Topology and dynamics of the Sun's magnetic field

Details Topology and dynamics of the Sun's magnetic field Topology and dynamics of the Sun's magnetic field

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..679..242g&link_type=abstract

SOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conference. AIP Conference Proceedings, Volume 679, pp. 242-2

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Particle Emission, Solar Wind, Electric And Magnetic Fields, Solar Magnetism, Diameter, Rotation, And Mass, Solar Wind Plasma, Sources Of Solar Wind

Scientific paper

The distribution of the magnetic field on the solar surface from 1975 up to 2002 is analyzed using the observations taken on the WSO observatory, revealing remarkable latitudinal zonal structure in both the northern and southern hemisphere. A preliminary model combining the dipole, quadrupole, octupole and other components for the longitude distribution is discussed. The active longitude problem has been investigated. The new active regions seem to appear with the sideral period of about 25.0 +/- .1 days, corresponding to the solar rotation rate at 10 degree latitude at the 0.85+/-.03 solar radii.

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