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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
Metadatasid.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 Date2021, July 25
Number of Files1
Size177 KiB
Context area
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 TypePRE PI
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
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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 > BDMCI > Fonds > Produção > DIDGE > Interplanetary origins of...
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Languageen
Target FileInterplanetary origins.pdf
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simone
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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
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