A New, Three-dimensional, Adaptive Mesh Refinement Code for Modeling Flows of Partially Ionized Plasma

Details A New, Three-dimensional, Adaptive Mesh Refinement Code for Modeling Flows of Partially Ionized Plasma A New, Three-dimensional, Adaptive Mesh Refinement Code for Modeling Flows of Partially Ionized Plasma

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..385..265k&link_type=abstract

Numerical Modeling of Space Plasma Flows: Astronum 2007 ASP Conference Series, Vol. 385, proceedings of the conference held 10-1

Astronomy and Astrophysics

Astronomy

3

Scientific paper

A milti-fluid, three-dimensional model of the heliospheric interface developed by tet{Kryukov:Pozaog04,Kryukov:Pozaog06,Kryukov:Pogo07} is implemented in the Chombo adaptive mesh refinement (AMR) framework. In this model, the charged component is described by ideal MHD equations, while different populations of neutral atoms are governed by separate sets of the Euler gas dynamic equations. The systems are coupled via source terms describing collisions and charge exchange between neutral and charged particles. We show the first 3D results of the application of our multi-fluid code to modeling the solar wind - interstellar medium interaction.

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