Ambipolar Diffusion Effects on Weakly Ionized Turbulence Molecular Clouds
Abstract
Ambipolar 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.
- Publication:
-
Computational Star Formation
- Pub Date:
- April 2011
- DOI:
- 10.1017/S1743921311000743
- Bibcode:
- 2011IAUS..270..421L
- Keywords:
-
- turbulence;
- ISM: magnetic fields;
- ISM: clouds;
- methods: numerical