Monday, October 12, 2026

Azad (Free) Kashmir Radio, Part 1

 
Photo via Wikipedia

AZAD (FREE) KASHMIR RADIO (AKR), Part 1

Thank you to Ray Robinson and Jeff White of Wavescan for sharing Adrian's nostalgic trek to the Pakistan border 

Jeff: Wavescan’s editor-in-chief as I’ve just mentioned, is Dr. Adrian Peterson, N9GW, who served with Adventist World Radio for decades, mostly in Asia.  He was primarily stationed in Poona, India, but during his time there, he visited many other countries in the region.  Among notes he has passed to Ray Robinson, we found a write-up of a trip Adrian had made in the 1980’s to the Pakistani side of the disputed territory of Kashmir, which is known as Azad Kashmir (or, ‘Free’ Kashmir).  He went station hunting, literally, and here to read Adrian’s report is Ray Robinson.

Ray: Thanks, Jeff.  Adrian wrote:

During the 1960's and 70's, there was a great deal of confusion and speculation among international radio monitors regarding the authenticity of a station identifying itself on air as "Azad Kashmir Radio".  This station had been logged in the tropical shortwave bands in several countries of Asia, as well as in Australia, New Zealand, and even occasionally in Europe and the United States.  Two different identification announcements had been heard stating, "Azad Kashmir Radio, Muzaffarabad", and "Azad Kashmir Radio, Trar Khel".

A partial answer to this intriguing situation had been supplied by two men well-known in the radio world, U. S. diplomat and DXer Gregg Calkins, and noted international radio monitor in Sri Lanka, Victor Goonetilleke.  Gregg visited the station in Muzaffarabad in 1975 while stationed in Pakistan, and Victor had made some astute monitoring observations from his residence in Colombo, Sri Lanka.

So what was the status of Azad Kashmir Radio?  In reality how many stations were there?  How many transmitters carried the AKR programs?  When was the station inaugurated?  All of these questions needed an answer.

Now, back in 1983, while stationed in India, I was making plans for an itinerary into neighboring Pakistan on AWR business.  So, I thought, why not make a side trip up into Azad Kashmir, and find out for myself just what the answer was to the mystery of Azad Kashmir Radio?

Historically, the large verdant vale of Kashmir, up against the foothills of the high Himalaya, has been fabled through the years in song and poem.  This productive valley has been the prize of king and conqueror, and at the height of its power and prosperity, was an independent mountain kingdom, with the two main towns being Jammu and Srinagar.  At the time of partition between India and Pakistan in 1947, Moslem claims to Kashmir became a major cause of dispute between the two neighboring powers, and a subsequent war erupted.  At the time of ceasefire in 1949, India held the major portion of the territory, including the prized valley, and Pakistan retained only a narrow mountainous strip along the western edge.  This small and rugged territory was given a new name, Azad Kashmir (in Urdu), or in English, Free Kashmir.  It’s a long, thin crescent-shaped territory, about 150 miles long north-south and maybe 30-50 miles wide, with a population of around 4½ million, and it’s administered as an autonomous territory by Pakistan.

Adrian continued:
Although I had been into Indian-held Kashmir on two previous occasions (and while there I saw India's Radio Kashmir), this was my first visit to Azad Kashmir.  When the appointed duties of my Pakistan itinerary were completed, I boarded a country bus in the capital city, Islamabad, for the arduous journey up into mountainous Azad Kashmir.  Soon we were in the hilly areas, and for many hours, the bus bumped over narrow winding, unpaved roads, cut into the rock along the edge of steep gorges, several thousand feet deep.  Here in these localities, it is the practice of drivers to pass each other slowly on the wrong side of the road, so that correct judgment can be made regarding the rising cliff on one side and the falling ravine on the other.

On a sunny Asian afternoon, the bus arrived in Muzaffarabad, the tiny capital city in the north of Azad Kashmir.  This is a typical Himalayan town located in a picturesque area of the mountains near the confluence of two large rivers.  The town hugs the sides of the hills and the usual bazaar runs the length of the main street.  I checked into what might euphemistically be called the “best” local hotel.

In the late afternoon, I walked the town, and the next morning I went up to the radio station, which was clearly identified by a large sign, "Azad Kashmir Radio".  It was located at the upper end of the bazaar area, with a delightful view of the valleys and mountains and an overview of the town.  I was received by the Director and he authorized an official tour of his station.  It had been inaugurated there on October 15, 1961.

