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Looking for evidence of mixing in the solar wind from 0.31 to 0.98 AU
dc.contributor.authorBorovsky, Joseph E.en_US
dc.date.accessioned2013-01-03T19:44:46Z
dc.date.available2013-08-01T14:04:41Zen_US
dc.date.issued2012-06en_US
dc.identifier.citationBorovsky, Joseph E. (2012). "Looking for evidence of mixing in the solar wind from 0.31 to 0.98 AU." Journal of Geophysical Research: Space Physics 117(A6): n/a-n/a. <http://hdl.handle.net/2027.42/95482>en_US
dc.identifier.issn0148-0227en_US
dc.identifier.issn2156-2202en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/95482
dc.publisherWiley‐Interscienceen_US
dc.subject.otherHomogenizationen_US
dc.subject.otherMixingen_US
dc.subject.otherPlasmaen_US
dc.subject.otherSolar Winden_US
dc.subject.otherChunk Mixtureen_US
dc.subject.otherTurbulenceen_US
dc.titleLooking for evidence of mixing in the solar wind from 0.31 to 0.98 AUen_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelAstronomy and Astrophysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDepartment of Atmospheric, Oceanic, and Space Sciences, University of Michigan, Ann Arbor, Michigan, USAen_US
dc.contributor.affiliationotherSpace Science Institute, Boulder, Colorado, USAen_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/95482/1/jgra21890.pdf
dc.identifier.doi10.1029/2012JA017525en_US
dc.identifier.sourceJournal of Geophysical Research: Space Physicsen_US
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