Jen's Eclectic Views & Real Deal, from March 22, is now available for YOU - to listen to or download.
Monday, March 23, 2026
Weekly Propagation Forecast Bulletins
Product: Weekly Highlights and Forecasts
:Issued: 2026 Mar 23 0245 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 16 - 22 March 2026
Solar activity reached moderate levels on 16-18 Mar, with low levels observed on 19-22 Mar. Region 4392 (S16, L=018, class/area=Csi/200 on 17 Mar) produced most of the flare activity observed throughout
the week, including three M-flares (R1-Minor). AR4392 produced an M2.7 flare at 16/1215 UTC with accompanying Type-II (est. 1,227 km/s), Type-IV, and Tenflare (380 sfu) emissions. The subsequent
asymmetric halo CME, first observed in LASCO C2 imagery at 16/1236 UTC, arrived at Earth on 20 Mar. AR4392 produced another M2.7 flare at 18/0842 UTC with accompanying Type-II (est. 860 km/s) and
Tenflare (229 sfu) emissions. The associated CME, first visible in LASCO C2 imagery at 18/0936 UTC, arrived simultaneously with the 16 Mar CME on 20 Mar.
No proton events were observed at geosynchronous orbit.
The greater than 2 MeV electron flux at geosynchronous orbit reached high levels on 16-20 and 22 Mar. Normal to moderate levels were observed on 21 Mar following a period of an elevated geomagnetic field
activity.
Geomagnetic field activity reached G1-G3 (Minor-Strong) geomagnetic storm levels on 20-22 Mar, following the arrival of multiple CMEs (that left the Sun on 16 and 18 Mar) on 20 Mar. The remainder of the
period was at quiet and quiet to unsettled levels under ambient solar wind conditions.
Forecast of Solar and Geomagnetic Activity 23 March - 18 April 2026
Solar activity is expected to be at low levels with a varying chance for M-class (R1-R2/Minor-Moderate) flares through 18 Apr.
No proton events are expected at geosynchronous orbit, barring significant flare activity.
The greater than 2 MeV electron flux at geosynchronous orbit is expected to reach high levels on 23-25, 27-28, 30-31 Mar and 04-09, 11-15 Apr. Normal to moderate flux levels are expected to prevail
throughout the remainder of the period.
Geomagnetic field activity is expected to reach G1-G2 (Minor-Moderate) geomagnetic storm levels on 23 Mar due to negative polarity CH HSS influences. Periods of G1 (Minor) storming are
likely on 03-04 Apr in response to negative polarity CH HSS influences. Periods of G1 (Minor) storming are likely on 09 and 11 Apr, with G2 (Moderate) storm periods likely on 10 Apr, due to
positive polarity CH HSS influences. G2 (Moderate) storm periods are likely again on 18 Apr following the onset of negative polarity CH HSS influences.
Product: 27-day Space Weather Outlook Table 27DO.txt
:Issued: 2026 Mar 23 0245 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 2026-03-23
#
# UTC Radio Flux Planetary Largest
# Date 10.7 cm A Index Kp Index
2026 Mar 23 120 34 6
2026 Mar 24 120 14 3
2026 Mar 25 122 12 3
2026 Mar 26 125 12 3
2026 Mar 27 130 8 3
2026 Mar 28 130 5 2
2026 Mar 29 128 8 3
2026 Mar 30 125 15 4
2026 Mar 31 125 10 3
2026 Apr 01 130 5 2
2026 Apr 02 120 5 2
2026 Apr 03 120 18 5
2026 Apr 04 115 24 5
2026 Apr 05 110 10 3
2026 Apr 06 120 15 4
2026 Apr 07 120 8 3
2026 Apr 08 118 7 2
2026 Apr 09 120 25 5
2026 Apr 10 110 40 6
2026 Apr 11 112 20 5
2026 Apr 12 115 12 3
2026 Apr 13 115 8 3
2026 Apr 14 110 7 2
2026 Apr 15 115 5 2
2026 Apr 16 115 4 2
2026 Apr 17 120 7 2
2026 Apr 18 122 48 6
(NOAA)
Sunday, March 22, 2026
Encore classical music from Radio Tumbril
Dear Listener
Regular Broadcast times of Encore By WRMI and Channel 292 are:
02:00 - 03:00 UTC Friday 5850 kHz WRMI to US
20:00 - 21:00 UTC Friday 15770 kHz WRMI to Europe
11:00 - 12:00 UTC Saturday 9670 kHz Channel 292 to Europe
01:00 - 02:00 UTC Sunday 5850 kHz WRMI to US and Canada
18:00 - 19:00 UTC Sunday 3955 kHz Channel 292 to Europe
02:00 - 03:00 UTC Monday 5950 kHz WRMI to the US and Canada
13:00 - 14:00 UTC Tuesday 15770 kHz WRMI to Europe, east
coast of US and Iceland. (Sometimes RTTY on the lower sideband. Suggest notch out or use USB.)
