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• W102304465 abstract "A brief overview is given of some of the current outstanding problems in solar physics with greatest emphasis on high energy phenomena in the atmosphere. The importance of plasma kinetic effects, as well as MHD, in understanding the complex finely structured and dynamic solar atmospheric plasma is stressed. Key results from the RHESSI Mission on energetic flare particle acceleration, propagation, and flare energy budgets are presented as are recent findings concerning the solar and stellar flare Neupert effect and the possible role of energetic particles in micro-events in the ‘non-flaring’ sun. Finally, evidence showing that magnetic fields are also important in hot star phenomena is mentioned." @default.
• W102304465 created "2016-06-24" @default.
• W102304465 creator A5072808639 @default.
• W102304465 date "2004-01-01" @default.
• W102304465 modified "2023-10-12" @default.
• W102304465 title "The Sun as a Stellar Laboratory: Unsolved Problems" @default.
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• W102304465 doi "https://doi.org/10.1017/s0074180900181914" @default.
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