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dc.contributor.advisorJohn W. Belcher.en_US
dc.contributor.authorChronopoulos, Chrisen_US
dc.contributor.otherMassachusetts Institute of Technology. Dept. of Physics.en_US
dc.date.accessioned2010-02-09T16:50:14Z
dc.date.available2010-02-09T16:50:14Z
dc.date.copyright2009en_US
dc.date.issued2009en_US
dc.identifier.urihttp://hdl.handle.net/1721.1/51604
dc.descriptionThesis (S.B.)--Massachusetts Institute of Technology, Dept. of Physics, 2009.en_US
dc.descriptionIncludes bibliographical references (p. 35).en_US
dc.description.abstractA new coordinate system (Interstellar Heliospheric Coordinates, or IHC) is introduced to enable the detailed study of the influence of the interstellar wind on the heliosheath. Recent, in situ measurements of plasma velocities in the heliosheath by Voyager 2 are projected into the IHC system and analyzed. We consider steady state flows as well as time dependent phenomena, and we show that a transient event with no obvious cause or direction takes a particularly simple form in IHC.en_US
dc.description.statementofresponsibilityby Chris Chronopoulos.en_US
dc.format.extent35 p.en_US
dc.language.isoengen_US
dc.publisherMassachusetts Institute of Technologyen_US
dc.rightsM.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.en_US
dc.rights.urihttp://dspace.mit.edu/handle/1721.1/7582en_US
dc.subjectPhysics.en_US
dc.titlePlasma velocities in the Heliosheath and the influence of the interstellar winden_US
dc.typeThesisen_US
dc.description.degreeS.B.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physics
dc.identifier.oclc495723562en_US


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