The numerical modelling of MHD astrophysical flows with chemistry

I. Kulikov, I. Chernykh, V. Protasov

Research output: Contribution to journalConference articlepeer-review

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 languageEnglish
Article number012132
Number of pages6
JournalJournal of Physics: Conference Series
Volume894
Issue number1
DOIs
Publication statusPublished - 22 Oct 2017

Keywords

  • MAGNETIC-FIELDS
  • SOLAR-WIND
  • SIMULATIONS
  • DYNAMICS
  • TURBULENCE
  • COLLISION
  • EMISSION
  • COLLAPSE
  • GAS

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