Monday, January 19, 2026

WRMI Winter Schedule Update-January 9, 2026

 


The current color grid program schedule,  dated January 9, 2026 is available at: https://docs.google.com/spreadsheets/d/1pcIEX8kisrOPqlXHDAq6gympKUgDj0SIb96qce2kGGQ/edit?gid=0#gid=0

The previously updated schedule was posted on November 8, 2025

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

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

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)

Weekly Propagation Forecast Bulletins

 Product: Weekly Highlights and Forecasts
:Issued: 2026 Jan 19 0216 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 12 - 18 January 2026


Solar activity ranged from low to strong levels. Forty-five C-class, three M-class (R1-Minor) and one X-class (R3-Strong) activity was observed from various regions on the disk during the period. A majority of the activity was observed from Regions 4341 (S11, L=046, class/area Dkc/840 on 16 Jan), 4342 (N17, L=041, class/area Dso/180 on 16 Jan) and 4343 (S11, L=097, class/area Dki/310 on 16 Jan). 

Region 4341 produced the following R1 (Minor) flare activity: an M1.6/1f at 14/2033 UTC, an M2.1/2b at 17/1029 UTC and an M1.1/2n at 17/2351 UTC. This region also produced an X1.9/3b long-duration event at 18/1809 UTC. Associated with this flare was a 693 km/s Type II sweep, a Type IV sweep, a 3,200 sfu Tenflare and a Castelli-U radio burst. An associated full-halo CME was first noted in GOES CCOR-1 imagery at about 18/1830 UTC. Additional coronagraph imagery will determine any Earth-directed component. 

A 10 MeV at 10 pfu proton event at geosynchronous orbit (S1-Minor) was first observed at 18/2255 UTC. This event occurred in association with the X1.9 flare at 18/1830 UTC. 

The greater than 2 MeV electron flux at geosynchronous orbit reached high levels on 12-18 Jan. A peak flux of 9,398 pfu was observed at 14/1645 UTC. 

Geomagnetic field activity was at quiet to minor storm levels (G1-Minor) throughout the period. Quiet to active levels were detected on 12-13 Jan associated with waning CME influence and effects from a negative polarity CH HSS. Mostly quiet levels were observed on 14 Jan. Unsettled to minor storm (R1-Minor) levels were detected on 15 through midday on 17 Jan. Unsettled to active levels were observed on the latter half of 17 Jan through 18 Jan due to positive polarity CH HSS. 

Forecast of Solar and Geomagnetic Activity 19 January - 14 February 2026

Solar activity is likely to remain at low levels, with a chance for R1-R2 (Minor-Moderate) and a slight chance for R3 (Strong) levels over the next forecast period, all due to multiple regions on the visible disk as well as regions expected to return. 

10 Mev at 10 pfu proton events (S1-Minor) are expected at geosynchronous orbit on 19-20 Jan. 

The greater than 2 MeV electron flux at geosynchronous orbit is expected to reach high levels on 19-27 Jan and 12-14 Feb, all due to the anticipated influence of multiple, recurrent coronal holes. 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 on 29 Jan and unsettled to active levels on 19-23, 27-28, 30-31 Jan, 04-11 and 13-14 Feb. All enhancements in activity are due to the anticipated influence of multiple, recurrent CH HSSs. The remainder of the outlook period is expected to be mostly quiet. 

:Product: 27-day Space Weather Outlook Table 27DO.txt
:Issued: 2026 Jan 19 0216 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 2026-01-19
#
#   UTC      Radio Flux   Planetary   Largest
#  Date       10.7 cm      A Index    Kp Index
2026 Jan 19     160          20          4
2026 Jan 20     165          16          4
2026 Jan 21     170          10          3
2026 Jan 22     175           8          3
2026 Jan 23     180           8          3
2026 Jan 24     180           5          2
2026 Jan 25     175           5          2
2026 Jan 26     170           5          2
2026 Jan 27     165          10          3
2026 Jan 28     160          15          4
2026 Jan 29     165          25          5
2026 Jan 30     165          12          4
2026 Jan 31     160          10          3
2026 Feb 01     155           5          2
2026 Feb 02     150           5          2
2026 Feb 03     145           5          2
2026 Feb 04     140          15          4
2026 Feb 05     130          12          4
2026 Feb 06     120          10          3
2026 Feb 07     125           8          3
2026 Feb 08     130           8          3
2026 Feb 09     135          10          3
2026 Feb 10     140           8          3
2026 Feb 11     135           8          3
2026 Feb 12     135           5          2
2026 Feb 13     135          20          4
2026 Feb 14     140          15          4
(NOAA)

BBC Daventry, part 2

 

Special thanks to Ray Robinson, Dr Adrian Peterson, and Jeff White for Part 2, of the BBC Daventry feature. Last week's Part 1 is available at: https://mt-shortwave.blogspot.com/2026/01/bbc-daventry-part-1.html

Jeff: Today we conclude our two-part feature about the large BBC shortwave transmission facility at Daventry in the English Midlands.  Last week, we reached about 1935, at the time when the BBC purchased an additional 95 acres and began the construction of a new transmitter building capable of holding three large shortwave transmitters, and erected 25 new antennas, 14 of which were reversible curtains.  Here’s Ray Robinson in Los Angeles to continue the story.


Ray: Thanks Jeff.  Yes, we also mentioned last week that the BBC had announced plans to acquire two new 100 kW transmitters.  They did indeed buy two new units made by STC, the British equivalent of the American Western Electric Company, although the transmitters weren’t quite as powerful as had been planned.  They were, in fact only capable of output power ranging between 50 and 80 kW, but they were duly installed and commissioned in 1937 as Senders 4 and 5.

