Semiannual and solar-cycle variation of sector structure

Details Semiannual and solar-cycle variation of sector structure Semiannual and solar-cycle variation of sector structure

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974georl...1..295s&link_type=abstract

Geophysical Research Letters, vol. 1, Nov. 1974, p. 295-297.

Physics

4

Annual Variations, Interplanetary Magnetic Fields, Solar Cycles, Solar Rotation, Geomagnetism, Magnetic Variations, Polarity, Satellite Observation, Solar Activity Effects

Scientific paper

The complexity of the interplanetary magnetic-field polarity pattern shows a semiannual variation, with more sectors per solar rotation in May and June, and again in November and December, times when the earth is close to the sun's equatorial plane. Complexity varies also through the solar activity cycle, in a manner consistent with contribution to the interplanetary field from both the polar field and long-lived, large-scale fields related to active regions.

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