On the geomagnetic response to high-speed solar-wind streams

Details On the geomagnetic response to high-speed solar-wind streams On the geomagnetic response to high-speed solar-wind streams

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988angeo...6..627b&link_type=abstract

Annales Geophysicae (ISSN 0980-8752), vol. 6, Dec. 1988, p. 627-634.

Physics

10

Coronal Holes, Geomagnetism, Solar Terrestrial Interactions, Solar Wind Velocity, Space Plasmas, Hysteresis, Kp Index, Plasma Density, Plasma Temperature, Solar Activity Effects

Scientific paper

The present investigation of geomagnetic response on a 24-hr scale to several well-identified quasi-stationary solar wing macrostructures over the 1965-1974 period groups the 60 high-speed solar wind streams originating in coronal holes into three classes, according to duration. For each class, the average 24-hr profiles of the interplanetary parameters and geomagnetic indices are obtained and evaluated for statistical reliability by means of a two-way variance analysis. The time-dependence of the geomagnetic index values on a single interplanetary parameter exhibits hysteresislike behavior due to the different stages of the geomagnetic perturbation development.

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