Recent work on the IMF control of geomagnetic activity is reviewed. The goal is to quantitatively express the temporal relation between the solar wind input and the ionospheric output from the magnetospheric system. Linear prediction filtering was used which treats the magnetosphere as a black box characterized by an impulse response. It is shown that an average impulse response can account for only about 40 percent of the variance in the AL index.
IMF control of geomagnetic activity
Advances in Space Research ; 8 , 9-10
1988-01-01
Sonstige
Keine Angabe
Englisch
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