A kinetic model for magnetogasdynamics
- 作者: Chetverushkin B.1, D’Ascenzo N.2, Saveliev A.3, Saveliev V.4
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隶属关系:
- Keldysh Institute of Applied Mathematics
- Deutsches Elektronen-Synchrotron
- Universität Hamburg
- Immanuel Kant Baltic Federal University
- 期: 卷 9, 编号 5 (2017)
- 页面: 544-553
- 栏目: Article
- URL: https://journals.rcsi.science/2070-0482/article/view/201883
- DOI: https://doi.org/10.1134/S2070048217050039
- ID: 201883
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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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