Solar wind variations as a source of short-term magnetic field perturbations in the dayside magnetosphere.

Details Solar wind variations as a source of short-term magnetic field perturbations in the dayside magnetosphere. Solar wind variations as a source of short-term magnetic field perturbations in the dayside magnetosphere.

Jun 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996kosis..34..248s&link_type=abstract

Kosmicheskie Issledovaniia, Tom 34, No. 3, p. 248 - 263

Computer Science

4

Solar Wind: Geomagnetic Field, Solar Wind: Variations, Solar Wind: Interplanetary Magnetic Field

Scientific paper

Short variations (about several minutes) in the dayside magnetospheric magnetic field measured by the GOES-5 and GOES-6 geosynchronous satellites were compared with simultaneous observations of the solar wind plasma and magnetic field aboard the Prognoz-10 and IMP-8 satellites. The results indicate that more than half of the events were caused by dynamic pressure variations in the solar wind. A considerable portion of the events can be associated with fluctuations in the orientation of the interplanetary magnetic field, influencing the foreshock plasma pressure.

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