Causes and Effects of Superstorms Associated With the Magnetic Field in the Corona and the Heliosphere

Details Causes and Effects of Superstorms Associated With the Magnetic Field in the Corona and the Heliosphere Causes and Effects of Superstorms Associated With the Magnetic Field in the Corona and the Heliosphere

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004agufmsa41b..01h&link_type=abstract

American Geophysical Union, Fall Meeting 2004, abstract #SA41B-01

Physics

7524 Magnetic Fields, 2134 Interplanetary Magnetic Fields

Scientific paper

The emergence of three strong active regions late last fall altered the configuration of the solar corona and launched major disturbances that were felt throughout the heliosphere. The effects of the superstorms were dramatic and far reaching, but did they permanently disrupt the morphology of the heliospheric magnetic field? The role such major active regions play in the solar-cycle evolution of coronal structure and the location of the heliospheric current sheet will be investigated.

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