The numerical modelling of MHD astrophysical flows with chemistry

I. Kulikov; I. Chernykh; V. Protasov

doi:10.1088/1742-6596/894/1/012132

The numerical modelling of MHD astrophysical flows with chemistry

I. Kulikov, I. Chernykh, V. Protasov

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

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.

Original language	English
Article number	012132
Number of pages	6
Journal	Journal of Physics: Conference Series
Volume	894
Issue number	1
DOIs	https://doi.org/10.1088/1742-6596/894/1/012132
Publication status	Published - 22 Oct 2017

Keywords

MAGNETIC-FIELDS
SOLAR-WIND
SIMULATIONS
DYNAMICS
TURBULENCE
COLLISION
EMISSION
COLLAPSE
GAS

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10.1088/1742-6596/894/1/012132

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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",

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AU - Kulikov, I.

AU - Chernykh, I.

AU - Protasov, V.

PY - 2017/10/22

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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 -

The numerical modelling of MHD astrophysical flows with chemistry

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Keywords

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