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Time delay between Hα and hard X-ray emissions during impulsive solar flares

✍ Scribed by V. K. Verma; M. C. Pande

Publisher
Springer
Year
1985
Tongue
English
Weight
318 KB
Volume
97
Category
Article
ISSN
0038-0938

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✦ Synopsis

This investigation shows that statistically there are significant time delays between Ha and hard X-ray (HXR) emissions during solar flares; most impulsive flares produce HXR emissions up to ~ 1 min before and up to 2 min after the onset of Hc~ emission. HXR emissions are also found to be peaked up to 2 min before the Hc~ emissions.

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