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Please use this identifier to cite or link to this item: http://arks.princeton.edu/ark:/88435/dsp01f4752k49x
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dc.contributor.advisorJi, Hantao-
dc.contributor.advisorRen, Yang-
dc.contributor.authorLo, Jensen-
dc.date.accessioned2018-08-17T15:38:22Z-
dc.date.available2018-08-17T15:38:22Z-
dc.date.created2018-04-30-
dc.date.issued2018-08-17-
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/dsp01f4752k49x-
dc.description.abstractObservations of magnetic reconnection events in the magnetopause by the Magnetospheric Multiscale Mission (MMS) show magnetic fluctuations and large electric fields possibly caused by electromagnetic drift instabilities, instabilities caused by a relative drift between electrons and ions within a magnetic field. Experiments in the MRX have also shown qualitatively similar magnetic fluctuations. We fully generalize a local, linear model originally published by Ji et. al, and extend it to cover these situations by carrying out a full calculation including guide field, magnetized ions, and kinetic effects.en_US
dc.format.mimetypeapplication/pdf-
dc.language.isoenen_US
dc.titleDescribing Drift Instabilities in Magnetic Reconnection Using a Local Linear Modelen_US
dc.typePrinceton University Senior Theses-
pu.date.classyear2018en_US
pu.departmentPhysicsen_US
pu.pdf.coverpageSeniorThesisCoverPage-
pu.contributor.authorid960961945-
Appears in Collections:Physics, 1936-2023

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