Dynamical problems in H-alpha flare loops on solar disc

Details Dynamical problems in H-alpha flare loops on solar disc Dynamical problems in H-alpha flare loops on solar disc

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992scsmp..35..463x&link_type=abstract

Science in China, Series A - Mathematics, Physics, Astronomy and Technological Sciences (ISSN 1001-6511), vol. 35, no. 4, April

Mathematics

Logic

H Alpha Line, Plasma Dynamics, Solar Flares, Solar Magnetic Field, Solar Spectra

Scientific paper

The dynamical process in H-alpha flare loops on solar disk is quantitatively discussed by using the observed data of the two-ribbon flare on May 16, 1981, taken with the H-alpha spectra-spectroheliograph and H-alpha chromospheric telescope at Yunnan Observatory, Kunming, PRC, as well as the X-ray data on the same flare from satellite HINOTORI. It is found that matter at the top of the H-alpha flare loops has initial velocity of several hundred km/s, and the falling velocity of matter within the loops decelerates. These dynamical problems are thought to be related to the physical mechanism of flare loops.

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