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Zhurnal Vychislitel'noi Matematiki i Matematicheskoi Fiziki, 2018, Volume 58, Number 5, Pages 716–725
DOI: https://doi.org/10.7868/S0044466918050046
(Mi zvmmf10732)
 

This article is cited in 5 scientific papers (total in 5 papers)

Kinetic model and magnetogasdynamics equations

B. N. Chetverushkina, N. D'Ascenzob, A. V. Savelievc, V. I. Savelievc

a Federal Research Center Keldysh Institute of Applied Mathematics, Russian Academy of Sciences, Moscow, Russia
b Deutsches Elektronensynchrotron, Hamburg, Germany
c Immanuel Kant Baltic Federal University, Kaliningrad, Russia
Citations (5)
References:
Abstract: An original kinetic model for the molecular velocity distribution function is considered. Based on this model, the equations of ideal magnetogasdynamics (MGD) are derived and an original model for dissipative MGD is obtained. The latter model can be used to construct algorithms easily adaptable to high-performance computer architectures. As an example, results of high-performance computations of astrophysical phenomena are presented, namely, the formation of cosmic jets is modeled.
Key words: magnetogasdynamics, kinetic models, kinetically consistent algorithms, high-performance computations.
Funding agency Grant number
Russian Science Foundation 14-11-00170
Received: 05.07.2017
English version:
Computational Mathematics and Mathematical Physics, 2018, Volume 58, Issue 5, Pages 691–699
DOI: https://doi.org/10.1134/S0965542518050068
Bibliographic databases:
Document Type: Article
UDC: 519.635
Language: Russian
Citation: B. N. Chetverushkin, N. D'Ascenzo, A. V. Saveliev, V. I. Saveliev, “Kinetic model and magnetogasdynamics equations”, Zh. Vychisl. Mat. Mat. Fiz., 58:5 (2018), 716–725; Comput. Math. Math. Phys., 58:5 (2018), 691–699
Citation in format AMSBIB
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  • This publication is cited in the following 5 articles:
    Citing articles in Google Scholar: Russian citations, English citations
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