A kinetic model for magnetogasdynamics


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详细

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.

作者简介

B. Chetverushkin

Keldysh Institute of Applied Mathematics

编辑信件的主要联系方式.
Email: office@keldysh.ru
俄罗斯联邦, Moscow

N. D’Ascenzo

Deutsches Elektronen-Synchrotron

Email: office@keldysh.ru
德国, Hamburg

A. Saveliev

Universität Hamburg

Email: office@keldysh.ru
德国, Hamburg

V. Saveliev

Immanuel Kant Baltic Federal University

Email: office@keldysh.ru
俄罗斯联邦, Kaliningrad

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