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

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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Цитировать

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

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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

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