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  5. Modeling the formation of current sheets in symmetric and asymmetric reconnection

Modeling the formation of current sheets in symmetric and asymmetric reconnection

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Author(s)
Montag, Peter Katsumi
Advisor(s)
Jan Egedal and John Belcher.
Date Issued
2018
Publisher
Massachusetts Institute of Technology
Abstract
In this thesis we investigate the nature of magnetic reconnection using analytic and numerical methods. We consider configurations which are symmetric across the reconnection layer relevant to the Earth magnetotail, as well as configurations asymmetric in density and temperature across the reconnection layer, important to reconnection in Earth's dayside magnetopause. We develop an analytic model for the evolution of the electron phase space distribution function based on adiabatic invariants. We then apply this two model problems-Fermi acceleration and electron trapping-to extend previous results in these areas and model their effects on parallel heating. Following this, we run a battery of simulations of reconnection using particle in cell (PIC) codes at several different values of density asymmetry and guide field. These simulations reveal a number of regimes of current sheet formation, all of which are associated with significant anisotropic heating. Finally, we take a closer look at the case of antiparallel reconnection, where small levels of asymmetry cause significant shortening in the current sheet that develops at the midplane. Analysis of the data suggests an asymmetry in the firehose condition is the cause. Running another battery of simulations that adds a temperature asymmetry, we find that elongated current sheets will again form when the temperature asymmetry is large enough to restore balance in the firehose condition across the layer.
Description
Thesis: Ph. D., Massachusetts Institute of Technology, Department of Physics, 2018.
Cataloged from PDF version of thesis.
Includes bibliographical references (pages 103-109).
Subjects
Physics.
MIT Department
Massachusetts Institute of Technology. Department of Physics
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MIT theses are protected by copyright. They may be viewed, downloaded, or printed from this source but further reproduction or distribution in any format is prohibited without written permission.
http://dspace.mit.edu/handle/1721.1/7582
Persistent DSpace Link
http://hdl.handle.net/1721.1/119927
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