Dual-peak solar cycle distribution of intense geomagnetic storms

Details Dual-peak solar cycle distribution of intense geomagnetic storms Dual-peak solar cycle distribution of intense geomagnetic storms

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990p%26ss...38..181g&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 38, Feb. 1990, p. 181-187.

Other

59

Geomagnetism, Magnetic Storms, Solar Cycles, Distribution (Property), Interplanetary Magnetic Fields

Scientific paper

This paper studies the features of the solar cycle distribution of intense storms (Dst) during cycles 20 and 21 (1965-1985). For these cycles, the distribution of intense storms (including moderate events for this time interval) in terms of Dst values below -50 nT, showed a dual-peak distribution, providing evidence for another enhancement of the intense storm distribution at the late ascending phase of the cycle. The origin of the dual-peak distribution of intense storms is associated with a similar dual-peak distribution obtained for large-amplitude and long-duration values of the negative Bz component of the IMF, computed for the interval 1970-1981.

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