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dc.contributor.authorWang, C.
dc.contributor.authorRichardson, John D.
dc.date.accessioned2015-02-17T15:45:09Z
dc.date.available2015-02-17T15:45:09Z
dc.date.issued2012-10
dc.date.submitted2012-09
dc.identifier.issn2041-8205
dc.identifier.issn2041-8213
dc.identifier.urihttp://hdl.handle.net/1721.1/94554
dc.description.abstractVoyager 2 (V2) entered the heliosheath in 2007 August at roughly the same time solar minimum conditions were reaching the outer heliosphere. Soon after crossing the termination shock the solar wind density at Voyager decreased by a factor of two and the temperature decreased by a factor of three. At the beginning of 2011 the plasma density in the heliosheath began to increase and in mid-2012 it was up by more than a factor of two. The temperature rose by about 50% and the speed remained constant, although the flow direction continues to turn tailward. These changes may signal the end of solar minimum conditions at V2 in the heliosheath, although we do not understand why the speed did not decrease. The increased dynamic pressure has lead to an outward movement of the termination shock from its very compressed state at solar minimum.en_US
dc.description.sponsorshipJet Propulsion Laboratory (U.S.) (United States. National Aeronautics and Space Administration Contract 959203)en_US
dc.description.sponsorshipUnited States. National Aeronautics and Space Administration (Grant NNX08AE49G)en_US
dc.language.isoen_US
dc.publisherIOP Publishingen_US
dc.relation.isversionofhttp://dx.doi.org/10.1088/2041-8205/759/1/l19en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceAmerican Astronomical Societyen_US
dc.titleVOYAGER 2 OBSERVES A LARGE DENSITY INCREASE IN THE HELIOSHEATHen_US
dc.typeArticleen_US
dc.identifier.citationRichardson, J. D., and C. Wang. “VOYAGER 2 OBSERVES A LARGE DENSITY INCREASE IN THE HELIOSHEATH.” The Astrophysical Journal 759, no. 1 (October 16, 2012): L19. © 2012 The American Astronomical Societyen_US
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Researchen_US
dc.contributor.mitauthorRichardson, John D.en_US
dc.relation.journalThe Astrophysical Journal. Lettersen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsRichardson, J. D.; Wang, C.en_US
mit.licensePUBLISHER_POLICYen_US
mit.metadata.statusComplete


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