought it was an American – either Charles Francis Jenkins (who I hadn’t heard of before), or Philo Farnsworth (who I had).  So, what was the true story?  It turns out it was a mixture of all of them, plus a number of others!  In fact, it became something of a race.  Let me explain.

Number 1519 Connecticut Avenue lies just north of Dupont Circle, about a 20-minute walk from the White House in Washington, DC.  In 1921, the inventor Charles Francis Jenkins set up his laboratory and offices there, upstairs from a car dealership.

Today there are no obvious external indications of this famous resident, nor of his exceptional achievements, awards and numerous patents.  Just over 100 years ago at his laboratory, on June 13, 1925, Jenkins gave a demonstration of a televised film sent by radio waves from a building about 4 miles away in what is now the US Naval Research Laboratory in Bellevue, on the southern outskirts of the District of Columbia.

The invited group of mostly government officials included the secretary of the Navy, Curtis D. Wilbur.  They watched with fascination a film that showed a silhouette of a toy windmill with its blades in motion.  The television picture comprised 48 lines, refreshed at the silent-movie rate of 16 frames per second.

By July 1925, Jenkins had demonstrated vision and sound transmitted together on a single short-wave radio frequency.  The published technical details indicate a high degree of sophistication in his designs, as might be expected from someone with a background in precision phototelegraphy (the transmission of images over wires).  In the early 1920’s he had developed a practical means of sending images of weather charts by radio to ships at sea.  It was this phototelegraphy work that led him into experiments in televising silhouettes of live and filmed scenes.

Parallel development
But, the Scottish inventor John Logie Baird beat him to become the first to perform a public demonstration of a similar mechanical television system, in London, over three weeks in March and April 1925.  Baird, who had been working on the technology since early 1923, showed live moving images in reflected light transmitted by radio to enthusiastic crowds in Selfridges department store on Oxford Street in London’s West End.  With only eight lines per picture, he carefully chose simple objects that would be easily identifiable.

For the demonstration, he had built a television studio in Covent Garden, less than half a mile away, and experimented with a small transmitter.  By January of the following year, 1926, he gained widespread recognition for being able to demonstrate 30-line television showing recognizable facial features in reflected light.

But in order to gain more funding which would require the sale of television receivers, he soon realized he needed a much more powerful transmitter to broadcast his programs.  The BBC had such a transmitter, 2LO, which was conveniently located on the roof of Selfridges.  2LO was used for daily 'wireless' programs, but the BBC service closed down in the evening at about 11pm and often didn’t re-start until mid-morning.  So, Baird approached the BBC for permission to use the transmitter during the overnight periods.  Eventually the BBC reluctantly agreed, and by the end of 1929 Baird was running a program of regular television broadcasts which would continue for the next six years.  Unfortunately, at first the BBC only had the one transmitter (for television you need two; one for the picture and one for the sound).  It meant that for the first six months, television programs comprised two minutes of picture, followed by two minutes of sound and so on.  By March 1930 the BBC had opened a second radio transmitter, and so simultaneous sound and picture transmissions began. 

In the United States, meanwhile, Jenkins had doubled down on improving the image quality for his demonstration.  He launched his silent silhouette video service for hobbyists on radio station W3XK in July 1928, around the same time as similar offerings from companies that included General Electric (GE) and the Radio Corporation of America (RCA).  By the end of 1928, there were thought to have been as many as 15 experimental television stations operating in the United States.

Like Baird’s and Jenkins’ methods, many of these early stations relied on mechanically rotating disks with patterns of holes to scan images line by line.  They were all very low on detail, but were still heralded as proof of concept for television.  A key factor in their acceptance was the uncanny ability of human vision to recognize facial expressions along with natural body motion in poor quality images.

Back in the UK in 1928, Baird went on to demonstrate color television, early 3D stereoscopic television, and transatlantic television all for the first time, though more as a way of attracting financial backing than presenting prototypes of future offerings.

