Flare Physics with the Nobeyama Radioheliograph and RHESSIs

Details Flare Physics with the Nobeyama Radioheliograph and RHESSIs Flare Physics with the Nobeyama Radioheliograph and RHESSIs

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006spnr.conf...39n&link_type=abstract

Solar Physics with the Nobeyama Radioheliograph, Proceedings of Nobeyama Symposium 2004, held in Kiyosato, Japan, October 26- 29

Physics

2

Scientific paper

In this article I review the present status of knowledge in areas of special interest for further study using solar flare observations at microwaves from the Nobeyama Radioheliograph and hard X-ray (HXR) observations from RHESSI. The most direct tracers of the electrons accelerated in a flare are the microwave and HXR emissions they produce. The combined microwave and hard X-ray data provide powerful diagnostics of the physical conditions in flaring regions and particularly the magnetic field configuration of the flare and the properties of the energetic electrons. I point out that in order to tackle better the fundamental problem of particle acceleration in solar flares, detailed comparison of the spatial and spectral data with models is needed.

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