Some Things to see on The Encore Website:
The Encore website is www.tumbril.co.uk where you will find:
Important information about funding of Encore - Radio Tumbril.
Up to date transmission times and frequencies.
The playlists for the most recent programmes.
An email link.
Informal reception reports as well as those requesting eQSL cards are welcome.
PLEASE MAKE A PAYPAL DONATION AND HELP KEEP ENCORE ON THE AIR - Go to - www.tumbril.co.uk
WRMI and Channel 292 are very generous with their air-time but Encore still costs around 130 Dollars/Euros a month to broadcast.
If you can - please send a small contribution to help Encore keep going.
THIS FORTNIGHT'S PROGRAMME - First broadcast on FRIDAY 20th March by WRMI at 0200 UTC on 5850, and 2000 UTC on 15770 and then Channel 292 on SATURDAY 21st March at 11:00 UTC on 9670 kHz:
Starts with part of the Concerto for Flute, Harp, and Orchestra by Mozart, some Tango inspired music from Argentina, and an example of music for high Baroque trumpet by J S Endler.
After that an arrangement for piano quartet of The Sea and the Seagulls from Rachmaninoff, and some film score by Caroline Shaw.
The last piece is the first movement of Borodin's Quartet No. 2.
Brice Avery - Encore - Radio Tumbril - www.tumbril.co.uk
GMØTLY
U.K. Propagation Update
RSGB
RadCom Assistant Editor | March 20, 2026
Last weekend’s Commonwealth Contest got off to a bad start, thanks to a Kp index of 6 that really affected the ionosphere.
As a result, HF conditions were not good with the maximum usable frequency over a 3,000km path below 21MHz until 1700UTC. Luckily, things improved a little on Sunday but overall scores were down compared with previous events.
The Kp index increase was due to a coronal hole stream which reached 600 to 700km/second and a Bz that pointed south. The equinox period hasn’t helped due to the Russell-McPherron effect, a phenomenon that occurs when the Earth’s magnetic field aligns with the Sun’s magnetic field during equinoxes, creating ‘cracks’ in the magnetosphere.
Otherwise, the week has been unremarkable. The solar flux index has remained firmly in the 110s and there have been no X-class solar flares, only a few M and lesser C-class events.
Next week, HF propagation may be dominated again by the solar wind. Coronal hole number 33 will begin to face Earth and a high-speed stream was predicted to reach us this weekend, ending today, 22 March. A coronal mass ejection was also predicted to arrive around Thursday, 19 March.
NOAA predicts the Kp index will rise to 5 this weekend and not decline to 3 until 26 March. Meanwhile, the solar flux is predicted to remain in the 105 to 120 range until 27 March. It may then increase slightly to be in the 120s until the end of the month.
As a result, expect lower maximum usable frequencies and poorer HF conditions until around next Thursday and Friday, 26-27 March.
VHF and up propagation news from G3YLA and G4BAO:
The high pressure that developed during the second half of last week formed on the warmer side of the front and as a result produced slightly better tropo conditions than looked possible the previous week.
The weather is probably going to try to change to a colder air high in the coming week, so expect conditions to decline. However, that’s not the only reason for a decline.
As the main high centre displaces west of Britain, we will find a colder and unsettled west or northwesterly pattern affecting the UK next week. So less tropo, but more chance of some rain scatter for the upper GHz bands.
Meteor scatter remains in the random activity domain, although we are edging closer to the next major shower of the late April Lyrids.