What came next
But, those mechanical systems were short-lived.  


Many scientists and engineers felt that mechanical television, using spinning discs, was not the answer to television.  They felt that the answer lay in a form of electronic television and its champions were:  Vladimir Zworykin at RCA in the USA; Isaac Shoenberg's team at EMI (Electric and Musical Industries) in the UK; and a fourteen-year-old farm boy from Idaho called Philo Farnsworth.

It took Farnsworth six years to take his system from first ideas to prototype – and by 1929 he was the first to demonstrate a complete electronic television system with no moving parts.  But he was soon overtaken by other inventors and faded from the scene.

RCA and EMI focused their respective resources on developing vastly superior electronic television systems.  These scanned and reproduced images using electron beams that are fired inside a cathode ray tube to capture and show the transmitted moving picture on the screens of people’s TV sets.  Those pictures had 


around 100 times the information content of the earlier mechanical systems, and they used ideas from scientists such as Boris Rosing in Russia and Alan Archibald Campbell-Swinton in the UK.

Sadly, Charles Jenkins didn’t live to see those new electronic systems.  His health began deteriorating in late 1930, and he died in 1934 aged 66, leaving behind a superb legacy of a career in inventions.

In the summer of 1934, the British government set up a committee, chaired by Lord Selsdon, to investigate the possibility of providing a high-definition television service to replace the low-definition 30-line transmissions already taking place.  At that time Baird's improved mechanical television system had had the benefit of nearly ten years of development since its invention whilst the EMI electronic system was still in its infancy.

The picture quality of the two systems at that time was similar, and so the Selsdon committee recommended that 'two television systems of High-Definition Television should be tried at the London Station'.  The London Station was to be built and operated by the BBC, and the two systems (Baird and EMI) would broadcast on alternate weeks for a trial period of six months.  The government defined High-Definition as 'not having less than 240 lines per picture' and Baird set to work to increase his system to meet the 240 line threshold.

At EMI, Isaac Shoenberg took the courageous decision to develop an electronic system which had 405 lines.  This leap of faith, based on advice from his research team (over 60 strong), would have financially ruined the company had it failed.
The Baird Company set to work to design and build all the equipment for a complete television station, including the transmitters.  EMI on the other hand felt that they didn't have the expertise in transmitter design, but they knew a man who did - Guglielmo Marconi - so a new company, Marconi-EMI, was formed to deliver the entire electronic station.

Alexandra Palace
Meanwhile the BBC, tasked with providing a suitable building complete with the studios, sound transmitter, mast and aerials - all within 18 months - began a frantic search for a suitable site.  Alexandra Palace, a run-down Victorian entertainment complex in North London, was not their first choice.  However it had a couple of significant advantages:
1) part of it was available for rent, and
2) it was on top of a hill.
The BBC knew that it was vital to get the transmitting aerials as high as possible. Calculations showed that to get a reliable range of 25 miles reception with a 34 kW transmitter in VHF band 1, the aerial had to be about 600 feet (180 metres) above sea level. Alexandra Palace was already half that, so the transmitting tower only needed to be another 300 feet (90 metres) tall.

The summer of 1936 saw a hive of activity as everyone worked frantically towards the official opening date of early November - but all that was about to change.

Olympia Broadcast
The 1936 Radio Show at Olympia, in London was scheduled for the end of August. RadiOlympia was an annual exhibition put on by the Radio Manufacturers' Association, and a number of the exhibitors were displaying new television sets. Concerned that there would be no programs to display on them at the show, the BBC came under pressure to provide demonstration transmissions during August.  A variety show was quickly put together called 'Here's Looking at You', and it went out twice a day for two weeks, with the two competing television systems alternating on a daily basis.

