Geomagnetic activity during minima of even and odd solar cycles

Details Geomagnetic activity during minima of even and odd solar cycles Geomagnetic activity during minima of even and odd solar cycles

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ge%26ae..33..137s&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 33, no. 1, p. 137, 138.

Computer Science

Earth Orbits, Magnetic Storms, Solar Activity Effects, Solar Terrestrial Interactions, Solar Wind, Magnetoactivity, Solar Cycles

Scientific paper

The cause of the observed increases in geomagnetic activity during solar activity minima following even solar cycles was investigated using results of an analysis of direct measurements of IMF parameters and of the solar wind velocity measurements for three latest solar activity cycles, together with results of studies of the modulation region geometry of the galactic cosmic rays. The results suggest that the observed phenomenon is caused by a higher solar wind velocity during even solar-activity cycles, rather than by the southward directed IMF component, as was suggested by Fel'dshtein et al. (1979).

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