Monday, January 27, 2025

A new CME is heading for Earth....maybe

 


The storm cloud was hurled into space by a dramatic filament eruption on Jan. 26th.

Most of the CME will sail south of our planet, but NOAA forecasters believe it could graze Earth as it passes by.

If so, a G1-class geomagnetic storm could occur on Jan. 29th.

Additional information at: https://spaceweather.com/
(Mike Terry, UK/BDXC)

Review of World Radio TV Handbook 2025

 

In the February edition of The Spectrum Monitor, I review the 2025 World Radio TV Handbook edition. This is the first published review and you don't want to miss it!! 

Not a subscriber ? Get the details at https://www.thespectrummonitor.com 

Gayle Van Horn W4GVH


An extra look at propagation from the U.K.

 
RSGB
GB2RS News Team
January 24, 2025

This week, ending today the 26 January, has looked a lot like a repeat performance of two weeks ago. The majority of the sunspots are in the western hemisphere with very few in the eastern side. This means that
the solar flux index could drop over the coming week unless there are sunspots ready to rotate into view to replace those being lost.

A look at the STEREO Ahead spacecraft imagery suggests that there are indeed sunspots over the Eastern limb, so all may not be lost.

Overall, the Sun has been fairly quiet. There were no X-class flares and only five M-class flares from the 19 to the 23 January. The Kp index has also been relatively low, only peaking at four for one three-hour period on the 20 January.

As a result, with the solar flux index in the 200s, HF conditions have been quite good. The maximum usable frequency over a 3,000km path has been consistently over 28MHz, from around 0830 to 1600UTC. However, the
20, 17, 15 and 12m bands, seem to be carrying most of the DX at the moment.

Next week, NOAA predicts that the solar flux index will remain in the mid-200s. Geomagnetic conditions are also predicted to be good until the end of the month, but a Kp index of 5 is forecast for the 31 January,
and this could last for a few days.

So, we urge you to make the most of the conditions now, before geomagnetic storming, if it occurs, makes a mess of HF as we enter February.

  VHF and up :

The weather pattern is being driven by a very strong winter jet stream across the Atlantic Ocean. This gives scope for rapid development of deep lows and consequent gales and damaging winds.

On Friday 24 January, the first big storm hit the northwest of Britain. We may find that the next low in the series is heading for southern Britain tomorrow, the 27 January.

This all makes tropo unlikely for much of the week ahead since it stays unsettled through most of the period, but with the smallest hint of higher pressure trying to return from Thursday.

Rain scatter will probably be worth some consideration on the GHz bands while meteor scatter remains driven by random activity rather than any major showers.

There have been further aurora alerts over the last week and it’s always worth keeping the Kp index in view to monitor any possible chances for aurora. High figures, above a Kp index of 4, are a good trigger point to get interested.

Moon declination reaches minimum in the northern hemisphere today, the 26 January, when Moon windows are at their shortest and peak Moon elevation is at its lowest.

Path losses are now falling as we passed apogee on Tuesday the 21 January. 144MHz sky noise is high, reaching over 3,000 Kelvin today, the 26 January, before dropping to moderate until Wednesday when the Moon and Sun are very close in the sky for the whole Moon pass. After this, it drops to low for the rest of the week.

(Mike Terry, UK/BDXC)

Weekly Propagation Forecast Bulletins

 Product: Weekly Highlights and Forecasts
:Issued: 2025 Jan 27 0230 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 20 - 26 January 2025



Solar activity ranged from low to moderate levels (R1-Minor). Moderate levels were observed on 21 Jan from Region 3967 (S14, L=148, class/area Eai/110 on 21 Jan) with an M3.3/Sf observed at  21/1039 UTC. This flare also produced a Type II sweep with an estimated shock velocity of 565 km/s. Region 3961 (S09, L=181, class/area Fkc/800 on 20 Jan) produced an M1.3/1f at 22/1108 UTC with a Type II sweep with an estimated shock velocity of 561 km/s. This region also produced an M2.7/1f flare at 24/2104 UTC. All other active regions were either quiet or contributed only C-class events. Potential Earth-directed CMEs were observed on 21 and 22 Jan. 

