Published in

Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S270(6), p. 421-424, 2010

DOI: 10.1017/s1743921311000743

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Ambipolar Diffusion Effects on Weakly Ionized Turbulence Molecular Clouds

Journal article published in 2010 by Pak Shing Li ORCID, Christopher F. McKee, Richard I. Klein
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

AbstractAmbipolar diffusion (AD) is a key process in molecular clouds (MCs). Non-ideal MHD turbulence simulations are technically very challenging because of the large Alfvén speed of ions in weakly ionized clouds. Using the Heavy-Ion Approximation method (Li, McKee & Klein 2006), we have carried out two-fluid simulations of AD in isothermal, turbulent boxes at a resolution of 5123, to investigate the effect of AD on the weakly ionized turbulence in MCs. Our simulation results show that the neutral gas component of the two-fluid system gradually transforms from an ideal MHD turbulence system to near a pure hydrodynamic turbulence system within the standard AD regime, in which the neutrals and ions are coupled over a flow time. The change of the turbulent state has a profound effect on the weakly ionized MCs.

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