Longitudinal Structure of Solar cycle 23

Details Longitudinal Structure of Solar cycle 23 Longitudinal Structure of Solar cycle 23

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004agufmsh13a1145b&link_type=abstract

American Geophysical Union, Fall Meeting 2004, abstract #SH13A-1145

Physics

7509 Corona, 7524 Magnetic Fields, 7536 Solar Activity Cycle (2162), 7549 Ultraviolet Emissions

Scientific paper

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.

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