In addition, a small 7.5 kW transmitter was also installed in the new ‘Empire Service Building’, and all three were on the air for the special broadcasts associated with the Coronation of His Majesty King George VI.  Sender 6, a Marconi 100 kW transmitter, was commissioned nearly a year later.

It should be remembered that similar progress was underway at the same time in other countries around the world.  Statistics during that era reveal that there were 131 shortwave transmitters on the air worldwide in May 1936, and by October in the following year 1937, there were then 245 shortwave transmitters on the air.  The number had almost doubled in less than 18 months.

During the late 30’s, BBC Daventry was usually on the air with two transmitters in parallel, though occasionally three were employed.  For very special occasions, they would sometimes activate as many as four of these shortwave transmitters with parallel programming.

In April 1938, the additional 100 kW Marconi transmitter (Sender 6) was shoe-horned into the Empire Service Building, and work commenced on the addition of an east wing to the building for the installation of two more new 100 kW Marconi units.  These were commissioned in February 1939 as Senders 8 and 9.

Back at this time, it was common practice to allocate a callsign to a specific transmitter (not to a station), and then to give supplementary callsigns for each channel or waveband used by that unit.  The primary callsign for BBC Daventry was GSE, with the "E" standing for Empire.  All 26 letters of the English alphabet were used for various shortwave channels, and then they began to allocate additional callsigns in a similar manner in the GR series.  Callsigns in the range GSA, GSB, GSC, etc, right down to GSZ were all taken up, one call per shortwave channel; and then they began to use the sequence in the GR series, beginning with GRZ and working backwards in the English alphabet, GRY, GRX, etc., right up to GRA.

With political events heating up on continental Europe, the BBC began to introduce foreign language programming into its external shortwave services.  The first additional language was Arabic which was inaugurated in January 1938.  Two months later, Spanish and Portuguese for South America were introduced, followed by several continental languages in the following year or two.  Studios for all of these external services were established in Bush House, London, which became the home of the BBC World Service for many decades.

At the time of the outbreak of hostilities in continental Europe in September 1939, BBC Daventry was on the air with nine shortwave transmitters, designated as follows:

Building Transmitters Make kW Identification
Original Shortwave Building 2 STC 10 Senders 1 & 2
5GB Medium Wave Building 1 Marconi 60 Sender 3
Two Wings of Empire Service Building 2 STC 80 Senders 4 & 5
Marconi 100 Senders 6, 8 & 9
Marconi 7.5 Standby


The designation Sender 7 was reserved for a bifurcated transmitter that was capable of radiating on two channels simultaneously, and that was installed more than a year later, in December 1040.  In BBC terminology, it was actually identified as Sender 7A and 7B.

A new relay service via the BBC commenced on Saturday April 25, 1942, and this was on behalf of the new Voice of America with its studios in Madison Avenue, New York City.  Programing was either taken off air and forwarded by landline to Daventry, or it was sent by undersea cable and re-transmitted from Daventry on shortwave.  Some programming was sent to England on recorded discs.  At this stage, the BBC initially incorporated the American programming into their own scheduling, rather than broadcasting the American programs as a separate relay.  

During this decisive era, the BBC began work on three additional large shortwave transmitter sites, at Skelton, Rampisham and Woofferton, and by the end of 1943, the BBC was capable of 

handling 43 different shortwave transmissions simultaneously.  By the end of the war in 1945, direct relays of the Voice of America had been transferred from Daventry to the new facility at Wooferton.

Following the war, Britain experienced a period of austerity, with rationing continuing into the early 1950’s, and the BBC was not immune.  Beginning on February 10, 1947, every BBC transmitter was required to drop its power output to 50 kW.  This was not only for economy, but also because the power generating equipment in England was getting quite old and it had not been possible to upgrade it for many years.  This requirement was in force for a period of two years and it was finally lifted on March 21, 1949.

On July 20, 1963, there was a total solar eclipse across the Atlantic and Radio Canada International made arrangements with the BBC to broadcast a special series of transmissions beamed towards Canada.  Three years later, RCI began regular relays via BBC Daventry for programming beamed towards continental Europe and the Mediterranean areas.  Then, in 1967, RCI actually bought two of the shortwave transmitters at Daventry for relay purposes.  Programming by this time was provided by a satellite link from Canada to England.

During the 1960’s, a modernization program was implemented at Daventry with the removal of several older transmitters which were replaced by more modern and higher-powered equipment.  Additionally, the antenna systems were also upgraded.  
However, time was moving on and the grand old facility at Daventry was beginning to show its age.  It was becoming evident that the entire facility would need to be rebuilt, or simply closed down in favor of other more modern locations.  A date was set for the final closure of the station and the sale of the land for other purposes.  This would finally come in 1992.

For a period of almost sixty years, the majestic station at Daventry had been on the air with up to two dozen shortwave transmitters, some as powerful as 250 kW, radiating through a bevy of around 50 different antenna systems.  

In preparation for the ultimate demise of BBC Daventry, usable equipment was removed and transferred to other locations.  And for the final closure of the last transmitter on air, a farewell party was held with dignitaries coming in from many different places and organizations.  It had to happen; and it took place at 1130 UTC on Sunday March 29, 1992.

Sender 24 was the last remaining transmitter still on the air; most of the others had already been removed.  That unit was radiating on the well-known BBC channel 15070 kHz, formerly designated as shortwave channel GWC.  The broadcast came to its end, and the transmitter was switched off.  The BBC Daventry shortwave site was now silent, forever.

The property was sub-divided, and some was sold for a housing development and a local park.  Two years later, all of the antenna towers were dropped, except one which is now in use for local phone communication.  In one of the still standing buildings, a radio museum was established, and you can now find information about that online at daventrymuseum.co.uk.

