NASA NTRS · 19890064574
A relation between Balmer and soft X-ray emission in flares
Abstract
Data are presented on 370 solar flares simultaneously observed and classified in H-alpha and in the GOES (1-8 A) soft X-ray band. SMM observations corroborate the association of the GOES and the H-alpha events in all cases. These flares are used to examine the correlation proposed recently by Butler, Rodono and Foing (1988).
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Haisch, B. M.. 1989-07-01. A relation between Balmer and soft X-ray emission in flares. https://ntrs.nasa.gov/citations/19890064574
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