The nature of rotation rates of the sector structure of the solar magnetic field.

Details The nature of rotation rates of the sector structure of the solar magnetic field. The nature of rotation rates of the sector structure of the solar magnetic field.

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989bsold..11..104m&link_type=abstract

Byulletin Solnechnye Dannye Akademie Nauk USSR, No. 1989/11, p. 104 - 111

Physics

Solar Magnetic Fields: Sector Structure, Interplanetary Magnetic Field: Sector Structure

Scientific paper

It is shown that the observed dominant rotation periods of the sector structure of the interplanetary magnetic field are associated with the distribution of the generating source of the magnetic field in the convective zone. The source is due to interaction of differential rotation and average helicity at different layers of the convective zone.

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