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Recent Experimental Results and Modelling of High-Mach-Number Jets and the Transition to Turbulence

dc.contributor.authorRosen, P. A.en_US
dc.contributor.authorWilde, B. H.en_US
dc.contributor.authorWilliams, R. J. R.en_US
dc.contributor.authorFoster, J. M.en_US
dc.contributor.authorKeiter, P. A.en_US
dc.contributor.authorCoker, R. F.en_US
dc.contributor.authorPerry, T. S.en_US
dc.contributor.authorTaylor, M. J.en_US
dc.contributor.authorKhokhlov, A. M.en_US
dc.contributor.authorDrake, R. Paulen_US
dc.contributor.authorBennett, G. R.en_US
dc.contributor.authorSinars, D. B.en_US
dc.contributor.authorCampbell, R. B.en_US
dc.date.accessioned2006-09-08T19:54:51Z
dc.date.available2006-09-08T19:54:51Z
dc.date.issued2005-07en_US
dc.identifier.citationRosen, P. A.; Wilde, B. H.; Williams, R. J. R.; Foster, J. M.; Keiter, P. A.; Coker, R. F.; Perry, T. S.; Taylor, M. J.; Khokhlov, A. M.; Drake, R. P.; Bennett, G. R.; Sinars, D. B.; Campbell, R. B.; (2005). "Recent Experimental Results and Modelling of High-Mach-Number Jets and the Transition to Turbulence." Astrophysics and Space Science 298 (1-2): 121-128. <http://hdl.handle.net/2027.42/42047>en_US
dc.identifier.issn0004-640Xen_US
dc.identifier.issn1572-946Xen_US
dc.identifier.urihttps://hdl.handle.net/2027.42/42047
dc.description.abstractIn recent years, we have carried out experiments at the University of Rochester’s Omega laser in which supersonic, dense-plasma jets are formed by the interaction of strong shocks in a complex target assembly (Foster et al., Phys. Plasmas 9 (2002) 2251). We describe recent, significant extensions to this work, in which we consider scaling of the experiment, the transition to turbulence, and astrophysical analogues. In new work at the Omega laser, we are developing an experiment in which a jet is formed by laser ablation of a titanium foil mounted over a titanium washer with a central, cylindrical hole. Some of the resulting shocked titanium expands, cools, and accelerates through the vacuum region (the hole in the washer) and then enters a cylinder of low-density foam as a jet. We discuss the design of this new experiment and present preliminary experimental data and results of simulations using AWE hydrocodes. In each case, the high Reynolds number of the jet suggests that turbulence should develop, although this behaviour cannot be reliably modelled by present, resolution-limited simulations (because of their low-numerical Reynolds number).en_US
dc.format.extent254807 bytes
dc.format.extent3115 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherKluwer Academic Publishers; Springer Science + Business Media, Inc.en_US
dc.subject.otherPhysicsen_US
dc.subject.otherAstronomyen_US
dc.subject.otherJetsen_US
dc.subject.otherTurbulenceen_US
dc.subject.otherLaboratory Astrophysicsen_US
dc.subject.otherSupernovaeen_US
dc.titleRecent Experimental Results and Modelling of High-Mach-Number Jets and the Transition to Turbulenceen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelAstronomyen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumUniversity of Michigan, USAen_US
dc.contributor.affiliationotherAWE, Aldermaston, UKen_US
dc.contributor.affiliationotherLos Alamos National Laboratory, USAen_US
dc.contributor.affiliationotherAWE, Aldermaston, UKen_US
dc.contributor.affiliationotherAWE, Aldermaston, UKen_US
dc.contributor.affiliationotherLos Alamos National Laboratory, USAen_US
dc.contributor.affiliationotherLos Alamos National Laboratory, USAen_US
dc.contributor.affiliationotherLawrence Livermore National Laboratory, USAen_US
dc.contributor.affiliationotherAWE, Aldermaston, UKen_US
dc.contributor.affiliationotherUniversity of Chicago, USAen_US
dc.contributor.affiliationotherSandia National Laboratories, Albuquerque, USAen_US
dc.contributor.affiliationotherSandia National Laboratories, Albuquerque, USAen_US
dc.contributor.affiliationotherSandia National Laboratories, Albuquerque, USAen_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/42047/1/10509_2005_Article_3921.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1007/s10509-005-3921-5en_US
dc.identifier.sourceAstrophysics and Space Scienceen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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