Monitoring of Pc3 pulsations in solar wind and at Earth by interplanetary magnetic field

Details Monitoring of Pc3 pulsations in solar wind and at Earth by interplanetary magnetic field Monitoring of Pc3 pulsations in solar wind and at Earth by interplanetary magnetic field

Nov 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987rpsct...2...58b&link_type=abstract

In its JPRS Report: Science and Technology. USSR: Space p 58 (SEE N88-16063 08-42) Transl. into ENGLISH from Geomagnetizm i Aero

Physics

Geomagnetic Micropulsations, Interplanetary Magnetic Fields, Shock Fronts, Solar Terrestrial Interactions, Solar Wind, Earth Surface, Field Strength, Periodic Variations, Statistical Analysis

Scientific paper

A significant statistical difference is found in Pc3 pulsations observed before the bow shock front and on the Earth surface. The properties were found to conform only for pulsations on the Earth surface and waves excited in the solar wind in the subsolar region of the shock front in the 9 to 13 LT range. The linear dimensions of this region were determined and found to coincide with an extended region of diffuse ion generation on the shock front.

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