Modeling the Heliosphere with an Adaptive MHD-kinetic Code

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

We combine an adaptive mesh refinement, axially-symmetric, MHD model of
the heliosphere with a fully kinetic model to treat the flow of neutral
particles. Results are presented of a comparison between MHD-kinetic and
multifluid models. The algorithm of coupling between the AMR fluid and
the kinetic codes is described.

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