Detailed comparison between H-alpha and YOHKOH soft X-ray images of a confined two-ribbon flare

Details Detailed comparison between H-alpha and YOHKOH soft X-ray images of a confined two-ribbon flare Detailed comparison between H-alpha and YOHKOH soft X-ray images of a confined two-ribbon flare

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992pasj...44l.129k&link_type=abstract

PASJ: Publications of the Astronomical Society of Japan (ISSN 0004-6264), vol. 44, no. 5, p. L129-L133.

Astronomy and Astrophysics

Astronomy

5

Coronal Loops, H Alpha Line, Solar Flares, Solar X-Rays, Spaceborne Astronomy, Japanese Spacecraft, Solar Magnetic Field, X Ray Imagery

Scientific paper

The spatial and temporal relationships between soft X-ray loops and H-alpha flare Kernels were studied for the 1B (M2.6) flare of December 5, 1991. Most of flare energy was released inside three soft X-ray loops whose footpoints were bright as H-alpha Kernels. We suggest that the interaction among preexisting or emerging magnetic loops is essential for the successive energy release in a confined two-ribbon flare.

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