Friday, August 24, 2018

Shortwave Radiogram, August 25-27

Hello friends,


Apologies to those of you who were tuned in to last Sunday’s 2330-2400 UTC broadcast on 7780 kHz. A few seconds after the broadcast began, another WRMI audio program came on and stayed for the rest of the half hour. I heard later from Rafael in Colombia that he heard Shortwave Radiogram on 5010 kHz, another of WRMI’s frequencies. WRMI was having a difficult day: Lightning in the area disrupted some of their systems.

You can still listen to program 61, and decode from the audio, thanks to videos provided by Ralf in Germany (Saturday 1600 UTC) and Scott in Ontario (Monday 0800 UTC – thanks to Scott for tuning in early Monday after the missing Sunday 2330 UTC show). The audio archive is maintained by Mark in the UK, and analysis is provided by Roger in Germany.

This weekend, Shortwave Radiogram will consist of our favorite combination of MFSK32, MFSK64, and MFSK128, with eight MFSK images and some interesting news stories.

Here is the lineup for Shortwave Radiogram, program 62, 24-27 August 2018, in MFSK modes as noted:

   1:37  Program preview
 2:53  MFSK32: U.S. Agency for Global Media is new name for BBG*
 6:28  MFSK128: New system for underwater-airborne comms*
11:56  MFSK64: Fake news detector algorithm better than human*
17:41  Cargo ship will attempt Russian Arctic voyage*
20:18  Images of the week*
28:31  MFSK32: Closing announcements

* with image

Please send reception reports to radiogram@verizon.net


Twitter: @SWRadiogram or https://twitter.com/swradiogram (visit especially during the weekend)



Shortwave Radiogram Program 62
(24-27 August 2018)

Friday
2030-2100 UTC
7780 kHz
5950 kHz
MFSK32
MFSK128
MFSK64
WRMI Florida
Saturday
1600-1630 UTC
9400 kHz
Space Line, Bulgaria
Sunday
2330-2400 UTC
7780 kHz
WRMI Florida
Monday
0800-0830 UTC

7730 kHz
5850 kHz
WRMI Florida

Slow Scan Radio transmits SSTV images and text modes Wednesdays at 1830-1900 UTC on 6070 kHz via Channel 292 in Germany. The website is http://www.slowscanradio.com. Reception reports to  x@xdv.me.

The Mighty KBC transmits to Europe Saturdays at 1500-1600 UTC on 9400 kHz (via Bulgaria), with the minute of MFSK at about 1530 UTC (if you are outside of Europe, listen via websdr.ewi.utwente.nl:8901/ ).  And to North America Sundays at 0000-0200 UTC (Saturday 8-10 pm EDT) on 9925 kHz, via Germany. The minute of MFSK is at about 0130 UTC.  Reports to Eric: themightykbc@gmail.com . See also http://www.kbcradio.eu/ and https://www.facebook.com/TheMightyKbc/. 

Italian Broadcasting Corporation (IBC)  Five minutes of MFSK32 is at the end of the 30-minute English-language “Shortwave Panorama. For the complete IBC transmission schedule visit  http://ibcradio.webs.com/  

Broad Spectrum Radio is transmitted by WRMI Florida Mondays at 0700-0800 UTC on 5850 and 7730 kHz. MFSK32 is broadcast during the second half hour of the show. Reports to broadspectrumradio@gmail.com.

Thanks for your reception reports! 

Kim

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


Airmail Postage & DX Supplies - Price List update



  +++  The Corrected Price for 1,000 forever stamps is $420.00 +++



 

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 VINTAGE FOUNTAIN PENS & MECHANICAL PENCILS -  For the past 18 months, I have been restoring vintage pens and pencils. Email me to list. Pens are lever fill, touchdown/plunger fill, vac-fil piston models.   A very nice selection of Sheaffer pens from the 1920s-1950s. Parker Duofolds and Challengers from the 1920s and 1930s. ALL pens and pencils have been restored to working condition. 





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Thursday, August 23, 2018

BBG rebrands as U.S. Agency for Global Media


Statement from CEO John F. Lansing on agency rebrand
by John F. Lansing August 22, 2018
Effective immediately, the Broadcasting Board of Governors (BBG), an independent U.S. government agency that employs thousands of talented journalists, storytellers, and media professionals, is now the U.S. Agency for Global Media (USAGM).

