The morphology of 20 X 10 exp 6 K plasma in large non-impulsive solar flares

Details The morphology of 20 X 10 exp 6 K plasma in large non-impulsive solar flares The morphology of 20 X 10 exp 6 K plasma in large non-impulsive solar flares

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992pasj...44l..71a&link_type=abstract

PASJ: Publications of the Astronomical Society of Japan (ISSN 0004-6264), vol. 44, no. 5, p. L71-L75.

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76

Plasma Spectra, Solar Flares, X Ray Telescopes, Chromosphere, Japanese Spacecraft

Scientific paper

We have examined images of 10 flares observed by the Soft X-ray Telescope on-board the Yohkoh spacecraft. These images show that the hottest portion of the soft X-ray flare is located in compact regions that appear to be situated at the tops of loops. These compact regions form at, or shortly after, flare onset, and persist well into the decay phase of the flares. In some cases, the compact regions are only a few thousand kilometers in size and are small compared to the lengths of flaring loops. This is inconsistent with the smoother intensity distribution along the loops expected from models of chromospheric evaporation.

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