Effect of the interplanetary secondary rarefaction waves on the geomagnetic field

Details Effect of the interplanetary secondary rarefaction waves on the geomagnetic field Effect of the interplanetary secondary rarefaction waves on the geomagnetic field

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ge%26ae..49..733g&link_type=abstract

Geomagnetism and Aeronomy, Volume 49, Issue 6, pp.733-740

Physics

Scientific paper

Based on the WIND and GOES satellite data on the solar wind and IMF parameters and the data on the surface magnetic field, it has been indicated that the secondary MHD rarefaction wave can affect the geomagnetic field during a storm sudden commencement (SSC) event. The secondary rarefaction wave originates in the magnetosheath when the shock wave interacts with the Earth's magnetosphere.

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