Tuesday, May 12, 2026

U.S. Military Radio Ship – Spindle Eye

 Special thanks to the Wavescan staff for this week's radio nostalgia feature on Spindle Eye

Jeff: This week, Ray Robinson in Los Angeles brings us the interesting story of a U.S. military radio ship which saw service in the Pacific in the 1940’s and was used to broadcast news of the American atom bomb tests on Bikini atoll in the Marshall Islands in 1946.

Ray: Thanks, Jeff.  Our editor-in-chief, Dr. Adrian Peterson, actually brought us this story first about 15 years ago, but recent research by Dr. Martin van der Ven in Germany now allows me to add more information.

The ship in question was called the Spindle Eye.  Plans for this new radio ship were developed during 1944, and she was originally intended to provide the master control for coverage of the projected invasion of Japan.

The ship was laid down in the Kaiser shipyards at Richmond, near San Francisco, California, and she was launched with the unassuming name Spindle Eye on May 25, 1945.  She was nearly 340 feet long and 50 feet wide (which by comparison is about one and a half times longer and wider than Radio Caroline’s current radio ship, the MV Ross Revenge).

The Spindle Eye was fitted out as a radio ship at the Todd shipyards in Seattle, Washington with a bevy of electronic equipment.  From a technical perspective, the Spindle Eye was a masterpiece of post-war engineering.  On board were, among other installations, a 7½ kW broadcast-quality RCA shortwave transmitter that had been made at their Camden Factory in New Jersey, a 500 watt Hallicrafters BC-610 shortwave transmitter that was used for local coordination, a 2½ kW Wilcox 96C four-channel shortwave transmitter, high-speed teletype equipment capable of up to 500 words per minute, Acme radiophoto transmission systems, as well as extensive recording and mixing facilities in two studios – one for broadcasting and one for recording and production.  Above the decks were also eight antennas.  A central control room had an extensive patching infrastructure, Western Electric compression amplifiers, numerous receivers (including Hammarlund Super-Pro and RCA AR-88 models), a fully equipped darkroom, and an air-conditioned press conference room with 120 typewriter positions.  In fact, all the studios and technical spaces were fully air-conditioned — quite an accomplishment for the time, and no small advantage in the tropical climate of the Marshall Islands.



Test transmissions from the Spindle Eye first took place during early September 1945 at the dockside in Seattle, using the 7.5 kW RCA transmitter.  On September 19, after only 64 days of fitting out, the ship sailed into the Pacific, bound for Japan.

The Spindle Eye arrived in Tokyo Harbor on October 15, and she took over the radio services previously provided by the Apache under the call sign WVLC; that vessel was still in the Philippines at the time.  The Spindle Eye was inspected by General MacArthur, after which she undertook a trial voyage off the coasts of China and Korea.  It was reported that the electronics aboard the Spindle Eye were working well.

On return to Japan just before Christmas, the Spindle Eye (operating under the transferred callsign WVLC), began a series of broadcasts on behalf of the Voice of America and the American Armed Forces Radio Service.  In addition, news dispatches from the post-War legal trials in Tokyo, which were convened on April 29, 1946, were relayed from the Spindle Eye to the United States for nationwide rebroadcast.


In July 1946, the Americans conducted two atomic tests in the Marshall Islands in the central Pacific, about halfway between Hawaii and the Philippines.  The umbrella codename for the tests was ‘Operation Crossroads’, and in this pre-television era, extensive plans were made for live radio coverage of the detonations.  Throughout the islands, a total of 150 radio transmitters and 300 receivers were in use for the coordination of the atomic detonations and for the broadcast of live news reports.

 The first test was an explosion in the air with the code name Able, and the second was an underwater test, code-named Baker.  On Able-Day, July 1, 1946, a U.S. Air Force B-29 dropped a bomb (named “Gilda”) over the Bikini Atoll in the far northwest of the group.  It detonated with a yield of 23 kilotons at an altitude of just over 500 feet, but it had been dropped about half a mile short of the intended destination.  A fleet of 73 obsolete ships had been moored around Bikini, but as a result of the targeting error, only five were sunk.

The Spindle Eye was given the task of co-ordinating all of the news transmissions from Operation Crossroads, including voice broadcasts, press dispatches and radio photos.  For this purpose, the ship was located at Kwajalein Atoll, about 200 miles southeast of Bikini, and the callsign WVLC was replaced by the Navy callsign NIGF.  The broadcasts from NIGF were beamed to RCA Bolinas and Press Wireless, Los Angeles for onward relay.

 One of the greatest technical challenges arose from the geographical orientation of Kwajalein and the prevailing winds in the area.  The conventional delta-fed doublet antennas that had been installed on board radiated their maximum power at right angles to the ship’s axis — which for most of the day was an unfavorable orientation for the desired link to the US West Coast.  So, using a four-point anchoring system, the ship was fixed on a heading of 143 degrees in order to align the main radiation lobe precisely with the great-circle path to San Francisco.  However, this was pretty uncomfortable for those on board with the swells hitting broadside, so a second solution was a remarkable piece of technical improvisation.  An inverted, unterminated V antenna was constructed, with its legs leading out to buoys that had been anchored in the lagoon.  Interestingly, the outcome was convincing:  an improvement in signal strength of approximately 30 per cent.

On Able-Day, July 1, program broadcasts from NIGF Spindle Eye began at 3:30 am local time with live news reports for NBC and CBS in the United States of the evacuation measures that were taking place.  The Voice of America also carried these same reports worldwide through their large network of shortwave and medium wave stations.  These were followed by outside broadcasts of the take-off of the B-29 bomber, and pooled broadcasts as the signal “Bombs Away” was received at 9:00 am.  Two voice transmitters on the Spindle Eye were used in parallel with all of the live news reports – the 7½ kW RCA and the 2½ kW Wilcox.  Subsequently the Wilcox was diverted for the transmission of news photos – the first photographs of the explosion which were sent via the army station WTJ in Hawaii and relayed onward to army station WVY in San Francisco.


One of the major news reporters on board for the occasion was Oliver Read who was the editor of the American radio journal, Radio News, and he published three lengthy articles about the Spindle Eye’s involvement in the operation in that magazine.

