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Paper: Implications of the Hall Effect for Turbulent Molecular Clouds
Volume: 385, Numerical Modeling of Space Plasma Flows: Astronum-2007
Page: 12
Authors: Downes, T.P.; O'Sullivan, S.
Abstract: We present the first study of turbulent decay in systems in which the Hall effect is important. We use a new, stable, explicit algorithm to integrate the multifluid MHD equations in the presence of the Hall effect.

We find that in Hall-dominated systems effect introduces more structure in density on all length scales, and marginally reduces the turbulent energy decay rate, than in equivalent systems which are ambipolar dominated.

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