4.6 Article

AN EXPLICIT SCHEME FOR INCORPORATING AMBIPOLAR DIFFUSION IN A MAGNETOHYDRODYNAMICS CODE

Journal

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
Volume 181, Issue 2, Pages 413-420

Publisher

IOP PUBLISHING LTD
DOI: 10.1088/0067-0049/181/2/413

Keywords

diffusion; ISM: clouds; methods: numerical; MHD; stars: formation; turbulence

Funding

  1. KASI
  2. Korea Science and Engineering Foundation
  3. Korea Foundation for International Cooperation of Science and Technology [K20702020016-07E0200-01610]
  4. National Research Foundation of Korea [2007-00342, 2002-0036978] Funding Source: Korea Institute of Science & Technology Information (KISTI), National Science & Technology Information Service (NTIS)

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We describe a method for incorporating ambipolar diffusion in the strong coupling approximation into a multidimensional magnetohydrodynamic (MHD) code based on the total variation diminishing scheme. Contributions from ambipolar diffusion terms are included by explicit finite-difference operators in a fully unsplit way, maintaining second-order accuracy. The divergence-free condition of magnetic fields is exactly ensured at all times by a flux-interpolated constrained transport scheme. The super time-stepping method is used to accelerate the time step in high-resolution calculations and/or in strong ambipolar diffusion. We perform two test problems, the steady-state oblique C-type shocks and the decay of Alfven waves, confirming the accuracy and robustness of our numerical approach. Results from the simulations of the compressible MHD turbulence with ambipolar diffusion show the flexibility of our method as well as its ability to follow complex MHD flows in the presence of ambipolar diffusion. These simulations show that the dissipation rate of the MHD turbulence is strongly affected by the strength of ambipolar diffusion.

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