An analysis for X-ray flare on July 14, 1980 and its comparison with the H-alpha flare

Details An analysis for X-ray flare on July 14, 1980 and its comparison with the H-alpha flare An analysis for X-ray flare on July 14, 1980 and its comparison with the H-alpha flare

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985chjss...5r..11x&link_type=abstract

Chinese Journal of Space Sciences, vol. 5, Jan. 1985, p. 11-18. In Chinese, with abstract in English.

Physics

H Alpha Line, Solar Flares, Solar Magnetic Field, Solar X-Rays, Spectrum Analysis, Bremsstrahlung, Energy Spectra, Magnetic Flux, Stellar Models

Scientific paper

The solar flare of July 14, 1980, is characterized on the basis of H-alpha observations obtained at Yunnan Observatory and X-ray data from the SMM satellite. The data are presented in graphs, maps, tables, and diagrams. It is found that the hard and soft X-ray bursts are produced by high-energy thermal electrons accelerated in the current sheet and by bremsstrahlung (of high-temperature sheet plasma and of nonthermal electrons), respectively. The relative positions of the H-alpha and X-ray events are shown to be consistent with the emerging-magnetic-flux theory of flare processes.

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