On the rotation of large-scale background fields in the 21st cycle of solar activity

Details On the rotation of large-scale background fields in the 21st cycle of solar activity On the rotation of large-scale background fields in the 21st cycle of solar activity

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992soph..138...23m&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 138, March 1992, p. 23-33.

Physics

11

Magnetic Field Inversions, Solar Activity, Solar Cycles, Solar Magnetic Field, H Alpha Line, Magnetic Dipoles, Solar Rotation

Scientific paper

The peculiarities of the large-scale organization of the background magnetic fields (BMFs) of the sun were investigated with special attention given to the variations of the BMF organization over the solar activity cycle. It was found that the lifetimes of the stable structures of the BMF were comparable with the cycle duration. It is suggested that processes with such large typical space-time scales are a global phenomenon and cover the entire convection zone of the sun.

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