Computer Science
Scientific paper
Mar 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.477..405o&link_type=abstract
In: Proceedings of the Second Solar Cycle and Space Weather Euroconference, 24 - 29 September 2001, Vico Equense, Italy. Editor:
Computer Science
Interplanetary Magnetic Field, Solar Magnetic Field
Scientific paper
It is shown that the sign and amplitude of the annual mean Bz component
of the interplanetary magnetic field (IMF) conforms with the structure
of the large-scale solar magnetic field at the poles. Therefore, the
recurrence of geomagnetic activity is best pronounced in the cycles when
the polar field in the Sun is positive.
Golyshev S.
Levitin A. E.
Obridko Vladimir N.
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