It’s not to say that exciting things can’t happen, however. Just after a HamSCI workshop on the subject of meteor scatter last weekend, a multi-ton meteoroid was reported from Cleveland, Ohio, on the HamSCI Google groups at around 1300UTC on 17 March.
This produced a sonic boom and was visible in broad daylight.
All is quiet on the Sporadic-E front, although we are slowly moving towards a period when the first glimmers of activity show themselves, particularly on digital modes.
Lastly, a comment on the chances of aurora. These are usually enhanced due to solar-terrestrial alignment around the equinoxes and with two coronal mass ejections predicted to arrive at the tail end of last week, ending today, 22 March. As usual, check for an increasing Kp index above 5.
For EME, yesterday saw the 5.7GHz section of the Dubus CW and SSB EME contest and associated all-mode activity weekend.
With Moon declination positive and rising, and path losses still low, it hopefully produced some nice contacts.
On VHF, 144MHz sky noise is low in the coming week.
https://rsgb.org/main/blog/news/gb2rs/propagation-news/2026/03/20/propagation-news-15-march-2026-2/
(Mike Terry, UK/BDXC)
Thursday, March 19, 2026
Uncle Bill's Melting Pot, March 2026
Uncle Bill's Melting Pot March 2026
We are going to feature music from Ghana, including a tribute to the memory of Ebo Taylor.
Friday, March 20, 2026, :3955 kHz, 1700 CET (1600 UTC), repeat 2300 CET (2200 UTC)
Our eQSL policy includes recognizing reports from remote SDRs as long as the entire program is reported and the location of both the remote SDR and the listener is included. Shorter reports will get a short note of thanks instead.
William "Bill" Tilford, Owner/Producer
Tilford Productions, LLC
email: bill@tilfordproductions.com
website: www.tilfordproductions.com
Tuesday, March 17, 2026
Radio in Antarctica-Part 1
.JPG)
Penguins and the remains of the wreck The Gratitude, Nuggets Beach, Macquarie Island, 1911, Frank Hurley
Part 1 – Macquarie Island & South Georgia
Thank you to the staff of Wavescan, for Part 1 of Part 3 in this series
Jeff: This week, we begin a two-part look at radio broadcasting in a part of the world few of us will ever get to visit – Antarctica. In part 1 this week, Ray Robinson looks at the history of broadcasting in two remote islands in the Antarctic region – Macquarie Island, governed by Australia, and South Georgia, governed by the British.
Ray: Thanks, Jeff. Macquarie Island is a cold, windswept island located halfway between the South Island of New Zealand and the Antarctic land mass. It is a long, thin island, 21 miles long and 3 miles wide, and is actually the exposed top of the Macquarie Ridge where the Australian and Pacific tectonic plates meet. Consequently, the area is prone to earthquakes, and two very large ones have occurred there so far this century, up around 8 on the Richter Scale. In spite of its remoteness and extreme climate, though, the island’s latitude is actually less than 55 degrees south – about the same latitude in the northern hemisphere as, say, Newcastle in England, or Copenhagen, Denmark.
The island has no permanent human population, but it has been governed as part of the Australian state of Tasmania since 1880. It is also home to the entire Royal Penguin population during their annual nesting season.
Macquarie Island has been noted as a place of shipwreck and as the temporary, unplanned home of shipwreck survivors. It was named in honor of a governor of New South Wales, Governor Lachlan Macquarie. The first known visitors to Macquarie Island were Polynesian sea travelers, most likely from New Zealand, although it’s not known when they initially encountered the island.
The first European to visit the island was Captain Frederick Hasselborough aboard the Perseverance who came across the island by chance on July 10, 1810. Ten years later, a Russian explorer, Thaddeus von Bellinghausen, also visited Macquarie. And then two years later again, Captain Douglass on the Mariner visited the island and pronounced it as unfit for human habitation. But, in 1825, Macquarie Island was declared to be part of Van Diemen’s Land, or Tasmania as we know it today.
For about 100 years, the island was used as a base for commercial companies harvesting animal oils, furs and skins. This commercial exploitation ended around 1920, by which time the animal populations had been hunted almost to extinction.
