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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/3AQNQ98
Repositorysid.inpe.br/mtc-m19/2011/11.17.16.49   (restricted access)
Last Update2011:12.06.16.59.59 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m19/2011/11.17.16.49.29
Metadata Last Update2022:03.05.04.16.46 (UTC) administrator
Secondary KeyINPE--PRE/
DOI10.1016/j.jastp.2010.07.024
ISSN1364-6826
Citation KeyAlvesEcheGonz:2011:GeSoWi
TitleGeoeffectiveness of solar wind interplanetary magnetic structures
ProjectFAPESP[2007/52533-1, 2008/06650-9]; CNPq/PQ[300211/2008-2]; CNPq[304865/2007-9]
Year2011
MonthJul
Access Date2024, May 04
Secondary TypePRE PI
Number of Files1
Size405 KiB
2. Context
Author1 Alves, M. V.
2 Echer, E.
3 Gonzalez, W. D.
Group1 GB-GB-INPE-MCT-BR
2 DGE-CEA-INPE-MCT-BR
3 DGE-CEA-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
e-Mail Addresstereza@sid.inpe.br
JournalJournal of Atmospheric and Solar-Terrestrial Physics
Volume73
Number11-12
Pages1380-1384
Secondary MarkB2_ASTRONOMIA_/_FÍSICA B1_CIÊNCIAS_BIOLÓGICAS_I B1_ECOLOGIA_E_MEIO_AMBIENTE B1_ENGENHARIAS_IV B1_GEOCIÊNCIAS A2_INTERDISCIPLINAR
History (UTC)2011-11-17 16:49:29 :: tereza@sid.inpe.br -> administrator ::
2011-11-17 16:49:30 :: administrator -> tereza@sid.inpe.br :: 2011
2011-12-08 16:24:27 :: tereza@sid.inpe.br -> marciana :: 2011
2011-12-08 16:39:35 :: marciana -> administrator :: 2011
2022-03-05 04:16:46 :: administrator -> marciana :: 2011
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsSolar wind
Geomagnetic storm
Interplanetary magnetic structures
Probability distribution functions
AbstractWe address the geoeffectiveness of three interplanetary structures in the interplanetary space: magnetic clouds (MCs), interplanetary shocks (IPSs), and corotating interaction regions (CIRs). The geoeffectiveness is evaluated using the geomagnetic indices Kp. AE, and Dst. We find that MCs are more geoeffective than IPSs, or CIRs. The average values of magnetic indices are significantly enhanced during disturbed periods associated with MCs, IPSs and CIRs, compared to the whole interval. The highest effect is noted for MC disturbed periods. Results obtained for the three data sets are used to derive a theoretical (continuous) probability distribution function (PDF) by fitting the histograms representing the percentage of events against the intervals of magnetic index. PDFs allow estimation of the probability of a given level of geomagnetic activity to be reached after the detection, by in situ solar wind observations, of a given interplanetary structure approaching the Earth.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Geoeffectiveness of solar...
Arrangement 2urlib.net > BDMCI > Fonds > Produção anterior à 2021 > GBDIR > Geoeffectiveness of solar...
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4. Conditions of access and use
Languageen
User Groupadministrator
marciana
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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
8JMKD3MGPCW/449S7R5
DisseminationWEBSCI; PORTALCAPES; AGU; MGA; COMPENDEX.
Host Collectionsid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notes
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