Spatial variations of background magnetic field polarity distribution on the sun

Details Spatial variations of background magnetic field polarity distribution on the sun Spatial variations of background magnetic field polarity distribution on the sun

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..109..233p&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 109, no. 2, 1987, p. 233-245.

Physics

1

Background Radiation, Interplanetary Magnetic Fields, Polarity, Solar Magnetic Field, Solar Rotation, H Alpha Line, Interplanetary Medium, Solar Activity

Scientific paper

Based on an analysis of the latitude and longitude regularities in the distribution of the sign of the background magnetic field (BMF) on the solar surface for 14 years (1969-1982), a classification of BMF distributions in the form of synoptic maps is proposed. The properties of the structure, interaction and rotation of the low- and high-latitude magnetic field details, taken together, provide a qualitative scheme for the formation and variation of the longitude-regular (sectoral) BMF distribution in the latitude range 40 deg S-40 deg N.

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