Solar cycle variations in IMF intensity

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

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979stin...7920959k&link_type=abstract

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Interplanetary Magnetic Fields, Magnetic Flux, Secular Variations, Solar Cycles, Autocorrelation, Data Reduction, Imp, Mariner 2 Space Probe

Scientific paper

Annual averages of logarithms of hourly interplanetary magnetic field intensities, obtained from geocentric spacecraft between November 1963 and December 1977, reveal the following solar cycle variation. For 2 to 3 years at each solar minimum period, the IMF intensity is depressed by 10-15 percent relative to its mean value realized during a broad nine-year period centered at solar maximum. No systematic variations occur during this nine-year period. The solar minimum decrease, although small relative to variations in some other solar wind parameters, is both statistically and physically significant.

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