The structure of the magnetic fields of active regions

Details The structure of the magnetic fields of active regions The structure of the magnetic fields of active regions

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989azh....66.1271k&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 66, Nov.-Dec. 1989, p. 1271-1282. In Russian.

Physics

3

Solar Activity, Solar Magnetic Field, Chromosphere, Field Theory (Physics), Magnetic Field Configurations, Plasma Pressure, Solar Prominences

Scientific paper

The inverse problem concerning the magnetic-field structure of a solar active region is solved. Tangential-field directions prescribed by fibril orientation are used as the initial data. The problem is shown to have a solution determined up to a factor common to the total distribution, both in terms of the potential approximation and in the case of a force-free field. Examples of field calculations for individual chromospheric structures are presented.

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