The U.S. Agency for Global Media is a modern media organization, operating far beyond the traditional broadcast mediums of television and radio to include digital and mobile platforms. The term “broadcasting” does not accurately describe what we do. The new name reflects our modernization and forward momentum while honoring our enduring mission to inform, engage and connect people around the world in support of freedom and democracy.

We recognize the overdue need to communicate the evolving, global scope of our work as well as our renewed, urgent focus on the agency’s global priorities, which reflect U.S. national security and public diplomacy interests. USAGM is an independent federal agency that provides accurate, professional, and objective news and information around-the-globe in a time of shifting politics, challenging media landscapes, and weaponized information. Our identity and name will now address these realities.

The decision to change our name was a result of thorough research and extensive consultation with numerous internal and external stakeholders, including the BBG Board of Governors, agency staff and leadership at all levels, the five networks, Congress, the Administration, and interagency colleagues.

As with the BBG, the U.S. Agency for Global Media encompasses five networks: the Voice of America (VOA), Radio Free Europe/Radio Liberty (RFE/RL), the Office of Cuba Broadcasting (Television and Radio Martí), Radio Free Asia (RFA), and the Middle East Broadcasting Networks (MBN). These networks collectively reach an unduplicated weekly audience of 278 million people in 59 languages and in more than 100 countries. Insulated by a firewall from political influence, these networks will continue to deliver truth and professional journalism to people living in some of the world’s most closed societies.

Now more than ever, people around the world need access to the truth. USAGM continues to tell the truth, and illuminate the world like no other news organization in the world.
(John Lansing/U.S. Agency for Global Media)

Deutsche Welle Bundesliga returns to shortwave on 25 August

All times UTC

Tune in for German football on Deutsche Welle. The Bundesliga gives viewers the goals, the action, the atmosphere and expert opinion on the best-attended soccer league in the world.

Transmitter locations as indicated
Effective: 25 August-01 September & 15 Sept-20 October 2018

All times UTC

Hausa
1325-1530 Sat. on 15195 ISS 500 kW / to WeAf Hausa Football (via Issoudun, France relay)
1325-1530 Sat. on 17840 ASC 250 kW / to WeAf Hausa Football (via Ascension Island relay)
(R Pearson)

Wednesday, August 22, 2018

Dxers Unlimited – midweek edition, August 21

By Arnie Coro CO2KK

 Hi amigos, I am Arnie Coro, radio amateur CO2KK, and your host at the middle of the week edition of Dxers Unlimited on the air and on the web from beautiful La Habana Cuba where we are experiencing thunderstorms every afternoon and early evening, with the most powerful ones lasting until late at night.

Cuban radio amateurs are well aware of the dangers of lightning, so it has become a ritual to disconnect all equipment after operating, and when on the air, at the slightest hint of an approaching thunderstorm you stop and disconnect everything, including your wires that go to the physical ground.

Since 1990 when they were recorded by on board cameras operating on the now retired Space Shuttles, sprites and elves have captured a lot of interests by geophysicists and space scientist. The most recent event recorded are:
  

Giant 'ELVE' over Russia 
On Aug. 16, high above a thunderstorm in central Russia, an enormous ring of light appeared in the night sky. Using a low-light video camera in the town of Irbit, amateur astronomer Ilya Jankowsky photographed the 300 km-wide donut hovering near the edge of space.

"It appeared for just a split second, surrounding the horns of the constellation Taurus," said Jankowsky.

This is an example of an ELVE (Emissions of Light and Very Low Frequency Perturbations due to Electromagnetic Pulse Sources). First seen by cameras on the space shuttle in 1990, ELVEs appear when a pulse of electromagnetic radiation from cloud-to-ground lightning propagates up toward space and hits the base of Earth's ionosphere. A faint ring of deep-red light marks the broad 'spot' where the Electromagnetic high intensity pulse hits.

"For this to happen, the lightning needs to be very strong-typically 150-350 kilo-Ampères," that is from one hundred and fifty thousand to three hundred thousand Amperes, says Oscar van der Velde, a member of the Lightning Research Group at the Universitat Politècnica de Catalunya. "For comparison, normal cloud-to-ground flashes only reach from 10 to 30 kiloAmperes."

ELVEs often appear alongside red sprites, which are also sparked by strong lightning and are under scrutiny by ionosphere researchers because they may be the cause of some particular form of Sporadic E layer clouds. By the way, during the ELVE event over Russia, Jankowsky's camera caught at least two clusters of sprites dancing nearby.

