Comparison of two high-latitude electrodynamic models during substorm intervals

Details Comparison of two high-latitude electrodynamic models during substorm intervals Comparison of two high-latitude electrodynamic models during substorm intervals

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002agusmsm42b..05v&link_type=abstract

American Geophysical Union, Spring Meeting 2002, abstract #SM42B-05

Physics

2784 Solar Wind/Magnetosphere Interactions, 2788 Storms And Substorms, 2431 Ionosphere/Magnetosphere Interactions (2736), 2447 Modeling And Forecasting

Scientific paper

High-latitude models provide us with dynamic maps of geomagnetic activity driven by the solar wind or a geomagnetic index. The main features of the substorm development are clearely traced out in these maps. They are quantified via derived magnetic indices and polar cap size. Further, the dynamic geomagnetic field models are used to drive the ionospheric E field response. For three small substorms in January 1997 we compare two different models, AMIE and Electra, in terms of spatial and temporal development of the magnetic field, derived conductance, and Joule heat.

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