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

Результат исследования: Научные публикации в периодических изданиях › статья по материалам конференции › рецензирование

Аннотация

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.

Язык оригинала	английский
Номер статьи	012132
Число страниц	6
Журнал	Journal of Physics: Conference Series
Том	894
Номер выпуска	1
DOI	https://doi.org/10.1088/1742-6596/894/1/012132
Состояние	Опубликовано - 22 окт 2017

Доступ к документу

10.1088/1742-6596/894/1/012132

Link to publication in Scopus

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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.

Результат исследования: Научные публикации в периодических изданиях › статья по материалам конференции › рецензирование

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KW - DYNAMICS

KW - TURBULENCE

KW - COLLISION

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