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 |
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Номер статьи | 012132 |
Число страниц | 6 |
Журнал | Journal of Physics: Conference Series |
Том | 894 |
Номер выпуска | 1 |
DOI | |
Состояние | Опубликовано - 22 окт. 2017 |