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A kinetic model for magnetogasdynamics

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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.

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Author information

Authors and Affiliations

  1. Keldysh Institute of Applied Mathematics, Russian Academy of Sciences, Moscow, Russia

    B. Chetverushkin

  2. Deutsches Elektronen-Synchrotron, Hamburg, Germany

    N. D’Ascenzo

  3. Universität Hamburg, Hamburg, Germany

    A. Saveliev

  4. Immanuel Kant Baltic Federal University, Kaliningrad, Russia

    V. Saveliev

Authors
  1. B. Chetverushkin
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  2. N. D’Ascenzo
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  3. A. Saveliev
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  4. V. Saveliev
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Corresponding author

Correspondence to B. Chetverushkin.

Additional information

Original Russian Text © B. Chetverushkin, N. D’Ascenzo, A. Saveliev, V. Saveliev, 2017, published in Matematicheskoe Modelirovanie, 2017, Vol. 29, No. 3, pp. 3–15.

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Chetverushkin, B., D’Ascenzo, N., Saveliev, A. et al. A kinetic model for magnetogasdynamics. Math Models Comput Simul 9, 544–553 (2017). https://doi.org/10.1134/S2070048217050039

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  • DOI: https://doi.org/10.1134/S2070048217050039

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