A kinetic model for magnetogasdynamics


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Abstract

In this work the equations of ideal magnetogasdynamics are derived based on the introduced local complex Maxwellian distribution function. Using this kinetic model, we obtain the analog of a quasi-dynamic system of equations for magnetogasdynamics, including dissipative processes. The resulting model and the algorithm of its solution have been tested by applying them to a number of well-known problems. The given algorithm can be easily adapted to an architecture of high performance systems with extramassive parallelism.

About the authors

B. Chetverushkin

Keldysh Institute of Applied Mathematics

Author for correspondence.
Email: office@keldysh.ru
Russian Federation, Moscow

N. D’Ascenzo

Deutsches Elektronen-Synchrotron

Email: office@keldysh.ru
Germany, Hamburg

A. Saveliev

Universität Hamburg

Email: office@keldysh.ru
Germany, Hamburg

V. Saveliev

Immanuel Kant Baltic Federal University

Email: office@keldysh.ru
Russian Federation, Kaliningrad

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