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 |
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Article number | 012132 |
Number of pages | 6 |
Journal | Journal of Physics: Conference Series |
Volume | 894 |
Issue number | 1 |
DOIs | |
Publication status | Published - 22 Oct 2017 |
Keywords
- MAGNETIC-FIELDS
- SOLAR-WIND
- SIMULATIONS
- DYNAMICS
- TURBULENCE
- COLLISION
- EMISSION
- COLLAPSE
- GAS