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Chen et al. 1995
Chen, J., Slinker, S., Fedder, J.A. and Lyon, J.G. (1995). Simulation of geomagnetic storms during the passage of magnetic clouds. Geophysical Research Letters 22: doi: 10.1029/95GL01520. issn: 0094-8276.

The response of the Earth's magnetosphere to the passage of interplanetary magnetic clouds is simulated using a three-dimensional magnetohydrodynamic (MHD) model. The input solar wind condition is given by the magnetic field, particle density, and plasma flow calculated from a model magnetic cloud. The cross-polar potential (&PHgr;p), Joule heating and electron energy precipitation into the polar cap are calculated. Synthetic magnetic indices Dst* and AE* are defined to serve as surrogates for the usual Dst and AE indices, respectively. We demonstrate that &PHgr;2p provides a good predictor of the energy deposition into the ionosphere during storm conditions and that Dst* and AE* behave qualitatively similarly to Dst and AE. ¿ American Geophysical Union 1995

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Abstract

Keywords
Magnetospheric Physics, Solar wind/magnetosphere interactions, Magnetospheric Physics, Storms and substorms, Magnetospheric Physics, Magnetosphere/ionosphere interactions, Space Plasma Physics, Numerical simulation studies
Journal
Geophysical Research Letters
http://www.agu.org/journals/gl/
Publisher
American Geophysical Union
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