Structure of solar wind velocity along the HCS and related geomagnetic field variations

Details Structure of solar wind velocity along the HCS and related geomagnetic field variations Structure of solar wind velocity along the HCS and related geomagnetic field variations

Aug 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ijrsp..22..273b&link_type=abstract

Indian Journal of Radio & Space Physics (ISSN 0367-8393), vol. 22, no. 4, p. 273-276

Physics

Space Physics

1

Azimuth, Current Sheets, Geomagnetism, Interplanetary Magnetic Fields, Solar Wind, Solar Wind Velocity, Correlation, Solar Longitude, Variations

Scientific paper

Azimuthal variation of solar wind velocity in the range 300-450 km/s has been found to exist along the heliospheric current sheet (HCS) during 1972-1977. The possibility of using the Ap index (when the earth goes through and IMF sector boundary crossing) to study the azimuthal structure of solar wind has been analyzed. The longitudinal variation of the Ap index terms of Carrington longitude is found to be similar to that of the solar wind velocity variation.

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