No proton events were observed at geosynchronous orbits.

The greater than 2 MeV electron flux at geosynchronous orbit reached high levels on 20, 22, and 23 Jan. Normal to moderate levels were observed on 21 and 24-26 Jan. 

Geomagnetic field activity was at quiet to active levels. Isolated active periods were reached on 20 Jan with unsettled levels observed on 20-24 Jan. Quiet levels were observed on 25-26 Jan. All elevations in geomagnetic activity were attributed to influence from multiple, negative polarity CH HSSs. 

Forecast of Solar and Geomagnetic Activity 27 January - 22 February 2025

Solar activity ranged from low to moderate levels (R1-Minor). Moderate levels were observed on 21 Jan from Region 3967 (S14, L=148, class/area Eai/110 on 21 Jan) with an M3.3/Sf observed at 21/1039 UTC. This flare also produced a Type II sweep with an estimated shock velocity of 565 km/s. Region 3961 (S09, L=181, class/area Fkc/800 on 20 Jan) produced an M1.3/1f at 22/1108 UTC with a Type II sweep with an estimated shock velocity of 561 km/s. This region also produced an M2.7/1f flare at 24/2104 UTC. All other active regions were either quiet or contributed only to C-class events. Potential Earth-directed CMEs were observed on 21 and 22 Jan. 

No proton events were observed at geosynchronous orbits.

The greater than 2 MeV electron flux at geosynchronous orbit reached high levels on 20, 22 and 23 Jan. Normal to moderate levels were observed on 21 and 24-26 Jan. 

Geomagnetic field activity was at quiet to active levels. Isolated active periods were reached on 20 Jan with unsettled levels observed on 20-24 Jan. Quiet levels were observed on 25-26 Jan. All elevations in geomagnetic activity were attributed to influence from multiple, negative polarity CH HSSs. 

Product:  27-day Space Weather Outlook Table 27DO.txt
:Issued: 2025 Jan 27 0230 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC web contact www.swpc.noaa.gov/content/subscription-services
#
#      27-day Space Weather Outlook Table
#                Issued 2025-01-27
#
#   UTC      Radio Flux   Planetary   Largest
#  Date       10.7 cm      A Index    Kp Index
2025 Jan 27     165           5          2
2025 Jan 28     160           5          2
2025 Jan 29     155          10          3
2025 Jan 30     150           5          2
2025 Jan 31     150          12          3
2025 Feb 01     145          12          3
2025 Feb 02     150          20          5
2025 Feb 03     165          15          4
2025 Feb 04     160          12          4
2025 Feb 05     165          12          4
2025 Feb 06     160          10          3
2025 Feb 07     155           5          2
2025 Feb 08     150           5          2
2025 Feb 09     145          10          3
2025 Feb 10     140          12          4
2025 Feb 11     140          18          5
2025 Feb 12     140          15          4
2025 Feb 13     140          20          5
2025 Feb 14     140          12          4
2025 Feb 15     145          15          4
2025 Feb 16     145          15          3
2025 Feb 17     150          10          3
2025 Feb 18     150          10          3
2025 Feb 19     155          10          3
2025 Feb 20     165           5          2
2025 Feb 21     170           5          2
2025 Feb 22     170           5          2
(NOAA)

Sunday, January 26, 2025

An update on demolition of Moosbrunn transmitters




The latestinformation from Top News

AUSTRIA   Heise Online (German article which has been translated to En.)

ORF has Austria's 500-kilowatt short-wave transmitter to be blown up.
{Made in Germany by AEG Telefunken Berlin of 1983 year, wb.)

The whole world can be reached with a unique short-wave antenna from
ORS Moosbrunn Austria site.

It could be blown up as early as Thursday Jan 30 at 13 UTC (wb.)
WWDXC Top Nx/25 jan 2025)

Demolition of the Moosbrunn transmitter postponed
 At the end of the year, the Austrian shortwave stopped broadcasting. For cost reasons and because there were hardly any broadcasts about them anymore. This morning it suddenly said: “There will be a blast today!” But nothing comes of it for the time being.

