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Current status and future prospects for laboratory study of angular momentum transport relevant to astrophysical disks

Published online by Cambridge University Press:  08 June 2011

Hantao Ji
Hantao Ji*
Affiliation:
Princeton Plasma Physics Laboratory, Princeton University, Princeton, New Jersey, U.S.A. email: [email protected]
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Abstract

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A concise review of the past and ongoing laboratory experiments on rotating flows and the associated angular momentum transport relevant to astrophysical disks is given in three categories: hydrodynamic, magnetohydrodynamic, gas and plasma experiments. Future prospects for these experiments, especially for those directly relevant to the magnetorotational instability (MRI), are discussed with an emphasis on a newly proposed swirling gas and plasma experiment.

Keywords

accretion diskshydrodynamicsmagnetohydrodynamics (MHD)instabilitiesplasmasturbulencemethods: laboratory
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S274: Advances in Plasma Astrophysics , September 2010 , pp. 18 - 25
Copyright
Copyright © International Astronomical Union 2011

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