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dc.contributor.authorGutynska, O.
dc.contributor.authorŠafránková, J.
dc.contributor.authorNěmeček, Z.
dc.contributor.authorRichardson, John D.
dc.date.accessioned2015-03-04T19:47:13Z
dc.date.available2015-03-04T19:47:13Z
dc.date.issued2010-10
dc.date.submitted2010-07
dc.identifier.issn2041-8205
dc.identifier.issn2041-8213
dc.identifier.urihttp://hdl.handle.net/1721.1/95817
dc.description.abstractThe crossing of the termination shock (TS) by Voyager 2 in 2007 at 84 AU allows a comparison of fluctuations in different heliosheath regions. The Letter concentrates on MHD waves that exhibit a significant correlation between the magnetic field strength and plasma density. The correlations between both quantities were computed on 2?hr time intervals in the frequency range of 1 × 10[superscript -4] to 4 × 10[superscript -3] Hz. We separate the data into two regions with different magnetic field behavior; the post-TS region with many crossings of the current sheet and the unipolar region where the magnetic field direction remains nearly constant. We find that typical correlation coefficients in these regions are about 0.55-0.65, larger than in Earth's magnetosheath. The largest correlations occur when the spectrum of magnetic field fluctuations is dominated by low frequencies.en_US
dc.description.sponsorshipGrant Agency of the Czech Republic (Contract 205/09/0170)en_US
dc.description.sponsorshipGrant Agency of the Czech Republic (Contract 205/07/0694)en_US
dc.description.sponsorshipGrant Agency of the Czech Republic (Contract 202/08/H057)en_US
dc.description.sponsorshipCzech Republic. Ministry of Education (Research Plan 0021620860)en_US
dc.description.sponsorshipUnited States. National Aeronautics and Space Administration (Voyager Project)en_US
dc.description.sponsorshipUnited States. National Aeronautics and Space Administration (Grant NNX08AC04G)en_US
dc.language.isoen_US
dc.publisherIOP Publishingen_US
dc.relation.isversionofhttp://dx.doi.org/10.1088/2041-8205/722/2/l228en_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.titleCORRELATIONS OF PLASMA DENSITY AND MAGNETIC FIELD STRENGTH IN THE HELIOSHEATHen_US
dc.typeArticleen_US
dc.identifier.citationGutynska, O., J. Šafránková, Z. Němeček, and J. D. Richardson. “CORRELATIONS OF PLASMA DENSITY AND MAGNETIC FIELD STRENGTH IN THE HELIOSHEATH.” The Astrophysical Journal 722, no. 2 (October 5, 2010): L228–L232. © 2010 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.journalAstrophysical 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.orderedauthorsGutynska, O.; Šafránková, J.; Němeček, Z.; Richardson, J. D.en_US
mit.licensePUBLISHER_POLICYen_US
mit.metadata.statusComplete


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