HR: 1340h
AN: SH13A-1145    [Abstracts]
TI: Longitudinal Structure of Solar cycle 23
AU: * Benevolenskaya, E E
EM: elena@quake.stanford.edu
AF: Benevolenskaya, E.E., 455 via Palou Stanford University, Stanford, CA 94305 United States
AB: The non-axisymmetrical pattern of solar activity during the 1996-2004 years has been studied using the SOHO/MDI, SOHO/EIT and WSO data. These data reveal close correlation between the non-axisymmetrical magnetic field and coronal structures. The long-lived complexees of solar activity have clusterred in preferred (active) longitudes and have shown an impulsive nature of the solar cycle. The nature of active longitudes or active longotudinal zones is discussed.
DE: 7509 Corona
DE: 7524 Magnetic fields
DE: 7536 Solar activity cycle (2162)
DE: 7549 Ultraviolet emissions
SC: SPA-Solar and Heliospheric Physics [SH]
MN: 2004 AGU Fall Meeting