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Kinetic‐Scale Turbulence in the Venusian Magnetosheath
dc.contributor.authorBowen, T. A.
dc.contributor.authorBale, S. D.
dc.contributor.authorBandyopadhyay, R.
dc.contributor.authorBonnell, J. W.
dc.contributor.authorCase, A.
dc.contributor.authorChasapis, A.
dc.contributor.authorChen, C. H. K.
dc.contributor.authorCurry, S.
dc.contributor.authorDudok de Wit, T.
dc.contributor.authorGoetz, K.
dc.contributor.authorGoodrich, K.
dc.contributor.authorGruesbeck, J.
dc.contributor.authorHalekas, J.
dc.contributor.authorHarvey, P. R.
dc.contributor.authorHowes, G. G.
dc.contributor.authorKasper, J. C.
dc.contributor.authorKorreck, K.
dc.contributor.authorLarson, D.
dc.contributor.authorLivi, R.
dc.contributor.authorMacDowall, R. J.
dc.contributor.authorMalaspina, D. M.
dc.contributor.authorMallet, A.
dc.contributor.authorMcManus, M. D.
dc.contributor.authorPage, B.
dc.contributor.authorPulupa, M.
dc.contributor.authorRaouafi, N.
dc.contributor.authorStevens, M. L.
dc.contributor.authorWhittlesey, P.
dc.date.accessioned2021-02-04T21:54:00Z
dc.date.available2022-02-04 16:53:58en
dc.date.available2021-02-04T21:54:00Z
dc.date.issued2021-01-28
dc.identifier.citationBowen, T. A.; Bale, S. D.; Bandyopadhyay, R.; Bonnell, J. W.; Case, A.; Chasapis, A.; Chen, C. H. K.; Curry, S.; Dudok de Wit, T.; Goetz, K.; Goodrich, K.; Gruesbeck, J.; Halekas, J.; Harvey, P. R.; Howes, G. G.; Kasper, J. C.; Korreck, K.; Larson, D.; Livi, R.; MacDowall, R. J.; Malaspina, D. M.; Mallet, A.; McManus, M. D.; Page, B.; Pulupa, M.; Raouafi, N.; Stevens, M. L.; Whittlesey, P. (2021). "Kinetic‐Scale Turbulence in the Venusian Magnetosheath." Geophysical Research Letters 48(2): n/a-n/a.
dc.identifier.issn0094-8276
dc.identifier.issn1944-8007
dc.identifier.urihttps://hdl.handle.net/2027.42/166266
dc.description.abstractWhile not specifically designed as a planetary mission, NASA’s Parker Solar Probe (PSP) mission uses a series of Venus gravity assists (VGAs) in order to reduce its perihelion distance. These orbital maneuvers provide the opportunity for direct measurements of the Venus plasma environment at high cadence. We present first observations of kinetic scale turbulence in the Venus magnetosheath from the first two VGAs. In VGA1, PSP observed a quasi‐parallel shock, β ∼ 1 magnetosheath plasma, and a kinetic range scaling of k−2.9. VGA2 was characterized by a quasi‐perpendicular shock with β ∼ 10, and a steep k−3.4 spectral scaling. Temperature anisotropy measurements from VGA2 suggest an active mirror mode instability. Significant coherent waves are present in both encounters at sub‐ion and electron scales. Using conditioning techniques to exclude these electromagnetic wave events suggests the presence of developed sub‐ion kinetic turbulence in both magnetosheath encounters.Key PointsObservations from Parker Solar Probe reveal kinetic scale turbulence in the Venus magnetosheathDifferences in kinetic range spectral indices between flyby‐encounters are possibly due to shock geometry and kinetic plasma instabilities
dc.publisherWiley Periodicals, Inc.
dc.publisherCambridge University Press
dc.subject.otherplasma
dc.subject.otherInstability
dc.subject.otherkinetic
dc.subject.otherPSP
dc.subject.otherturbulence
dc.subject.otherVenus
dc.titleKinetic‐Scale Turbulence in the Venusian Magnetosheath
dc.typeArticle
dc.rights.robotsIndexNoFollow
dc.subject.hlbsecondlevelGeological Sciences
dc.subject.hlbtoplevelScience
dc.description.peerreviewedPeer Reviewed
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/166266/1/grl61662.pdf
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/166266/2/grl61662_am.pdf
dc.identifier.doi10.1029/2020GL090783
dc.identifier.doihttps://dx.doi.org/10.7302/189
dc.identifier.sourceGeophysical Research Letters
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dc.working.doi10.7302/189en
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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