A kinetic model for magnetogasdynamics
- Authors: Chetverushkin B.1, D’Ascenzo N.2, Saveliev A.3, Saveliev V.4
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Affiliations:
- Keldysh Institute of Applied Mathematics
- Deutsches Elektronen-Synchrotron
- Universität Hamburg
- Immanuel Kant Baltic Federal University
- Issue: Vol 9, No 5 (2017)
- Pages: 544-553
- Section: Article
- URL: https://journals.rcsi.science/2070-0482/article/view/201883
- DOI: https://doi.org/10.1134/S2070048217050039
- ID: 201883
Cite item
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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