The Austrian shortwave broadcasting center Moosbrunn has existed since 1959 and was used for a long time to broadcast Austria's foreign service. A modern, efficient system was built for this purpose.
After Radio Österreich International was discontinued, the system stayed alive through broadcasting time rentals. However, as of fall 2024, the primary airtime tenant, Adventist World Radio, has withdrawn from shortwave. A hit below the belt for the shortwave center.
 
Should be saved
 Since the technical systems and the existing antennas are still in full working order, the Moosbrunn shortwave center would continue to be fully operational. Above all, the large rotating antenna offers the system a very high level of flexibility, which allows it to broadcast to almost any region of the world.
As recently as December 2024, it was said that efforts were being made to save the system and the 320-ton rotating antenna. The same thing could still be heard at the beginning of January 2025. In addition, the ORF general director is said to have said at the end of 2024 that the facility would not be blown up.
 
Surprising turnaround?
 We don't (yet) know the exact background of what happened behind the scenes over the last few weeks. In any case, this morning it was surprisingly announced that the large rotating antenna would be blown up.
 
Inquired
 We asked the Moosbrunn municipal office. An employee there confirmed to us that the demolition of the facility was scheduled for today, but had been canceled for the time being. He couldn't give the reasons for this. The gentleman in the Moosbrunn municipal office did not know a new date for the demolition of the facility.
 
What's next?
 This is completely open. Based on what we have been able to find out over the last few weeks, it seems to us that some decision maker is trying to ignore all ongoing efforts and create facts. True to the motto: “The system has to go, so BOOM”.
 
Cheers from Bremerhaven,
Lesley Illingworth
(photo via Wikipedia)

QSLing Alaska and Madagascar in January 2025

 
photo via Mt Evelyn DX Report

Alaska &Madagascar paper QSLs

Hello! If anyone is interested in receiving PAPER QSL cards from KNLS at Anchor Point-ALS and MWV New Life Station, Mahajanga, Madagascar stations, send reports in January 2025 to knlsradio@gmail.com  and  mwvradio@gmail.com

Mailing of QSL cards will be made in February from Russia. 
(Alexander Berezkin, St. Petersburg-RUS, Radio reception - Telegram;
via RUSdx #1325 via wwdxc BC-DX TopNews Jan 19)

Friday, January 24, 2025

Shortwave Radiogram, Program 386

 

Program 386

Hello friends,

I hope you have been able to withstand our stretch of cold and snow (unusual in some places) during the past few days in North America. At our house, the outdoor thermometer showed 10°F/-12°C during the early morning hours -- not as bad as many places, but about as cold as we have ever been.

Last week's experiment with Olivia 64-2000 and Olivia 32-2000 was interesting. It was difficult to find signals that were poor enough that MFSK32 showed errors, while Olivia 64-2000 was 100% (or nearly so). But I have audio of two examples, which you can access, and from which you can decode. The first is January 19, 0330 UTC, 9265 kHz from WINB Pennsylvania. The signal is very weak because the signal is too close (200 km) to my receiver in northern Virginia.  The second is January 19, 2300 UTC, 7570 kHz from WRMI Florida. Here, the reception is challenging via an SDR in Bermuda because Voice of (North) Korea is co-channel and stronger.

A video of last week's Shortwave Radiogram (program 385) is provided by Scott in Ontario (Wednesday 1330 UTC). Mark maintains the audio archive in the UK. (This link now works) Analysis is provided by Roger in Germany. Roger shows us the comparative bandwidths of the MFSK32, Olivia 64-2000, Olivia 32-2000 and MFSK64 ..



Here is the lineup for Shortwave Radiogram, program 386, 24-29 January 2025, in MFSK modes as noted:

 1:41  MFSK32: Program preview
 2:51  MFSK32: NZ mayor objects to Trump 'split the atom' claim
 5:35  MFSK64: NASA develops a 3D-printed antenna*
10:46  MFSK64: Images of the week*
27:40  MFSK32: Closing announcements 

* with image(s)

Please send reception reports to radiogram@verizon.net
Twitter: @SWRadiogram or https://twitter.com/swradiogram
(visit during the weekend to see listeners’ results)



Other Shortwave broadcast programs that include digital text and images include The Mighty KBC, Pop Shop Radio and Radio North Europe International (RNEI). Links to these fine broadcasts, with schedules, are posted here.
 Thanks for your reception reports!