Since shortly before World War I, a total of four different communication stations have been established on Macquarie Island and its claim to fame is that the very first wireless station in the Antarctic region was installed on this forbidding island. The story goes back to the year 1911.
It was in December of 1911 that a small convoy of sailing ships, led by the Aurora, left Hobart, Tasmania, bound for Macquarie Island. A little over a week later, these venturing ships arrived off the coast of Macquarie, only to find several seafarers already on the island, survivors of a ship that had been wrecked there just the day before.
On board the Aurora was all of the apparatus intended for the new wireless station; a 1½ kW Telefunken spark transmitter & receiver, masts & wires, and a petrol generator. All of this electrical equipment was installed in a newly built wooden hut at the northern end of the island, for operation by the commercial companies engaged in animal hunting and processing there. Twin wooden masts were erected on top of a nearby hill which was 350 ft above sea level.
The first historic wireless contact with the outside world was made on the evening of February 13, 1912 when station MQI talked with shipping south of Australia and New Zealand in spark gap Morse Code. Soon afterwards, Morse Code contact was made with wireless stations AAM in Melbourne, AAA in Sydney & WN in Wellington. However, the Macquarie Island wireless station didn’t fare well. The aerial system was damaged and destroyed by high winds on three or four occasions, and there was always difficulty in making adequate contact with the Antarctic mainland as well as with Australia and New Zealand.
Finally, at the end of nearly three years of difficult service, the station was dismantled and shipped back to Australia, but the ship carrying it was sunk in a naval skirmish soon after the commencement of World War I in 1914, and all of the equipment was lost. Both New Guinea and Samoa were German colonies at that time, and naval engagement with Australia and New Zealand began as early as August 1914.
The second wireless station for Macquarie Island was planned after World War I, and was listed with the callsign VIQ in 1921. However, available records indicate that it may only have been on the air for a short period of time, if indeed it was ever erected at all.
A third station, this time for voice communication, was planned for Macquarie Island in 1947. This was to be a shortwave station with the callsign VJM, and it was finally installed by a contingent of amateur radio operators five years later in 1952. This station, again using 1½ kW, was in intermittent usage, depending on the availability of personnel, until communication on shortwave was phased out in 1988 in favor of satellite communication.
However, the shortwave station on Macquarie was re-activated in 1992 under the same callsign, VJM, but with a batch of new equipment, including a 1 kW Racal transmitter. Thus, Macquarie Island has been on the air with communication equipment during four widely separated eras under three different callsigns, MQI, VIQ & VJM. Wireless and radio messages from Macquarie Island were mainly for the benefit of passing shipping and other isolated wireless stations, with the home base on the island of Tasmania.
It is understood that a few QSL’s do exist verifying the VJM callsign, and in addition, several amateur radio operators who served on the island also issued their own amateur QSL cards.
And then there’s another very remote island near the continent of Antarctica – South Georgia in the far South Atlantic Ocean. Like Macquarie, this island is also less than 55 degrees south, but is often covered by snow, and famously was where Ernest Shackleton finally made landfall in 1916 following the disastrous Imperial Trans-Antarctic Expedition.
South Georgia is larger than Macquarie, being about 100 miles long and 25 miles wide, but it is equally as forbidding. The first settlement on the island was established in 1904 by a colony of Norwegian seafarers, and it ultimately became the hub of the whaling industry with some 2,000 permanent residents.
In 1925, a shortwave wireless station with the call sign ZBH was established by the British administration to enable communication with the outside world.
In 1938, a solar eclipse occurred over South Georgia on Sunday morning, May 28. The British arranged for special broadcasts from the island for the occasion and two small portable transmitters were stationed at two different locations, one on South Georgia itself, and the other further south on South Orkney, much closer to the Antarctic landmass. It is understood that these transmitters operated in the old Apex Hi-Fidelity Band, 30-40 MHz, feeding live transmissions to a more powerful relay station in Argentina, probably at Monte Grande.
Records also indicate that the communication station ZBH, located at King Edward Point on South Georgia Island, was also used to relay the live broadcasts from the two small portable transmitters. At the time of the eclipse, ZBH was on the air with 1 kW, on 8205 kHz.
