Distributions of Charged Particles for Non-storm Time Substorm Events from THEMIS observations

Physics

Scientific paper

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2790 Substorms, 7807 Charged Particle Motion And Acceleration, 7845 Particle Acceleration, 7859 Transport Processes, 7899 General Or Miscellaneous

Scientific paper

THEMIS mission has provided plentiful observational data including fluxes and angular distributions for both ions and electrons at lower energy (< 30 keV) and higher energy (> 30 keV) from the instrument ESA and SST, respectively. The separation of the five composed satellites at the equatorial plane at different L-shells provides simultaneous observations at multi-points to study the spatial structure and temporal evolution of these charged particles. We will present case studies on analysis of the observed charged particle data for non- storm time substorm events. The evolution of pitch-angle distributions is specifically investigated. The local magnetic field data from the instrument FGM and upstream solar wind data (e.g. from ACE) will also be adopted to identify the magnetospheric environment. This will enhance our understanding on the possible mechanism for charged particles occurred during non-storm time substorms and benefit to future tudies on storm time substorm events.

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