Speaker
Viviane Pierrard
(Belgian Institute for Space Aeronomy)
Description
Recent progress of kinetic models for space plasmas will be reported. Concerning the solar wind, exospheric model based on kappa distributions for the electrons are coupled with coronal conditions deduced from spacecraft observations and from MHD models. Dynamical simulations are also developed for particles trapped in the inner magnetosphere and the results are compared with satellite observations and especially with the Energetic Particle Telescope (EPT) flux measurements.
Primary author
Viviane Pierrard
(Belgian Institute for Space Aeronomy)