ELVEs are elusive, and that's an understatement. Blinking in and out of existence in only a millisecond, they are completely invisible to the human eye. For comparison, red sprites tend to last for hundredths of a second and regular lightning can scintillate for a second or more. Their brevity explains why ELVEs are a more recent discovery than other lightning-related phenomenon.

Despite the poor propagation conditions during the weekend, the international event dedicated to lighthouses and lightships was a success, and I think that all participants did enjoyed the relaxed atmosphere prevailing while operating their stations because of the non-contest nature of the event. It did provide a nice opportunity for newcomers to the Dxing world to work the rarely used T4 prefix, authorized for the special occasion to several Cuban radio club stations that operated from lighthouses. Among them, at the Santiago de Cuba Morro Castle Lighthouse T48SC, tango forty-eight sierra charlie accumulated a good number of contacts.

Now we must wait for the final report from the organizers of the ILLW International event to see the results. Let me add that to calculate the short propagation conditions for the weekend I had to use the number 1, yes 01 Sunspot Number feeding the forecasting software, that I regularly use because its simplicity and accuracy, the nice job of W6EL, who made it freely available. W6EL HF propagation forecasting software runs fast and when I compare results with other much more sophisticated programs, the results achieved, are good indeed.

The non-conversational digital communications mode FT8 has already brought a lot of controversy, and the saga goes on and on, something that, in my opinion, has benefitted amateur radio during this extended period of extremely low solar activity and its associated very poor HF bands propagation conditions.
  
Item # 2 - of special interest to short wave listeners that enjoy catching DX on the tropical broadcasts bands and good news coming from Brazil. A new station on 90 meters, Rádio Cultura de Araraquara is on 3365 kHz in the   tropical band.

The station has just announced that starting last Friday, August 17, it began transmitting, using 3365 kHz, and running one kW, but not specifying the type of antenna in use. The broadcast schedule will be from 2100-0300 UTC and to make the best possible use of both greyline and night-time propagation at that location of Brazil.

As anyone monitoring the HF bands on a day to day basis, will easily find out, the low solar activity continues to limit the chances of shortwave propagation on frequencies above 20 megahertz, even during the best times of the day at any given location. The exception comes when sporadic E layer openings move the maximum usable frequency up past the 25 MHz range.

Recent observations confirm that solar cycle 24 continues to show very weak activity as compared with any of the previous five solar cycles and some scientists are calling for an extended tail end of the cycle to last even two more years, while other solar researchers are telling us that we are now already well into solar minimum.

Si amigos, I receive many radio related questions coming to the ASK ARNIE section of Dxers Unlimited ... and they have helped me to learn more about the radio hobby, making possible to share with my listeners some very interesting findings.

Peter, from Birmingham in the United Kingdom, wrote asking about how he could replace worn out vacuum tubes on a nice 1950's vintage radio receiver that he is bringing back to life. Peter explains that the wooden cabinet is simply beautiful, and the radio was kept in a dry place for storage after it broke down.

After exploring the circuit diagram, Peter found out that the valve or vacuum tube marked ECH81 showed a whitish dust inside the glass bulb, indicating the loss of vacuum, fortunately the ECH81 tube is still available from Russia where it was manufactured in large quantities under the designation 6 INDIA ONE P.

This is Radio Havana Cuba, the name of the show is Dxers Unlimited and here is news about a little known amateur radio satellite the first Phase 5 amateur payload is already operational in an elliptical orbit around the Moon.

Yes, you heard it right ... there is a Chinese satellite carrying amateur radio transponders that is orbiting around the Moon...The last transmissions from LongJiang 2 were on 2018-08-05 from 00:30 to 02:30 UTC and from 07:30 to 09:30 UTC on 435.400 MHz and 436.400 MHz.

Various experiments are being carried out with GMSK and JT4G downlink signals. Stations with 'normal' amateur equipment can receive the downlinks quite well. Downlink signals have even been received with no more than an Arrow antenna, no preamp.

DK5LA was the first to have his signals relayed through LongJiang 2 on 2018-07-15. On August 4, the first picture of an onboard camera was downlinked with SSDV. Other experiments will follow later. Why not give LongJiang 2 a try?

Thanks to Nico, PA0DLO for the above information.