However, in spite of the elaborate plans for extensive live news coverage from the atomic test areas, on Able-Day there had been times when the voice relays were inferior and difficult to understand.  This was due to the fact that the shortwave transmitters used had only modest output power considering the distance and propagation challenges with the local effects on the ionosphere immediately after the explosion.

For the underwater test, Baker, which was conducted 3½ weeks later, the radio ship Spindle Eye was moved to Honolulu, as a more central relay point between the atomic test sites in the Marshall Islands and the American mainland.  On July 25, a second bomb of the same size was detonated at a depth of 90 feet below the waves, creating a vast radioactive column of water and debris that sank several ships – including the USS Saratoga – and caused extreme and unexpected contamination of the fleet.  The Spindle Eye, operating under the call sign NIGF, received the shortwave reports from Bikini and relayed this programming on to RCA Bolinas and Press Wireless, Los Angeles for further distribution.

Following the two atomic tests, the Spindle Eye returned to the Pacific coast of the United States, and operation of the RCA transmitter as WVLC-NIGF came to an end at the close of 1946.

One year later, the Spindle Eye was renamed the Sgt. Curtis F. Shoup and it was then used in the Pacific as a helicopter freighter.  After that spate of service came to an end, the ship was transferred to the Mediterranean for oceanographic studies.  Finally, she was sold for scrap on May 9, 1973.

It is known that a few QSL letters were issued for the WVLC-NIGF broadcasts, and the Voice of America also issued their regular QSL’s confirming the relay of the atomic tests at Bikini Atoll.  In addition, special QSL cards were printed to commemorate the atomic tests, and these showed an artistic version of the sinking of a ship.

Back to you, Jeff.

Jeff: Thanks, Ray, and again, we are grateful to Dr. Martin van der Ven in Germany for his additional research on this feature.








 



Monday, May 11, 2026

Audio now available for Jen's & GB's Mum's Day Special on Unique Radio

 



Audio for the May 10 edition of Jen's special Mum's Day programming is now available for your listening nd downloading.

Link: 


For contact pleasure.

Thanks.
Jen In The RAD

For your contact pleasure.

Jen In The RAD

Weekly Propagation Forecast Bulletins, May 11, 2026

 Product: Weekly Highlights and Forecasts
:Issued: 2026 May 11 0150 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  04 - 10 May 2026


Solar activity reached high levels on 10 May due to an M5.7/2b flare (R2-Moderate) at 10/1339UTC from Region 4436 (N19, L=330, class/area=Dao/beta on 10 May), the strongest of the period.
Associated with the event was a Type II radio sweep (est. 650 km/s), Tenflare (550sfu), and a CME signature first observed in coronagraph imagery at 10/1348UTC towards the NE. Analysis and modeling of the event is ongoing at the time of this writing. 

Region 4424 (N17, L=192, class/area=Eai/160 on 30 Apr) also produced an M-class event with an M1.8 flare (R1-Minor) observed at 04/0133 UTC. The other 10 numbered active regions on this visible disk were either mostly quiet or only produced C-class activity during the past week 

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 the summary period. 

Geomagnetic field activity reached G2 (Moderate) geomagnetic storm levels on 04 May and G1 (Minor) levels on 05 May due to the influence of a passing CME. Total magnetic field strength only reached a peak of 11 nT during that time, but Bz rotated as far southward as -10 nT and was sustained southward from late on 04 May through midday on 05 May. Despite the influence of a positive polarity A coronal hole beginning late on 07 May, the mostly northward Bz component results in only quiet to unsettled conditions through the end of the reporting period. 

Forecast of Solar and Geomagnetic Activity 11 May - 06 June 2026

Solar activity is expected to be at low levels, with a chance for M-class activity (R1/R2-inor/Moderate), and a slight chance for X-class (R3-Strong), throughout the outlook period due to the flare potential of several active regions both currently on the visible disk and those expected to return from the Sun's  farside. 

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 17-20 May due to the influence of a recurrent, negative polarity coronal hole. The remainder of the 
outlook period is likely to be at normal to moderate levels. 

Geomagnetic field activity is likely to reach G1 (Minor) geomagnetic storm levels over 15-17 May; active conditions are likely on 18 May, 23 May, 27 May, and 03 Jun; unsettled conditions are likely over 11 May, 13 May, 21-22 May, and 28 May - 31 May. All enhancements in geomagnetic activity are due to the anticipated influence of multiple, recurrent, coronal hole HSSs. The remainder of the outlook. The period is likely to be mostly quiet. 

Product: 27-day Space Weather Outlook Table 27DO.txt
:Issued: 2026 May 11 0150 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 2026-05-11
#
#   UTC      Radio Flux   Planetary   Largest
#  Date       10.7 cm      A Index    Kp Index
2026 May 11     128           8          3
2026 May 12     128           5          2
2026 May 13     122          10          3
2026 May 14     130           5          2
2026 May 15     125          25          5
2026 May 16     125          20          5
2026 May 17     120          18          5
2026 May 18     122          15          4
2026 May 19     130           5          2
2026 May 20     130           5          2
2026 May 21     130           8          3
2026 May 22     120          10          3
2026 May 23     125          12          4
2026 May 24     125           5          2
2026 May 25     125           5          2
2026 May 26     130           5          2
2026 May 27     135          12          4
2026 May 28     135          10          3
2026 May 29     130           8          3
2026 May 30     125           8          3
2026 May 31     122           8          3
2026 Jun 01     118           5          2
2026 Jun 02     115           5          2
2026 Jun 03     120           5          2
2026 Jun 04     120          12          4
2026 Jun 05     120           5          2
2026 Jun 06     120           5          2
(NOAA)

Friday, May 08, 2026

U.K. Propagation Update

 

RSGB
RadCom Assistant Editor | May 8, 2026
Compiled by G0KYA, G3YLA and G4BAO on Thursday, 7 May 2026

We had another mixed week of HF propagation, with a Kp index of 6 one day and then three days later a Kp of less than 1.

The index hit 6.33 on the evening of Monday, 4 May, sparking aurora and poor HF conditions. But by Wednesday, 6 May it was back down to 0.67.

So, you can see why it is hard to predict what HF conditions are going to be like with ionospheric propagation being driven by the geomagnetic status rather than the solar flux index.

