Gjermund, LB5GI has been added to M0OXO QSL Service. Gjermund lives on Sandsøya Island, (IOTA EU-079), just off the coast of Norway.
The Team are back home after a successful Dxpedition to Prins Karls Forland Island, Norway, (IOTA EU-063) having made just under 16,000 contacts in the four day trip.
Harald (DF2WO) will be qrv as 9X2AW from Kigali, Rwanda between the 13th & 28th September 2021 from Grid KI48xe.
Listen for the guys from the Royal Omani Amateur Radio Society this week operating as A44M from Masirah Island (IOTA AS-014), Sultanate of Oman during the RSGB IOTA Contest.
Listen out for the Team Friuli Venezia Giulia this weekend as they activate Barbana Island (IOTA EU-130) Italy as II3Y in the RSGB IOTA Contest.
Henry NL0H is preparing to be active for the next few days including during the RSGB IOTA contest from St. Lawrence Island IOTA NA-040.
Harald (DF2WO) will be qrv as 9X2AW from Kigali, Rwanda between the 13th & 28th September 2021 from Grid KI48xe.
Well just a week away from the RSGB IOTA Contest 2021.
Imagine an explosion on the farside of the sun so powerful, we could feel it here on Earth. It happened on July 13th. The debris emerged in a circular cloud known as a ‘halo CME. When space weather forecasters first saw this explosion, there was a moment of excitement. It appeared to be heading directly toward Earth. However, data from NASA’s STEREO-A spacecraft indicated otherwise. The CME was heading directly away from us–a farside event.
Dust storms on Mars are bigger than we thought; they even spill into space. According to a recent paper in JGR Planets, Mars appears to be leaking dust, filling a huge volume of the inner solar system with gritty debris. You can see it with your naked eye. The bright triangle in this image from the Haleakalā Observatory in Hawaii is marsdust.
It’s called Zodiacal Light, and astronomers have long wondered what causes it. The usually faint triangle is sunlight scattered by dust in the plane of our solar system. The dust, it turns out, comes from Mars.
NASA’s Juno spacecraft flew through the dust cloud en route to Jupiter between 2011 and 2016. Dust grains smashed into Juno at about 10,000 mph, chipping off submillimeter pieces of spacecraft. Juno’s oversized solar arrays turned out to be excellent dust detectors, registering as many as 200 hits per day.
Ironically, the sandblasting allowed researchers to map the cloud for the first time. One theory of Zodiacal Light held that asteroids were responsible. Yet, as Juno flew through the asteroid belt toward Jupiter, impact rates sharply dropped, sometimes to zero. Asteroids were not the answer. Instead, they realized, the dust must be coming from Mars. Orbital elements of the dust grains essentially match that of the Red Planet.
Mars is the dustiest place in the Solar System, with dust storms that envelop the entire planet for months. But how does this dust escape? During storms, dust is sometimes launched to very high altitudes in the Martian atmosphere; researchers call it ‘rocket dust’. However, leaving Mars requires overcoming escape velocity (~5 km/s), and even rocket dust has trouble doing that. Dust grains would have an easier time launching from Phobos and Deimos; however, those small moons don’t produce enough dust to explain the Zodiacal Light.
So, there’s still a mystery here. Mars has the dust, but researchers haven’t yet figured out how Mars delivers it. Lead author John Leif Jørgensen (Technical University of Denmark) and colleagues hope other scientists will help them solve this final piece of the puzzle.
credit spaceweather.com
