Dynamics of open solar magnetic fields, active longitudes, and near earth disturbances

Details Dynamics of open solar magnetic fields, active longitudes, and near earth disturbances Dynamics of open solar magnetic fields, active longitudes, and near earth disturbances

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.506..141i&link_type=abstract

In: Solar variability: from core to outer frontiers. The 10th European Solar Physics Meeting, 9 - 14 September 2002, Prague, Cze

Physics

1

Solar Magnetic Fields, Solar-Terrestrial Relations, Dynamics

Scientific paper

Open magnetic field lines in the solar corona are calculated in order to study their relationship to solar activity and near Earth disturbances in 2000. Slow, rotation by rotation, dynamics of photospheric regions with open fields show a correlation with generating and decay of active complexes located at longitudes 280-360 degrees, and with the series of the near Earth recurrent extra storms on May 24, July 15, August 12, and October 5.

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