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Direct Monte Carlo simulation of development of the Richtmyer-Meshkov instability on the Ar/He interface. / Kashkovsky, A. V.; Kudryavtsev, A. N.; Shershnev, A. A.

In: Journal of Physics: Conference Series, Vol. 1404, No. 1, 012109, 06.12.2019.

Research output: Contribution to journal › Conference article › peer-review

Harvard

Kashkovsky, AV, Kudryavtsev, AN & Shershnev, AA 2019, 'Direct Monte Carlo simulation of development of the Richtmyer-Meshkov instability on the Ar/He interface', Journal of Physics: Conference Series, vol. 1404, no. 1, 012109. https://doi.org/10.1088/1742-6596/1404/1/012109

APA

Kashkovsky, A. V., Kudryavtsev, A. N., & Shershnev, A. A. (2019). Direct Monte Carlo simulation of development of the Richtmyer-Meshkov instability on the Ar/He interface. Journal of Physics: Conference Series, 1404(1), [012109]. https://doi.org/10.1088/1742-6596/1404/1/012109

Vancouver

Kashkovsky AV, Kudryavtsev AN, Shershnev AA. Direct Monte Carlo simulation of development of the Richtmyer-Meshkov instability on the Ar/He interface. Journal of Physics: Conference Series. 2019 Dec 6;1404(1):012109. doi: 10.1088/1742-6596/1404/1/012109

Author

Kashkovsky, A. V. ; Kudryavtsev, A. N. ; Shershnev, A. A. / Direct Monte Carlo simulation of development of the Richtmyer-Meshkov instability on the Ar/He interface. In: Journal of Physics: Conference Series. 2019 ; Vol. 1404, No. 1.

BibTeX

@article{22265854c6924ac7988d1e72bd44d9e6,
title = "Direct Monte Carlo simulation of development of the Richtmyer-Meshkov instability on the Ar/He interface",
abstract = "The Richtmyer-Meshkov instability developing on the interface between helium and argon gases hit by a propagating shock wave is simulated numerically. In contrast with conventional approach based on the Navier-Stokes equations, the simulation in the current paper is performed on the molecular level using the Direct Simulation Monte Carlo method. The data averaging over short time periods is employed to decrease statistical scattering. The instability development is successfully reproduced with relatively moderate computer resources used. The time evolution of the transmitted shock wave and contact surface velocities are retrieved from numerical data as well as the instability growth rates.",
author = "Kashkovsky, {A. V.} and Kudryavtsev, {A. N.} and Shershnev, {A. A.}",
note = "Publisher Copyright: {\textcopyright} 2019 IOP Publishing Ltd. Copyright: Copyright 2020 Elsevier B.V., All rights reserved.; 16th All-Russian Seminar with International Participation on Dynamics of Multiphase Media, DMM 2019 ; Conference date: 30-09-2019 Through 05-10-2019",
year = "2019",
month = dec,
day = "6",
doi = "10.1088/1742-6596/1404/1/012109",
language = "English",
volume = "1404",
journal = "Journal of Physics: Conference Series",
issn = "1742-6588",
publisher = "IOP Publishing Ltd.",
number = "1",

}

RIS

TY - JOUR

T1 - Direct Monte Carlo simulation of development of the Richtmyer-Meshkov instability on the Ar/He interface

AU - Kashkovsky, A. V.

AU - Kudryavtsev, A. N.

AU - Shershnev, A. A.

N1 - Publisher Copyright: © 2019 IOP Publishing Ltd. Copyright: Copyright 2020 Elsevier B.V., All rights reserved.

PY - 2019/12/6

Y1 - 2019/12/6

N2 - The Richtmyer-Meshkov instability developing on the interface between helium and argon gases hit by a propagating shock wave is simulated numerically. In contrast with conventional approach based on the Navier-Stokes equations, the simulation in the current paper is performed on the molecular level using the Direct Simulation Monte Carlo method. The data averaging over short time periods is employed to decrease statistical scattering. The instability development is successfully reproduced with relatively moderate computer resources used. The time evolution of the transmitted shock wave and contact surface velocities are retrieved from numerical data as well as the instability growth rates.

AB - The Richtmyer-Meshkov instability developing on the interface between helium and argon gases hit by a propagating shock wave is simulated numerically. In contrast with conventional approach based on the Navier-Stokes equations, the simulation in the current paper is performed on the molecular level using the Direct Simulation Monte Carlo method. The data averaging over short time periods is employed to decrease statistical scattering. The instability development is successfully reproduced with relatively moderate computer resources used. The time evolution of the transmitted shock wave and contact surface velocities are retrieved from numerical data as well as the instability growth rates.

UR - http://www.scopus.com/inward/record.url?scp=85077818412&partnerID=8YFLogxK

U2 - 10.1088/1742-6596/1404/1/012109

DO - 10.1088/1742-6596/1404/1/012109

M3 - Conference article

AN - SCOPUS:85077818412

VL - 1404

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

SN - 1742-6588

IS - 1

M1 - 012109

T2 - 16th All-Russian Seminar with International Participation on Dynamics of Multiphase Media, DMM 2019

Y2 - 30 September 2019 through 5 October 2019

ER -

ID: 23120809