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 details of the numerical
method are described; the main tests and the scheme of parallel implementation
are shown. The chemodynamics of the hydrogen while the turbulent formation of
molecular clouds is modeled.
%0 Generic
%1 citeulike:14130132
%A Kulikov, Igor
%A Chernykh, Igor
%A Protasov, Viktor
%D 2016
%K imported
%T A New Code for Numerical Simulation of MHD Astrophysical Flows With Chemistry
%U http://arxiv.org/abs/1608.08748
%X 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 details of the numerical
method are described; the main tests and the scheme of parallel implementation
are shown. The chemodynamics of the hydrogen while the turbulent formation of
molecular clouds is modeled.
@misc{citeulike:14130132,
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 details of the numerical
method are described; the main tests and the scheme of parallel implementation
are shown. The chemodynamics of the hydrogen while the turbulent formation of
molecular clouds is modeled.}},
added-at = {2019-03-25T08:20:55.000+0100},
archiveprefix = {arXiv},
author = {Kulikov, Igor and Chernykh, Igor and Protasov, Viktor},
biburl = {https://www.bibsonomy.org/bibtex/2c81cb18cf54586f9ce20f1c881f06379/ericblackman},
citeulike-article-id = {14130132},
citeulike-linkout-0 = {http://arxiv.org/abs/1608.08748},
citeulike-linkout-1 = {http://arxiv.org/pdf/1608.08748},
day = 31,
eprint = {1608.08748},
interhash = {79e9863b01cbc3d038a87427d44e78ee},
intrahash = {c81cb18cf54586f9ce20f1c881f06379},
keywords = {imported},
month = aug,
posted-at = {2016-09-05 06:41:19},
priority = {2},
timestamp = {2019-03-25T08:20:55.000+0100},
title = {{A New Code for Numerical Simulation of MHD Astrophysical Flows With Chemistry}},
url = {http://arxiv.org/abs/1608.08748},
year = 2016
}