X-ray and gamma-ray emission from solar flares
A Tsvetkova;
2020-01-01
Abstract
We present a brief review of the contemporary understanding of and topical problems in solar flare physics that can be clarified by methods of X-ray and gamma-ray astronomy. The review focuses on several issues, including the conditions and mechanisms of electron acceleration in solar flares, the flare energy distribution between thermal and nonthermal components, the gamma-ray emission from solar flares and its dynamics, and the spatial structure of X-ray and gamma-ray sources. Discussed in this context are the latest data obtained by the joint Russia-US experiment Konus-Wind, which in 2019 celebrated the 25th anniversary of continuous operation in space.File | Size | Format | |
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2020_Lysenko_UFN_eng_pu_63_818.pdf Solo gestori archivio
Description: Articolo principale
Type: versione editoriale
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