17 and 34 GHz Observations of the Sun with The Nobeyama Radioheliograph

Details 17 and 34 GHz Observations of the Sun with The Nobeyama Radioheliograph 17 and 34 GHz Observations of the Sun with The Nobeyama Radioheliograph

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999spro.proc..249f&link_type=abstract

Solar Physics with Radio Observations, Proceedings of the Nobeyama Symposium, held in Kiyosato, Japan, Oct. 27-30, 1998, Edited

Physics

1

Scientific paper

Since the beginning of dual-frequency observations with the Nobeyama Radioheliograph, many flares and related energetic phenomena have been observed. Some of them are sufficiently intense in microwave and mm-wave ranges that it is possible to synthesize 34 GHz images together with the corresponding 17 GHz images. Dual-frequency analyses of them provide us with spectral information which reflects physical conditions in flare regions such as energy distribution of high-energy electrons, magnetic fields, and density of heated plasmas. In this paper, we briefly present observations of two flares and a prominence eruption which were obtained by the Nobeyama Radioheliograph at 17 and 34 GHz.

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