How does the magnetic field of an usual active region develop?

Details How does the magnetic field of an usual active region develop? How does the magnetic field of an usual active region develop?

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983baicz..34..219b&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 34, July 1983, p. 219-229.

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9

Magnetic Field Configurations, Solar Activity, Solar Magnetic Field, Sunspot Cycle, Gyromagnetism, Lines Of Force, Magnetoactivity

Scientific paper

The existence of a regular pattern of development in a single solar active region's magnetic field, at least in some of its evolutionary stages, and the pattern's dependence on the heliographic position or on the phase of the solar activity cycle is investigated using about 36 sets of 'qualitative' maps of the longitudinal field distribution. Evidence of the influence of solar differential rotation on the shape of the magnetic field and of other dynamical forces arising from the flow of photospheric matter around the active region is obtained. It is shown that magnetic lines of force in the active region's 'center' form a subsystem which is lower than and perpendicular to the main system of magnetic lines of force joining the leading and following main spots.

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