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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/37JU35E
Repositorysid.inpe.br/mtc-m19@80/2010/06.01.18.11   (restricted access)
Last Update2010:06.01.18.11.10 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m19@80/2010/06.01.18.11.11
Metadata Last Update2021:07.18.04.02.29 (UTC) administrator
Secondary KeyINPE--PRE/
DOI10.1016/j.jastp.2009.02.009
ISSN1364-6826
Citation KeyEcherTsurGuar:2010:InOrNo
TitleInterplanetary origins of November 2004 superstorms
Year2010
MonthMar.
Access Date2024, Apr. 24
Secondary TypePRE PI
Number of Files1
Size177 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)
JournalJournal of Atmospheric and Solar-Terrestrial Physics
Volume72
Number4
Pages280-284
Secondary MarkB2_ASTRONOMIA_/_FÍSICA B1_CIÊNCIAS_BIOLÓGICAS_I B1_ECOLOGIA_E_MEIO_AMBIENTE B1_ENGENHARIAS_IV B1_GEOCIÊNCIAS A2_INTERDISCIPLINAR
History (UTC)2010-07-05 14:54:46 :: simone -> marciana :: 2010
2011-05-23 03:01:38 :: marciana -> administrator :: 2010
2021-07-18 04:02:29 :: administrator -> marciana :: 2010
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsSuperstorms
Magnetosphere
Solar wind
Space weather
AbstractThe sun was very active in the declining phase of solar cycle 23. Large sunspot active regions gave origin to multiple flare and coronal mass ejection (CME) activity in the interval 20032005. On November 2004, the active region AR 10696 was the origin of dozens of flares and many CMEs. Some events of this solar activity region resulted in two large geomagnetic storms, or superstorms (Dst−250 nT) on November 8, peak Dst=−373 nT, and on November 10, peak Dst=−289 nT. It is the purpose of this article to identify the interplanetary origins of these two superstorms. The southward-directed interplanetary magnetic fields (IMF Bs) that caused the two superstorms were related to a magnetic cloud (MC) field for the first superstorm, and a combination of sheath and MC fields for the second superstorm. However, this simple, classic picture is complicated by the presence of multiple shocks and waves. Six fast-forward shocks and, at least, two reverse waves were observed in the period of the two superstorms. A detailed analysis of these complex interplanetary features is performed in this work.
AreaCEA
Arrangementurlib.net > Fonds > Produção anterior à 2021 > DIDGE > Interplanetary origins of...
doc Directory Contentaccess
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4. Conditions of access and use
Languageen
Target FileInterplanetary origins.pdf
User Groupadministrator
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; 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 documentstage e-mailaddress electronicmailaddress format isbn label lineage mark nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype
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