Tracking Solar Shocks and Fast Electrons from Sun to Spacecraft (SolShocks)

Bidragets beskrivning

The Sun is an active star that produces the most powerful explosions in the Solar System such as solar flares and solar storms. These explosions are often accompanied by fast particles with speeds comparable to the speed of light, sometimes directed towards Earth. The fast particles can have a harmful impact on satellites and technology in space. Some of these particles can be observed remotely as radio emission but they can also be directly detected by spacecraft. A number of mechanisms can produce these fast particles during solar storms. However, it is currently not known which type of storms and mechanisms produce the particles observed. The project aims to answer these unknown questions by using observations from international radio telescopes combined with direct detections of these particles from a newly launched fleet of spacecraft.
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Startår

2023

Slutår

2027

Beviljade finansiering

Diana Morosan Orcid -palvelun logo
602 205 €

Finansiär

Finlands Akademi

Typ av finansiering

Akademiforskare

Beslutfattare

Forskningsrådet för naturvetenskap och teknik
16.05.2023

Övriga uppgifter

Finansieringsbeslutets nummer

354409

Vetenskapsområden

Geovetenskaper

Forskningsområden

Avaruusfysiikka

Identifierade teman

space, physics