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Does a ‘two-stream’ flow model apply to wakes of large bodies in space?

dc.contributor.authorSamir, Urien_US
dc.contributor.authorStone, Nobie H.en_US
dc.contributor.authorOran, W. A.en_US
dc.date.accessioned2006-09-08T19:56:03Z
dc.date.available2006-09-08T19:56:03Z
dc.date.issued1974-11en_US
dc.identifier.citationSamir, Uri; Stone, N. H.; Oran, W. A.; (1974). "Does a ‘two-stream’ flow model apply to wakes of large bodies in space?." Astrophysics and Space Science 31(1): L1-L8. <http://hdl.handle.net/2027.42/42066>en_US
dc.identifier.issn0004-640Xen_US
dc.identifier.issn1572-946Xen_US
dc.identifier.urihttps://hdl.handle.net/2027.42/42066
dc.description.abstractStructural patterns of ion and electron currents observed on the wake axes of the Ariel J and the Gemini 10 space vehicles are re-examined, together with relevant theoretical and laboratory ‘simulation’, studies. Some insight into existing in-situ data is provided. The possibility that ‘converging-stream’ models describe structural features of current enhancements in the wake region of large spacecraft is discussed.en_US
dc.format.extent398622 bytes
dc.format.extent3115 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherKluwer Academic Publishers; D. Reidel Publishing Company ; Springer Science+Business Mediaen_US
dc.subject.otherPhysicsen_US
dc.subject.otherAstronomyen_US
dc.titleDoes a ‘two-stream’ flow model apply to wakes of large bodies in space?en_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelAstronomyen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumSpace Physics Research Laboratory, Univ. of Michigan, Mich., USA; Dept. of Environmental Sciences, Tel-Aviv Univ., Israelen_US
dc.contributor.affiliationotherSpace Sciences Laboratory, Marshall Space Flight Center, Huntsville, Ala., USAen_US
dc.contributor.affiliationotherSpace Sciences Laboratory, Marshall Space Flight Center, Huntsville, Ala., USAen_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/42066/1/10509_2004_Article_BF00642618.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1007/BF00642618en_US
dc.identifier.sourceAstrophysics and Space Scienceen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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