See you all at the weekend edition of Dxers Unlimited next Sunday and early Monday UTC days just after the top of the hour news...send your signal reports and comments about this and other Radio Havana Cuba's programs as well as your radio hobby related questions to inforhc@enet.cu and via air mail postage to: Arnie Coro, Radio Havana Cuba. Havana, Cuba
(Arnie Coro)


Monday, August 20, 2018

Dxers Unlimited – weekend edition, August 19, 2018


Special thanks to Arnie Coro, for sharing his program script with our blog followers

(GVH)

 Hola amigos radioaficionados, I am Arnie Coro, radio amateur CO2KK bringing to you the week-end edition of Dxers Unlimited, and here is our first news item:

The International Lighthouse and Lightships Weekend took place on August 18-19, and several Cuban amateur radio clubs stations participated using the special prefix T4.

For your information the International Lighthouse and Lightships Weekend, is one of the largest yearly operating events in the amateur radio calendar, with more than 400 lighthouse/lightship activations in 40 countries, and tens of thousands of amateur stations wanting to work them.

By the way...this year is the 25th anniversary of the event from which it all began. The very first Northern Lighthouse Weekend was organized in 1993 by the Ayr Amateur Radio Group with activity from just 10 lighthouses in Scotland and the Isle of Man. But something about 'the romance of lighthouses' found a resonance with radio amateurs; the idea quickly spread world-wide and grew into the remarkable event we know it today.

The solar activity is at very low levels... although a single solitary small sunspot broke the sequence of days without sunspots. Experts explained to me that the small active region is not expected to produce powerful solar flares and is expected to fade out soon.

The present summer season of the northern hemisphere has brought a rather normal sporadic E layer activity, with several good days when transatlantic contacts were possible on the 6 meters band.

More information about HF propagation conditions at the end of the show when you will receive the latest Arnie Coro's HF plus low band VHF propagation update.

Answering another question from Dxers Unlimited listeners, they all want to learn more about Trans Equatorial Propagation, also known by its acronym TEP. Amigos TEP is a propagation mode that sometimes even makes possible, two meters band contacts between Caribbean stations and Brazil, Argentina, Chile, Bolivia, Uruguay and Paraguay, while using low power stations.

Well, I must say that the TEP, the Trans Equatorial Propagation opening here in Cuba are not as good as those enjoyed by my amateur radio friends located in Trinidad and Tobago, Saint Lucia and Barbados and Puerto Rico.

Here three band openings start usually are around 20 hours UTC and the peak months are March and September, coinciding with the spring and autumn equinoctal periods and are at a minimum during the summer solstice. I usually monitor six meters on the international DX window frequency of 50.110 kHz, where experienced operators call CQ DX using single side band voice.

Sometimes you can even tell from where the signals are coming, before even picking up a callsign, by paying attention to that very peculiar way of speaking Spanish that is typical of the Argentineans and Uruguayans or the Portuguese language spoken by the Brazilian radio amateurs.

Once again for your information the TEP can link up with Sporadic E propagation and place signals from the far end of South America into the United States and Mexico, and sometimes even as far as Canada.

If you are an amateur radio operator you can make very nice two-way contacts while running low power and a very simple two to three elements Yagi or cubical quad antennas, that can be easily built at home and without expending a lot of money as readily available materials are used.

Again, for those of you radio amateurs that live in the Southern United States and in southern Mexico, and Central America, September will very probably bring in many Trans Equatorial Propagation events that will open up the 10 and six-meter bands during your local afternoon and early evening hours, although I have made contacts with Chile and Argentina on
six meters past midnight my local time here in Havana.

This is the weekend edition of your favorite listener oriented and technically minded radio hobby program, with yours truly Arnie Coro radio amateur CO2KK as your host.

Here is now our next topic... more information about simple end-fed antennas now in use here by several Cuban radio amateurs that operate on the shortwave ham bands from 40 to 10 meters. Operators are achieving good results with a very simple wire antenna that has the advantage over a dipole that it is fed at one end using a balanced to unbalanced broadband transformer.

There are ongoing discussions about the impedance transformation ratio required for this end-fed antenna, and all I can say that my tests using  a second such antenna 25 meters long installed horizontally show that using a standard factory built four to one balun and 50 or 75 coaxial cable makes possible to operate on the 40, 30, 20, 17, 15, 12 and 10 meter bands using my wide range PI network antenna tuner.