Kim
Kim Andrew Elliott, KD9XB
Producer and Presenter
Shortwave Radiogram
Reporting on international broadcasting at https://twitter.com/kaedotcom


Special weekend broadcast from Vatican Radio

 


Vatican Radio will be again on Sshortwave this weekend:

Saturday January 25t, for the Celebration of Second Vespers.  1625-1800 UTC  English on 13830, French on 17525 and Portuguese on 15565 kHz

Sunday January 26, for the Holy Mass to mark the Sunday of the Word of God. French on 17525, Portuguese on 15565 and English to Africa on 17540 and English to India on 15490 kHz (Tinang).
(BDXC/C Ghibaudo, France)

Encore classical music on Radio Tumbril

 


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, 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 programs.
An email link.
Informal reception reports as well as those requesting eQSL cards are welcome.
 
ENCORE IS A ONE-MAN OPERATION -  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 100 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.
 
(Please don't be put off by the POWR security wall when using the PAYPAL button - it is a harmless requirement of WIX the website hosting service.)
 
THIS FORTNIGHT'S PROGRAM - First broadcast this FRIDAY 24th January by WRMI at 0200 UTC on 5850, and 2000 UTC on 15770 and then Channel 292 on SATURDAY 25th January at 11:00 UTC on 9670 kHz:



Begins with some of a sonata by C P E Bach - one of J S Bach's sons - for Viola da Gamba, the piano trio by Ravel, and a three voice Agnus Dei by Firminus Caron - Renaissance composer.
After that the Elegy for Horn and Piano written by Poulenc and dedicated to the horn player's horn player - Dennis Brain, and some of Mozart's concerto for flute and harp.
The programme finishes with part of a late Beethoven string quartet.
  
Brice Avery - Encore - Radio Tumbril - www.tumbril.co.uk
GMØTLY

Thursday, January 23, 2025

WRMI Winter Schedule Update

 

WRMI - Winter schedule update - effective 11 January 2025

The current winter color grid, which includes programming information is available at:


All times UTC
Programming in English/French/Portuguese/Russian

0000-0100 5010ca 5050la 5800la 5850na 5950na 7570na 9455na 15770eu
0100-0200 5050la 5800la 5950na 7570na 7870ca 9455na 15770eu
0200-0300 5010ca 5050la 5950na 7780ca 9455na 15770eu
0300-0400 5010ca 5050la 5800la 5850na 5950na 9455na 9955sa 15770eu
0400-0500       5010ca    5050la    5850na    5950na    7570na    7730na    7780ca    9955ca 15770eu
0500-0600 5010ca 5850na 7570na 7730na 9395na 9955sa 15770eu
0600-0700 5010ca 5850na 7570na 7730na 7780ca 9395na 9955sa 15770eu
0700-0800 5010ca 5850na 7570na 7730na 7780ca 9395na 9955sa 15770eu
0800-0900 5010ca 7730na 7780ca 9395na 9955sa 15770eu
0900-1000 5010ca 5850na 7730na 7780ca 9395na 9955sa 15770eu
1000-1100 5010ca 7570na 7730na 7780ca 9395na 9955sa 15770eu
1100-1200 5010ca 5850na 7570na 7730na 7780ca 9395na
1200-1300 5010ca 5850ca 7570na 7730na 9395na 15770eu
1300-1400 5010ca 5850na 7570na 7730na 7780ca 9395na
1400-1500 5010ca 5850na 7570na 7730na 7780ca 9395na 15770eu 17790la
1500-1600 7570na 7730na 9395na 9955sa 17790la
1600-1700 7570na 7730na 9395na 9955sa 17790la
1700-1800 7570na 7730na 9395na 15770eu 17790la
1800-1900 7570na 7730na 9395na 15770eu 17790la
1900-2000 7570na 7730na 9395na 15770eu 17790na
2000-2100 7570na 9395na 17790la
2100-2200 7570na 7730na 9395na
2200-2300 5850na 5950na 7570na 7730na 15770eu
2300-0000 5800la 5850na 5950na 7570na 7730na 7780ca 9455na 15770eu
(WRMI)