The main building on the small AKR estate housed the studios and offices for "Azad Kashmir Radio, Muzaffarabad".  At the time of my visit, a music recording session was under way, with several local musicians sitting in little clumps on the carpeted floor.  It was reminiscent of music recordings in my own radio studio for Adventist World Radio back in Poona, India.

The second and smaller building contained two transmitters, a 1 kW unit radiating in the 3 MHz tropical shortwave band, and a 10 kW AM unit radiating on 1510 kHz.  As I left the property, I glanced at the three masts which support the low-slung AM and shortwave antennas.

At the time of my visit, a new 150 kW transmitter was radiating test transmissions on 792 kHz medium wave.  This unit was at a new location on a knoll overlooking the highway just before entering the other end of the town.  This new unit was testing on air at midday local time on 792 kHz and it was brought into regular service a month later.  The antenna appeared to be a 5/8th wave vertical radiator.  It is probable that the older 10 kW AM unit was removed from service soon after the new 150 kW transmitter assumed regular broadcasting.

This was a sign-on of Azad Kashmir Radio, Muzaffarabad in September 2006:

Audio Clip - 2006 09 03 - Pakistan - Azad Kashmir Radio, Muzzafarabad - sign on available at: https://www.podomatic.com/podcasts/wavescan

So, at least, part of the mystery was now solved.  Azad Kashmir Radio, Muzaffarabad was indeed a legitimate radio broadcasting station, radiating local programs on a tropical band channel.  The low power output accounted for the fact that the station was not heard regularly at great distances.  But, what about the other station with the identification of "Azad Kashmir Radio, Trar Khel"?

The next day, I boarded another bus for the rugged return journey back into Pakistan, but this time traversing the southern route out of Azad Kashmir, via Trar Khel.  Although Trar Khel was briefly the capital "city" of Azad Kashmir, it is in reality no more than a small, unheralded village.

While in this second locality I enquired about AKR Trar Khel, and several people knew nothing about it, perhaps intentionally.  I then talked with the postmaster, and he told me that all mail addressed to AKR Trar Khel is bundled up and forwarded to an address in Rawalpindi.  So that, then, was the answer.  AKR Trar Khel is not located in Trar Khel at all, but rather in Rawalpindi, Pakistan.

Before leaving the area, I tuned in to the channels used for the broadcasts from the two AKR stations, and was surprised that reception from both stations was particularly poor in Trar Khel.

When I returned to the twin city complex in Pakistan, Islamabad - Rawalpindi, I discovered that AKR Trar Khel is indeed located in Rawalpindi.  Program production for this station takes place in its own studio complex, which is located on a main thoroughfare running through the city.  On many occasions I had seen this modest and unidentified white building without realizing its significance to the radio world.  It is located within walking distance of the city's only regular radio station, Radio Pakistan, Rawalpindi.

The programs of Azad Kashmir Radio, Trar Khel were broadcast from a 10 kW transmitter located at the large shortwave base operated by Radio Pakistan.  This base, 15 miles out of town along the Grand Trunk Road towards Lahore, was actually two bases side by side.  There were believed to be eight active transmitters at that location, with output powers of 10, 100 and 250 kW.  One of the original 10 kW transmitters in the older of the two bases was the one used for the programs of Azad Kashmir Radio, Trar Khel.  (The WRTH and other international radio publications listed the "Trar Khel" - Rawalpindi transmitter as being 100 kW, but my experience would suggest that usually a 10 kW transmitter was used.)

Interestingly, even though this was supposed to be a somewhat clandestine operation, the local village people near the transmitter base were ‘in-the-know’ and listened to Azad Kashmir Radio, "Trar Khel" on their small transistor receivers.  Although this outlet purports to be located in Trar Khel, half a day's journey by bus across the mountains, it is in reality broadcasting to Trar Khel and not from Trar Khel.

