Analysis of geomagnetic activity with regard to different solar causes

Details Analysis of geomagnetic activity with regard to different solar causes Analysis of geomagnetic activity with regard to different solar causes

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989angeo...7..311c&link_type=abstract

Annales Geophysicae (ISSN 0980-8752), vol. 7, June 1989, p. 311-317.

Physics

8

Geomagnetism, Solar Activity Effects, Solar Terrestrial Interactions, Annual Variations, Coronal Holes, Solar Flares, Solar Wind, Sunspot Cycle

Scientific paper

Geomagnetic activity between 1973-80 is divided into a basic part generated by slow solar wind and parts generated by coronal holes and flares. Recurrence tendency and semiannual variation are examined in these parts. Coronal holes are shown to produce the main part of geomagnetic activity and the semiannual wave. Recurrence tendency is completely determined by coronal holes, in particular the 27-day period in 1973-75, and the 28-period in 1977.

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