In 1947, ZBH was again noted on 8 MHz with an irregular schedule that included a relay of the BBC news at 6:00 am. Station ZBH in South Georgia was later shown on a set of postage stamps, issued in 2006.
Reception reports for the special eclipse broadcasts from South Georgia were requested and these were to be addressed to the Colonial Secretary at Port Stanley in the Falklands. However, it is unknown whether any QSL’s were ever issued for the event. It is also unknown whether any QSL’s were issued for the relay of the BBC news via ZBH, or for any of its regular communications on shortwave.
Well, next week, I’ll be looking at the history of broadcasting on the Antarctic landmass itself, and there is quite a bit more to that than you might think.
Back to you, Jeff.
(Ray Robinson/Jeff White)
Monday, March 16, 2026
Audio available for Jen &GB's St. Patrick program from March 15
If you missed it .... no problem !
Jen & GB's St Patrick's Day Annual Cast On Unique audio for Sunday, March 15, is up and ready for listening and downloading. Programming includes a variety of Irish tunes, reels, jigs, and other goodies from the Celtic world, plus an all-green edition of Real Deal.
Audio available at:
Tiny URL link:
Contact at:
Trump nominates new head of VOA's parent agency after court ruling against Kari Lake
President Donald Trump nominated a senior State Department official on Thursday for the top post at the U.S. Agency for Global Media after a federal judge ruled that Kari Lake's leadership violated federal law.
Trump nominated Sarah Rogers, the undersecretary of state for public diplomacy, less than a week after U.S. District Judge Royce Lamberth ordered that all actions Lake took as acting CEO from July 31 to Nov. 19 be considered void, including an Aug. 29 reduction-in-force that eliminated jobs for more than 500 employees at Voice of America and elsewhere within USAGM.
Additional story at:
Tiny URL: https://tinyurl.com/5x96yssw
Weekly Propagation Forecast Bulletins
Product: Weekly Highlights and Forecasts
:Issued: 2026 Mar 16 0302 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC cweb ontact www.swpc.noaa.gov/content/subscription-services
#
# Weekly Highlights and Forecasts
#
Highlights of Solar and Geomagnetic Activity 09 - 15 March 2026
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Solar activity was at low to moderate levels with a total of 37 C-class flares and 2 M-class flares observed. The largest flares of the period were an M1.2 flare on 13/0955 UTC from Region 4384 (N10, L=150, class/area Eho/300 on 03 Mar), a C8.9/1n flare on 13/2023 from Region 4392 (S15, L=017, class/area Cso/170 on 15 Mar), and an M1.0/Sf flare on 15/0939 UTC from Region 4392. The most active region of the period was Region 4381 (N08, L=173, class/area Eao/220 on 03 Mar), which produced a long-duration C8.0 flare on 13/1518 UTC in addition to 11 other weak C-class events.
No proton events were observed at geosynchronous orbit.
The greater than 2 MeV electron flux at geosynchronous orbit reached high levels on 09 - 13 Mar and 15 Mar with a peak flux of 2,940 pfu observed at 12/1545 UTC. Normal to moderate levels were observed on 14 Mar.
Geomagnetic field activity ranged from quiet to G2 (Moderate) storm levels throughout the 09-15 Mar period. The week began at quiet to unsettled levels on 09 Mar, with active conditions observed on 10-11 Mar due to the influence of a negative polarity coronal hole high speed stream (CH HSS). Conditions returned to mostly quiet to unsettled levels by 12 Mar. Activity intensified midday on 13 Mar, reaching G1 (Minor) to G2 (Moderate) storm levels following the onset of a positive polarity CH HSS. These storming levels continued through the first half of 14 Mar before waning to unsettled and active levels later in the day. On 15 Mar, the field reached active levels early in the period, followed by a return to quiet and unsettled conditions as positive polarity CH HSS effects gradually diminished.
Solar wind parameters reflected the influence of two distinct CH HSS regimes during the period. The week began under the influence of a negative polarity CH HSS, with solar wind speeds initially ranging between 450-500 km/s before gradually declining to ambient levels near 400 km/s by 12 Mar. Total magnetic field (Bt) remained mostly around 6 nT during this interval, while the North-South (Bz) component saw periodic southward deflections to -7 nT. A solar sector boundary crossing (SSBC) occurred early on 13 Mar, indicated by a shift in the phi angle from the towards to away sector. This was immediately followed by the onset of a more powerful positive polarity CH HSS. Solar wind speeds rose sharply from 400 km/s to a peak of 725 km/s on 14 Mar. During this period, Bt reached 13 nT and the Bz component reached a maximum southward deflection of -10 nT.
