A Problem with the Global Plasmasphere Ionosphere Density (GPID) Model

Physics

Scientific paper

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2753 Numerical Modeling, 2760 Plasma Convection, 2768 Plasmasphere, 2788 Storms And Substorms

Scientific paper

The Global Plasmaspheric Ionospheric Density (GPID) model has been developed to simulate the cold, dense plasma that surrounds the Earth out to a distance of some four Earth radii. This highly dynamic region, located above the ionosphere, is called the plasmasphere. One of the main characteristics of the plasmasphere is the plasmapause, where the plasma density drops by around an order of magnitude over a short spatial distance. GPID models the formation of the plasmapause using a new empirical method, which accurately reproduces the experimental observed location of the plasmapause across all geomagnetic storm conditions. However, no physical explanation has yet been found to account for this agreement. This presentation will describe the approach used by GPID to model the formation of the plasmapause and attempts to find a physical reason for the success of this method.

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