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Solar cycle variations in IMF intensity

Journal Article · · J. Geophys. Res.; (United States)
Annual averages of logarithms of hourly interplanetary magnetic field (IMF) intensities, obtained from geocentric spacecraft between November 1963 and December 1977, reveal the following solar cycle variation. For 2--3 years at each solar minimum period, the IMF intensity is depressed by 10--15% relative to its mean value realized during a broad 9-year period contered at solar maximum. No systematic variations occur during this 9-year period. The solar minimum decrease, although small in relation to variations in some other solar wind parameters, is both statistically and physically significant.
Research Organization:
NASA/GSFC, Laboratory for Extraterrestrial Physics Greenbelt, MD 20771
OSTI ID:
5631335
Journal Information:
J. Geophys. Res.; (United States), Journal Name: J. Geophys. Res.; (United States) Vol. 84:A10; ISSN JGREA
Country of Publication:
United States
Language:
English

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