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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZGivnJVY/M2hk9
Repositorysid.inpe.br/mtc-m16@80/2006/08.01.19.11   (restricted access)
Last Update2013:02.06.11.06.14 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m16@80/2006/08.01.19.11.50
Metadata Last Update2021:07.28.21.27.13 (UTC) administrator
Secondary KeyINPE--PRE/
DOI10.1029/2005SW000200
ISSN1539-4956
Citation KeyEcherGonzAlve:2006:GeEfSo
TitleOn the geomagnetic effects of solar wind interplanetary magnetic structures
Year2006
Access Date2024, May 02
Secondary TypePRE PI
Number of Files1
Size447 KiB
2. Context
Author1 Echer, Ezequiel
2 Gonzalez, Walter Demétrio
3 Alves, Maria Virgínia
Group1 DGE-INPE-MCT-BR
2 DGE-INPE-MCT-BR
3 DGE-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais, Divisão de Geofísica Espacial (INPE.DGE)
2 Instituto Nacional de Pesquisas Espaciais, Divisão de Geofísica Espacial (INPE.DGE)
3 Instituto Nacional de Pesquisas Espaciais, Divisão de Geofísica Espacial (INPE.DGE)
JournalSpace Weather
Volume4
Number6
Pages1-11
History (UTC)2006-08-01 19:11:50 :: simone -> administrator ::
2008-06-10 22:43:12 :: administrator -> banon ::
2008-11-05 17:59:18 :: banon -> administrator ::
2012-11-24 01:56:35 :: administrator -> simone :: 2006
2013-02-06 11:06:14 :: simone -> administrator :: 2006
2021-07-28 21:27:13 :: administrator -> marciana :: 2006
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Keywordsmagnetosphere
solar wind
space weather
AbstractWe present in this work a statistical study of the geoeffectiveness of the solar wind magnetic interplanetary structures over the entire observational period (19642003). The structures studied were magnetic clouds (MCs, 170 events), corotating interaction regions (CIRs, 727 events) and interplanetary shocks (830 events). The geoeffectiveness was assessed in terms of the geomagnetic index Kp, AE, and Dst peak values within 2 days after the interplanetary structure had passed near Earth's orbit. Frequency distributions were obtained that give the probability of every interplanetary structure being followed by intense, moderate, weak, or quiet (none) magnetic activity levels. The knowledge of probability distribution is important in schemes to forecast space weather conditions after the detection, by in situ solar wind observations, of an interplanetary structure approaching Earth. We observed that magnetic clouds are more efficient than shocks or CIRs in producing all the geomagnetic activity disturbances; CIRs are themselves more geoeffective as measured by the AE activity. We have confirmed that compound structures (shocks plus MCs) are more geoeffective in every type of magnetospheric activity than isolated structures.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > On the geomagnetic...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
User Groupadministrator
banon
simone
Visibilityshown
Archiving Policydenypublisher denyfinaldraft
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
DisseminationWEBSCI
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress electronicmailaddress format isbn label lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject targetfile tertiarymark tertiarytype typeofwork url versiontype
7. Description control
e-Mail (login)marciana
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