Back to you Jeff




:


Sunday, January 18, 2026

Radio Mystery Theater programming schedule on WRMI

 



WRMI Facebook Post on 10 January:
Radio Mystery Theater Listings for January-March 2026:

Jan. 24 Quiet Please Radio Show, "Calling All Souls" 1948
Jan. 31 The Hermit's Cave Radio Show, "Hanson's Ghost" 1944
Feb. 7 Suspense Radio Show, "Flesh Peddler" 1957
Feb. 14 Johnny Madero Pier 23 Radio Show, "The Fatal Auction" 1947
Feb. 21 Weird Circle Radio Show, "Frankenstein" 1944
Feb. 28 The Whistler Radio Show, "Death Laughs Last" 1945 
Mar. 7 The Hermit's Cave Radio Show, "The Nameless" 1940
Mar. 14 Hall Of Fantasy Radio Show, "Dance Of The Devil Dolls" 1953
Mar. 21 Hall Of Fantasy Radio Show, "The Automaton" 1953
Mar. 28 Favorite Story Radio Show, "The Bottled Imp" 1948
You can hear Martin Dawson's Radio Mystery Theater Saturdays at 1300 UTC on 15770 kHz and at 11:00 pm Eastern Time Saturdays [Sundays 0400 UT*] on 9395 kHz. There is a repeat on Thursdays at 7:00 pm Eastern Time [Fridays 0000 UT*] on 5950 kHz.
* = One hour earlier from 8 March with DST change in US
(WRMI via Alan Roe, Teddington, UK/BDXC)

Saturday, January 17, 2026

January 18 programming from Jen's Eclectic Views & Real Deal

 


Don't miss it - live link for January 18 - Jen's Eclectic Views & Real Deal


Jen's Eclectic Views & Real Deal For Jan 11th heard on Unique Radio Australia is up & ready for downloading and listening

Jan. 11th Cast 


Jan. 11th Cast short link.



For your contact pleasure

Happy & Healthy New Year to All.

Jen 

Thursday, January 15, 2026

Shabname Radio to Iran available on video


Shabname Radio, a new clandestine station targeting Iran, and broadcasting as the Voice of Freedom, is available as a five-minute video, at the Shortwave Central YouTube channel. Broadcasts are uncensored and report from beyond Iran's borders, designed to reach listener's inside Iran, as well as outside.

Video of January programming on 9680 kHz from 1830 UTC is available at:  

January programming from Uncle Bill's Melting Pot

 


Uncle Bill's Melting Pot, January 2026


January's show will feature music of Venezuela.
All broadcasts are on Radio Channel 292 from Germany as follows:

Friday, January 16:
3955 kHz at 1600 UTC, repeats 2200 UTC 
In addition to direct radio reception, we do honor reception reports for both programs using remote SDRs as long as the whole program is described and which SDR is specified. All QSLs are e-QSLs only.
 

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

Wednesday, January 14, 2026

BBC Daventry, part 1

 
Transmitters of Daventry
Special thank you to Ray Robinson, Dr Adrian Peterson, and Jeff White, for sharing this week's episode - next week will feature part 2

Jeff: Those of you who collect antique radios, particularly ones made in Europe, may have noticed stations marked on the dial often included one called “Daventry”.  Well, as we mentioned last week, we are now going to present the story of that major BBC transmitting station at Daventry in England.  The story begins with the launch of the BBC Empire Service in 1932.  Here’s Ray Robinson.

Ray: Thanks, Jeff.  Daventry is a small town located in the English Midlands about 40 miles southeast of Birmingham.  The history of the town goes way back even before the era of the Roman Empire.  In the year 51 AD, the Roman army conquered the area and established an encampment at the village which already existed there.  Then in the year 1006, Danish invaders attacked the area, and they planted an oak tree to mark the exact center of England.  Hence the name, as they say locally, Dane-Tree, or as we know it on the map of England today, Daventry.

The BBC facility was established just outside the town at a location called Borough Hill, and the first transmitter to be activated there was actually a shortwave one that had been previously licensed at the Marconi factory in Chelmsford as G5SW, and which remained in service for an incredible 32 years.

By the mid-1920’s, the use of shortwave transmissions for international communication as well as for program broadcasting was already proving to be quite successful.  Guglielmo Marconi himself had performed several successful long-range tests, and experimental shortwave broadcasting was already on the air from stations in the United States and Australia, as well as from amateur operators in England itself.

With this in mind, Marconi constructed a 10 kW shortwave transmitter in 1927, and the first broadcast transmission from the new unit took place on Armistice Day 1927.  This inaugural broadcast on November 11 commemorated the end of what we now call World War I, and the programming was shaped to honor this occasion.
This new shortwave transmitter was hurriedly assembled from already available equipment and the two aerial masts, 475 ft. high, supported an aerial that was omni-directional and vertically polarized.  The original channel was around 12500 kHz, though this was changed in the following year to 11750 kHz in accordance with new regulations enacted at the 1927 International Radiotelegraph Conference in Washington, D.C.

Thus began a regular international radio broadcasting service that was heard around the world, and which was reported quite frequently in radio magazines published in England, the United States, Australia and New Zealand.  Programming for this shortwave broadcasting service was usually a relay from 2LO in London, and these shortwave transmissions from Chelmsford were on the air for a little over three years.

The BBC then made arrangements with Marconi to rent the shortwave transmitter at Chelmsford to provide a preliminary program service while their own large station at Daventry was under construction.  The BBC took over the programming for shortwave G5SW in 1931, and on January 5, 1932, the BBC used it to introduce their new expanded Empire Service.


It was in October 1931 that the BBC had decided to establish their own large new shortwave station near Daventry, and they co-sited it with the six year old 25 kW longwave station 5XX.  The initial plans called for two STC transmitters rated at 10 to 15 kW to be installed in a new building, together with a total of 18 antenna systems, both directional and omni-directional.