BBC Television formally opened a regularly scheduled service on 2 November 1936 at 3pm, with speeches by the Postmaster General, the Chairman of the BBC, and Lord Selsdon.  The opening ceremony actually took place twice; first (on the toss of a coin) in front of the Baird cameras, and then again with the Marconi-EMI system.  In this way, BBC television's second programme was also its first repeat.  The first program following the official opening on 2 November was a bulletin of British Movietone News.  Other programs transmitted on that day included variety pieces and the first TV documentary, Television Comes to London.

The new BBC Television Service had started, and it was the first regularly scheduled true high-definition television service in the world.  With the two systems alternating on a weekly basis, it was soon clear that Marconi-EMI were offering superior performance.  The decision was taken to end the competition early, and after only three months the final Baird transmission went out at the end of January 1937.  John Logie Baird continued to work as a TV pioneer in the late 1930’s and early 1940’s, dedicated to exploring color television and cinema projection.  He died in 1946 at the age of just 57.


In the USA, by the late 1930’s, RCA had developed a 441 line system which was adopted by their NBC TV network, but then in 1941, under pressure from competing technologies, the FCC formed a committee called the NTSC, which decided to standardize on a 525 line system.  That of course was black and white, but a compatible standard for color television was adopted in 1953, and the first program broadcast coast-to-coast in color was the January 1st 1954 coverage on NBC of the Rose Parade from Pasadena, California.



After a short break during World War II, the British 405-line television service continued for several decades.  It was supplemented in 1955 by the introduction of a commercial TV service – Independent Television, or ITV, in VHF Band 3.  And that 405 line black and white system is what I grew up with in England during the 1950s and 60’s.  Alongside the 405 line system, a superior quality 625 line system was introduced on UHF in 1964, and then color television using the compatible PAL standard was gradually introduced, program by program, from 1967 onwards.  The 405 line black and white VHF service was finally shut down at the start of 1985, more than 48 years after it had officially been launched.

Jenkins’ and Baird’s original pioneering efforts, and the excitement they generated, are still rightly heralded by many people today.  We can now only imagine how it must have felt to see moving images transmitted from miles away for the first time. It’s incredible to reflect that what was once considered magic so quickly became mundane.  Back to you, Jeff.

Norway is back on 190 metres!

 