The length of the coaxial cable downlead is at my station is less than 15 meters losses due to high standing wave ratio are minimal. The antenna behaves as an omnidirectional system on 40, 30 and 20 meters, but starts to show up some directivity above the 20 meters band...

Si amigos, my friends, oui mes amis, this is the weekend edition of Dxers Unlimited, now ASK ARNIE the second most popular section of this show.

Today answering a question sent by listener Herman from Bogota, Colombia who monitors Radio Havana Cuba via our Internet streaming audio, and via shortwave on 11840 kHz. Herman lives outside the city in a residential neighborhood, so he can install a wire antenna from a 10 meters mast on his roof going to another similar mast at the end of the backyard. I recently told him to try a center fed group of dipoles, cut for the 40, 20 and 15-meter bands, that can also be tuned to 17, 12 and 10 meters with the aid of his antenna tuner. The dipoles are separated from each other by insulators that are 15 centimeters long, made from the dielectric that is used by RG213 coaxial cable, by removing the center conductor using heat from the soldering iron.

Ys, radio amateurs from many different countries that are QRP or low power fans can be heard on the air on the 15 meters band frequency of 21.060, using CW Morse Code with their very low power rigs. Plans are now in the work to make a special operating event next October the fourth to celebrate the 57th anniversary of the launching of the first ever artificial satellite, Sputnik One, that had on board the first radio transmitter that went into space and sent radio signals from an orbiting space satellite. 

Several of the radio amateurs involved in the Sputnik One anniversary in recent years will be again celebrating, having already built a small vacuum tubes transmitter that is an exact replica of the rig that went up and sent its signals on two frequencies, 20.005 and 40.005.

The original Sputnik frequency of 20.005 MHz is not assigned to the amateur radio service, it was decided that the replica transmitters will operate on the nearby 15 meters band, on the frequency internationally agreed to be used by low power, or QRP CW amateur radio stations, that is 21.060 MHz. The transmitter designed by the Soviet radio engineers for the first man made satellite, Sputnik One, used very ruggedly built subminiature vacuum tubes.

Poor propagation conditions on the HF bands continue and solar activity is expected to be extremely low during the next several days.

See you all at the middle of the week Dxers Unlimited edition next Tuesday and Wednesday UTC days.

Send your signal reports, comments about this and other programs, and radio hobby related questions to inforhc@enet.cu, and via air mail to: Arnie Coro, Radio Havana Cuba, Havana, Cuba.
(Arnie Coro/R Havana)




Highest Powered Mediumwave Station in the Southern Hemisphere - 2YA


2CO Corowa transmitter and aerial
When it was officially opened on December 16, 1931, mediumwave station 2CO in Corowa New South Wales  Australia, was accorded honor as the highest powered mediumwave radio broadcasting station in the Southern Hemisphere with 7½ kW on 560 kHz.  Then on March 15 of the following year 1932, 5CK in Crystal Brook South Australia was officially opened on 635 kHz, also with 7½ kW, thus sharing honor with 2CO as equal highest powered mediumwave radio broadcasting station in the Southern Hemisphere.

          
However five years later again, a bright new mediumwave station near Wellington in New Zealand, 2YA with a 60 kW transmitter, became the highest powered mediumwave station in the Southern Hemisphere, thus eclipsing the two Australian stations for that honor.  Since that time, 2YA has always held the honor, at least as equal highest powered mediumwave station in the South Pacific.    
Let’s go back now to the month of February in the year 1922, which was when the first mediumwave station in Wellington commenced broadcasting.  This new station was constructed and  operated by Charles Forrest at the International Electric Company in Courtenay Place, Wellington and it was on the air two evenings a week, Monday and Wednesday, for an hour and a half on each occasion.

Six months later, Forrest merged with Hope Gibbons to form Wellington Broadcasters Ltd with their small cramped radio studio at the top of the Ford Building in Courtenay Place.  This building had been constructed earlier for the assembly of American made Model T Ford motor cars.
     
During the following year (1923), the New Zealand government began issuing callsigns to radio broadcasting stations and this first station in Wellington was accorded the callsign 2YB.  However one year later again, in November 1924, this station 2YB merged with the second broadcasting station in Wellington that had been accorded the sequential callsign 2YK.
   
