Magnetospheric storm dynamics in terms of energy output rate

Details Magnetospheric storm dynamics in terms of energy output rate Magnetospheric storm dynamics in terms of energy output rate

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992p%26ss...40..581p&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 40, no. 4, April 1992, p. 581-588.

Physics

20

Earth Magnetosphere, Energy Transfer, Magnetic Storms, Solar Terrestrial Interactions, Solar Wind, Energy Dissipation, Ring Currents

Scientific paper

Using hourly values of both the global magnetospheric disturbance characteristic DR, and AE index of auroral ionospheric currents during magnetic storm intervals, the energy output rate dynamics is evaluated for a magnetic storm main/recovery phase and a whole storm interval. The magnetospheric response to the solar wind energy input rate under varying interplanetary and magnetospheric conditions is considered from the temporal variability point of view. As far as quantitative characteristics of energy output rate are concerned, the time dependence pattern of the ring current decay parameter is shown to be fairly important.

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