Relationship between the geomagnetic disturbance level, high-speed solar wind streams, and coronal holes

Details Relationship between the geomagnetic disturbance level, high-speed solar wind streams, and coronal holes Relationship between the geomagnetic disturbance level, high-speed solar wind streams, and coronal holes

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ge%26ae..23..968o&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 23, Nov.-Dec. 1983, p. 968-971. In Russian.

Physics

Coronal Holes, Geomagnetism, Magnetic Disturbances, Solar Terrestrial Interactions, Solar Wind, Solar Corona, Solar Corpuscular Radiation

Scientific paper

The relationship between coronal holes, high-speed solar wind streams, and the geomagnetic disturbance level is examined on the basis of available data. It is shown that magnetic disturbances near the solar minimum are due to high-speed corpuscular streams associated with coronal holes. The character of the magnetic disturbance depends on stream parameters, particularly the maximum stream velocity.

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