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Observational Studies of the X-Ray Quasi-Periodic Oscillations of a Solar Flare

✍ Scribed by Y. P. Li; W. Q. Gan

Publisher
Springer
Year
2007
Tongue
English
Weight
466 KB
Volume
247
Category
Article
ISSN
0038-0938

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πŸ“œ SIMILAR VOLUMES

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A new series of solar flare energetic X-ray events has been detected by an ionization chamber on the OGO-I and OGO-III satellites in free space. These X-rays lie in the range 10-50 keV, and a study has been made of their relationship to 3 and 10 cm radio bursts and with the emission of electrons and

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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