According to the CDXC Slack group, DX worked over the past week
included:

TZ4AM in Mali on 10m CW
T31TTT from Central Kiribati on 12m and 15m FT8 XQ6CF in Chile on 17m CW VP8A on the Falkland Islands on 60m CW 3B9G on 20m CW TL8BNW from Central African Republic on 40m SSB So, there is DX about if you hunt for it. Interestingly, all of the above, apart from T31TTT, were on southward paths, perhaps reflecting poorer conditions on polar paths at times due to the elevated Kp index.

Next week, NOAA predicts that the solar flux index will remain around
115 to 130 with calm geomagnetic conditions for the first half of the week.

However, unsettled geomagnetic conditions are forecast for 15-18 May with a possible Kp index of 5.

With five sunspot groups visible on the Sun’s surface and active region
4419 the source of two X-Flares on Friday, 24 April now about to turn back into Earth’s view, it is anyone’s guess what could happen next.

As we enter mid-May, we are getting closer to summer HF conditions. So Sporadic-E on the higher HF bands, lower maximum usable frequencies overall but perhaps 14MHz staying open all night are all features to watch out for.

Also look out for 10m band openings to Southern Africa around midday and paths to South America during early and late evening.

VHF and up propagation news from G3YLA and G4BAO:

The current period of weather seems to be a mix of weak high pressure and low pressure systems vying for dominance.

Therefore it implies that a mix of radio conditions will share our attention, with weak tropo from ridges of high pressure but no big highs on the chart while frontal rain bands or heavy showers bring a chance of rain scatter for GHz operators.

The prospects for meteor scatter may remain elevated for a while since we have only just passed the peak of the Eta Aquarids on Wednesday, 6 May. Remember the early morning hours tend to be best for meteor activity in general.

The aurora alerts have continued to provide a glimmer of hope but mostly for weak enhancements, so look for a Kp value of 5 or greater and signs of ‘watery’ sounding signals on the HF bands before turning the VHF beams to the north.

As we move into the early part of the Sporadic-E season, it will become the mode of choice for us during the next few months.

The general rule is to check for the two main periods of activity: in mid-morning and again late afternoon or early evening.

Listen for strong signals on the 10m band from Europe and then, as the event develops, the higher frequency bands will open up too.

In a strong event, the 2m band can even show up sounding like 20m. 
However, early season events tend to favour the 10 and 6m bands.

EME now. The Moon is past minimum declination and increasing, giving lengthening Moon windows and increasing peak elevation.

Path losses are decreasing now after apogee on Monday, 4 May. 144MHz sky temperature is low all week until Saturday, 16 May when the Sun and Moon are close in the sky.

(Mike Terry, UK/BDXC)

Radio Caroline North, set for May 9-10 broadcasts

Ross Revenge

 Radio Caroline North's next broadcast is between 9th and 10th of May, live from our radio ship Ross Revenge.

You'll hear some great music from the 60s to 90s – plus you could win a stunning music-themed wall clock in this month's competition draw.

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 north@radiocaroline.co.uk and remember, it's the only email address that gets you straight through to our 'North' broadcasters.

(Mike terry, UK/BDXC)
(photo/Wikipedia)

Thursday, May 07, 2026

Throwback Thursday - Australian Army Radio

 Australian Army Radio

In recent times, many DXers and international radio monitors worldwide have reported hearing the unique shortwave service for Australian troops serving in the peacekeeping forces in Timor and elsewhere. Over a period of time, these broadcasts have been radiated over transmitters located at three different radio bases in Australia, and they form an interesting update to the entire story of radio broadcasting by the Australian Army Amenities Service (AAAS). This is the story, that begins way back during World War II.

The first radio broadcasting unit for Australian Forces was a mobile studio, which was commissioned in Australia in June 1942 and shipped to the Middle East. Originally, it was intended that this mobile radio studio would broadcast back to Australia with war news and information from North Africa and the Middle East. However, because the shortwave transmitter had an output of only 1 kw, these intended broadcasts became impractical. Consequently, the mobile studio was used mainly for producing programs in the battle areas and for broadcasting them over local radio transmitters.

During the Pacific theater of World War II, a series of 21 mobile radio stations were constructed in Australia, tested late at night from locations in Melbourne and Sydney, and then shipped to forward areas. These stations were rated with a power output ranging from 10 to 200 watts.

On one occasion, and quite by chance, I heard one of these stations at a distance of some 500 miles. It was 9AF, with 200 watts on 1440 kHz, broadcasting a test program from Melbourne late at night.

These AAAS stations were based in the main areas of Australian troop deployment in the Pacific islands, and were supplementary to the larger number of American Armed Forces Radio Stations in the same areas. The whole series of callsigns for the AAAS stations at the time ranged from 9AA to 9AP.

Many of these stations were transported from place to place according to the movement of the armed forces in the various stages of the Pacific war. One of the stations, 9AG with 200 watts on 1340 kHz, was established at Balikpapan in Borneo. When the Australian troops moved forward, this station was handed over to the Dutch authorities, and it became the local station in the NIROM network.


In addition, several other stations were constructed locally in forward battle areas or were taken over from a retreating enemy. Such stations as "Radio RAAF Milne Bay" and "RAAF Radio Madang" were well known in the area at the time.

At Port Moresby, New Guinea, a 500-watt station on 1250 kHz was officially opened by General Douglas MacArthur on February 26, 1944. The first allotted callsign was 9PA, but this was soon changed to 9AA, signifying its status as the parent station for all of the forward stations with callsigns in the 9A series. The QSL letter that I received from this station lists the call as 9PA, when, in reality, as an army station at the time, it was really 9AA.

In addition to the testing of the mobile MW stations in the two cities, Melbourne and Sydney, additional army stations have been established in other areas of mainland Australia. These have operated generally on the medium wave band, though one in particular was a shortwave broadcaster.

At Darwin in Australia's Northern Territory, an MW station was established in 1944. This was 5DR, standing for Darwin Radio. It was in use as an army station for two years, and then it was taken over by the government broadcasting service, the Australian Broadcasting Commission, as the Northern Territory relay station for the ABC home service network. This station was later designated as 8DR, and its callsign has since been changed to 8RN.

