Abstract This paper deals with a preliminary study of two flares observed by the PHEBUS instrument and by the Nancay Multifrequency Radioheliograph in the hard X-ray/gamma-ray and in the decimeter-meter radio wave domains respectively. For both flares the radio emission associated with individual hard X-ray/gamma-ray peaks show different characteristics. This is discussed in terms of temporal changes of the large scale magnetic structure involved in the region of particle acceleration.
Radio and X-ray/gamma-ray observations of two solar flares
Advances in Space Research ; 13 , 9 ; 285-288
1993-01-01
4 pages
Article (Journal)
Electronic Resource
English
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