The Bergen Broadcasting Association (FBK), where I am CEO/Editor-in-chief, is operating a local radio station on FM (88.6/93.8/100.3 MHz) and an AM/medium wave station on 1314 kHz. We also have a Shortwave station on 5895 kHz.
FBK is actually operating the only remaining AM stations on the Norwegian mainland*).
The second AM/medium wave transmitter on "Askøysenderen" operated on the Norwegian frequency 1611 kHz from the summer of 2014 to August 2019 with 70 watts, and then with 750 watts until the end of 2023.
It is now back on the air. Yes, we have moved the fine station Radio Northern Star (RNS) a bit further down the medium wave band to 1575 kHz, 190 metres!
The station is radiating the international program of RNS, with announcements in 8 languages //5895 kHz.
We started on Thursday, August 21st at 1940 UTC thanks to great efforts from LB6II and a couple of sponsors. Adjustments followed on Friday, August 22nd.
1575 kHz was allocated to us in early June 2025 after we had applied to NKOM in 2024 with three frequency alternatives. A 6-year licence was subsequently granted by the Norwegian Media Authority.
The 1575 licence is for 6 years and currently allows a transmitter power of 1 kW ERP.
The application and coordination process took a very long time and required a lot of patience, but was carried out very professionally by NKOM with strict adherence to all deadlines for objections from neighbouring countries. However, there were no objections and no competing applications.
We are very grateful to the Norwegian media authorities who have shown us so much trust for 13 years now by granting another broadcast license to transmit from the old Askøy Kringkaster/Bergen Mellombølgesender which originally broadcast NRK Bergen Lokal until May 22, 1966 and NRK Riks until November 1, 1978.
Our fine radio amateurs have been crucial in making this happen.
At the same time as 1575 started, we announced in the DX press and to DX correspondents that we intended to start broadcasting on the new 1575 in early autumn 2025, initially //5895 kHz.
It is possible that more AM frequencies will be advertised in Norway in due course. It is good that the media authorities are still focusing on this band.
Initially, our 2 kW transmitter will be used, initially with approx. 500 watts, eventually up to @750 watts, and the previous inverted V antenna from 2014 that was used for 1611 has been put back into use. Any need for modifications to the antenna will be considered over time.
At 1611, the "inverted V" antenna had a modest performance over Western Norway during the day, but it had a very good skywave and was heard in Canada and 15++ other countries, between Finnmark and Sicily.
The antenna seems to have the best coverage towards the northwest/southeast.
The 1611/1575 and 5895 stations have been operated by a Co-Op within FBK for the past 3 years, which has contributed a lot of effort and finances.
The 1314 station with FBK's Bergen Kringkaster program is running with better sound and higher power than before.
We hope for support from radio amateurs, DXers, the local radio stations, as well as more sponsors and other radio enthusiasts who want to contribute.
It is important to be on the AM bands. The range is unmatched and it is becoming more and more important to be on the alert.
Finally a little history: According to the Copenhagen Plan which was in force until 23rd November 1978, Norway had two transmitters (LKF Fredrikstad 10 kW and LKN3 "Nordkapp" (Honningsvåg) 2 kW) on 1578 kHz and these shared the channel with RAI Genova/Portofino in Italy 50 kW (+19 low-power transmitters) and Emissora Ass. do Lisboa in Portugal 10 kW. These former Norwegian sites were even monitored in Australia and New Zealand.
On the side was 1575 Sharjah Broadcasting 50 kW and 1580 VOA Ban Pachi 1000 kW which were also often heard. So the channel will be less crowded now!
We send our best regards to other official users of 1575 in Italy, Spain and England.
We hope we are heard far away!
So far listener reports have been received from Norway, Sweden, Denmark and Finland.
Correct reception reports should be sent to styret2025 at bergenkringkaster.no and 1000 at northernstar.no and will be answered with eQSL.
*) Svalbard Kringkaster on 1485 kHz in Longyearbyen, which broadcasts NRK P1, is still broadcasting. It has been improved and is now heard regularly in North America.
SvennM
CEO/Chief Editor
Bergen Broadcasting As
(Facebook post by Svenn Martinsen, August 24th)
(Mike Barraclough/BDXC)_

Mediumwave news update

 
After its tower was swept away in the flooding caused by Hurricane Helene last September, Jet Broadcasting has completed the rebuild of the former “SportsRadio 1420” WEMB Erwin, Tennessee. .

WEMB is now operating from the tower site of co-owned “Livewire 103.9” WXIS and stunting with sounds of jets taking off along with prerecorded announcements hyping the station’s new format. WEMB will debut programming on Friday, August 22 with the start of the Unicoi County High School football season.

Owner Maria True stated in a Facebook live video discussing the rebuild that WEMB will flip to a Talk format focusing on “positive, non-political” topics.
https://radioinsight.com/headlines/307134/

Lance Venta, Radio Insight (2025-08-21)
(Ydun's MW)

Weekly Propagation Forecast Bulletins

 Product: Weekly Highlights and Forecasts
:Issued: 2025 Aug 25 0309 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 18 - 24 August 2025

Solar activity was at low levels on 18, 20, and 21 Aug with only C-class flares observed. Activity increased to moderate levels on 19 Aug following an M1.1 flare at 19/0439 UTC from an area beyond the Eastern limb. Moderate levels were also observed on 22 Aug as Region 4191 (N11, L=172, class/area=Ehi/360 on 24 Aug) produced a long-duration M1.7/Sf flare at 22/1851 UTC. Associated with this flare was a Type II radio sweep with an estimated shock speed of 521 km/s. The associated CME was deemed to be behind the Sun-Earth line. Moderate levels continued into 23 and 24 Aug with an M1.9 at 23/2006 UTC and an M1.3 flare at 24/0836 UTC, both originating from beyond the NE limb. While multiple CMEs were observed in coronagraph imagery over the period, nearly all were at or beyond the Eastern limb and none were considered to have an Earth-directed component. 

