Polar Coronal and Magnetic Activity in Solar Cycle 23

Details Polar Coronal and Magnetic Activity in Solar Cycle 23 Polar Coronal and Magnetic Activity in Solar Cycle 23

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003agufmsh42b0531b&link_type=abstract

American Geophysical Union, Fall Meeting 2003, abstract #SH42B-0531

Physics

2162 Solar Cycle Variations (7536)

Scientific paper

The results of investigation of the polar coronal activity using EUV data from SOHO/EIT and its relations to the magnetic activity studied from SOHO/MDI for 1996-2002 are presented. The observations of formation and evolution of polar coronal structures during the current activity cycle reveal close correlations between eruptive magnetic flux, coronal topology and changes of the global magnetic field, which have interesting implications for understanding the mechanism of the solar cycle.

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