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Vertical structure of hard X-ray flare

✍ Scribed by S. Tsuneta; T. Takakura; N. Nitta; K. Ohki; K. Makishima; T. Murakami; M. Oda; Y. Ogawara

Publisher: Springer
Year: 1983
Tongue: English
Weight: 630 KB
Volume: 86
Category: Article
ISSN: 0038-0938
DOI: 10.1007/bf00157204

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✦ Synopsis

This paper presents studies of the vertical structure of hard X-ray flares for two contrasting examples. The 1981 May 13 flare contained a coronal hard X-ray source which was located above 50000 km above the photosphere. On the other hand, the 1981 July 20 flare had a chromospheric double source structure in the initial phase. Electrons in this case were able to stream freely from the corona to the chromosphere.

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