Energetic Electrons and Magnetic Field Structures in the Corona

Details Energetic Electrons and Magnetic Field Structures in the Corona Energetic Electrons and Magnetic Field Structures in the Corona

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994kofu.symp..263p&link_type=abstract

In: Proceedings of Kofu Symposium, Kofu, Japan, Sept. 6-10, 1993, p.263-266.

Physics

3

Scientific paper

The Nancay Radioheliograph provides imaging observations of the low middle corona. Such observations combined with X-ray and gamma ray observations constitute an unique way to get informations on the coronal structures in which electrons propagate. This is illustrated on two examples: 1)the first joint observation of a coronal structure between the soft X-ray telescope aboard the Yohkoh satellite and the Nancay multifrequency radioheliograph; a radioburst was used as a tracer of a coronal structure and its spectral identification was obtained with the radiospectrograph of the University of Porto 2)the magnetic structures involved in the flare acceleration processes.

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