BCS Spectra from Flares on 6TH September 1992

Details BCS Spectra from Flares on 6TH September 1992 BCS Spectra from Flares on 6TH September 1992

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994kofu.symp..191k&link_type=abstract

In: Proceedings of Kofu Symposium, Kofu, Japan, Sept. 6-10, 1993, p.191-194.

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Scientific paper

We have studied time evolution of BCS spectra of He - like S XV, Ca XIX and Fe XXV ions observed by the Yohkoh satellite for two flares on 6th September 1992 at 05:05 (M2.4 class) and 08:59(M3.3 class). Electron temperatures of S XV, Ca XIX and Fe XXV ions are derived through synthetic spectra. Apparent ion temperatures are derived from the line width of S XV and Ca XIX spectra. The blue shifted components in the rising phase are separated from the main component in Ca XIX spectra. The emission measures and other parameters derived from the spectra are compared with HXT and radio data. The ion ratios derived from the ratios of line intensities are studied relating to the ionization equilibrium.

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