Plasma velocities in the Heliosheath and the influence of the interstellar wind

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.

Department dc:contributor.department

Massachusetts Institute of Technology. Dept. of Physics.

Grantor dc:publisher

Massachusetts Institute of Technology

Year dc:date.issued

2009

Author dc:creator

• Chronopoulos, Chris

Advisor dc:contributor.advisor

• John W. Belcher.

• Physics.

Statement 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.

Licence dc:rights.uri

• http://dspace.mit.edu/handle/1721.1/7582

Language dc:language.iso

eng

Handle dc:identifier.uri

http://hdl.handle.net/1721.1/51604

OAI identifier oai:identifier

oai:dspace.mit.edu:1721.1/51604