A method for evaluating the total magnetospheric energy output independently of the epsilon parameter

Details A method for evaluating the total magnetospheric energy output independently of the epsilon parameter A method for evaluating the total magnetospheric energy output independently of the epsilon parameter

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987georl..14.1183v&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 14, Dec. 1987, p. 1183-1186.

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16

Earth Magnetosphere, Energy Distribution, Solar Terrestrial Interactions, Ring Currents, Solar Wind

Scientific paper

A method for calculating the magnetospheric energy output parameter U(T) that is completely independent of the epsilon parameter or any analogous solar wind quantity is described. This method may be used to generate time series of U(T) values for comparison with epsilon or any other assumed form of the solar wind energy input function. This would allow a test of epsilon = U(T) or similar hypotheses without encountering the problems of circular reasoning or artificial interdependence of variables.

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