Bursts of solar X-rays in the energy range 5-15 keV are associated with flares and are due to thermal emission from a hot coronal plasma. In this paper we present the results of the first study of a large sample of separate bursts, 197 events associated with subftares and a few importance 1 events.
โฆ LIBER โฆ
Reduction in the intensity of solar X-ray emission in the 2- to 15-keV photon energy range and heating of the solar corona
โ Scribed by I. K. Mirzoeva
- Book ID
- 120808580
- Publisher
- SP MAIK Nauka/Interperiodica
- Year
- 2013
- Tongue
- English
- Weight
- 629 KB
- Volume
- 39
- Category
- Article
- ISSN
- 1063-780X
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