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

WRMI website  http://wrmi.net/
Reception Reports: info@wrmi.net (or post online)

Wednesday, January 22, 2025

FCC Raises Maximum Pirate Radio Fines in Fifth Report

 

The Federal Communications Commission has released its fifth annual report to Congress detailing the implementation and enforcement activities of the PIRATE Act, as the maximum penalty for repeated infractions increases to match inflation in 2025.


The Preventing Illegal Radio Abuse Through Enforcement Act, signed into law in January 2020, grants the FCC increased enforcement tools to deal with and punish unlicensed broadcasters.

Additional text to: 

Tuesday, January 21, 2025

Pop Shop Radio schedules for January

 


January 2025 program relay sites as indicated

All times UTC/frequency kHz

January 22-27 program theme Glamrock 

22 January 17.00-18.00, 3955 9670 Rohrbach, Germany
25 January 14.00-15.00, 6160 Winsen, Germany 
25 January 23.00-24.00, 3955 9670 Rohrbach, Germany 
26 January 20.00-21.00, 6160 Winsen, Germany {3975?}
27 January 02.00-03.00: 5950, Okeechobee, FL/WRMI 

Email Reception Reports to: radiopopshop@gmail.com

Inside the Third Reich's Radio

Thank you to Ray Robinson and Jeff white for sharing last week's Wavescan script


 Inside the Third Reich’s Radio

Joseph Goebbels commissioned a stylish, mass-producible radio to channel Nazi propaganda into German homes


By Allison Marsh, professor at the University of South Carolina



Introduced in 1933, the inexpensive Volksempfänger helped spread Nazi propaganda to an eager audience.


Jeff: Joseph Goebbels understood the art of persuasion.  As propaganda minister for the Nazis, he sought to exploit radio's tremendous potential to broadcast Hitler's messages.  But first he needed a way for people to tune in.  Here’s Ray Robinson with the story of his ‘people’s receiver’ or ‘people’s radio’.


Ray: Thanks, Jeff.  Like the story we told two weeks ago about the first transistor radio, we are again indebted to Professor Allison Marsh at the University of South Carolina for researching and documenting our story today.


Radio helped bring the Nazis to power and keep them there

On 18 August 1933, Joseph Goebbels opened the 10th International Radio Show, in Berlin, with a speech declaring “Radio as the Eighth Great Power" — a nod to Napoleon's notion that the press was the seventh great power.  Goebbels argued that “the radio will be for the twentieth century what the press was for the nineteenth century." He noted the failure of the Weimar Republic to embrace radio, and claimed that the National Socialists would not have been able to take power without it.


He proclaimed:  “We want a radio that reaches the people, a radio that works for the people, a radio that is an intermediary between the government and the nation, a radio that also reaches across our borders to give the world a picture of our character, our life, and our work."


To make that happen, Geobbels had seized control of the Reichs-Rundfunk-Gesellschaft — the Reich Broadcasting Corporation — a national network of regional broadcasting companies.  After solidifying control of the broadcast infrastructure, he imposed rules on permissible content.  His final task was to make sure everyone had access to an affordable radio receiver.  But radios in Germany in the early 1930’s were expensive, easily exceeding a month's wages for ordinary workers.


Goebbels approached electrical engineer Otto Griessing to design a radio that was technically simple, easy to mass-produce, and inexpensive.

 The result was the Volksempfänger  (“people's receiver" or “people's radio") which was housed in a tall rectangular case, that Goebbels introduced at the Berlin show.  At a subsidized price of 76 Reichsmarks (then the equivalent of about US$250), it was around half the cost of the cheapest radios then on the market.  More than 100,000 units were sold during the first two days of the exhibition.  The radio could also be purchased on an installment plan.  By 1941, nearly two-thirds of German households owned a Volksempfänger, and Goebbels had succeeded in giving Hitler a direct conduit into people's homes via the airwaves.

