Abstract
A kinetic model based on the use of a single-particle distribution function is used to describe dissipative magnetogasdynamic phenomena. Along with the original quasi-gasdynamic model, a simplified version that is more convenient for numerical implementation is considered and justified. Numerical results for a number of problems are presented.
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Notes
Here, we do not consider cases where the QGD system yields results that are in better agreement with experimental data than the Navier–Stokes equations, for example, flows with moderate Knudsen numbers \(Kn \leqslant 0.1\) [7, 17, 20–22]. In that case, the complete QGD system (3.14)–(3.19) has to be used.
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ACKNOWLEDGMENTS
This work was supported by the Russian Science Foundation, grant no. 14-11-00170.
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Translated by I. Ruzanova
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Chetverushkin, B.N., Saveliev, A.V. & Saveliev, V.I. A Quasi-Gasdynamic Model for the Description of Magnetogasdynamic Phenomena. Comput. Math. and Math. Phys. 58, 1384–1394 (2018). https://doi.org/10.1134/S0965542518080055
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DOI: https://doi.org/10.1134/S0965542518080055