This was a sign-on from Azad Kashmir Radio, Trar Khel in October 2016:

Audio clip - 2016 10 00 - Pakistan - Azad Kashmir Radio, Trar Khel - sign-on available at: https://www.podomatic.com/podcasts/wavescan

Ironically, there once was a small radio station actually located in the village of Trar Khel – a mobile unit which began broadcasting on April 16, 1948.  The studio was housed in an army truck and a low-powered tropical-band transmitter was in another.  Although it is not known how long the station was on the air, it is probable the station was in use for no more than a few months at the most.  It is not known exactly when programming was transferred from the mobile units in Trar Khel back to the permanent site in Rawalpindi, although still announced as AKR Trar Khel. However, an FIBS listing shows two shortwave channels in use for AKR Trar Khel in 1949, so it is probable the Rawalpindi facility of AKR came into operation at the end of 1948.

Use of shortwave for broadcasting in and from Pakistan ended in 2021.  But they do still make quite a lot of use of medium wave in that part of the world, and if you open this year’s edition of the WRTH, what do you find?  Azad Kashmir Radio, Muzaffarabad still on 792 kHz in the north but now with 100 kW, and also Azad Kashmir Radio from a new location, Mirpur, in the south, with 40kW on 936 kHz, plus a small number of low-power FM stations.

There’s also a very interesting story about Adrian’s attempts to obtain QSL’s from these stations in Azad Kashmir, but we’re out of time for today.  Perhaps I can bring that another week.

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


Questions Circulate on the Future of WBCQ

 


The National Association of Shortwave Broadcasters posted on Facebook:

10 October 2026

WBCQ is a commercial shortwave radio station in Maine, USA. The station is selling its 500-kilowatt Continental transmitter, its 360-degree rotatable antenna, a 2-megawatt generator, 3000 square foot transmitter and studio building, and 100 acres of land near Monticello, Maine -- all for US$2 million. The price includes these assets, but if the buyer would like to operate the station in this location, he/she would have to obtain a new license from the U.S. Federal Communications Commission. Or the buyer could take the equipment and move it to another location. WBCQ will continue to operate an adjacent lower-power shortwave facility under its license, and that portion of the station is not for sale. 

Inquiries may be made to Allan Weiner at wbcq@wbcq.com

https://www.facebook.com/nasbshortwave





Interference over the UVB-76 frequency

 Frequency: 4625 kHz.




Pirate radio operators have been increasingly interfering with the UVB-76 frequency at night using music, whistling, and conversations.
Pirate radio operators have recently begun appearing more frequently on the 4625 kHz frequency, home to the shortwave station UVB-76. They play music, talk to one another, and create interference over the main signal, 
according to a radio monitoring researcher who runs the "UVB-76 Efir" Telegram channel-which broadcasts the station 24/7 and publishes its messages.
According to radio enthusiasts, the most active offender is the Russian-speaking "Kilohertz." "RC4," "E12," and "Sneg-05" also appear on the frequency. The extraneous signal may sound like music, whistling, or hissing, and sometimes multiple participants engage in open radio exchanges.
"The pirates' disruptive behavior is immediately noticeable because an extraneous radio signal appears on the frequency-which could be music, whistling, or hissing-while sometimes several radio hooligans conduct open conversations with each other, and some use digital modulation modes to overlay patterns and images onto the spectrogram (a visual representation of the signal - Ed.)," the researcher explained.
The pirates have their own habits. For example, before going off-air, "Kilohertz" invariably plays Viktor Tsoi's song "Quiet Night." Other participants greet listeners and wish them a good evening, or-conversely-simply switch on the music and display images on the spectrogram without a word.
https://vk.ru/radioreceiver)
(RUS-DX)

K-Love To Grow Internationally With Trans World Radio Partnership

 

By Lance Venta
October 12, 2026
Educational Media Foundation K-Love K-Love K-Love Inc. has announced a partnership with Trans World Radio with plans to bring K-Love programming to up to 190 countries globally.

K-Love, which began international partnerships earlier this year with stations in Italy and Zambia which have since expanded to Lithuania, will work with Trans World Radio’s local ministry teams to adapt K-Love’s content for different cultures and languages, with an emphasis on countries that are closed or restricted to Christian missionary efforts.

