Dynamical problems in Hα flare loops on the solar disc.

Details Dynamical problems in Hα flare loops on the solar disc. Dynamical problems in Hα flare loops on the solar disc.

Apr 1992

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

Science in China, Series A, Vol. 35, No. 4, p. 463 - 471

Physics

Scientific paper

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

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