Soon after the war was over, an experimental broadcasting service was launched from an air force base at Higgensfield in North Queensland. This station announced as "Radio RAAF No. 2," identifying the air force unit that was operating it. The 100 watt transmitter on 1470 kHz was on the air in August 1945 with the intent of launching an entertainment/information radio service, but the project was abandoned.

Then, in 1955, the first army shortwave station came onto the air unannounced, from Puckapunyal in Victoria. This station radiated 25 watts on 7850 kHz, and it was on the air just two hours per week in November 1955.

Towards the end of the Pacific war, a 50 year old wooden ship, the "Apache," was fitted out in Sydney Harbour as a radio station and sent up to the Philippines. This station, announcing as WVLC, took over some of the Australian shortwave broadcasts from VLC, Shepparton, and it also relayed American AFRTS and VOA programs over a channel in the 7 MHz band.

HMS Grenville

In addition, several warships in the Pacific, British, Australian, and American, began to relay programs from Australian MW stations to surrounding areas on shortwave. One of these, for example, was the HMS Grenville, which was heard relaying the commercial programs from 2KY Sydney in January 1946.

More recently, some of the larger Australian navy vessels have incorporated a radio station as part of their onboard entertainment facilities. In some cases these stations have radiated programs over a MW transmitter, and in other cases programs are available on board the ship via closed circuit cable. One of the ships, HMAS Canberra, for example, was stationed off the coast of Vietnam during the South East Asian conflict.

During the era of occupation in Japan, at least four of the mobile 9A stations were taken to Japan. These were incorporated into existing Japanese stations and were allocated callsigns in the American W series. For example, the 10 watt station 9AQ was located near Kure in Japan. It was first identified as WVTX, and later as WLKU. All of these stations were broadcasting on MW, but one of them, 9ALWVTV/WLKSwas also broadcasting for a while on shortwave.

When the Korean offensive began, Australian troops also moved into the peninsula, and so too did some of their radio stations, as many as four of them.

Along with the American "Good Morning Vietnam" series of AFRTS stations, there were a couple of Australian stations located in Vietnam as well. One of these was a 500-watt station broadcasting from Vung Tau on 1040 kHz. Another station was located for a while at Hue, near the larger VOA and AFRTS stations.


Back in 1960, on July 1 to be exact, a rather substantive radio station was established by the Royal Australian Air Force at Butterworth on the Malay Peninsula, just across from the island of Penang. This AAAS station broadcast from two 500-watt transmitters, using each on alternate days, both at 50 percent power. They also had a choice of two simple antennas, an inverted L and a folded dipole. This station was occasionally heard further afield, and on several occasions, I heard it in India and Sri Lanka. Radio RAAF Butterworth served some 5,000 Australian personnel at the air base, and it left the air when Butterworth was closed in the late 1980's.

The latest endeavor in AAAS broadcasting made its appearance unheralded, unannounced and unexpected. A few years back, a new shortwave service for Australian forces serving in Somalia came onto the air. At first, the half hour programs were broadcast from one of the 250 kw shortwave transmitters of Radio Australia located on Cox Peninsula near Darwin in the Northern Territory. A while afterwards, DXers in Europe and elsewhere reported hearing similar programming on other channels not listed for Radio Australia.

Subsequent information revealed that these transmissions were coming from two different locations. One is VHP, the large Navy radio station located at Belconnen near Canberra, Australia's capital city. The other is NMCVLF, the American radio facility located near Exmouth at North West Cape in a Western Australian coastal area. These transmissions were on the air several times a day from both locations. Studio facilities are housed in one of the government offices in Canberra, and the first broadcast each day was presented live.

The broadcasts from Exmouth were directed towards Somalia, and the broadcasts from Belconnen were directed towards Kampuchea. Programming consisted of contemporary music interspersed with calls from relatives in Australia to servicemen on ships and in Somalia and Kampuchea.
(Wavescan/May 7, 2000)
(photos/Wikipedia)

Wednesday, May 06, 2026

WKRP Is Back in Cincinnati

(graphics by Gayle Van Horn)



Series star Gary Sandy kicks off new era for 97.7 FM

By Nick Langan 

Published: May 4, 2026

Nearly 50 years after the iconic “WKRP in Cincinnati” premiered, the call letters have finally found their way back to the Queen City.

The voice of Gary Sandy — who played program director Andy Travis on the CBS sitcom — welcomed listeners to the new WKRP(FM) 97.7 on the Cincinnati radio dial at 6 a.m. on Monday, according to a report filed by John Kiesewetter of Cincinnati’s WVXU(FM).

The pair of Randy Michaels — whose many decades in the radio industry include time as the former CEO of Jacor and Clear Channel — and Jeff Ziesmann operate the three-station oldies-formatted network known as “The Oasis.”

Michaels’ Radioactive LLC bought the rights to use the call sign in April. Lance Venta of RadioInsight was first to report the move of the calls.


RNZ New Zealand summer Schedule

 
requested by contributor, Rod Pearson - the summer schedule for RZ Pacific - New Zealand

classic QSL

New Zealand, RNZ Pacific - A26 Summer schedule

29 Mar 2026 - 24 Oct 2026

All times UTC/kHz/Target Area to Pacific regions

**********************************
00:00-04:58 17675 Pacific Daily
04:59-06:58 13690 Pacific Daily
06:59-10:58 11725 Pacific Daily
10:59-12:58  9700 Solomon Islands, PNG Mon - Fri
10:59-12:58  9700 Pacific Sat-Sun
12:59-16:50  7440 Pacific Daily
16:51-18:58  9700 Pacific Sat
18:59-19:58 13690 Pacific Sat
19:59-20:58 15720 Pacific Sat
20:59-23:59 17675 Pacific Daily

DRM
16:51-18:58  9700 AM 9780 DRM Pacific/Cook Is, Samoa, Tonga Sun-Fri
18:59-19:58 13690 AM 11690 DRM Pacific/Cook Is, Samoa, Tonga Sun-Fri
19:59-20:58 15720 13840 DRM Pacific/Cook Is, Samoa, Tonga Sun-Fri

QSL- Reception Reports
RNZ welcomes QSL reports from listeners using this form  :
(RNZ Pacific)

The Freedom Stations of World War II

 


Thanks to the staff of Wavescan. Nostalic radio stories from World War II continue to be popular.

