A comprehensive analysis of the loop prominence of 1981 April 27

Details A comprehensive analysis of the loop prominence of 1981 April 27 A comprehensive analysis of the loop prominence of 1981 April 27

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985cha%26a...9..226c&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 9, Issue 3, p. 226-231.

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

We make comprehensive analysis of morphological tracings and positional measurements of Hα images, white-light sunspot photographs and chromosphere velocity field, obtained at Yunnan Observatory, and hard X-ray images obtained by the Hinotori satellite, of the loop prominence of 1981 April 27. It seems likely that the observed loop is the projection of a post-flare loop system, and the associated flare occurred on the rear side of the solar disk. A two-ribbon flare such as in the Kopp-Pneuman model can satisfactorily explain all the observed features. The occurrence of such a flare seems likely from the evidence given by the data.

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