Additional story at: 

Jen's Eclectic Views & Real Deal audio for Oct. 11 is available

 
Audio is available for listening to or downloading the October 11 edition of Jen's Eclectic Views & Real Deal 

Extended link: 

Tiny URL: 

For contact, go to:

Thanks.
Jen In The Rad

Weekly Propagation Forecast Bulletins, October 12, 2026

 

Product: Weekly Highlights and Forecasts
:Issued: 2026 Oct 12 0344 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
05 - 11 October 2026

Solar activity was at very low to (R1-R2 - Minor-Moderate) levels
throughout the summary period. Region 4545 (N17, L=222, class/area
Dso/070 on 08 Oct) produced an impulsive M1.0 (R1 - Minor) flare at
05/1848 UTC. Region 4547 (N15, L=274, class/area Cri/030 on 06 Oct)
produced an M1.3 flare at 09/1409 UTC as the region exited the west
limb. The majority of the activity was observed from Region 4549
(N10, L=216, class/area Eki/260 on 09 Oct). During the period, the
region produced 39 C-class, 3 R1-Minor, and 2 R2-Moderate flares. It
produced an M6.7/2b flare at 08/1548 UTC with an associated Type II
Sweep with an estimated velocity of 4,125 km/s and a Type IV Sweep.
At 10/1510 UTC, this region produced an M6.4/1n flare with an
associated Type II Sweep with an estimated velocity of 929 km/s and
a 240 sfu Tenflare. The largest region on the disk, Region 4551
(S15, L=102, class/area Eko/400 on 11 Oct) produced 3 C-class
flares. In total, 50 C-class and 7 M-class events were observed. 

No proton events were observed at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit reached
high levels on 05-08 Oct and 10 Oct with a peak of 11,300 pfu
observed at 08/1250 UTC. Normal to moderate levels were observed on
09 and 11 Oct. 

Geomagnetic field activity ranged from quiet to G3-Strong levels
during the period. Quiet to G1-Minor levels were observed on 05 Oct
and quiet to unsettled levels were observed on 06 Oct, all due to
influences from a positive polarity CH HSS. Mostly quiet levels were
observed on 07-08 Oct. Activity increased on 09 Oct when unsettled
to active levels were observed due to weak influence from a 06 Oct
CME. Activity levels increased further on 10 Oct when unsettled to
G3-Strong levels were observed due to continued influence from CME
activity observed on 06 and 07 Oct. During this level of high
activity, total magnetic field strength increased to a peak of 45 nT
at about 10/1500 UTC and Bz observed some southward deflections to
30 nT at about 10/1630 UTC. Solar wind speeds rapidly increased from
about 380 km/s at 10/1500 UTC to a peak of about 890 km/s at 10/1755
UTC. Associated with this CME activity was some influence from a
negative polarity CH HSS. 

Forecast of Solar and Geomagnetic Activity
12 October - 07 November 2026

Solar activity is likely to continue at very low to low levels with
isolated R1-Minor levels possible throughout the period. 

No proton events are expected at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit is
expected to be at high levels on 14-15 Oct, 23-28 Oct, and 01-04
Nov, all due to anticipated influence from multiple, recurrent CH
HSSs. 

Geomagnetic field activity is expected to be reach G1-Minor
geomagnetic storm levels on 13 and 31 Oct , and 01 Nov. Active
levels are likely on 12, 22, and 23 Oct. Unsettled levels are likely
on 14-15, 21, and 24 Oct and 02 and 06-07 Nov. All increases in
goemagnetic activity are associated with anticipated influence from
multiple, recurrent, coronal hole HSSs. The remainder of the outlook
period is likely to be at mostly quiet levels. 

:Product: 27-day Space Weather Outlook Table 27DO.txt
:Issued: 2026 Oct 12 0345 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC web contact www.swpc.noaa.gov/content/subscription-services
#
#      27-day Space Weather Outlook Table
#                Issued 2026-10-12
#
#   UTC      Radio Flux   Planetary   Largest
#  Date       10.7 cm      A Index    Kp Index
2026 Oct 12     120          16          4
2026 Oct 13     115          28          5
2026 Oct 14     110          14          3
2026 Oct 15     105           8          3
2026 Oct 16     100           5          2
2026 Oct 17      95           5          2
2026 Oct 18      95           5          2
2026 Oct 19     100           5          2
2026 Oct 20     100           5          2
2026 Oct 21     105          15          3
2026 Oct 22     100          20          4
2026 Oct 23     100          15          4
2026 Oct 24      95          10          3
2026 Oct 25      95           5          2
2026 Oct 26     105           5          2
2026 Oct 27     110           5          2
2026 Oct 28     110           5          2
2026 Oct 29     110           5          2
2026 Oct 30     110           5          2
2026 Oct 31     105          30          5
2026 Nov 01     105          25          5
2026 Nov 02     105          10          3
2026 Nov 03     100           5          2
2026 Nov 04     105           5          2
2026 Nov 05     105           5          2
2026 Nov 06     110          10          3
2026 Nov 07     110          10          3
(NOAA)

Friday, October 09, 2026

Calling All Radio NUTZ, audio available

 


For the HF Enthusiast in you, Jen & GB's CARN for Saturday 10/03 is up & ready for listening and downloading.


