HR: 1330h
AN: SH42B-0531    [PDF]
TI: Polar Coronal and Magnetic Activity in Solar Cycle 23
AU: * Benevolenskaya, E E
EM: elena@quake.stanford.edu
AF: Stanford University, 455 via Palou, Stanford, CA 94305 United States
AB: 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.
DE: 2162 Solar cycle variations (7536)
SC: SPA - Solar and Heliospheric Physics [SH]
MN: 2003 Fall Meeting