{"id":{"repo_id":"mit","oai_identifier":"oai:dspace.mit.edu:1721.1/51604"},"canonical_url":"https://search.dev.ndltd.org/etd/mit/oai:dspace.mit.edu:1721.1/51604","repository":{"repo_id":"mit","name":"MIT","base_url":"https://dspace.mit.edu/oai/request"},"display":{"title":"Plasma velocities in the Heliosheath and the influence of the interstellar wind","abstract":"A 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.","abstract_html":"A 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.","abstract_has_math":false,"creators":["Chronopoulos, Chris"],"institution":"Massachusetts Institute of Technology","degree_name":null,"degree_level":null,"degree_discipline":null,"degree_department":"Massachusetts Institute of Technology. Dept. of Physics.","school":null,"contributors":[],"advisors":["John W. 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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."],"dc:description.degree":["S.B."],"dc:identifier.uri":["http://hdl.handle.net/1721.1/51604"],"dc:language.iso":["eng"],"dc:publisher":["Massachusetts Institute of Technology"],"dc:rights":["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."],"dc:rights.uri":["http://dspace.mit.edu/handle/1721.1/7582"],"dc:subject":["Physics."],"dc:title":["Plasma velocities in the Heliosheath and the influence of the interstellar wind"],"dc:type":["Thesis"]},"updated_at":"2026-07-22T22:22:08Z"}