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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/38U7EQ8
Repositorysid.inpe.br/mtc-m19/2011/01.10.15.46   (restricted access)
Last Update2011:12.06.17.37.40 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m19/2011/01.10.15.46.11
Metadata Last Update2021:07.18.04.01.58 (UTC) administrator
Secondary KeyINPE--PRE/
DOI10.1016/j.jastp.2010.09.020
ISSN1364-6826
Citation KeyEcherTsurGuarKozy:2011:CAEv
TitleInterplanetary fast forward shocks and their geomagnetic effects: CAWSES events
ProjectCNPq agency (PQ-300211/2008-2); FAPESP (project 2008/05607-2)
Year2011
MonthJuly
Access Date2024, May 01
Secondary TypePRE PI
Number of Files1
Size1024 KiB
2. Context
Author1 Echer, E.
2 Tsurutani, B. T.
3 Guarnierid, F. L.
4 Kozyrae, J. U.
Group1 DGE-CEA-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
3 Universidade do Vale do Paraiba (UNIVAP), Sao Jose dos Campos, SP, Brazil
4 University of Michigan, Ann Arbor, MI, USA
e-Mail Addresstereza@sid.inpe.br
JournalJournal of Atmospheric and Solar-Terrestrial Physics
Volume73
Number11-12
Pages1330-1338
Secondary MarkB2_ASTRONOMIA_/_FÍSICA B1_CIÊNCIAS_BIOLÓGICAS_I B1_ECOLOGIA_E_MEIO_AMBIENTE B1_ENGENHARIAS_IV B1_GEOCIÊNCIAS A2_INTERDISCIPLINAR
History (UTC)2011-01-10 16:59:07 :: marciana :: 2010 -> x
2011-08-01 11:56:17 :: marciana :: x -> 2011
2011-11-01 11:45:46 :: marciana -> tereza@sid.inpe.br :: 2011
2011-12-06 17:37:49 :: tereza@sid.inpe.br -> administrator :: 2011
2021-07-18 04:01:58 :: administrator -> tereza@sid.inpe.br :: 2011
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsInterplanetary shocks
AE indices
Substorms
Magnetotail
AbstractThe seven CAWSES interplanetary fast forward shocks and their geomagnetic effects during 20042005 have been analyzed. It is found that the arrival time of the shocks at Earth can be estimated within an accuracy of 5 min. Furthermore, AL decreases are found to occur within 10 min of shock impingement on the magnetopause. It was also determined that there is a direct correlation between the interplanetary magnetic field southward directed (IMF Bs) prior to shock arrival and substorms triggered by the shocks. If the IMF is northward prior to shock arrival, the geomagnetic activity is present but is low. One interpretation of this result is that the preconditioning energy stored in the magnetotail leaks away rapidly. A correlation between substorm peak AL and shock strength (Mach number) has also been noted, which could imply that shock strength is important for the amount of energy released into the magnetosphere/ionosphere.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Interplanetary fast forward...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
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4. Conditions of access and use
Languageen
User Groupadministrator
marciana
tereza@sid.inpe.br
Visibilityshown
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
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
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel electronicmailaddress format isbn label lineage mark nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress readergroup resumeid rightsholder schedulinginformation secondarydate session shorttitle sponsor subject targetfile tertiarymark tertiarytype typeofwork url
7. Description control
e-Mail (login)tereza@sid.inpe.br
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