While the Daventry site was being built, early the following year, in 1932, radio monitors in the USA, Australia and New Zealand reported hearing test broadcasts from a shortwave station that announced the callsign G5RX.  These originated from a new GPO site at Rugby, only 10 miles from Daventry.  Rugby was primarily a communication station, but some phone-capable transmitters had been installed, and these were being tested.

Ten months later on October 25, 1932, just a year after the BBC’s plans had been announced, the first tests were heard from the two new STC transmitters at Daventry, designated as Sender 1 and Sender 2.  Interestingly, they used the same Chelmsford callsign G5SW – all while the Marconi transmitter G5SW was still located at Chelmsford, 100 miles away.

By mid-November, more tests were heard under the now regularized callsign GSE, with the “E” in the callsign standing for “Empire”.  As you might expect, though, from 10-15 kW units, signal strength as received in Australia was not good, and the transmissions did not initially live up to the previously announced high expectations.  Regardless, the five-year-old Marconi transmitter in Chelmsford was closed down on December 17, 1932 in favor of the two new transmitters located at Daventry, and then two days later on Monday, December 19, the BBC began its famous “Empire Service”.  The first two-hour transmission began at 9:30 am UK time, introduced by announcer William Shewen.  J.H. Whitley, Chairman of the BBC and Director General Sir John Reith both participated, explaining their aspirations for the new service.  It was directed primarily towards Australia and New Zealand, with Sender 1 using the callsign GSC on 9585 kHz, and Sender 2 using GSD on 11750 kHz.  This is how the broadcast began:

Additional information and videos on Daventry are available for a search at www.youtube.com 

The production studio for those live broadcasts was in the new “Broadcasting House” in London, with a program feed to Daventry via dedicated telephone lines.

Sir John Reith and Rt. Hon. J.H. Witley

As a historic first, His Majesty, King George 5 made a radio broadcast on Christmas Day, December 25 in the same year, 1932, and as photos taken at the time reveal, the microphone for this occasion was installed in Buckingham Palace, London.  However, to ensure the King’s Speech was heard reliably throughout the world, arrangements were made for it also to be relayed via the shortwave transmitters at Rugby.

In January 1935, the Marconi transmitter, which by then had been off the air for two years, was refurbished and re-engineered up to 20 kW, with the capability of operating on several different shortwave bands.  It was then transferred to Daventry, and installed in an available open space in what was known as the 5GB Medium Wave Building.  At this new BBC location, the historic Marconi transmitter was designated as Sender 3 (the two STC units being Sender 1 and Sender 2) and it was brought back into regular broadcast service on May 19, 1935.  Callsigns used by this transmitter now depended on what frequency was in use, with a different callsign for each waveband.  At the same time, the BBC announced that two additional high-powered shortwave transmitters would be installed at Daventry, with a power rating of 100 kW.

An additional 95 acres adjoining the radio facility at Daventry was purchased, and a new building large enough to hold three transmitters was constructed, the “Empire Service Building”.  An additional 25 antennas were installed, 14 of which were reversible curtains.

In 1937, the former Marconi transmitter was upgraded again, this time to 60 kW.

During the intense events of 1940 with the Allied Expeditionary Force in northern France, Sender 3 was used for carrying the Forces Program on 6150 kHz.

However, as time went by, this historic transmitter became increasingly unreliable, and ultimately, it was withdrawn from service and removed from the 5GB Building in 1959.  We assume at that point, it was simply scrapped.

And we’ll continue the BBC Daventry story next week.  Back to you, Jeff.
































(Ray Robinson/Wavescan)

RFE/Radio Liberty resumes Radio Farda service to Iran

 

(WASHINGTON) — Radio Free Europe/Radio Liberty (RFE/RL) has today resumed shortwave radio broadcasts into Iran following the imposition of an internet blackout by the Islamic Republic. Working with several commercial vendors, RFE/RL’s Persian-language service Radio Farda is once again providing an alternative to state-controlled media. Radio Farda reaches 6.5 million Iranians.

As nationwide protests in Iran continue, Radio Farda remains a lifeline for the people of Iran, providing vital news and insight, amplifying the voices of activists, verifying the deaths of protesters, and delivering expert analysis on the developing U.S. response. 

President & CEO Stephen Capus said:

“At this historic moment, when the Iranian people have been plunged into digital darkness by their government, Radio Farda’s return to the airwaves is an essential breakthrough. We’re reaching the people of Iran with the facts they need to stay safe – and ensuring their voices continue to be heard. Our journalists at Radio Farda are working nonstop to fulfill our commitment to the people of Iran.”

In the week leading up to the Islamic Republic’s internet blackout, Radio Farda’s digital reach surged. Between January 2-8, Radio Farda’s Instagram content was viewed at least 30 million times per day – 241.8 million views total – with 96% coming from Iran. Between December 28-January 5, Instagram video viewership rose by 411% over the previous seven-day period, with engagements soaring by 481%.

Radio Farda is a primary source of international perspectives on the crisis for Iranians, providing the latest statements from U.S. President Donald Trump, Secretary of State Marco Rubio, the House Foreign Affairs Committee Majority, and Sen. Lindsey Graham (R-S.C.), as well as analyses of the crisis and its impact on U.S. and foreign policy debates and analysis by experts such as Jack Goldstone, Michael Sobolik, Michael Rubin, and Ilan Berman.

For the latest information on the protests, follow Radio Farda’s live blogs in English and Persian.