The greater than 10 MeV proton flux at geosynchronous orbit was at background levels from 18-22 Aug. Beginning around midday on 22 Aug, flux levels began to rise following the long-duration M1.7 flare event, mentioned above. Levels continued to rise, eventually reaching a peak of 8.3 pfu at 24/2330 UTC, but never exceeded the greater than 10 pfu levels. 

The greater than 2 MeV electron flux at geosynchronous orbit was at normal to moderate levels on 19-20 Aug, and 22-23 Aug. Activity reached high levels on 18, 21, and 24 Aug, with the peak observed value of 2,200 pfu at 18/0830 UTC. 

Geomagnetic field activity was at quiet to unsettled levels on 18 and 24 Aug, bookending a negative polarity coronal hole high speed stream. Unsettled to active conditions were observed on 20-23 Aug as CH HSS activity elevated, with active to minor storm levels observed on 19 Aug. 



Forecast of Solar and Geomagnetic Activity 25 August - 20 September 2025

Solar activity is expected to be at low levels, with varying chances for M-class flares (R1-R2/Minor-Moderate events) through 20 Sep. 

The greater than 10 MeV proton levels are expected to be at or above 10 pfu levels on 25 Aug before dropping below the 10 pfu level by 26 Aug. Levels should remain below thresholds through 20 Sep, with no additional events expected at geosynchronous orbit. 

The greater than 2 MeV electron flux at geosynchronous orbit is expected to be at moderate levels on 25-26 Aug, 29 Aug-5 Sep, and 15-19 Sep. Conditions are likely to see high levels on 27-28 Aug, 6-14 Sep, and again on 20 Sep. 

Geomagnetic field activity is expected to be at mostly quiet levels on 29 Aug-3 Sep and again on 11-14 Sep. Unsettled levels are likely on 25-28 Aug, 7-10 Sep, and 17-20 Sep. Active conditions are likely on 4-9 Sep and 15-16 Sep, with possible minor storming on 4-6 Sep and 15 Sep. All increased activity levels are associated with coronal hole high speed stream influence. 

Product: 27-day Space Weather Outlook Table 27DO.txt
:Issued: 2025 Aug 18 0120 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 2025-08-18
#
#   UTC      Radio Flux   Planetary   Largest
#  Date       10.7 cm      A Index    Kp Index
2025 Aug 18     115          12          3
2025 Aug 19     110          30          5
2025 Aug 20     110          18          4
2025 Aug 21     110           8          3
2025 Aug 22     110           8          3
2025 Aug 23     120           5          2
2025 Aug 24     125           5          2
2025 Aug 25     120           8          3
2025 Aug 26     120           8          3
2025 Aug 27     125          10          3
2025 Aug 28     125          12          4
2025 Aug 29     130           8          3
2025 Aug 30     130          10          3
2025 Aug 31     140          10          3
2025 Sep 01     150           8          3
2025 Sep 02     150           5          2
2025 Sep 03     140           5          2
2025 Sep 04     140          20          4
2025 Sep 05     135          35          6
2025 Sep 06     130          20          4
2025 Sep 07     130          15          3
2025 Sep 08     130          15          3
2025 Sep 09     120          15          3
2025 Sep 10     120          10          3
2025 Sep 11     115           5          2
2025 Sep 12     110           5          2
2025 Sep 13     110           5          2
(NOAA)

Saturday, August 23, 2025

Jen's Ecletic Views & Real Deal audio for August 17, now available

 

Jen's Eclectic Views & Real Deal for  August 17, is up and ready for downloading or listening 

Due to Personal issues, last Sunday's Cast is now coming out.


Live Stream Next Week, 
Jen's Eclectic Views & Real Deal for Sunday August 24, at 1800-2100 UTC.


For your contact pleasure

Jen In The Rad.