Analysis of the Simple Inner Magnetosphere Model

Details Analysis of the Simple Inner Magnetosphere Model Analysis of the Simple Inner Magnetosphere Model

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agufmsm53a1432m&link_type=abstract

American Geophysical Union, Fall Meeting 2006, abstract #SM53A-1432

Physics

Space Physics

2722 Forecasting (7924, 7964), 2730 Magnetosphere: Inner, 2732 Magnetosphere Interactions With Satellites And Rings, 2740 Magnetospheric Configuration And Dynamics, 2753 Numerical Modeling

Scientific paper

The Simple Inner Magnetosphere Model (SIMM) is a particle trace model designed to specify magnetospheric particle fluxes for particles up to 100 keV at geosynchronous orbit. Based on the Magnetospheric Specification Model (MSM), SIMM is designed to take advantage of the improvements in empirical and data assimilative modeling since initial development of the MSM. In particular, SIMM uses electric potential patterns created by the Assimilative Mapping of Ionospheric Electrodynamics (AMIE) technique as the electric field driver for the semi-empirical plasma sheet model. The SIMM model output provides a valuable tool for evaluation of spacecraft exposures, calibration of particle measurement instrumentation, biological effects on organisms on- board spacecraft, and provides an advanced tool for space weather modeling. The model output is being archived at the National Geophysical Data Center, and is available for viewing through the Space Physics Interactive Data Resource (SPIDR). We will present the model verification results and compare them to output from the MSM and present the geomagnetic conditions under which using AMIE for the electrodynamics provides more reliable results than direct input from remote sensing data.

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