Solar-wind disturbances and the solar wind-magnetosphere energy coupling function

Details Solar-wind disturbances and the solar wind-magnetosphere energy coupling function Solar-wind disturbances and the solar wind-magnetosphere energy coupling function

Feb 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ssrv...34..173a&link_type=abstract

(COSPAR, IAU, IUGG, IUPAP, and URSI, International Symposium on Progress in Solar-Terrestrial Physics, 5th, Ottawa, Canada, May

Physics

15

Dynamo Theory, Earth Magnetosphere, Magnetic Disturbances, Solar Activity Effects, Solar Terrestrial Interactions, Solar Wind, Auroras, Energy Dissipation, Geomagnetism, Ionospheric Currents, Solar Corona, Solar Flares

Scientific paper

An examination of the results of recent studies of solar wind-magnetosphere interaction in terms of the input-output relationship indicates that the magnetosphere is primarily a directly driven system in which this interaction constitutes a dynamo. Attention is given to the chain of processes by which the dynamo-generated power is transmitted to the polar ionosphere, leading to auroral phenomena. The present analyses suggest that the solar activity-magnetosphere disturbance relationship should be considered to be a single process sequence, involving the solar wind generation, sunspot, solar wind-magnetosphere, and auroral dynamos. The importance of a study of the causes of the north-south solar wind magnetic field component, including its time variations, is emphasized as a missing link between solar activity and magnetospheric disturbances.

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