CARN # 1 for Oct.3rd.

CARN Long Link.


CARN  Tiny URL .


For your contact pleasure


The Bands Are Alive !!

73's & 33's
Jen & GB

Thursday, October 08, 2026

Throwback Thursday-The Radio Scene in Shanghai

 
This week's edition originally aired on June 10, 2001

During the era under review in this edition of Wavescan, the city of Shanghai in China was an important international city. These days it is listed as the world's largest city, with a population in excess of 10 million people. However, the beginnings of Shanghai go back more than a thousand years when it was just a small trading center. 

After the Opium War in 1842, England was granted trading rights in Shanghai. Soon afterwards, other European powers were also granted the same trading privileges in Shanghai, and each country was given its own territory, a "concession," in an area to the north of the city. In this way, Shanghai truly became an international city, with separate residential areas for England, France, Germany, Italy, America and Japan.

When radio stations were established in the city of Shanghai, each of the foreign concessions established its own station, though mostly with Chinese callsigns. Many of these stations were heard throughout the world on shortwave.

A few struggling experimental stations with irregular callsigns were launched on mediumwave by commercial enterprises in the Chinese area of Shanghai in the mid 1920s, but most of them failed soon afterwards. More substantial mediumwave stations began to appear on the radio dial in the early 1930s, and these were all licensed with callsigns in the X series.

The first shortwave station in Shanghai was launched in 1931 on the channel 5000 kHz exactly and given the regular callsign XCTE. This station also disappeared soon afterwards. 

Japanese forces occupied Shanghai in 1937, but each of the foreign concessions was permitted to retain its area of influence and to continue in its regular activities, at least for a while. In early 1938, the Japanese occupation forces took over a mediumwave station previously owned by a Japanese merchant in Shanghai. This was station XQHA, with 250 watts on 580 kHz.

During the Pacific War, there were five different and important international shortwave stations located in Shanghai, all owned and operated by different nations.

Early in the year 1939, station XMHA was installed in the American concession in Shanghai with its identification announcement as "The Call of the Orient." Early in the year 1942, this station was taken over by the Japanese, still with the same identification announcements, XMHA and "The Call of the Orient." This station was monitored frequently by Arthur Cushen in New Zealand for news and information of interest to the South Pacific. 

Early in the year 1940, station XGRS was installed in the German concession in Shanghai. It could be presumed that the callisgn XGRS stood for "German Radio Station." Programming from this station was violently anti-British, and it carried significant news and information from both Germany and Japan. 

When peace was declared in Europe, Japan took over this station, giving it the callsign XGOO. Three months after peace was declared in the Pacific, the Chinese took over the station, giving it a new callsign, XORA. This 5 kw. crystal controlled transmitter was the only shortwave station that remained on the air in Shanghai after the war.

The Italians also erected a station in their concession in Shanghai with the callsign XIRS; and likewise, it could be presumed that XIRS stood for "Italian Radio Station."

The French erected a mediumwave station in their concession some years before the hostilities began in Europe, though this station identified with the French callsign FFZ rather than a Chinese callsign. Early in the year 1940, a 400 watt shortwave unit was installed, and after the German occupation of France this station became the Asian voice for the Vichy government.

For a period of a year or so, a shortwave station in Shanghai purported to be located "somewhere in India." This station announced on air as "The Voice of Free India" and "The Voice of Indian Independence," and it was first noted in New Zealand in March 1942. This station was heard frequently with two channels in parallel. Towards the end of the same year, programming was revamped and the station identified as "The Voice of the Indian Independence League."

Thus for half a dozen decisive years around the middle of the last century, many of the major powers in conflct in Europe and Asia were represented on the shortwave scene in Shanghai.
(Wavescan 337)
(photo via UnSplash)

Wednesday, October 07, 2026

From the Isle of Music, October 9

 

From the Isle of Music, October 2026
This month, we will air the postponed episode covering the career of accordionist/bandleader/arranger/composer/producer Eddy Gaytan, born in Argentina but moved to Cuba and had an impact on several styles of Cuban music.  We hope to have his son, Eddy Gaytan, an accomplished musician in his own right, to guide us through an interesting and, to many North Americans, unexpected mix of music. .  