This second station in Wellington was owned and financed by a group of five interested men who operated as the Federal Telephone Company.  The transmitter for this new radio station was constructed locally on information provided by Professor Robert Jack who had been experimenting with wireless for the past year or more in Dunedin on the South Island. 
    
The new Wellington station was installed at the back of Mr. A. H. Simpson’s home in suburban Wellington, quite near to the local post office, and it was launched in August 1922, when the previously mentioned first station 2YB was just six months old.  The New Zealand government issued the callsign 2YK to this now second station in Wellington.
    
In November (1923) this station, with its staff-built new transmitter, was moved to the 5th floor in the Dominion Building on Plimmers Steps, just off Lambton Quay, hence a new company name, the Dominion Radio Company.  Waterside workers cut a tree and hauled it to the roof of the building to support the antenna system.  This station was on the air two or three evenings a week for a total of just a few hours altogether.
  
During the year 1924, the New Zealand government began to subsidize four key radio broadcasting stations in New Zealand, including 2YK in Wellington.  Then In November of that same year, the first station in Wellington (2YB) was merged into the more substantial and now more successful second station 2YK. 
       
On August 30 of the next year (1925) the government took over tall four of the subsidized stations (1YA Auckland, 2YK Wellington, 3AQ Christchurch, 4YA Dunedin), though the Wellington station went silent instead.  As an interim measure, the Post Office personnel provided some form of spasmodic programming for the 2YK transmitter.

Station 2YK returned to the air for the November (1925) elections, and again for special Christmas programming.  Then during the following year (1926), this station began to carry a regular programming schedule.  In June 1927, station 2YK was given a change in callsign, and thus 2YK became the now highly regarded and well known 2YA.
    
Actually, the 2YA callsign had previously been allocated to a small battery operated station in Nelson.  This small regional city of Nelson is located on the north coast of the South Island almost opposite Wellington, and Wellington is located across the Cook Straits on the southern edge of the North Island.  In 1923, Mr. D. Field established this radio station in Nelson which was allocated at that stage the callsign 2YA.  
  
This small radio station operated without mains electricity, and it required 300 torch batteries soldered together to provide electricity for it to go on the air.  This 2YA radio station broadcast from a hardware shop, Wilkins & Field Ltd., in Hardy Street, Nelson.
  
During the mid 1920s, a big new 2YA in the national capital city Wellington was planned as the most powerful mediumwave broadcasting station in the world.  However when it was officially opened by Prime Minister Joseph G. Coates on July 9, 1927, its power level was only 5 kW, not even as powerful as the two stations in Australia; 2CO & 5CK with 7½ kW each. 
    
Studios for this new 2YA were installed in the Wellesley Club Building on the corner of Waring Taylor & Featherstone Streets in Wellington.  The transmitter was installed in a new building under two  
self-supporting towers on Mt. Victoria, towering over the city of Wellington.
  
However soon afterwards. another new 2YA was built on a small promontory at Titahi Bay, Whitireia Head, and this one really did become the most powerful in the Southern Hemisphere.  In addition, its single tower was also the tallest in the Southern Hemisphere standing 700 feet high.  The tower was manufactured in Australia and shipped to New Zealand in sections.
   
The transmitter building at Titahi Bay was constructed to withstand sustained wind speeds of 100 miles an hour, and the end roofing trussets were specially designed to retain the roof in gale force winds.  The earthing system was composed of 10 miles of copper wire laid underground in a special counterpoise pattern.  An emergency on-air studio was installed in the transmitter building, and subsequently, so was an emergency power generator.

The new 2YA transmitter was manufactured by AWA at their Sydneyside factory in suburban Ashfield, and it was rated at the unusual power level of 60 kW.  The antenna system for this new high powered radio station was configured to provide maximum coverage of New Zealand north-south, with a minimum of skywave propagation.

This high powered 2YA on 570 kHz in New Zealand was easily heard one thousand miles away in Australia, particularly in the evenings with programming at a listening level, due to the saltwater pathway.  In fact, on one occasion, mediumwave 2YA was heard on a car radio at a listenable level while a family was traveling up towards the center of Australia when the time at the transmitter site was already late morning.  
   
This new 2YA was officially opened by the Prime Minister of New Zealand, Mr Michael Savage, on January 25, 1937.  The old 5 kW 2YA transmitter was retuned to 840 kHz and it returned to the air under a new callsign 2YC.
    