The Volksempfänger was a model of German engineering

The Volksempfänger was designated model VE301, a reference to 30 January, the day in 1933 that Adolf Hitler assumed power.  It was a three-tube receiver that operated in the long-wave and medium-wave bands — 150 to 350 kilohertz and 550 to 1700 kilohertz, respectively — and had a built-in magnetic loudspeaker.  The radio came in three versions:  The VE301 W ran on alternating current, the VE301 B was battery powered, and the VE301 G operated on direct current.  The W and B sold for 76 RM, while the G was priced at 65 RM.  All of the models had sockets on the left side for plugging in antennas of different lengths.  A later model, the VE301 Dyn, introduced in 1938, featured an electrodynamic loudspeaker.


The Volksempfänger's radio dial was not marked with frequencies but rather listed the names of cities, such as Frankfurt and Heidelberg.  [These can be seen on the model in the Deutsches Museum's Volksempfänger, pictured at top].  This made tuning into foreign broadcasts such as those from the BBC a little more challenging.


Beneath the speaker grill on the front enclosure, there was an on/off/band select knob, a volume knob, and two tuning knobs which had to be turned in tandem to acquire a new station.  An ear-splitting screech could result if the receiver drifted out of tune.  The Volksempfänger did have the sensitivity to pick up foreign broadcasts, but after the start of World War II in 1939, listening to them became punishable by fines, imprisonment, and even death.


Low cost was not the only reason for the Volksempfänger's popularity.  The original VE301 had an attractive art deco-inspired design.  Industrial designer Walter Maria Kersting fabricated the cabinet out of Bakelite, a plastic that could be easily molded.  Bakelite also had insulating properties that made it ideal for the electronics industry, replacing the heavy and more expensive wood cabinetry that was then common.  Unfortunately, the later VE301 Dyn lacked some of the radio's original flair.  It had a rectangular speaker and tuning window, giving it a much more utilitarian aesthetic.


The government pressured 28 German radio manufacturers, including Philips, Siemens, and Telefunken, into producing the VE301.  They were required to adhere to strict standards and could not alter the circuitry or housing.  The only distinguishing mark they were allowed was a stamp of the company name on the



A brochure for the Volksempfänger highlights the radio's especially beautiful tone and its adherence to safety standards set by the Federation of German Electrical Engineers.  Note the swastika.


back cover.  A committee of experts from the radio industry, the Institute for Oscillation Research (known as the Heinrich Hertz Institute before and after Nazi control), and the Reich Broadcasting Corporation assured quality control and technical compliance.  But the Volksempfänger didn't hold a total monopoly.  Manufacturers were still allowed to produce other radios and to price them at market rates.


For the German people, the Volksempfänger offered welcome distraction

The original marketing materials for the VE301 made no secret of Goebbels's plan to bring radio to as many Germans as possible.  One brochure claimed that, through broadcasting, the radio brought together “city and country, people and government, manual laborers and office workers, old and young."


Ads positioned the Volksempfänger as the intermediary for the greater German community that would make the country strong and prosperous again by bringing political, cultural, and economic ideas into every household.  The national emblem of the eagle near the tuning dial identified the product as part of state propaganda efforts.  Later models also included a swastika.  An even cheaper version of the radio, the Kleinemfänger, came out in 1938 and sold for 35 Reichsmarks.


Goebbels knew better than to simply broadcast the Third Reich's agenda nonstop.  People welcomed the inexpensive receivers into their homes precisely because they also provided entertainment and distraction.  Regular programming included operas, classical concerts, light dance music, games, jokes, and popular arts.  To be sure, programming was highly censored. 



Goebbels ended his speech at the 1933 Berlin radio show with a high-minded wish: to unite science, industry, and intellectual leadership with a common goal of a “glorious German future."  His success in this effort helped trigger a world war while concealing an architected program of genocide, mass murder, and oppression.


