Ionospheric Convection Pattern for Sawtooth Events from AMIE Simulation

Details Ionospheric Convection Pattern for Sawtooth Events from AMIE Simulation Ionospheric Convection Pattern for Sawtooth Events from AMIE Simulation

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004agufmsm31b1224c&link_type=abstract

American Geophysical Union, Fall Meeting 2004, abstract #SM31B-1224

Physics

2708 Current Systems (2409), 2712 Electric Fields (2411), 2736 Magnetosphere/Ionosphere Interactions, 2784 Solar Wind/Magnetosphere Interactions, 2788 Storms And Substorms

Scientific paper

Sawtooth events are quasi-periodic, large-amplitude oscillations of energetic particle flux enhancement with a periodicity of 2-4 hours, which are observed globally and simultaneously at the geosynchronous orbit. Statistical studies of sawtooth events imply an enhanced solar wind - magnetosphere - ionosphere coupling. Herein the ionosphere convection potentials and currents systems are examined using the Assimilative Mapping of Ionospheric Electrodynamics (AMIE) simulation results. Comparison of convection pattens for sawtooth events with isolated substorms, steady magnetosphere convection (SMC) events are also made.

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