A kinetic model for magnetogasdynamics
- Авторлар: Chetverushkin B.1, D’Ascenzo N.2, Saveliev A.3, Saveliev V.4
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Мекемелер:
- Keldysh Institute of Applied Mathematics
- Deutsches Elektronen-Synchrotron
- Universität Hamburg
- Immanuel Kant Baltic Federal University
- Шығарылым: Том 9, № 5 (2017)
- Беттер: 544-553
- Бөлім: Article
- URL: https://journals.rcsi.science/2070-0482/article/view/201883
- DOI: https://doi.org/10.1134/S2070048217050039
- ID: 201883
Дәйексөз келтіру
Аннотация
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.
Негізгі сөздер
Авторлар туралы
B. Chetverushkin
Keldysh Institute of Applied Mathematics
Хат алмасуға жауапты Автор.
Email: office@keldysh.ru
Ресей, Moscow
N. D’Ascenzo
Deutsches Elektronen-Synchrotron
Email: office@keldysh.ru
Германия, Hamburg
A. Saveliev
Universität Hamburg
Email: office@keldysh.ru
Германия, Hamburg
V. Saveliev
Immanuel Kant Baltic Federal University
Email: office@keldysh.ru
Ресей, Kaliningrad
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