By 15 Mar, solar wind speeds began a slow decline but remained elevated near 600 km/s through the end of the period.
Forecast of Solar and Geomagnetic Activity 16 March - 11 April 2026
Solar activity is expected to be at low levels, with a slight chance for M-class (R1-R2/Minor-Moderate) flares throughout the outlook period. Elevated probabilities are related to the flare potential of both currently observed spot groups as well as the potential from returning regions.
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 16-20, 22-30 Mar, 04-09, and 11 Apr due to the influence of multiple, recurrent, CH HSSs. The remainder of the outlook period is likely to be at normal to moderate levels.
Geomagnetic field activity levels are likely to reach G1 (Minor) geomagnetic storm levels on 22 Mar, 04 Apr, 09 Apr, and 11 Apr due to CH HSS influences. G2 (Moderate) geomagnetic storm levels are likely on 11 Mar and 10 Apr due to CH HSS influences. Unsettled to active levels are likely on 16-18, 20, 23-27, 30-31 Mar, and 03 and 05-07 Apr. All elevated levels of geomagnetic activity are associated with the anticipated influence of multiple, recurrent, CH 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 Mar 16 0302 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 2026-03-16
#
# UTC Radio Flux Planetary Largest
# Date 10.7 cm A Index Kp Index
2026 Mar 16 108 15 4
2026 Mar 17 108 10 3
2026 Mar 18 105 8 3
2026 Mar 19 105 5 2
2026 Mar 20 105 10 3
2026 Mar 21 100 35 5
2026 Mar 22 102 25 5
2026 Mar 23 105 15 4
2026 Mar 24 110 15 4
2026 Mar 25 100 18 5
2026 Mar 26 110 10 3
2026 Mar 27 120 8 3
2026 Mar 28 125 5 2
2026 Mar 29 125 5 2
2026 Mar 30 125 15 4
2026 Mar 31 125 10 3
2026 Apr 01 130 5 2
2026 Apr 02 135 5 2
2026 Apr 03 140 18 5
2026 Apr 04 135 20 5
2026 Apr 05 135 8 3
2026 Apr 06 130 15 4
2026 Apr 07 135 8 3
2026 Apr 08 130 5 2
2026 Apr 09 125 25 5
2026 Apr 10 120 40 6
2026 Apr 11 115 20 5
(NOAA)
Sunday, March 15, 2026
Info on WEWN website update
USA. The WEWN/ETWN website has updated (after 2 years) its frequency schedule page at https://www.ewtn.com/radio/frequency-guide and is now showing the schedule for 28 March to 24 October 2026, as follows: 12050 from 1400-0600 UT and 15610 from 1900-0600 UT. No languages listed, but 12050 is Spanish, and 15610 would be English but is still, I think, currently off-air.
)Alan Roe, Teddington UK/BDXC)
Saturday, March 14, 2026
Jen' & GB's Annual St. Patrick's Day program
 |
| (designs by Gayle Van Horn) |
Get your green on !! Jen and GB's St. Patrick's Day Annual Cast On Unique, Sun March 15th at 18:00 -23:00 UTC and beyond!
First intro to 18:15 UTC
Then GB takes over with his Irish Variety Selection to around 1930 UTC, then I finish up to past 2300 UTC with reels, jigs,and other goodies from the Celtic world, plus my all-green edition of the Real Deal.
Then GB takes over with his Irish Variety Selection to around 1930 UTC, then I finish up to past 2300 UTC with reels, jigs,and other goodies from the Celtic world, plus my all-green edition of the Real Deal.
Live Stream:
Join us in our "Green" chat room
Click on connect, then web chat
Please put in the following:
For Nick: name or like me radionutresss
Then the next line channel, that's the following:
#eyeradiojd
and you are in the room.
Slaint !
Jen & GB
For contact pleasure.
Jen In The Rad.
73'' & 33''
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