Magnetohydrodynamics, magnetogenesis, and magnetorotational instabilities with adaptive mesh refinement

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Abstract/Contents

Abstract
While the presence of magnetic fields seems ubiquitous in cosmic structures of all scales, the mechanisms of their formation are still debated. Using the adaptive mesh refinement (AMR) code Enzo, we touch on three major topics in the study of magnetic fields in computational astrophysics. We first describe the features of magnetohydrodynamic algorithms, and develop a technique to computationally maintain the divergence free nature of the magnetic field in an AMR hierarchy. Second, we analyze the generation of magnetic seed fields in protogalaxy formation via a plasma physics phenomenon called the Biermann Battery, and discuss its dependence on turbulence during large scale structure formation in the early universe. Finally, we discuss the magnetorotational instability that causes the saturation of magnetic field generation in differentially rotating objects such as accretion disks. We adapt the shearing box, a local 3D simulation of differentially rotating disks, to the AMR formalism and analyze the resolution and simulation box size dependence of these instabilities.

Description

Type of resource text
Form electronic; electronic resource; remote
Extent 1 online resource.
Publication date 2010
Issuance monographic
Language English

Creators/Contributors

Associated with Zhao, Fen
Associated with Stanford University, Department of Applied Physics
Primary advisor Abel, Tom G, 1970-
Primary advisor Petrosian, Vahe
Thesis advisor Petrosian, Vahe
Thesis advisor Blandford, Roger D
Advisor Blandford, Roger D

Subjects

Genre Theses

Bibliographic information

Statement of responsibility Fen Zhao.
Note Submitted to the Department of Applied Physics.
Thesis Thesis (Ph. D.)--Stanford University, 2010.
Location electronic resource

Access conditions

Copyright
© 2010 by Fen Zhao
License
This work is licensed under a Creative Commons Attribution Non Commercial 3.0 Unported license (CC BY-NC).

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