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Insight into theory-experiment comparisons of wake measurements in the plasmasphere

dc.contributor.authorSamir, Urien_US
dc.contributor.authorComfort, R. H.en_US
dc.contributor.authorSingh, N.en_US
dc.contributor.authorHwang, K. S.en_US
dc.contributor.authorStone, Nobie H.en_US
dc.date.accessioned2006-04-07T20:46:35Z
dc.date.available2006-04-07T20:46:35Z
dc.date.issued1989-07en_US
dc.identifier.citationSamir, U., Comfort, R. H., Singh, N., Hwang, K. S., Stone, N. H. (1989/07)."Insight into theory-experiment comparisons of wake measurements in the plasmasphere." Planetary and Space Science 37(7): 873-880. <http://hdl.handle.net/2027.42/27873>en_US
dc.identifier.urihttp://www.sciencedirect.com/science/article/B6V6T-46YCYDP-9T/2/4cc5156533e4555e9777f1158a8c4339en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/27873
dc.description.abstractCalculated results from a modified one-dimensional time-dependent plasma expansion model are compared with wake measurements of low energy H+ ions made in the plasmasphere which consists of 77-90% H+ and 23 10% He+. The variation of the theoretical-to-experimental results with the H+ ionic Mach number (SH+) in the range 0.5 H+ &lt; 1.2 is shown. It is found that the theoretical model used overestimates the particle flux in the wake by factors of 2 to 6. Possible causes for these differences are examined. Discussions regarding; (1) the shortcomings of using one-dimensional models and other simplifications commonly used in theoretical modeling, (2) the use of measurements from probes having finite angular acceptance in wake studies, and (3) a relative comparison between a three-dimensional neutral approximation and the modified one-dimensional model used here are given. This comparison shows that for the plasmaspheric parameters used here, the application of a neutral particle model yields reasonable results, since the ion thermal motion rather than the local electric field dominates the filling of the wake (particularly for weakly charged bodies). These discussions provide additional insight into such theory-experiment comparisons and should be of practical use.en_US
dc.format.extent650252 bytes
dc.format.extent3118 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherElsevieren_US
dc.titleInsight into theory-experiment comparisons of wake measurements in the plasmasphereen_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, University of Michigan, Ann Arbor, MI 48109, USA; Department of Geophysics and Planetary Sciences, Tel-Aviv University, Israel.en_US
dc.contributor.affiliationotherCenter for Space Plasma and Aeronomic Research, University of Alabama in Huntsville, Huntsville, AL 35899, USA; Department of Physics, NASA/Marshall Space Flight Center, Huntsville, AL 35812, USA.en_US
dc.contributor.affiliationotherCenter for Space Plasma and Aeronomic Research, University of Alabama in Huntsville, Huntsville, AL 35899, USA; Department of Electrical & Computer Engineering, NASA/Marshall Space Flight Center, Huntsville, AL 35812, USA.en_US
dc.contributor.affiliationotherCenter for Space Plasma and Aeronomic Research, University of Alabama in Huntsville, Huntsville, AL 35899, USA; Department of Mechanical Engineering, NASA/Marshall Space Flight Center, Huntsville, AL 35812, USA.en_US
dc.contributor.affiliationotherSpace Science Laboratory, NASA/Marshall Space Flight Center, Huntsville, AL 35812, USA.en_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/27873/1/0000287.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1016/0032-0633(89)90138-4en_US
dc.identifier.sourcePlanetary and Space Scienceen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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