Jeff: To begin today’s show, Ray Robinson in Los Angeles has a very interesting story regarding an aspect of shortwave broadcasting during World War II that is very little understood – that of the so-called ‘Freedom Stations’.

Ray: Thanks, Jeff.  I’ve recently been reading a fascinating book written during World War II by Harold Ettlinger, called ‘The Axis on the Air’.  Harold was a columnist for the Chicago Star newspaper and a keen monitor of the shortwave bands.  In late 1943, he published the book, which details his observations of the propaganda broadcasts being made from Germany, Italy, and Japan targeting the home audiences of the Allies and their fighting men on the battlefield.

One very interesting chapter deals with what were referred to as the ‘Freedom Stations’.  These appeared to be clandestine in nature and most operated on shortwave (in Europe at least, mainly in what was often termed the ‘49 meter European Band’), but the interesting thing was that they were made to appear as if they were being operated by underground resistance fighters, while in reality it was the Axis powers who were behind them.  It was all very devious and cunning, so I’d like to read part of that chapter for you today.  Remember Harold wrote this in late 1943 when the outcome of the war was still far from certain.  He said:

“The Germans do not confine themselves to a single freedom station for each of their enemies.  England receives broadcasts from at least four, each of them broadcasting frequently, and there are others for the dominions.  Those beamed at England are the New British Broadcasting Station, the Workers’ Challenge, Radio Caledonia and the Christian Peace Movement.  Among those aimed at the Empire are Free India, Free Egypt and Anzac Tattoo.  One of the stations aimed at England is keyed to a middle-class audience and another to factory workers.  Each plays up what the Germans imagine to be the prejudices of the class they are addressing.  As they appeal to different audiences, they have to differ not only in their method of going after their objectives but even in the objectives themselves.  For example, on the second-front issue in 1942 and early 1943 (the ‘second front’ was the anticipated Allied invasion of the European continent from the west), on the second-front issue in 1942 and early 1943 the middle-class freedom station for Britain exploited what the Nazis believed to be British middle-class fear of Communism.  The station followed the line that it was the Communists who wanted the second front in order to (take the pressure off the eastern front and) save Communism, no matter how many lives it cost.  The station aimed at British workers actually appeared to favor a second front, but it used the issue to try to hinder British production.  “Russia wants the second front in western Europe,” it said, “but she won't get it from the capitalists.  Workers of Britain, strike for a second front!”

“A station called ‘Debunk’ is a typical fake clandestine station.  When it first began broadcasting, Debunk went to elaborate lengths to make us believe it originated in the American Midwest.  Its speakers made their accents as twangy as they could, announced the time as Central Standard, opened with a few bars of the “Star-Spangled Banner,” and generally sought to create a cracker-barrel atmosphere.  Joe Scanlon, the principal Debunk speaker, is probably Otto Koischwitz, who has persuaded Goebbels that he is the very man to put a fake Midwestern radio station across with us yokels out here.

“Among the more recent efforts of the Nazis to exploit the freedom-station technique was the creation shortly after the Anglo-American landing in North Africa of three ostensibly clandestine transmitters which had the special job of trying to cause dissension and interfere with Allied plans.  These stations were Brazzaville Two, which was supposed to be a Fighting French outlet in North Africa, the Voice of Truth and Radio Patrie, all of them broadcasting from France or Italy.  Brazzaville Two was designed to be confused with the authentic Fighting French station broadcasting from Brazzaville in Equatorial Africa and used the latter's wavelength.  It issued contradictory orders to try to cause confusion, and appealed to French soldiers in the name of the Fighting French.

“In one broadcast, Brazzaville Two sought to create panic by announcing the spread of a plague of typhus in the zones occupied by American troops.  The speaker, purporting to be a De Gaullist, said: “We are dumfounded at the administration’s inability to check this scourge.”  The so-called Voice of Truth went on the air to Africa with a strong anti-Semitic line, announcing in one of its first broadcasts that “all Jewish officers who were in the French army and had been dismissed by the Vichy administration have been called up [in North Africa] and made high officers and advisers, but were never sent to the front.”

“For purposes of creating animosity between Arabs and Jews and creating enmity against the occupation forces among the native population, Vichy Arab-language transmitters, parading as authentic Arab mouthpieces, went on the air with broadcasts like this: “The Allied nations and the French traitors are delivering you to the Jews.  Your fathers were masters of the Jews.  The Allied nations are now making the Jews your masters.  Will you stand for this?”

“Fake freedom stations have been used with increasing frequency throughout Asia in recent months.  Afghanistan has been a favorite nesting spot for them, as Axis secret agents and even diplomatic missions have been able to work there with comparative freedom, broadcasting irresponsible, false news items and diatribes against Britain and the United States in the form of news commentaries.  These transmitters are usually not very powerful and are not designed to carry very far. Their principal job is to influence the more uncivilized natives of northwest India, Persia, Iraq and Arabia rather than the city populations of Asia.  For the latter the Axis has powerful transmitters located in its own capitals which parade as freedom stations.  Radio Himalaya, which is supposed to operate from New Delhi, actually originates in Rome; India Independence broadcasts from Tokyo; and Free India originates in Berlin.

“From time to time a freedom station does appear which has an unmistakably authentic ring, but it is rarely heard from more than a few times.  Such a station appeared in Belgium in June 1942 and called itself the Flemish Freedom Station.  The best recommendation for its authenticity was the fact that the Germans tried so hard to jam its broadcasts, and usually succeeded after the first minute or two.  It was rarely able to get more than a few sentences across before the jammer cut it out.  “This is the free transmitter of oppressed Belgium!” it would say.  “Hang all the traitors! Tear down all the swastikas!”  And that is about as far as it could get before the interference became too great for it to be heard.

