Research output: Contribution to journal › Conference article › peer-review
The numerical modelling of MHD astrophysical flows with chemistry. / Kulikov, I.; Chernykh, I.; Protasov, V.
In: Journal of Physics: Conference Series, Vol. 894, No. 1, 012132, 22.10.2017.Research output: Contribution to journal › Conference article › peer-review
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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