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Characteristics of solar X-ray flares registered by the CORONAS-PHOTON satellite

✍ Scribed by Yu. D. Kotov


Book ID
111502286
Publisher
Allerton Press Inc
Year
2011
Tongue
English
Weight
178 KB
Volume
75
Category
Article
ISSN
1062-8738

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It is now more than ten years since the first x-ray emitting stellar corona was discovered (Catura, Acton, and Johnson 1975). Since then, rapid progress has been made in cataloging the incidence and range of stellar x-ray emission, most notably with the Einstein Observatory (see, eg., reviews by Ste