Meridional Drift of the Large-Scale Solar Magnetic Fields in Different Phases of Solar Activity

Details Meridional Drift of the Large-Scale Solar Magnetic Fields in Different Phases of Solar Activity Meridional Drift of the Large-Scale Solar Magnetic Fields in Different Phases of Solar Activity

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996soph..163..241l&link_type=abstract

Solar Physics, Volume 163, Issue 2, pp.241-247

Physics

10

Scientific paper

An analysis is made of mean latitudinal profiles of the meridional drift of the large-scale solar magnetic fields. The previously detected equatorward migration of the drift pattern in the course of a cycle is confirmed. Evidence for the existence of a near-equatorial narrow zone ±7° with an equatorward drift with a rate of about 1 m s-1 is obtained. The study revealed a significant difference in shapes and variations of average drift profiles for the large-scale magnetic field and small magnetic features (Komm, Howard, and Harvey, 1993).

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