The relationship between filament appearance and active-region magnetic-field changes

Details The relationship between filament appearance and active-region magnetic-field changes The relationship between filament appearance and active-region magnetic-field changes

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987azh....64..841m&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 64, July-Aug. 1987, p. 841-849. In Russian.

Statistics

Computation

3

Solar Activity, Solar Magnetic Field, Solar Prominences, Computational Astrophysics, Magnetic Field Configurations

Scientific paper

A study has been made of the dynamical behaviour of the longitudinal magnetic field gradient distribution in the nearest vicinity of the polarity inversion line. It is shown that a necessary condition for a filament to appear within an active region is the displacement of grad H∥ distribution toward lower gradient values as well as the homogeneity of the polarity inversion line with respect to the magnetic field. Also, maximum values of grad H∥ must not exceed a certain limiting value.

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