The Volksempfänger was an elegant and inexpensive piece of engineering that gave ordinary Germans access to entertainment and culture, but that sadly also became an instrument of hate.  Back to you, Jeff.







Monday, January 20, 2025

Weekly Propagation Forecast Bulletins


Product: Weekly Highlights and Forecasts
:Issued: 2025 Jan 20 0136 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 13 - 19 January 2025

Solar activity ranged from low to high levels (R1-R2/Minor-Moderate). High levels were observed on 17 Jan following an M7.4 (R2) flare at 17/1335 UTC from Region 3964 (N06, L=247, class/area=Dki/475 on 17 Jan). The region also produced ten
R1 (Minor) events over 17-19 Jan. Region 3961 (S09, L=181, class/area=Eki/600) also produced an M1.1 (R1) flare at 17/0320 UTC. All other active regions were either quiet to contributed only C-class events. No Earth-directed CMEs were observed in available
coronagraph imagery. 

No proton events were observed at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit was normal to moderate levels. 

Geomagnetic field activity was at quiet to active levels. Active conditions were reached on 13 Jan, 15 Jan, 17 Jan, and 19 Jan. Unsettled to quiet conditions were observed for the remainder of the summary period. All elevations in geomagnetic activity were
attributed to influence from multiple, negative polarity CH HSSs. 

Forecast of Solar and Geomagnetic Activity 20 January - 15 February 2025

Solar activity is likely to reach moderate levels
(R1-R2/Minor-Moderate), with a chance for high levels of activity (up to R3-Strong), throughout the outlook period. This potential is driven primarily by Regions 3964 (N06, L=249, class/area=Dki/475 on 17 Jan) and 3961 (S09, L=181, class/area=Eki/600 on 17 Jan) on the Earth-facing side of the Sun as well as multiple regions on the Sun's farside that are due to rotated back onto the visible disk later during the outlook period. 

There is a slight chance for proton events of S1 or greater at geosynchronous orbit due primarily to the flare potential from Regions 3964 and 3961 over 20-28 Jan. 

The greater than 2 MeV electron flux at geosynchronous orbit is likely to be at high levels on 02-05 Feb due to recurrent CH HSS activity. The remainder of the outlook period is expected to be at normal to moderate levels. 

Geomagnetic field activity is expected to be at quiet to G1 (Minor) geomagnetic storm levels. G1 conditions are likely on 31 Jan - 02 Feb, 11 Feb, and 13 Feb. Active conditions are likely on 20 Jan, 03-05 Feb, 10 Feb, 12 Feb, and 14-15 Feb. Unsettle levels are likely
over 21 Jan, 06 Feb, and 09 Feb. All elevations in geomagnetic activity are anticipated due to multiple, recurrent CH 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: 2025 Jan 20 0136 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC web contact www.swpc.noaa.gov/content/subscription-services
#
#      27-day Space Weather Outlook Table
#                Issued 2025-01-20
#
#   UTC      Radio Flux   Planetary   Largest
#  Date       10.7 cm      A Index    Kp Index
2025 Jan 20     235          12          4
2025 Jan 21     235           8          3
2025 Jan 22     235           5          2
2025 Jan 23     230           5          2
2025 Jan 24     230           5          2
2025 Jan 25     235           5          2
2025 Jan 26     240           5          2
2025 Jan 27     245           5          2
2025 Jan 28     245           5          2
2025 Jan 29     245           5          2
2025 Jan 30     240           5          2
2025 Jan 31     235          20          5
2025 Feb 01     230          20          5
2025 Feb 02     225          20          5
2025 Feb 03     225          15          4
2025 Feb 04     225          12          4
2025 Feb 05     230          12          4
2025 Feb 06     225          10          3
2025 Feb 07     215           5          2
2025 Feb 08     205           5          2
2025 Feb 09     195          10          3
2025 Feb 10     190          12          4
2025 Feb 11     185          18          5
2025 Feb 12     185          15          4
2025 Feb 13     185          20          5
2025 Feb 14     185          12          4
2025 Feb 15     190          15          4
(NOAA)