Flare-related relaxation of magnetic shear as observed with the Soft X-ray Telescope of YOHKOH and with vector magnetographs

Details Flare-related relaxation of magnetic shear as observed with the Soft X-ray Telescope of YOHKOH and with vector magnetographs Flare-related relaxation of magnetic shear as observed with the Soft X-ray Telescope of YOHKOH and with vector magnetographs

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992pasj...44l.123s&link_type=abstract

PASJ: Publications of the Astronomical Society of Japan (ISSN 0004-6264), vol. 44, no. 5, p. L123-L127.

Astronomy and Astrophysics

Astronomy

42

Magnetic Field Configurations, Magnetic Signatures, Solar Flares, Solar Magnetic Field, X Ray Telescopes, Japanese Spacecraft, Solar Corona

Scientific paper

The Soft X-ray Telescope of Yohkoh observed an M-class flare on 1992
February 6. As the flare progressed, an initially sheared coronal loop
structure was seen to evolve toward a relaxed magnetic configuration. In
association with this evolution, the vector magnetograph observations
detected a decrease in the electric currents.

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