Radio Farda 

Effective: 14 Jan 2026 
Farsi 
0530-0800   15430
0530-1400   15615
0800-1400   15110
1400-1500  15310
1500-2100   7500
1500-1700   13755
 (TH/Teak Publishing)

U.K. Propagation Update

 

RSGB
RadCom Assistant Editor | January 9, 2026
Now that the dust has settled after the New Year’s celebrations, we can get back to our regular propagation reports.
The New Year has started with minor disturbed geomagnetic conditions at times, plus lots of C-class solar flares, and a healthy dose of sunspots. As we slide down the slope towards sunspot minimum, we can expect more geomagnetic disturbances and raised Kp indices. But we should still have good HF conditions for a couple of years.
The Kp index hit 5 on 2 January, but has otherwise been relatively quiet, often registering less than 1 or 2. And the lack of M- and X-class solar flares means we have had no solar fade-outs.
With the solar flux index at more than 150 for much of the time, this bodes well for HF propagation and, as Propquest shows, the maximum usable frequency over 3,000km during daylight has often been more than 28MHz.
Unfortunately, this does decline quite quickly after sunset, leaving the maximum usable frequency below 10MHz most of the time. As we head towards spring, we can expect this to improve.
DX has been available. Stations worked include V51WH in Namibia on the 12m band using SSB, TZ4AM in Mali on 30m using CW, and ZS7ANF in Antarctica using CW on the 17m band.
Next week, NOAA predicts that the solar flux index will be in the 130 to 150 range.
Geomagnetic conditions are forecast to be variable, with the Kp index predicted to hit 5 on 13-14 January, and again 17-20 January.
So, we recommend you get your HF DXing in before 13 January and around 15-16 January, as propagation and maximum usable frequencies will no doubt be affected if the Kp index rises.
With the three-week 3Y0K Bouvet Island DXpedition set for early February, now may be a good time to sort out your antennas. Remember that Bouvet is almost due south from the UK, so plan accordingly. More propagation details will be made available nearer the time.
VHF and up propagation news from G3YLA and G4BAO:
The unsettled weather pattern continues to provide a variety of challenging weather types with heavy snow and rain, plus strong winds at times.
The nature of such patterns in January is that the timing and track of the lows are critical for the rain and snow outcome. Overall, it’s likely to be a cold system week with occasional brief milder interludes as Atlantic fronts move through in the middle of the coming week.
The effect on VHF and UHF propagation is limited with tropo unlikely, but there is a significant chance of rain or snow scatter at times for GHz operators.
There have been some slight increases in the Earth’s Kp index, which responds to solar activity. However, as we are between the peak periods of autumn and spring for aurora, it’s probably not a major player this time.
Meteor scatter has been a bit more interesting lately due to the peak of the Quadrantids meteor shower on 4 January. The shower has a short, intense peak, but spans the period from 28 December to 12 January. The next major shower isn’t until April, so it’s back to random activity from this weekend through to the late April Lyrids.
Lastly, a reminder that mid-winter Sporadic-E does happen. 6 January saw a nice early evening 6m band opening to the Baltic states, moving round to Ukraine and the Balkans later.
Recent Quadrantids meteors may have contributed some long-lived metallic ions, which can be focused into thin Sporadic-E patches. It’s always worth checking the Sporadic-E Layer Critical Frequency values plotted on the Propquest graphs for short spikes in the purple trace, which could be a sign of potential interest in Sporadic-E on the 10 and 6m bands.
For EME operators, Moon declination is negative again and we are past perigee, so path losses are increasing and Moon window length and peak elevation are reducing. 144MHz sky noise remains low but rising to high by Friday, 16 January.
And that’s all from the propagation team this week.
(Mike Terry, UK/BDXC)

Monday, January 12, 2026

Weekly Propagation Forecast Bulletins

 Product: Weekly Highlights and Forecasts
:Issued: 2026 Jan 12 0311 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 January 2026

Solar activity ranged from low to moderate levels. Forty-five weak to middle-level C-class activity was observed from various regions on the disk during the period. A majority of the activity was observed from Regions 4334 (S16, L=200, class/area Dao/150 on 08 Jan), 4336 (S10, L=166, class/area Eko/430 on 09 Jan) and 4337 (N25, L=243, class/area Dao/020 on 08 Jan). At 11/2314 UTC, a long-duration M3.3 (R1-Minor) flare was observed from behind the ESE limb. Several potential Earth-directed CMEs were observed leaving the Sun on 08 Jan with possible impact on late 10 Jan to early on 11 Jan. 

No proton events were observed at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit was at normal to moderate levels on 05, 08, 09 and 11 Jan with high levels observed on 06, 07, and 10 Jan. A peak flux of 2,507 pfu was observed on 10/1635 UTC. 

Geomagnetic field activity was at quiet to active levels on 05 Jan in response to declining CH HSS influence. Quiet levels were observed on 06 and 07 Jan. Quiet to active levels were observed on 08, 09 and early 10 Jan due to CH HSS influence. Activity levels increased to G1 (Minor) to G2 (Moderate) activity levels during late 10 Jan through 11 Jan due to CME effects from the 08 Jan CME coupled with CH HSS effects. 

Forecast of Solar and Geomagnetic Activity 12 January - 07 February 2026

Solar activity is likely to remain at low levels, with a chance for R1 (Minor) conditions and a slight chance for R2/R3 (Moderate/Strong) over the next forecast period due to multiple regions on the visible disk as well as regions expected to return. 

No proton events are expected at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit is expected to reach high levels on 12, 14-15, 21-27, and 30-31 Jan and 01-03 and 05-07 Feb due to the anticipated influence of multiple, recurrent coronal holes. 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 on 12 and 29 Jan; unsettled to active levels on 13-16, 19-23, 27-28, 30-31 Jan and 04-07 Feb. All enhancements in geomagnetic activity are due to the anticipated influence of
multiple, recurrent CH HSSs. The remainder of the outlook period is expected to be mostly quiet. 

