Sometimes one QSO is enough, if it is the right one.
Last year I had already watched Kev from Gibraltar, ZB2GI, during his meteor scatter tests and got short reflections from him. Unfortunately, there was not enough time for a test and a long year passed.
During the Perseid shower ZB2GI (IM76hd) resides on Top of the Gibraltar Rock with a free Takeoff into Europe. With his small station, a 5 element Yagi antenna and 50 watt output power, he has already had many successful meteor scatter contacts in the past. But would that be enough this year for a QSO over the distance of 2,130 km?
For a long, very long time I watched Kev’s frequency as he tested with southern European stations. And there were reflections, not many, not loud and not long. But it was enough for decoding.
When he was free I started a call. Hopefully the reflections will continue and we will hear each other. To make a long story short: Finally, after almost 90 minutes and my pulse near a heart attack, he got my final RRR and the QSO was finished with 26 reports on both sides.
Contacts above 2,000 km via meteor scatter are usually difficult with few reflections. So I’m all the more happy about this special contact and a new DXCC # 97 for me on 2m. Many thanks Kevin for your patience and perseverance!
After 2016, the MRASZ – Hungarian Radio Amateur Society – offers again a nice short time award, commemorating the 230th anniversary of the birth of Samuel F.B. Morse, the creator of the Morse alphabet. The Award is free of charge and could be downloaded as pdf-file.
2021 will mark the 60th anniversary of the first manned flight into space, one of the most important milestones in the history of all mankind. The first manned flight took place on April 12, 1961. Cosmonaut Yuri Gagarin made one complete turn in Earth orbit and returned safely to Earth.
For this anniversary the special call signs R1994YU, R1996VK, R2014NC, RG21DS, RU21DS, RA60YG – RZ60YG, R60MCC, R60CTC, R60YAG and several others are in the air and the Miller-DX-Club “M-DX-C” has developed an interesting Award program. The period is from April 12th to 25th, 2021.
From January 28, 2021 to January 29 2021 the ISS send again pictures in Slow Scan Television. The images are always transmitted in Mode PD 120 on 145.800 MHz in Frequency Modulation. The following images were received with a 14 Element Yagi and decoded with MMSSTV software. More information about Amateur Radio on the ISS can be found on the ARISS website and the ARISS Blogspot. A nice Tracker could be find here.
Another milestone in my 48 years of Ham Radio: After WAC 432 MHz (1983) and WAC 144 MHz (2018), the WAC 1296 MHz arrived today. Of all these it was the fastest and all Continents were in the log after just 2 months of activity.
Nice surprise: The ARRL DXCC Challenge Medallion 2500 was in the mailbox today. Just a small round sticker, but so much time and work went into it. Challenge 2500 means an average of 250 DXCC Entities on each of the 10 Bands from 160m to 6m. The next and final level is 3000, but I’m out of business now. Unfortunately it is more difficult nowadays to get the confirmation for a QSO than to make the contact itself. Not to mention the cost of requesting QSL cards or LotW confirmations. Now it has a dignified place on the wall and will remind me of so many nice contacts.
The Perseids come around once a year in mid-August, when the Earth passes through a trail of comet dust on its way around the sun. The dust burns up in the Earth’s atmosphere and ionizes the E-layer. The Perseids are caused by debris from comet 109P / Swift-Tuttle, which loops around the sun on a 133-year orbit.
This year they should peak on Wednesday, Aug. 12 between 0800 and 2100 UTC. The Perseids typically deliver up to 110 meteors per hour at their peak. According to scientific predictions, the reflection numbers should start to rise again in 2027.
After a two-year absence, I decided to be active on 144 MHz this year for the Perseids Meteor shower. At the end a total of 44 QSOs could be logged, including 13 new QTH locators. In retrospect, I have to say that the shower had significantly worse reflections this year compared to previous years.
This picture shows my signal, recorded by Nick US8AR in KO60RR and Andy UT4UEP in KN49WV. It is the same burst with a duration of over 30 seconds, recorded by both on August 11, 2020 at 10:45:30 UT. Thanks to Nick and Andy for these interresting screenshots.
From August 04, 2020 until August 05 2020 the ISS send again pictures in Slow Scan Television. The images are always transmitted in Mode PD 120 on 145.800 MHz in Frequency Modulation. The following images were received with a 14 Element Yagi and decoded with MMSSTV software. More information about Amateur Radio on the ISS can be found on the ARISS website and the ARISS Blogspot.
50 MHz: Seasonally 6m was open every day within Europe. In addition, there were very long openings to Asia and North America. Towards the US and Canada, the terrain of my QTH rises to 10 degrees elevation, so at all again only a few stations from the west have been heard and worked.
In total, six new DXCC entities could be worked in May: 4S7VG (Sri Lanka), BU2EL (Taiwan), DU1IST (Philippines), HL2ZN (South Korea), JT1CO (Mongolia) and VR2XYL (Hong Kong).
144 MHz: Regarding Sporadic E, this June was a real disappointment. Only on June 21st there was a brief opening to the east and just two contacts could be logged. RU3GX, R3KBF, UA3QHF were heard only.