A story of real heroism is connected with an unquestionably authentic station, operated in Holland.  Early in 1942, a Dutch Nazi was killed in Utrecht.  That night, an underground broadcasting station in the Netherlands gave a description of the murder, complete in every detail, even to the license number of the murdered Nazi’s car.  After that broadcast, the station was silent for a time, while the Gestapo scoured Holland in search of it.  Then, obligingly, it came on the air again.  This time it taunted the Nazis by giving a circumstantial report of a visit to Gestapo headquarters in Amsterdam.  The speaker described the interior of the building fully, mentioning the pictures on the wall, the dirt spots on the tile floors, and other striking details.  Weeks went by, but the Germans were unable to find the station.  The programs never came from the same source twice.  Jamming the transmitter proved impossible because its wavelength was always being changed.  That, of course, made it difficult for listeners to pick it up, but the men who ran the station realized that it was better to have a small, haphazard audience than to be shot.

“Probably the best known of all the fake freedom stations operating today is the one called Gustav Siegfried Eins, which broadcasts in German, ostensibly from Berlin. While it is clear that the Gustav Siegfried Eins station is not what it pretends to be, I cannot say what it actually is.  It purports to be operated by high officers of the German army who are opposed to the Nazis but want to win the war.  It is patriotically German, never says anything favorable to our side but consistently picks at Nazi party officials for their inefficiency, corruption and general mishandling of the war.  In December 1942, the station urged Germany not to waste men and material helping “the weak-sister Italians” on the African front and warned that the only vital front was Russia.  In this connection, the station made frequent attacks on Rommel for his unsuccessful African campaign.”

“The fact that the station has remained in existence for many months and has made frequent broadcasts shows that either the Nazi government does not want to suppress it, or cannot get at it.  And so it is likely the station originates somewhere in Europe outside of Germany, probably England.”

And that was an extract from the book ‘The Axis on the Air” by Harold Ettlinger, published in 1943.  In his assumption about the Gustav Siegfried Eins station (or GS1 for short), he was right on the money.  It was indeed a black psy-op station that broadcast from powerful shortwave transmitters at Signal Hill, Buckinghamshire and Potsgrove, Bedfordshire, England, a little northwest of London, beginning in May 1941.  It was the brainchild of journalist Sefton Delmer, who, having been born and  Sefton Delmer
raised in Berlin was a native German speaker, and together with a team of intelligence officers and German émigrés, dissidents, and POW’s, they created the station, which successfully masqueraded as an underground German station, to break the Nazi spirit and morale.

The main speaker in the broadcasts was called ‘The Chief’ (‘Der Chef’ in German), who in reality was a German Jewish refugee.  In late 1943, after Harold’s book was published, Sefton Delmer decided The Chief should be martyred.  A GS1 broadcast was abruptly interrupted by the sound of shouting, scuffling and gunshots, and then a different panicked voice came on saying “They’ve got him.  The Gestapo has silenced The Chief!”  The station then went dead, and the illusion was complete.  The Gestapo was credited with a murder they did not commit, but The Chief was transformed from a voice into a legend.  I wish I could bring you an audio recording of it, but sadly, none are known to exist.

But, from the ashes of GS1 rose several successors, including Soldatenzender Kalundborg, purporting to be a Wehrmacht station broadcasting from occupied Denmark, and playing the latest American jazz and swing music.  This had been banned by the Nazis, but was adored by the German troops.  Another successor was Soldatensender Calais which broadcast on 390 meters (833 kHz), 420 meters (714 kHz) and 490 meters (612 kHz) with an associated shortwave station Kurzwellensender Atlantik (Shortwave Station Atlantic) created to broadcast to U-boat crews.  It used a 500 kW medium wave transmitter originally constructed for the Newark, New Jersey station WJZ, although it had never been delivered due to the FCC imposing a maximum 50 kW power limit on U.S. stations.  So, RCA was glad to be able to sell it to the British Secret Service who codenamed it ‘Aspidistra’ and installed it near Crowborough, Sussex.  Soldatensender Calais operated from 6pm to dawn, and unlike its predecessor Gustav Siegfried Eins, all programs were broadcast live until it ceased operation on April 30, 1945.  And so the psychological warfare continued on the airwaves not just in Europe, but around the world, until the end of the war.  In the 1950’s, a different kind of psychological broadcasting took shape during the Cold War, but that’s a whole different story!

Back to you, Jeff.
(Wavescan-Ray Robinson)



India's Akashvani Summer Schedule 2026

 


INDIA/BHARAT   Akashvani External Summer Service A26 schedule

UTC        Language    kHz   Tx site      Target Area   Old kHz

0030-0830  Bangla        594(C)           Bangladesh
0100-0130  Sindhi       1071(R)  9870(B)  Pakistan       9860
0100-0230  Tibetan     11710(D)           Tibet
0130-0230  Indonesian  15260(B)           Indonesia
0145-0230  Nepali      15410(B)
                       103.2(N) 103.7(G)  Nepal
0230-0245  Hindi         "                 "
0245-0300  English       "                 "
0300-0315  Nepali        "                 "
0300-0430  Baluchi      9740(D)           Pakistan      11805
0315-0415  Burmese     15410(B)           Myanmar
0400-0530  Farsi       15130(B)           Iran          15280
0400-0745  Urdu         1071(R)
                       100.8(F) 103.6(A)  Pakistan
0430-0600  Dari         9740 (D)          Afghanistan   11805
0430-0600  Pashtu      15185(B)           Afghanistan
0530-0630  Arabic      15130(B)           Middle East   15280
0830-0845  English       594(C)           Bangladesh
0845-0900  Hindi          "                "
0900-1030  Nepali      11865(D) 15410(B)
                       103.2(N) 103.7(G)  Nepal
0930-1130  Urdu         1071(R)
                       100.8(F) 103.6(A)  Pakistan
1000-1515  Bangla        594(C)           Bangladesh
1030-1200  Chinese     15410(B)           China
1045-1215  Tibetan     11865(D)           Tibet
1130-1200  Saraiki      1071(R) 103.6(A)  Pakistan
1200-1330  Punjabi      1071(R) 103.6(A)  Pakistan
1215-1315  Swahili     15410(B)           East Africa
1230-1330  Baluchi      9870(D)           Pakistan
1230-1400  Pashtu      11750(B)           Afghanistan   11810
1330-1500  Dari         9870(D)           Afghanistan
1515-1530  Hindi         594(C)           Bangladesh
1530-1545  English       594(C)            "
1545-1830  Bangla        594(C)            "
1545-1930  Urdu         1071(R)
                       100.8(F) 103.6(A)  Pakistan
1600-1730  Farsi        9620(B)           Iran          11900
1730-1930  Arabic       9620(B)           Middle East   11900
1930-2030  French       9620(B)           We. Europe    11900
2330-0100  Punjabi      1071(R) 103.6(A)  Pakistan
2345-0115  Chinese     15410(B)           China         15280