Friday, October 9, 2026, 9670 kHz, 1800 CEST (1600 UTC), repeats on 3955 kHz at 2400 CEST (2200 UTC)
 
Programming from Channel 292 in Germany. In addition to terrestrial listening, we do accept reception reports using remote SDRs, provided both your own physical location and the location of the SDR are included. EQSLs only for either.

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

Monday, October 05, 2026

Weekly Propagation Forecast Bulletins-October 5, 2026

 Product: Weekly Highlights and Forecasts
:Issued: 2026 Oct 05 0139 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 28 September - 04 October 2026


Solar activity was at very low to low levels throughout the summary
period. Region 4535 (N11, L=351, class/area Dao/060 on 30 Sep)
produced the strongest flare of the period; an impulsive C8.6/1f
event at 30/0246 UTC. This event also produced a 523 km/s Type II
and a Type IV Sweep. All other regions remained simple and absent of
any significant activity. No Earth-directed CMEs were observed in
available coronagraph imagery. 

No proton events were observed at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit reached
high levels on 28-30 Sep and 01 Oct with a peak of 5,620 pfu
observed at 29/1620 UTC. Moderate levels were observed on 02-04 Oct. 

Geomagnetic field activity was at quiet levels on 28-30 Sep and
01-03 Oct with some isolated unsettled periods observed early on 03
Oct. On 04 Oct, solar wind parameters became enhanced due to the
influence of a positive-polarity CH HSS. Total magnetic field
strength increased to a peak of 22 nT and Bz observed several
southward deflections, the maximum being -20 nT early on 04 Oct.
Solar wind speeds steadily increased from about 300 km/s to a peak
of 644 km/s later on 04 Oct. The phi angle was predominantly
positive. 

Forecast of Solar and Geomagnetic Activity 05 October - 31 October 2026

Solar activity is likely to continue at very low to low levels
throughout the outlook period. 

No proton events are expected at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit is
expected to be at high levels on 06-11 Oct, 14-17 Oct, and 23-28 Oct
due to anticipated incluence from multiple, recurrent CH HSSs. 

Geomagnetic field activity is expected to reach G1 (Minor)
geomagnetic storm levels on 22 and 31 Oct. Active levels are likely
on 06, 21, and 23 Oct. Unsettled levels are likely on 07, 11-14, and
24 Oct. All increases in geomagnetic activity are associated with
anticipated influence from multiple, recurrent, coronal hole HSSs.
The remainder of the outlook period is likely to be at mostly quiet
levels. 

:Product: 27-day Space Weather Outlook Table 27DO.txt
:Issued: 2026 Oct 05 0139 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC web contact www.swpc.noaa.gov/content/subscription-services
#      27-day Space Weather Outlook Table
#                Issued 2026-10-05
#
#   UTC      Radio Flux   Planetary   Largest
#  Date       10.7 cm      A Index    Kp Index
2026 Oct 05      92          18          5
2026 Oct 06      90          12          4
2026 Oct 07      90          10          3
2026 Oct 08      90           8          3
2026 Oct 09      92           5          2
2026 Oct 10      92           5          2
2026 Oct 11      90          10          3
2026 Oct 12      90           8          3
2026 Oct 13      95           8          3
2026 Oct 14     100           8          3
2026 Oct 15     105           5          2
2026 Oct 16     105           5          2
2026 Oct 17     105           5          2
2026 Oct 18     105           5          2
2026 Oct 19     110           5          2
2026 Oct 20     105           5          2
2026 Oct 21     105          18          5
2026 Oct 22     100          22          5
2026 Oct 23      95          15          4
2026 Oct 24      90          10          3
2026 Oct 25      90           5          2
2026 Oct 26      85           5          2
2026 Oct 27      80           5          2
2026 Oct 28      75           5          2
2026 Oct 29      75           5          2
2026 Oct 30      75           5          2
2026 Oct 31      80          30          5
(NOAA)

Saturday, October 03, 2026

Saturday show from Jen & GB's Calling All Radio Nutzz (CARN)

 


Jen & GB's Calling All Radio Nutzz (CARN) Saturday Oct 3rd 

18:00 - 21: 00 UTC on Unique


It's time for a new season of the CARN show. In the first program, we commence the regular features at lesson one, or part one, and put them together in a block. 

