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Reference TypeJournal Article
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/3822JU5
Repositorysid.inpe.br/mtc-m19@80/2010/08.02.15.05   (restricted access)
Last Update2010:08.02.15.07.44 (UTC) administrator
Metadatasid.inpe.br/mtc-m19@80/2010/08.02.15.05.02
Metadata Last Update2021:07.18.04.02.31 (UTC) administrator
Secondary KeyINPE--PRE/
DOI10.1016/j.jastp.2010.06.007
ISSN1364-6826
Citation KeyTsurutaniEchVerLakGua:2011:MiInUp
TitleMirror instability upstream of the termination shock (TS) and in the heliosheath
Year2011
MonthJuly
Access Date2021, July 25
Number of Files1
Size604 KiB
Context area
Author1 Tsurutani, Bruce T.
2 Echer, Ezequiel
3 Verkhoglyadovar, Olga P.
4 Lakhina, Gurbax S.
5 Guarnieri, F. L.
Resume Identifier1
2 8JMKD3MGP5W/3C9JH3D
Group1
2 DGE-CEA-INPE-MCT-BR
Affiliation1
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3
4 ndian Institute of Geomagnetism, Navi Mumbai, India
5 UNIVAP, Sao Jose dos Campos, SP, Brazil
Author e-Mail Address1 Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
2
3 CSPAR, University of Alabama, Huntsville, AL, USA
e-Mail Addresslise@dpi.inpe.br
JournalJournal of Atmospheric and Solar-Terrestrial Physics
Volume73
Number11–12
Pages1398–1404
Secondary TypePRE PI
Secondary MarkB2_ASTRONOMIA_/_FÍSICA B1_CIÊNCIAS_BIOLÓGICAS_I B1_ECOLOGIA_E_MEIO_AMBIENTE B1_ENGENHARIAS_IV B1_GEOCIÊNCIAS A2_INTERDISCIPLINAR
History (UTC)2011-02-21 17:55:30 :: marciana -> lise@dpi.inpe.br :: 2010
2011-09-13 12:40:32 :: lise@dpi.inpe.br -> marciana :: 2010
2011-12-27 15:23:57 :: marciana -> tereza@sid.inpe.br :: 2010
2012-01-26 11:33:01 :: tereza@sid.inpe.br -> administrator :: 2010 -> 2011
2021-07-18 04:02:31 :: administrator -> tereza@sid.inpe.br :: 2011
Content and structure area
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsMirror instability, Pickup ions, Heliosheath, Magnetosheaths.
AbstractWe experimentally identify mirror mode (MM) structures in the Voyager 1 heliosheath data for the first time. This is done using the magnetic field data alone. The heliosheath MM structures are found to have the following characteristics: (1) quasiperiodic spacings with a typical scale size of not, vert, similar57 ñp, (2) little or no angular changes across the structures (not, vert, similar3° longitude and not, vert, similar3° latitude), and (3) a lack of sharp boundaries at the magnetic dip edges. It is demonstrated that the pickup of interstellar neutrals in the upstream region of the termination shock (TS) and quasiperpendicular TS plasma compression are the causes of MM instability during intervals when the IMF is nearly orthogonal to the solar wind flow direction. Concomitant additional injection of pickup ions (PUIs) throughout the heliosheath will lead to further MM amplification. MM structures in planetary magnetosheaths and interplanetary sheaths are discussed for comparative purposes. Multiple sources of free energy are often involved.
AreaCEA
ArrangementMirror instability upstream...
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Languageen
Target Fileecher.pdf
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lise@dpi.inpe.br
marciana
tereza@sid.inpe.br
Visibilityshown
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Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
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Mirror Repositorysid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
Next Higher Units8JMKD3MGPCW/3EU29DP
DisseminationWEBSCI; PORTALCAPES; AGU; MGA; COMPENDEX.
Host Collectionsid.inpe.br/mtc-m19@80/2009/08.21.17.02
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