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The numerical modelling of MHD astrophysical flows with chemistry. / Kulikov, I.; Chernykh, I.; Protasov, V.

в: Journal of Physics: Conference Series, Том 894, № 1, 012132, 22.10.2017.

Результаты исследований: Научные публикации в периодических изданиях › статья по материалам конференции › Рецензирование

Harvard

Kulikov, I, Chernykh, I & Protasov, V 2017, 'The numerical modelling of MHD astrophysical flows with chemistry', Journal of Physics: Conference Series, Том. 894, № 1, 012132. https://doi.org/10.1088/1742-6596/894/1/012132

APA

Kulikov, I., Chernykh, I., & Protasov, V. (2017). The numerical modelling of MHD astrophysical flows with chemistry. Journal of Physics: Conference Series, 894(1), [012132]. https://doi.org/10.1088/1742-6596/894/1/012132

Vancouver

Kulikov I, Chernykh I, Protasov V. The numerical modelling of MHD astrophysical flows with chemistry. Journal of Physics: Conference Series. 2017 окт. 22;894(1):012132. doi: 10.1088/1742-6596/894/1/012132

Author

Kulikov, I. ; Chernykh, I. ; Protasov, V. / The numerical modelling of MHD astrophysical flows with chemistry. в: Journal of Physics: Conference Series. 2017 ; Том 894, № 1.

BibTeX

@article{b97c541c28ea47ad9acd6372714cf458,
title = "The numerical modelling of MHD astrophysical flows with chemistry",
abstract = "The new code for numerical simulation of magnetic hydrodynamical astrophysical flows with consideration of chemical reactions is given in the paper. At the heart of the code - the new original low-dissipation numerical method based on a combination of operator splitting approach and piecewise-parabolic method on the local stencil. The chemodynamics of the hydrogen while the turbulent formation of molecular clouds is modeled.",
keywords = "MAGNETIC-FIELDS, SOLAR-WIND, SIMULATIONS, DYNAMICS, TURBULENCE, COLLISION, EMISSION, COLLAPSE, GAS",
author = "I. Kulikov and I. Chernykh and V. Protasov",
note = "Funding Information: The research work was supported by the Grant of the President of Russian Federation for the",
year = "2017",
month = oct,
day = "22",
doi = "10.1088/1742-6596/894/1/012132",
language = "English",
volume = "894",
journal = "Journal of Physics: Conference Series",
issn = "1742-6588",
publisher = "IOP Publishing Ltd.",
number = "1",

}

RIS

TY - JOUR

T1 - The numerical modelling of MHD astrophysical flows with chemistry

AU - Kulikov, I.

AU - Chernykh, I.

AU - Protasov, V.

N1 - Funding Information: The research work was supported by the Grant of the President of Russian Federation for the

PY - 2017/10/22

Y1 - 2017/10/22

N2 - The new code for numerical simulation of magnetic hydrodynamical astrophysical flows with consideration of chemical reactions is given in the paper. At the heart of the code - the new original low-dissipation numerical method based on a combination of operator splitting approach and piecewise-parabolic method on the local stencil. The chemodynamics of the hydrogen while the turbulent formation of molecular clouds is modeled.

AB - The new code for numerical simulation of magnetic hydrodynamical astrophysical flows with consideration of chemical reactions is given in the paper. At the heart of the code - the new original low-dissipation numerical method based on a combination of operator splitting approach and piecewise-parabolic method on the local stencil. The chemodynamics of the hydrogen while the turbulent formation of molecular clouds is modeled.

KW - MAGNETIC-FIELDS

KW - SOLAR-WIND

KW - SIMULATIONS

KW - DYNAMICS

KW - TURBULENCE

KW - COLLISION

KW - EMISSION

KW - COLLAPSE

KW - GAS

UR - http://www.scopus.com/inward/record.url?scp=85033227980&partnerID=8YFLogxK

U2 - 10.1088/1742-6596/894/1/012132

DO - 10.1088/1742-6596/894/1/012132

M3 - Conference article

AN - SCOPUS:85033227980

VL - 894

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

SN - 1742-6588

IS - 1

M1 - 012132

ER -

ID: 10066245