The flare as a result of cross-interaction of loops - Causal relationship with a prominence

Details The flare as a result of cross-interaction of loops - Causal relationship with a prominence The flare as a result of cross-interaction of loops - Causal relationship with a prominence

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..127..253u&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 127, June 1990, p. 253-265.

Physics

6

Coronal Loops, Magnetic Field Configurations, Solar Flares, Solar Magnetic Field, Solar Prominences, Magnetic Field Reconnection, Magnetohydrodynamic Stability, Photosphere

Scientific paper

The helical bend of magnetic loops of an emerging arcade leads to their cross-interaction. If the longitudinal magnetic field and longitudinal electric field in the arcade loops are antiparallel, then a rapid formation of a horizontal magnetic filament is possible. Its subsequent decay can have a flare character. In the opposite case (B-parallel i) greater than the magnetic filament cannot form rapidly.

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