Reorganization of the solar corona following a C4.7 flare

Details Reorganization of the solar corona following a C4.7 flare Reorganization of the solar corona following a C4.7 flare

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997adspr..19.1883v&link_type=abstract

Advances in Space Research, vol. 19, p. 1883

Physics

5

Solar Corona, X Ray Imagery, Solar Flares, Coronal Loops, Solar Radio Bursts, Magnetic Field Reconnection, Two Dimensional Models, Brightness Distribution, Solar Magnetic Field, Magnetic Field Configurations

Scientific paper

X-ray images, multifrequency 2D observations and magnetogram data are used to study a C4.7 long-duration flare, seen near the solar equator, that began with the expansion of spectacular twisted loops and was followed by sporadic radio bursts and two remote X-ray brightenings on opposite hemispheres of the sun. The timing and location of these events, combined with the overall magnetic configuration, furnish evidence for a large-scale magnetic reconnection between the expanding twisted loops and large overlying loops.

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