Product: 27-day Space Weather Outlook Table 27DO.txt
:Issued: 2026 Jan 12 0312 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 2026-01-12
#
#   UTC      Radio Flux   Planetary   Largest
#  Date       10.7 cm      A Index    Kp Index
2026 Jan 12     110          28          6
2026 Jan 13     110          18          4
2026 Jan 14     112          12          4
2026 Jan 15     110           8          3
2026 Jan 16     108           8         
2026 Jan 17     106           5          2
2026 Jan 18     106           5          2
2026 Jan 19     110          18          4
2026 Jan 20     115          15          4
2026 Jan 21     125          12          4
2026 Jan 22     135           8          3
2026 Jan 23     140           6          2
2026 Jan 24     135           6          2
2026 Jan 25     135           6          2
2026 Jan 26     135           6          2
2026 Jan 27     130          10          3
2026 Jan 28     125          15          4
2026 Jan 29     125          25          5
2026 Jan 30     130          12          4
2026 Jan 31     130          10          3
2026 Feb 01     125           5          2
2026 Feb 02     120           5          2
2026 Feb 03     115           5          2
2026 Feb 04     110          15          4
2026 Feb 05     105          12          4
2026 Feb 06     105          10          3
2026 Feb 07     110           8          3
(NOAA)

Saturday, January 10, 2026

Jen's Eclectic Views & Real Deal programming on January 11

 


Another great program is waiting for you !! Tune in on Sunday, January 11

19:00 -21:00 UTC


For your contact pleasure


Happy & Healthy New Year to All.

Jen 

Thursday, January 08, 2026

Encore classical music from Radio Tumbril

 


Dear Listener
Radio Tumbril - www.tumbril.co.uk

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
03:00 - 04:00 UTC Monday 5950 kHz WRMI to the US and Canada
13:00 - 14:00 UTC Tuesday 15770 kHz WRMI to Europe, the east coast of the 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 the funding of Encore - Radio Tumbril.
Up-to-date transmission times and frequencies.
The playlists for the most recent programs. 

An email link.
Informal reception reports as well as those requesting eQSL cards, are welcome.

WRMI and Channel 292 are very generous with their airtime 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.

THE DONATION BUTTON is on the homepage of the website - www.tumbril.co.uk - which folks can use if they would like to support Encore.

THIS FORTNIGHT'S PROGRAM  - First broadcast on FRIDAY 9th January by WRMI at 0200 UTC on 5850, and 2000 UTC on 15770 and then Channel 292 on SATURDAY 10th January at 11:00 UTC on 9670 kHz:
Starts with Diliges Dominum by William Byrd, the first movement of Beethoven's 3rd concerto 'Eroica', and a startling motet from Anton Bruckner.
After that - the 2nd movement of the 'Eroica', and the first movement of the Violin Sonata in E Minor by Mozart.
The programme finishes with the 3rd and final movement of Beethoven's 'Eroica'.

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

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


From the Isle of Music's January programming

 


Happy New Year! 

January 2026 - From the Isle of Music, broadcast will be as follows: 

¡Feliz año nuevo! January's show will feature music from two of the most prominent living jazz pianists in Cuba, Alejandro Falcón and Ernán López Nussa.

Friday, January 9:
3955 kHz at 1700 UTC, repeats 2200 UTC 


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


Monday, January 05, 2026

Wavescan's focus on U.S. Coast Guard Cutter ‘Courier’

 
USCGC Courier

Thank you to Ray Robinson, Dr Adrian Peterson, and Jeff White for this week's Wavescan episode.

US Coast Guard Cutter ‘Courier’

Jeff: For 12 years during the Cold War from 1952 to 1964, the United States used a Coast Guard vessel in the Mediterranean Sea to broadcast Voice of America programming via medium wave and shortwave to Eastern Europe, the Balkans, the Middle East and North Africa in up to 16 different languages.  Those operating the ship-based station always had to contend with the forces of nature, technical challenges and deliberate jamming from the East.  Once again, our contributor, Dr. Martin van der Ven in Germany has been digging into the history of this rather unique enterprise, and here’s Ray Robinson in Los Angeles to bring us what Martin has uncovered.

Ray: Thanks, Jeff.  Yes, Martin has produced a very informative article, and I also found some great information about this project at the website theradiohistorian.org, so we’re very much indebted to both.

The Voice of America began broadcasting during World War II, and by the late 1940’s, a number of powerful VOA shortwave transmitting facilities were broadcasting from within the United States.  But in 1949, the Soviet Union began jamming those signals, creating walls of noise and interference that largely wiped out reception of the VOA in eastern bloc countries.  The signals from North America were considerably weaker than the jammers because of the long transmission distances, so to break through the jamming, the US State Department began setting up VOA relay transmission facilities that were closer to its target areas.  Beginning in the early 1950s, overseas relay stations were built or leased in Tangier, the Philippines and Okinawa.

At the same time, the VOA proposed to build a fleet of shipboard radio transmitters that could quickly and easily move to wherever they were needed to serve as temporary relay stations.  In response to the proposal, the Department of State created the program “Operation Vagabond” in April, 1951.  At first six vessels were contemplated, but in the end budget constraints imposed by Congress limited the project to just one ship.  To avoid political controversy, this ship would be unarmed and would operate under the command of the US Coast Guard, not the Navy.  It would not broadcast from International Waters on the high seas, but only from inside the territorial coastal waters of friendly countries that had granted permission.

In 1952, the State Department acquired a mothballed ship, the 340 ft. M/V Coastal Messenger.  She’d been built in Milwaukee in early 1945 as a wartime transport vessel, but the war was over before the ship could be placed into service.  After the war, she plied the coastal waters of South America, but on one voyage ran aground off the coast of Venezuela – an incident that ultimately led to her being laid up in the reserve fleet.

The Coastal Messenger was duly chosen to be converted into the first of the proposed six new VOA relay ships.  And for this mission, she was given a new name:  U.S. Coast Guard Cutter Courier.  She was equipped with two 35 kW Collins 207B shortwave transmitters and a 150 kW RCA BT-105 medium wave transmitter – the most powerful medium wave transmitter ever installed on a ship.


