Geomagnetic activity and Hale sector boundaries

Details Geomagnetic activity and Hale sector boundaries Geomagnetic activity and Hale sector boundaries

Feb 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980stin...8022222l&link_type=abstract

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Computer Science

Polarization Characteristics, Solar Activity, Solar Magnetic Field, Equinoxes, Northern Hemisphere, Polarity, Seasons, Solar Wind Velocity, Southern Hemisphere

Scientific paper

The variation of the geomagnetic activity index Ap at the IMF sector boundaries (+ to - and - to +) is examined for three solar cycles, separating data into vernal and autumnal equinoxes. It is found that a reported increase in Ap as an effect of a Hale boundary can be better attributed to the occurrence of a negative IMF Bz component in the geocentric solar magnetospheric coordinate system and to the occurrence of high speed solar wind streams.

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