(D) Delhi      100 kW
(B) Bengaluru  250 kW
(R) Rajkot    1000 kW
(C) Chinsurah 1000 kW

Note:
a) Home Service and other languages may be heard briefly for a few minutes prior to the start/end of some of the scheduled External Services languages.

b) A 15-minute program in English, "Spotlight," is broadcast on various services.

c) Reception Reports to: spectrum-manager@prasarbharati.gov.in
QSL cards are issued by postal mail
( Jose Jacob (VU2JOS)
(photo-Vceety)

Recent Brazilian monitoring on mediumwave

BRAZIL 

 With a considerable exodus of Brazilian stations from medium wave, following the nationally encouraged migration program to FM, which is still in effect,an excellent space opens up for tuning in to a good number of South American stations (on practically all frequencies).

Sometimes, two or three stations from more than one country are heard on the same frequency, making it a good exercise in using a good loop antenna. The vast majority of stations that arrive are from Argentina, Uruguay, and Paraguay, but on nights 'blessed' by the opening of propagation, we
have received stations from Chile, Peru, Bolivia, Colombia, Cuba, and the United States. Before the migration process to FM, it was impractical to have this contact with an extensive number of South American stations and beyond.

Some carriers (some weaker, some stronger) have been present in recent days: 639, 657, 828, 891, 1134, 1179, and 1498 kHz. The 828 kHz frequency, in particular, has shown the best results in recent
days (with only a few bursts of music and male voice communication), which, in a first preliminary analysis, we can think of as'Radio Magic 828 AM', South Africa. This station has been arriving occasionally. In 2021 after listening to it in better conditions,I sent them a reception report,
and was rewarded with a reply via email in just one day.

It is suspected that we can even create imaginations about the other carriers, but in radio listening, responsible patience makes us try to listen to them in better conditions to have new information that leads us to success. Eyes and ears are wide open !
(Rudolf Grimm, Ibiuna-SP-BRA #479, hcdx via wwdxc BC-DX TopNews April 24)

BRAZIL   670 kHz  'Radio Montanhesa', Ponte Nova MG, April 23 at 00.05 UT. Advertisements, ID. 'ZYL347 670 kHz Radio Montanhesa ...'. S5.

1240 kHz  'Radio Iracema', Cunha Pora SC, April 22 at 23.18 UT. Commentaries talking about 'Cunha Pora', Brazilian songs. S2. A strong QRM from 1240 kHz 'Rede Aleluia', Santos, SP.

1260 kHz  'Radio Cultura', Sao Borja RS, April 22 at 23.02UT. Commentaries about Sao Borja, announcements. S4.

1500 kHz  'Radio Aparecida do Sul MG', Ilicinea MG, April 20 at 20.06 UT. Brazilian songs, ID. 'em todo o lugar, Radio Aparecida do Sul'. S6.

1550 kHz  'Radio Cacique', Capivari SP, April 20 at 19.36 UT. A pop song, jingle 'Radio Cacique', advs Camara Municipal de Capivari. S4.(Rudolf Grimm, Ibiuna-SP-BRA #479, hcdx via wwdxc BC-DX TopNews April 24)
(WWDXC Top Nx 1652/06 May 2026)

May programming from Tilford Productions

 

From the Isle of Music, Friday, May 8, 2026, 3955 kHz, 1600 UTC, repeats 2200 UTC 
This month, we present some Cuban rock and pop from the 60s, 70s, and 80s..  

Uncle Bill's Melting Pot, Friday, May 15, 2016,: 3955 kHz at 1600 UTC, repeats 2200 UTC 
This month, we present some Persian classical music.  

In addition to direct radio reception, we do honor reception reports using remote SDRs as long as the whole program is described, and which SDR is specified. All QSLs are e-QSLs only.
 
(Bill  Tilford, Owner/Producer 
Tilford Productions, LLC )

Monday, May 04, 2026

Weekly Propagation Forecast Bulletins-May 4, 2026

Product: Weekly Highlights and Forecasts
:Issued: 2026 May 04 0142 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 27 April - 03 May 2026

Solar activity reached moderate levels on 27 and 18 Apr due to M-class (R1-Minor) activity from Region 4425 (N05, L=162, class/area=Ekc/320 on 28 Apr) and 4420 (S18, L=246, class/area=Eki/300 on 21 Sep). Region 4420 produced the strongest flare of the period, an M1.5/Sn (R1) flare at 28/1353 UTC. The region also produced two Type II radio sweeps alongside C-class activity. The ejecta associated with the activity originated from near the NW limb and was not suspected to contain an Earth-directed component. 

The other 13 numbered active regions on the visible disk were either mostly quiet or only produced C-class X-ray activity. No other Earth-directed CMEs were identified in available coronagraph imagery. 

No proton events were observed at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit was normal to moderate levels over the past seven days. 

Geomagnetic field activity reached G1 (Minor) geomagnetic storm levels on 30 Apr and active levels on 01 May due to the influence of a negative polarity CH HSS. Total magnetic field strength reached a brief peak of 14 nT on 30 Apr, with Bz reaching as far south as -12 nT. Solar wind speeds peak at just over 500 km/s early on 01 May and gradually waned over the next two days. The remainder of the period was at quiet to unsettled levels. 

Forecast of Solar and Geomagnetic Activity 04 May - 30 May 2026

Solar activity is likely to be at low levels with a chance for M-Class (R1/R2-Minor/Moderate) throughout the outlook period due to the flare potential of multiple regions on the visible disk as well as multiple complex regions due to return from the farside.  

No proton events are expected at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit is likely to reach high levels on 15-20 May due to influence from a recurrent, negative polarity coronal hole. The remainder of the outlook period is expected to at normal to moderate levels. 

