Radio and X-ray manifestations of a bright point flare

Details Radio and X-ray manifestations of a bright point flare Radio and X-ray manifestations of a bright point flare

Jun 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..374..408g&link_type=abstract

High energy solar physics. AIP Conference Proceedings, Volume 374, pp. 408-415 (1996).

Physics

Solar Electromagnetic Emission

Scientific paper

We have found remarkably different manifestations of a bright point flare in X-ray and radio (microwave) wavelengths, unlike previous observations. In X-rays, the BP flare was relatively simple while in radio, the bright point flare had a large scale component and a transient moving component. The large scale structure may be the radio counterpart of large scale structures sometimes seen during X-ray BP flares. The transient component was also compact and moved away from the location of the X-ray BP flare with a speed of ~60 km s-1. The compact source also showed fast time structure which suggests nonthermal emission mechanism for the transient sources.

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