There will be live tuning during the Oceania DX contest and hunting the 9T0MD Dxpedition to the DRC. All the usual news, diary dates, station recordings, plus music.

Contributions Of The HF of kind are welcome - please email the show.

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So Join Us..

Jen & GB

Friday, October 02, 2026

Sunday'sJen's Eclectic & Real Deal program

 

On Sunday, October 4, 2026 - tune in to the live stream for Jen's Eclectic & Real Deal 

17:00 - 20:00 UTC + 


For contact, pleasure.


Thanks.
Jen In The RAD

U.K. Propagation Update-October 2, 2026

 

 RSGB

RadCom Assistant Editor | October 2, 2026

Compiled by G0KYA, G3YLA and G4BAO on Thursday, 1 October 2026.

As we enter October, we think it’s time to get excited about HF again.

Some of the best HF conditions can occur this month as MUFs rise. It might take a couple of weeks to get going but it will, we promise – there’s a good reason why the CQ Worldwide SSB contest is held in October after all.

Solar conditions have been surprisingly calm. The solar flux index has been ranging from 90 to 100 but geomagnetic conditions have been quiet, with the Kp index usually around one to two.

We had a brief excursion to a Kp index of 4 on 26 and 27 September but this was relatively short-lived.

Daytime Maximum Usable Frequencies, or MUFs, over a 3,000km path have been touching 25 to 28MHz at times, but we can expect this to improve over the next few weeks.

As long as the Solar Flux Index can stay around 100 we should see some transatlantic paths opening up on 28MHz but they may not be as good as previous years.

Ten-metre openings at the start of this month may be fleeting and unreliable.

What we do have is a massive coronal hole on the Sun’s equator, which could send the Kp index up this weekend as solar plasma impacts the Earth. Keep an eye on solarham.com for updates.

If this comes to pass, expect lower MUFs and poor DX for a day or two.

DX to be worked this week include 5W0AF from Samoa; 9T0MD from the Democratic Republic of Congo; JW6VM, JW7XK and JW9DL on Svalbard; 7P8JL, 7P8LZ and 7P8TR in Lesotho; 6O2M (Somalia), C5R from The Gambia and FW1P from Wallis and Futuna.

NOAA predicts that the SFI this coming week may bottom out at around 90, before rising again, perhaps reaching 100 to 102 by next weekend.

As mentioned earlier, we can expect the Kp index to rise, perhaps hitting four on 5-7 October. After this, it should settle to a more reasonable Kp index of 2 for the rest of the week.

VHF and up propagation news:

Compiled by G3YLA and G4BAO.

The autumn season is typically a mix of still, quiet weather with high pressure on the charts and, in contrast, a few days later deep Atlantic lows roll by with wind and rain.

The coming ten days or so will follow that script and offer a mix of propagation modes for the VHF/UHF fraternity.

The Tropo conditions will dominate in the south and should probably be in control up to the middle of next week. Northern Britain will have activity from weather fronts and possible rain scatter for the GHz bands, which becomes more general from midweek onwards.

The autumn season is also a prime time for aurora, so keep that mode on the ‘to do’ list and be aware of changes in the Kp index to values higher than Kp index 5. Meteor scatter is mostly in the realm of random activity.

Lastly, a surprise mention of Sporadic-E, which for CW and SSB modes is pretty much done, but last week on Thursday, 24 September there was some activity for FT8 within Europe.

This was mixed in with Tropo paths so it was difficult to pinpoint the exact mode being used without looking at detailed measurements from radiosondes and ionosondes.

The end result is that ‘out of season’ may still produce Es for digital modes but it’s probably a rare occurrence.

EME now, and the Moon is at maximum declination on Friday, 2 October so Moon windows are at their longest and peak Moon elevation is at its highest.

Path losses are low after perigee on 1 October but will start to increase. 144 MHz sky noise starts the week moderate, dropping back to low for the rest of the week.

https://rsgb.org/main/blog/news/gb2rs/propagation-news/2026/10/02/propagation-news-04-october-2026/

(Mike Terry, UK/BDXC)