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Global simulations of heat-flux-driven buoyancy and magnetothermal instabilities, and their astrophysical implications

Author(s)
Kulchoakrungsun, Ekapob
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Massachusetts Institute of Technology. Department of Physics.
Advisor
Mark Vogelsberger.
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M.I.T. theses are protected by copyright. They may be viewed from this source for any purpose, but reproduction or distribution in any format is prohibited without written permission. See provided URL for inquiries about permission. http://dspace.mit.edu/handle/1721.1/7582
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Abstract
In this thesis, we investigate the convective instabilities induced by anisotropic conduction in a rapidly conducting plasma. We simulate the magneto-thermal instability (MTI), and the heat-flux-driven buoyancy instability (HBI) in two- and three- dimensional, global hydrodynamic simulations performed by the AREPO code, and verify the results of previous works. Our results have important astrophysical implications, such as the conductive heat transport in galaxy clusters.
Description
Thesis: S.B., Massachusetts Institute of Technology, Department of Physics, 2016.
 
Cataloged from PDF version of thesis.
 
Includes bibliographical references (page 36).
 
Date issued
2016
URI
http://hdl.handle.net/1721.1/105598
Department
Massachusetts Institute of Technology. Department of Physics
Publisher
Massachusetts Institute of Technology
Keywords
Physics.

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