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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/37JTUH8
Repositorysid.inpe.br/mtc-m19@80/2010/06.01.17.52   (restricted access)
Last Update2010:06.01.17.52.40 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m19@80/2010/06.01.17.52.41
Metadata Last Update2018:06.05.04.36.43 (UTC) administrator
Secondary KeyINPE--PRE/
DOI10.1016/j.asr.2009.11.011
ISSN0273-1177
Citation KeyEcherTsurGuar:2010:FoReCI
TitleForward and reverse CIR shocks at 4–5 AU: Ulysses
Year2010
MonthMar.
Access Date2024, Apr. 28
Secondary TypePRE PI
Number of Files1
Size688 KiB
2. Context
Author1 Echer, Ezequiel
2 Tsurutani, Bruce T.
3 Guarnieri, Fernando L.
Resume Identifier1 8JMKD3MGP5W/3C9JH3D
Group1 DGE-CEA-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Jet Propulsion Laboratory
3 Universidade do Vale do Paraiba (UNIVAP)
JournalAdvances in Space Research
Volume2010
Number6
Pages798-803
Secondary MarkB4_ASTRONOMIA_/_FÍSICA B3_CIÊNCIAS_BIOLÓGICAS_I B1_ENGENHARIAS_III B1_ENGENHARIAS_IV B1_GEOCIÊNCIAS B1_INTERDISCIPLINAR
History (UTC)2010-07-05 14:54:46 :: simone -> marciana :: 2010
2011-05-20 15:11:33 :: marciana -> administrator :: 2010
2012-11-20 18:34:13 :: administrator -> banon :: 2010
2013-02-19 13:54:28 :: banon -> administrator :: 2010
2018-06-05 04:36:43 :: administrator -> marciana :: 2010
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsSolar wind
Ulysses
Interplanetary shocks
Corotating interaction regions
AbstractIn this article, we study fast shocks at CIR boundaries during an extended interval of 15 consecutive major high speed solar wind streams in 19921993. Ulysses was 45 AU from the sun. The Abraham-Schrauner shock normal method and the Rankine-Hugoniot relations were used to determine fast shock directions and speeds. Out of 33 potential CIR shocks, 14 were determined to be fast forward shocks (FSs) and 14 were fast reverse shocks (RSs). Of the remaining 5 events, 2 were forward waves and 3 were reverse waves. CIR edges at latitudes below 30o were, for the most part, bounded by fast magnetosonic shocks. The forward shocks were generally quasi-perpendicular (average ènBo = 67o). The reverse shocks were more oblique (average ènBo = 52o), but they extended to all angles. Both FSs and RSs had magnetosonic Mach numbers ranging from 1 to 5 or 6. The average Mach numbers were 2.4 and 2.6 for FSs and RSs, respectively. The shock Mach numbers were noted to generally decrease with increasing latitude. The non-shock events or waves were noted to occur preferentially at high (−30° to −35°) heliolatitudes where stream-stream interactions were presumably weaker. These results are consistent with expectations, indicating the general accuracy of the Abraham-Schrauner technique.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Forward and reverse...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target Fileforward and reverse cir.pdf
User Groupadministrator
banon
simone
Visibilityshown
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Mirror Repositorysid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
Next Higher Units8JMKD3MGPCW/3EU29DP
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionsid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notes
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7. Description control
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