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Intercomparison among plasma wake models for plasmaspheric and ionospheric conditions

dc.contributor.authorSamir, Urien_US
dc.contributor.authorComfort, R. H.en_US
dc.contributor.authorWright, Jr. , K. H.en_US
dc.contributor.authorStone, Nobie H.en_US
dc.date.accessioned2006-04-07T19:45:31Z
dc.date.available2006-04-07T19:45:31Z
dc.date.issued1987-12en_US
dc.identifier.citationSamir, U., Comfort, R. H., Wright, Jr., K. H., Stone, N. H. (1987/12)."Intercomparison among plasma wake models for plasmaspheric and ionospheric conditions." Planetary and Space Science 35(12): 1477-1487. <http://hdl.handle.net/2027.42/26496>en_US
dc.identifier.urihttp://www.sciencedirect.com/science/article/B6V6T-46YJYWK-1D8/2/c04c04eec79bf0136d23477223fd2119en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/26496
dc.description.abstractIntercomparisons are made among the angular distributions of ions in the wake of a body moving through a space plasma as computed from three different expressions (models). Both subsonic and supersonic relative flows are considered in order to examine the wake current depletion ratios under conditions realistic for the topside ionosphere and plasmasphere. Results of these comparisons demonstrate the importance of including the thermal flux at low Mach numbers and of taking into account the angular acceptance of ion detectors in making theory-experiment comparisons. Gradients in the angular variations of the fluxes are found to be steeper near the wake-ambient interface than closer to the maximum rarefaction region of all models, although quantitatively there is considerable variation among the models. From examining the variations of the wake depletion ratio parametrically with Mach number and normalized potential over ranges characteristic of the plasmasphere and topside ionosphere, we find considerable variation with both parameters, with sensitivity to normalized potential increasing dramatically with Mach number. Overall, however, the Mach number variation appears to be the more significant over this range of parameters.en_US
dc.format.extent1221999 bytes
dc.format.extent3118 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherElsevieren_US
dc.titleIntercomparison among plasma wake models for plasmaspheric and ionospheric conditionsen_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelAtmospheric, Oceanic and Space Sciencesen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumSpace Physics Research Laboratory, The University of Michigan, Ann Arbor, MI 48109, U.S.A.; Department of Geophysics and Planetary Science, Tel-Aviv University, Ramat-Aviv, Israel.en_US
dc.contributor.affiliationotherDepartment of Physics, The University of Alabama in Huntsville, Huntsville, AL 35899, U.S.A.en_US
dc.contributor.affiliationotherDepartment of Physics, The University of Alabama in Huntsville, Huntsville, AL 35899, U.S.A.en_US
dc.contributor.affiliationotherSpace Sciences Laboratory, NASA/Marshall Space Flight Center, Huntsville, AL 35812, U.S.A.en_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/26496/1/0000032.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1016/0032-0633(87)90074-2en_US
dc.identifier.sourcePlanetary and Space Scienceen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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