Erosion of the inner magnetosphere during geomagnetic storms

Using the empirical magnetic field model dependent on the <i>Dst</i> index and solar wind dynamic pressure, we calculated the behaviour of the contour <i>B</i> = <i>B<sub>s</sub></i> in the equatorial plane of the magnetosphere where <i>B<s...

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Bibliographic Details
Main Authors: E. Y. Feshchenko, Y. P. Maltsev
Format: Article
Language:English
Published: Copernicus Publications 1997-12-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/15/1532/1997/angeo-15-1532-1997.pdf