Evidence for magnetic field rearrangement in a solar flare

Details Evidence for magnetic field rearrangement in a solar flare Evidence for magnetic field rearrangement in a solar flare

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...281..884z&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 281, June 15, 1984, p. 884, 885.

Astronomy and Astrophysics

Astrophysics

11

H Alpha Line, Solar Flares, Solar Magnetic Field, Chromosphere, Photosphere

Scientific paper

The author presents an example of the change in transverse magnetic field in the course of a solar flare. A filament consisting of sheared field lines along an inversion line of longitudinal field is replaced by a set of much shorter field transition arches across the inversion line. The eruption itself results from the invasion of the area by fields associated with a moving sunspot.

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