Large-scale transport of magnetic flux on the Sun and flare productivity

Details Large-scale transport of magnetic flux on the Sun and flare productivity Large-scale transport of magnetic flux on the Sun and flare productivity

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.477...73a&link_type=abstract

In: Proceedings of the Second Solar Cycle and Space Weather Euroconference, 24 - 29 September 2001, Vico Equense, Italy. Editor:

Computer Science

Solar Magnetic Fields, Solar Flares

Scientific paper

Horizontal transport of the large-scale magnetic field during the last three solar activity cycles was studied. The specific displacement of the magnetic regions was followed and the horizontal velocity field was inferred. A non-homogeneous transport of the magnetic flux over the solar surface, superposed on the global differential rotation and meridional circulation was discovered. Large-scale velocities with the axially symmetric component and also with the large-scale non-axially symmetric component of the horizontal velocity field varies during the 11-year activity cycle. A spatial distribution of the available magnetic energy was computed and the relationship with the flare productivity was found.

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