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Design Considerations for Unmagnetized Collisionless-shock Measurements in Homologous Flows

dc.contributor.authorDrake, R. P.en_US
dc.contributor.authorGregori, G.en_US
dc.date.accessioned2013-06-28T15:25:35Z
dc.date.available2013-06-28T15:25:35Z
dc.date.issued2012en_US
dc.identifier.citationDrake, R. P.; Gregori, G. (2012). "Design Considerations for Unmagnetized Collisionless-shock Measurements in Homologous Flows." The Astrophysical Journal 749(2): 171. <http://hdl.handle.net/2027.42/98554>en_US
dc.identifier.urihttp://stacks.iop.org/0004-637X/749/i=2/a=171en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/98554
dc.description.abstractThe subject of this paper is the design of practical laser experiments that can produce collisionless shocks mediated by the Weibel instability. Such shocks may be important in a wide range of astrophysical systems. Three issues are considered. The first issue is the implications of the fact that such experiments will produce expanding flows that are approximately homologous. As a result, both the velocity and the density of the interpenetrating plasma streams will be time dependent. The second issue is the implications of the linear theory of the Weibel instability. For the experiments, the instability is in a regime where standard simplifications do not apply. It appears feasible but non-trivial to obtain adequate growth. The third issue is collisionality. The need to keep resistive magnetic-field dissipation small enough implies that the plasmas should not be allowed to cool substantially.en_US
dc.publisherIOP Publishingen_US
dc.titleDesign Considerations for Unmagnetized Collisionless-shock Measurements in Homologous Flowsen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/98554/1/0004-637X_749_2_171.pdf
dc.identifier.doi10.1088/0004-637X/749/2/171en_US
dc.identifier.sourceThe Astrophysical Journalen_US
dc.owningcollnamePhysics, Department of


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