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Riunione Gruppo gestione documentale
14:30
Riunione Gruppo gestione documentale
Lug 4@14:30–18:30
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“First X-ray detection of plasma motions in a stellar flare and in the associated CME”, Costanza Argiroffi (Dip. di Fisica & Chimica, Universita` di Palermo)
15:00
“First X-ray detection of plasma motions in a stellar flare and in the associated CME”, Costanza Argiroffi (Dip. di Fisica & Chimica, Universita` di Palermo)
Lug 12@15:00–16:00
The comprehension of magnetically-related phenomena occurring in stellar atmospheres is one of the long-standing issues of astrophysics. The solar corona has always been the starting point to understand coronal physics, because the high spatial structuring of coronal plasmas complicate stellar observations. Stars however show activity levels up to 10^4 times higher than the Sun, and it is not clear how
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