Implications of the Hall Effect for Turbulent Molecular Clouds

Details Implications of the Hall Effect for Turbulent Molecular Clouds Implications of the Hall Effect for Turbulent Molecular Clouds

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..385...12d&link_type=abstract

Numerical Modeling of Space Plasma Flows: Astronum 2007 ASP Conference Series, Vol. 385, proceedings of the conference held 10-1

Astronomy and Astrophysics

Astronomy

2

Scientific paper

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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