These days, the magnificent 2YA is still on the air with 50 kW on 567 kHz at Titahi Bay, and studios in Radio New Zealand House on the Terrace in Wellington.  Over the years, many hundreds of QSL cards have been sent to listeners living in countries within, and beyond, the Pacific arena.
(AWR/Wavescan-NWS 492)
(photo/ABC Archive/Flickr)

Weekly Propagation Forecast Bulletins


Product: Weekly Highlights and Forecasts
:Issued: 2018 Aug 20 0445 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC link http://www.swpc.noaa.gov/weekly.html
#
#                Weekly Highlights and Forecasts
#
Highlights of Solar and Geomagnetic Activity 13 - 19 August 2018

Solar activity was very low. Two small regions developed on the visible disk this period. Region 2718 (S07, L=191, class/area Hrx/020 on 17 Aug) developed on 14 Aug and decayed to plage by 19 on Aug. Region 2719 (S06, L=133, class/area Bxo/010 on 19 Aug)  developed in the SE quadrant on the 19 August. No significant flare events occurred from either region. Other activity included a filament eruption centered near S11W04 observed lifting off the solar disk at approximately 19/0538 UTC. An associated coronal mass ejection was observed off the SW limb in SOHO/LASCO C2 imagery at 19/0812 UTC. WSA/Enlil modelling of the event suggested the ejecta was primarily directed to the westward of the Sun-Earth line and is not expected to cause any significant effects.

No proton events were observed at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit was at normal levels on 13-15 Aug, moderate levels on 16-17 Aug, and at high levels on 18-19 Aug. The largest flux of the period was 18,287 pfu observed at 19/1800 UTC.

Geomagnetic field activity ranged from quiet to active levels over the period. Solar wind speed was at nominal levels at the beginning of the period with solar wind speed ranging from 310-430 km/s while the total field was between 1-4 nT. The geomagnetic field was quiet on 13-14 Aug. By 15 Aug, solar wind speed increased to approximately 450-500 km/s with total field increasing to a maximum of 14 nT by 16/1005 UTC as a positive polarity coronal hole high speed stream (CH HSS) moved into geo effective position. A further increase in solar wind speed to near 570 km/s was observed late on 17 Aug before slowly receding to nominal levels by midday on 19 Aug. The geomagnetic field that responded with quiet to active levels on 15-18 Aug. By late on 19 Aug, total field increase again to 12 nT along with an increase in solar wind to near 550 km/s as a negative polarity CH HSS was becoming geoeffective. However, only quiet levels were observed on 19 Aug.

Forecast of Solar and Geomagnetic Activity 20 August - 15 September 2018

Solar activity is expected to continue at very low levels.

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 22-27 Aug and again on 13-15 Sep due to CH HSS influence.

Geomagnetic field activity is expected to be unsettled to active levels on 20-25 Aug, 03-04 Sep, 07 Sep, and 11-15 Sep with a chance for G1 (Minor) geomagnetic storm levels on 20-21 Aug due to the recurrent of CH HSS activity.

Product: 27-day Space Weather Outlook Table 27DO.txt
:Issued: 2018 Aug 20 0445 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC link http://www.swpc.noaa.gov/wwire.html
#
#      27-day Space Weather Outlook Table
#                Issued 2018-08-20
#
#   UTC      Radio Flux   Planetary   Largest
#  Date       10.7 cm      A Index    Kp Index
2018 Aug 20      67          20          4
2018 Aug 21      67          18          4
2018 Aug 22      67          12          4
2018 Aug 23      67          12          4
2018 Aug 24      66          10          3
2018 Aug 25      66           8          3
2018 Aug 26      66           5          2
2018 Aug 27      66           5          2
2018 Aug 28      66           5          2
2018 Aug 29      66           5          2
2018 Aug 30      66           5          2
2018 Aug 31      66           5          2
2018 Sep 01      66           5          2
2018 Sep 02      66           5          2
2018 Sep 03      66          12          4
2018 Sep 04      66           8          3
2018 Sep 05      66           5          2
2018 Sep 06      67           5          2
2018 Sep 07      67           8          3
2018 Sep 08      67           5          2
2018 Sep 09      67           5          2
2018 Sep 10      67           5          2
2018 Sep 11      68          15          4
2018 Sep 12      68          15          4
2018 Sep 13      68          12          4
2018 Sep 14      68          12          4
2018 Sep 15      68          10          3
(NOAA)