Latitude-time distribution of 3 types of magnetic field activity in the global solar cycle

Details Latitude-time distribution of 3 types of magnetic field activity in the global solar cycle Latitude-time distribution of 3 types of magnetic field activity in the global solar cycle

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992soph..141..381c&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 141, no. 2, p. 381-390.

Physics

21

Geomagnetism, H Alpha Line, Solar Activity, Solar Cycles, Solar Magnetic Field, Angular Momentum, Solar Atmosphere, Sunspots

Scientific paper

Large-scale solar activity is considered as a manifestation of 3 types of magnetic field activity which is demonstrated in the 22-year cycle: (a) of small-scale flux emergence (polar faculae at latitudes greater than 40 deg); (b) of somewhat larger scale flux emergence (sunspots at latitudes less than 40 deg; and (c) of the global magnetic neutral lines at all latitudes. The migration (poleward or equatorward) of the place of birth and/or of the phenomena themselves of these three types of manifestation of magnetic field is discussed. The poleward migration of the global field is explained in a phenomenological way.

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