                            USCGC Courier – Transmitter Hold (Collins SW on left, RCA MW on right)

On the forward deck, four inverted pyramid steel lattice antennas were used for shortwave transmissions – a larger pair for lower frequencies on the port bow, and a slightly smaller pair for higher frequencies on the starboard bow.  These were omnidirectional, and all were painted red and duly guyed to the deck.  Medium wave transmissions, also omnidirectional, were to be made through a resonant steel cable held aloft by a huge helium balloon,which it also tethered.  The balloon was winched up to some 900 feet above the deck during broadcasts.  Three 500 kW three-phase generators supplied the power, any two of which could run the entire station at full load.

On February 15, 1952, the ship was officially commissioned in Hoboken, New Jersey, after which she sailed to Washington, D.C. where on March 4, 1952, she was inspected by President Harry S. Truman, and he made a short broadcast from her deck.  Then, before entering full service, the Courier undertook a six-week shakedown cruise through the Caribbean to the Panama Canal.

On April 18, 1952, the first test transmissions took place from the Canal Zone using the callsign KU2XAJ on 6110 and 9690 kHz shortwave and on 1510 kHz medium wave.  Broadcasts ran daily from 5-11pm local time, and were well received as far afield as Europe and New Zealand.  The announcements identified the test broadcasts as:  “Voice of America broadcasting via the Courier, the floating station KU2XAJ in the waters of the Panama Canal.  This transmitter is testing its electronic equipment with programmes in the Spanish language on 1510 kHz, 9690 and 6110 kHz.  VoA technicians welcome reception reports to:  Courier, Apartado 2016, Balboa, Canal Zone.”

The reason the then American territory of the Canal Zone was chosen for the test broadcasts was to covertly support a CIA operation to overthrow the then communist government of Guatemala.  Whilst outwardly it was presented as a goodwill mission, it was in reality a tactical propaganda operation, known only to a small circle of VOA personnel at the time.  The evening broadcasts in Spanish on the powerful medium wave transmitter easily reached Guatemala by sky wave, and perhaps partly as a result of the Courier’s targeted political influence campaign for a few months in 1952, there was indeed eventually a successful coup d’etat in Guatemala two years later on June 27, 1954.

A month later, she set out for the eastern Mediterranean — via Tangier, Naples and Piraeus — finally arriving in the harbor of Rhodes on August 22, 1952.  The location just 11 miles off the south coast of Turkey was both strategic and symbolic:  Greece had just joined NATO, and the presence of the American broadcast ship stood as a visible sign of Western solidarity.  On September 7, she officially began broadcasting.

Although the ship often moored in the port, when broadcasting, she usually lay at anchor about one mile offshore within territorial waters, by agreement with the Greek government.

USCGC Courier off Rhodes


The red inverted-pyramid ‘discone’ antennas at the bow were for shortwave transmission.
A Faraday cage was constructed at the stern to shield the receivers from RF interference.
The helium balloon was launched from the platform at midships.

The helium balloons used to raise the medium wave antenna were 69 feet long and 35 feet wide – similar in size to the barrage balloons that had been used over London during the Blitz.  Five of these expensive balloons were kept on board, along with 600 bottles of helium.  It took many coastguardsmen to inflate the balloons and send them aloft.  But the system proved unreliable:  strong winds often tore the balloons loose, sending them drifting — sometimes over Turkey, where private property was damaged.  Eventually, the fragile system was replaced by an inverted delta-loop antenna, which used three wires strung between the ship’s forward and aft masts.  The primary medium wave frequency from Rhodes was 1259 kHz, using the callsign NFKW.

Balloon About to Lift AM Antenna

News and current affairs programming was received via shortwave either from Tangier or direct from Washington D.C. through a bank of Collins 51-J

receivers.  News bulletins were generally relayed directly, while other programming was recorded onto transcription discs for later rebroadcast.  The turntables were actually mounted in gimbals on specially-designed gyroscopic cradles that stabilised the decks and kept them level as the ship pitched and rolled with the sea – an innovation that sadly was not copied by the offshore stations of the 1960’s – they just taped a coin on top of the stylus to keep it tracking in the grooves of a record. 



VOA music programming from the Courier was played on reel-to-reel tapes that were taken to the ship regularly.  Adjacent to the control room on board was also a small broadcast studio, which was mainly used for continuity announcements, although local broadcasts were occasionally made too.

Problems were experienced with the reception of VOA broadcasts from Washington due to RF interference from the ship’s own transmitters, and to try to counter that, a Faraday shield was constructed around the stern of the ship, but that was only partially successful.  So, in later years, a separate receiving station was built on land, on a hill overlooking the harbor, and news relays were then sent by VHF link from there to the ship in better quality than could be obtained on board.

But the airwaves were contested territory:  from the East, jammers in the Soviet Union and Eastern European countries tried to block her transmissions.  It was a constant game of cat and mouse, and small frequency changes to adjacent channels were often made during broadcasts to try to get a clear signal through.

Married crew members were permitted to bring their families to Rhodes.  A small American community soon developed on the island, complete with homes, shops and an American school.  The Courier community stimulated the local economy, created jobs — and not infrequently led to friendships or even marriages between islanders and crew members.


But in the long run, having a movable seagoing transmitter proved not to be as useful as was originally hoped, and the Courier’s signal range was hampered by the limitations of its shipboard antennas.  As the Soviets increased their jamming power, higher transmitting power and more efficient, directional antennas were needed.  Finally, in 1964, the VOA inaugurated a land-based transmitting station on the Island of Rhodes.  It was equipped with a 500 kW medium wave transmitter and two 50 kW shortwave units.  A second relay station at Kavala in northeastern Greece, just south of the Bulgarian border, was commissioned in 1972.

