Solar cycle variations in IMF intensity

Details Solar cycle variations in IMF intensity Solar cycle variations in IMF intensity

Oct 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979jgr....84.5938k&link_type=abstract

Journal of Geophysical Research, vol. 84, Oct. 1, 1979, p. 5938-5940.

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16

Interplanetary Magnetic Fields, Magnetic Flux, Solar Cycles, Satellite Observation, Solar Activity Effects, Solar Wind

Scientific paper

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 centered 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.

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