Response of the DCF field to variations of the dynamic pressure of the solar wind

Details Response of the DCF field to variations of the dynamic pressure of the solar wind Response of the DCF field to variations of the dynamic pressure of the solar wind

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ge%26ae..29..664z&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 29, July-Aug. 1989, p. 664, 665. In Russian.

Computer Science

Numerical Analysis

Dynamic Pressure, Magnetopause, Pressure Oscillations, Solar Wind, Dynamic Response, Numerical Analysis, Pressure Gradients

Scientific paper

The relationship between increases of the Dst field over 1 hr at a relatively quiet level and corresponding variations in the dynamic pressure of the solar wind is examined on the basis of mean hourly values of the Dst index and solar-wind parameters. It is shown that the proportionality factor between these parameters is not constant, but decreases as the dynamic-pressure gradient increases.

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