YouTube link to VOA Rhodes  https://www.youtube.com/watch?v=IPaGfkzeXlU

After twelve years of service, the Courier prepared to return to the United States in 1964.  Final maintenance work was carried out at a shipyard near Piraeus — and even there, while in dry dock, she remained “on the air”, earthed via a massive cable to the quay.  On May 17, 1964, the final broadcast went out over the airwaves.  The technical equipment was then offloaded and handed over to the Greek government, and the ship began her voyage home — via Naples, Barcelona and the Azores.  On August 13, 1964, the Courier reached the American east coast.  Two years later in 1966, she was recommissioned as a training vessel for the Coast Guard, a role she filled until 1972 when she was finally decommissioned.  In 1975 the vessel was scrapped, ending a colorful career as one of the world’s most unique broadcast facilities.

What remained was her legacy:  a ship that fought not with weapons, but with words — and whose aerials for many years stood as symbols of a free and uncensored world.

Back to you, Jeff.

Jeff: Thanks, Ray.  And again, we thank Dr. Martin van der Ven in Germany for much of the input to that item.  Next week, Ray will begin a short two-part series on the history of the BBC transmitting station at Daventry in England.








Jan.4th broadcast audio from Jen's Eclectic Views & Real Deal now available

 


Jen's Eclectic Views & Real Deal For Jan 4th, and heard on Unique Radio Australia, is up and ready for downloading & listening

Yes, folks, the Gremlins hit us. hi

Here's the new link.


This is today's cast.

Jen's Eclectic Views & Real Deal For January 4, 2026


Or Tiny URL link: 


New for 2026 program links will be available for 60 days after broadcast.

Sunday, January 04, 2026

Weekly Propagation Forecast Bulletins, January 5, 2026

 Product: Weekly Highlights and Forecasts
:Issued: 2026 Jan 05 0224 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC web contact www.swpc.noaa.gov/content/subscription-services
#
#                Weekly Highlights and Forecasts
#
Highlights of Solar and Geomagnetic Activity 29 December - 04 January 2026

Solar activity ranged from low to high levels. High levels were observed on 31 Dec following an M7.1/1N flare at 31/1351 UTC from Region 4324 (N25, L=288, class/area=Dao/230 on 29 Dec). Associated with the event was Type IV and Type II radio sweeps, a Tenflare, and a CME signature to the NE in subsequent coronagraph imagery.

Modeling of the CME event suggested passage by Earth late on 03 Jan. Moderate levels were observed on 01 Jan following an M1/Sf flare at 29/0651 from Region 4325 (S08, L=296, class/area=Eki/330 on 01 Jan). The other 21 numbered active regions across the visible disk this week were either quiet or only produced C-class activity. A Type II radio sweep was reported on 02 Jan but was associated with a CME that erupted from beyond the W limb. 

No proton events were observed at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit reached high levels over the past seven days. 

Geomagnetic field activity was mostly at quiet to unsettled levels on day, but 02 Jan. G1 (Minor) geomagnetic storm levels were observed on late on 02 Jan, following the arrival of the last of a set of weak CMEs that left the Sun over 28-31 Dec. Total magnetic
field strength reached a peak of 09 nT as the CME passed. Bz reached as far south as -8 nT. Solar wind speeds peaked between ~600-700 km/s. While influence from a negative polarity coronal hole was observed beginning on 31 Dec, no significant geomagnetic activity was observed from the feature over the following days. 

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

Solar activity is likely to remain at low levels, with a chance for moderate (R1-Minor) conditions and a slight chance for high (R2/R3-Moderate-Strong) over the next solar rotation due to multiple regions on the visible disk as well as regions 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 reach high levels on 05 Jan and 15 Jan - 13 Jan due to the anticipated influence of multiple, recurrent coronal holes. The remainder of the outlook period is likely to at normal to moderate levels. 

Geomagnetic field activity is likely to reach G1 (Minor) geomagnetic storm levels on 13-14 Jan, 17-20 Jan, and 29 Jan; active levels are likely on 05 Jan and 28 Jan; unsettled levels are likely on 09-10 Jan, 12 Jan, 21-22 Jan, 27 Jan, and 30-31 Jan. All enhancements in geomagnetic activity are due to the anticipated influence of
multiple, recurrent, coronal holes. The remainder of the outlook period is expected to be mostly quiet. 

Product: 27-day Space Weather Outlook Table 27DO.txt
:Issued: 2026 Jan 05 0224 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC  web contact www.pc.noaa.gov/content/subscription-services
#
#      27-day Space Weather Outlook Table
#                Issued 2026-01-05
#
#   UTC      Radio Flux   Planetary   Largest
#  Date       10.7 cm      A Index    Kp Index
2026 Jan 05     155          10          3
2026 Jan 06     150           5          2
2026 Jan 07     145           5          2
2026 Jan 08     140           5          2
2026 Jan 09     135           8          3
2026 Jan 10     135           8          3
2026 Jan 11     130           5          2
2026 Jan 12     135          10          3
2026 Jan 13     135          15          5
2026 Jan 14     140          15          5
2026 Jan 15     145           5          2
2026 Jan 16     145           5          2
2026 Jan 17     145          20          5
2026 Jan 18     140          20          5
2026 Jan 19     145          18          5
2026 Jan 20     150          18          5
2026 Jan 21     155           8          3
2026 Jan 22     160           8          3
2026 Jan 23     165           6          2
2026 Jan 24     170           6          2
2026 Jan 25     175           6          2
2026 Jan 26     175           6          2
2026 Jan 27     170           8          3
2026 Jan 28     165          12          4
2026 Jan 29     160          20          5
2026 Jan 30     155          10          3
2026 Jan 31     160           8          3
(NOAA)