Coronal holes and the large-scale solar magnetic field

Details Coronal holes and the large-scale solar magnetic field Coronal holes and the large-scale solar magnetic field

Jul 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....59...73s&link_type=abstract

Astronomy and Astrophysics, vol. 59, no. 1, July 1977, p. 73-78.

Astronomy and Astrophysics

Astronomy

3

Dynamo Theory, Magnetic Field Configurations, Solar Corona, Solar Magnetic Field, Harmonic Analysis, Solar Physics, Spaceborne Astronomy, Spherical Harmonics, Turbulence Effects

Scientific paper

The spherical harmonic coefficients of the solar magnetic field are used to divide the observed field into 'normal modes', the independent solutions of the turbulent solar dynamo. The modes S 1 and S 3, which are symmetric with respect to the equator and have two and six magnetic sectors, respectively, were dominant during 1973. It is suggested that these two modes essentially controlled the position of the three most conspicuous coronal holes observed during the Skylab period.

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