Heliospheric electrojets: their structure and magnetospheric impacts

Details Heliospheric electrojets: their structure and magnetospheric impacts Heliospheric electrojets: their structure and magnetospheric impacts

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.506...37v&link_type=abstract

In: Solar variability: from core to outer frontiers. The 10th European Solar Physics Meeting, 9 - 14 September 2002, Prague, Cze

Physics

Planetary Magnetic Fields, Solar Wind, Solar Magnetic Fields

Scientific paper

The planetary magnetospheres can intercept electric currents flowing in
the heliosphere. The strongest heliospheric currents - electrojets are
sufficient to produce appreciable geomagnetic perturbations in this way.
Corresponding estimates are presented.

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