Geomagnetic field activity is expected to reach G1 (Minor) geomagnetic storm levels on 15-17 May; active levels are likely on 08 May, 18 May, 23 May, and 27 May; unsettled levels are likely on 04 May, 09 May, 21-22 May, and 27 May. All enhancements in geomagnetic activity are forecast in anticipation of influence fron multiple, recurrent, coronal hole HSSs. The remainder of the outlook period is expected to be at mostly quiet levels. 

:Product: 27-day Space Weather Outlook Table 27DO.txt
:Issued: 2026 May 04 0142 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC web www.swpc.noaa.gov/content/subscription-services
#
#      27-day Space Weather Outlook Table
#                Issued 2026-05-04
#
#   UTC      Radio Flux   Planetary   Largest
#  Date       10.7 cm      A Index    Kp Index
2026 May 04     140           8          3
2026 May 05     140           6          2
2026 May 06     135           6          2
2026 May 07     130           6          2
2026 May 08     135          12          4
2026 May 09     130          10          3
2026 May 10     130           6          2
2026 May 11     125           5          2
2026 May 12     125           5          2
2026 May 13     120           5          2
2026 May 14     115           5          2
2026 May 15     120          25          5
2026 May 16     120          20          5
2026 May 17     125          20          5
2026 May 18     130          15          4
2026 May 19     130           5          2
2026 May 20     130           5          2
2026 May 21     130           8          3
2026 May 22     120          10          3
2026 May 23     125          12          4
2026 May 24     125           5          2
2026 May 25     125           5          2
2026 May 26     130           5          2
2026 May 27     135          12          4
2026 May 28     135          10          3
2026 May 29     130           8          3
2026 May 30     125           8          3
(NOAA)

Friday, May 01, 2026

A nostalgic journey from SM Dessau

 


The May 1, 2026, special broadcast from SM Dessau began with a nostalgic journey from former days on shortwave. 

The 1600 UTC broadcast, relayed from Gavar, Armenia, on 12060 kHz, began with a classic sign-on from Germany's Radio Berlin International. 


Shortwave Central YouTube channel has the video athttps://youtu.be/0KrsMXx07dQ

WRMI Schedule Update, April 23, 2026

 




WRMI A-26 Summer Schedule Update

The current color grid program schedule, dated April 23, 2026, is available at: 

Previous schedule post on  April 13, 2026


QSL - 2016

All times UTC
Programming in English, French, Italian, Japanese, Portuguese, Russian, Slovak, Spanish

0000-0100   5010ca  5050la  5850na  5950na  7730na  7780na  9455na  15770eu  17790va     
0100-0200   5050la  5800sa  5950na  7730na  7780ca  15770eu  17790va
0200-0300   5010ca  5050la  5950na  7780ca  9955la  15770eu
0300-0400   5050la  9955la  15770eu
0400-0500   7730na  7570na  7780ca  15770eu
0500-0600   7570na  7730na  7760ca  9395na  15770eu
0600-0700   5850na  7570na  7730na  7780ca  9395na  15770eu
0700-0800   5850na  7570na  7730na  7780ca  9395na  15770eu
0800-0900   7730na  7780ca  9395na  15770eu
0900-1000   5850na  7730na  9395na  15770eu
1000-1100   7570na  7730na  7780ca  9395na  15770eu
1100-1200   5850na  7730na  9395na
1200-1300   7730na  9395na
1300-1400   7730na  9395na
1400-1500   7730na  9395na  15770eu
1500-1600   7730na  9395na  17790va
1600-1700   7730na  9395na  17790va
1700-1800   7730na  9395na  15770eu  17790va 
1800-1900   7730na  9395na  15770eu  17790va
1900-2000   7730na  9395na  17790va
2000-2100   9395na  17790va
2100-2200   7730na  17790va
2200-2300   5850na  7730na  15770eu  17790va
2300-0000   5010ca  5850na  7730na  9455na17790va

Target Areas:
ca  Central America
eu  Europe
la  Latin America
na North America
sa  South America
va  Africa/South America

WRMI website:  http://wrmi.net/
Reception Reports: info@wrmi.net 
Rapid E-QSL: Send a reception report and receive an immediate e-QSL to: wrmiqsl@gmail.com
(GVH/Teak Publishing)

Texas Radio Shortwave- May 2-3, 2026 programs

 

May 2, 2026
1400-1500, 6160 Shortwave Radio Gold to Europe - Michael Strah on Texas Radio Shortwave: The Music of Tommy Taylor
1800-1900, 3975, 6160 Shortwave Radio Gold to Europe - Michael Strah on Texas Radio Shortwave: The Music of Tommy Taylor

May 3, 2026
1200-1300, 9670,  Channel 292 to Europe - Michael Strah on Texas Radio Shortwave: The Music of Tommy Taylor
2300-0000, 9670, Channel 292 to North America - Michael Strah on Texas Radio Shortwave: The Music of Tommy Taylor

This schedule is subject to change based on listener requests for specific Texas artists or music genres, propagation conditions, and other things beyond our control.
Texas Radio Shortwave is an independent producer of musical and topical shows, usually about Texas.
Unless otherwise shown, programs are one hour long.
Programs for Europe (Eur) and beyond on 3975 and 6160 kHz over Shortwave Radio Gold in Winsen, Germany, are transmitted with 1 kW into crossed dipole antennas.
Programs for Europe (Eur) and beyond on 6070 and 9670 kHz over Channel 292 in Rohrbach, Germany, are transmitted with 10 kiloWatts into an inverted V antenna.
Programs for North America (NAm) and beyond on 9670 kHz over Channel 292 are transmitted with 10 kW into a 10.5 dB gain beam antenna.
Texas Radio Shortwave uses a version of The Yellow Rose of Texas as its Interval Signal/Signature Song.

Texas Radio Shortwave verifies correct, detailed reception reports by electronic QSL. This includes reports from listeners using remote receivers (SDRs). Texas Radio
Many TRSW programs are archived at www.mixcloud.com/texasradiosw.
Texas Radio Shortwave's Facebook page is www.facebook.com/texasradiosw.
Texas Radio Shortwave's Listeners' Group Facebook page is www.facebook.com/groups/580199276066655/.
(TRSW) 
(photo/Wikipedia)