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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/36HQJT5
Repositorysid.inpe.br/mtc-m19@80/2009/12.10.18.05   (restricted access)
Last Update2009:12.10.18.05.38 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m19@80/2009/12.10.18.05.39
Metadata Last Update2018:06.05.04.36.03 (UTC) administrator
Secondary KeyINPE--PRE/
DOI10.1016/j.asr.2009.05.003
ISSN0273-1177
Citation KeyEcherTsurGuar:2009:SoInOr
TitleSolar and interplanetary origins of the November 2004 superstorms
Year2009
MonthSept.
Access Date2024, Apr. 27
Secondary TypePRE PI
Number of Files1
Size410 KiB
2. Context
Author1 Echer, Ezequiel
2 Tsurutani, Bruce T.
3 Guarnieri, Fernando Luis
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)
JournalAdvances in Space Research
Volume44
Number5
Pages615-620
Secondary MarkB3_CIÊNCIAS_BIOLÓGICAS_I B1_ENGENHARIAS_III B2_ENGENHARIAS_IV B1_GEOCIÊNCIAS A2_INTERDISCIPLINAR
History (UTC)2009-12-10 18:05:59 :: simone -> administrator ::
2010-05-11 01:02:52 :: administrator -> simone ::
2011-05-23 02:40:36 :: simone -> administrator ::
2012-11-20 18:34:03 :: administrator -> banon :: 2009
2013-02-19 13:54:21 :: banon -> administrator :: 2009
2018-06-05 04:36:03 :: administrator -> marciana :: 2009
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsGeomagnetic storms
Solar flares
CMEs
Shocks
Magnetic clouds
AbstractDuring the first half of November 2004, many solar flares and coronal mass ejections (CMEs) were associated with solar active region (AR) 10696. This paper attempts to identify the solar and interplanetary origins of two superstorms which occurred on 8 and 10 November with peak intensities of Dst = −373 nT and −289 nT, respectively. Southward interplanetary magnetic fields within a magnetic cloud (MC), and a sheath + MC were the causes of these two superstorms, respectively. Two different CME propagation models [Gopalswamy, N., Yashiro, S., Kaiser, M.L. et al. Predicting the 1-AU arrival times of coronal mass ejections. J. Geophys. Res. 106, 2920729219, 2001; Gopalswamy, N.S., Lara, A., Manoharan, P.K. et al. An empirical model to predict the 1-AU arrival of interplanetary shocks. Adv. Space Res. 36, 22892294, 2005] were employed to attempt to identify the solar sources. It is found that the models identify several potential CMEs as possible sources for each of the superstorms. The two Gopalswamy et al. models give the possible sources for the first superstorm as CMEs on 2330 UT 4 November 2004 or on 1454 UT 5 November 2004. For the second superstorm, the possible solar source was a CME that on 0754 UT 5 November 2004 or one that occurred on 1206 UT 5 November 2004. We note that other propagation models sometimes agree and other times disagree with the above results. It is concluded that during high solar/interplanetary activity intervals such as this one, the exact solar source is difficult to identify. More refined propagation models are needed.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Solar and interplanetary...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target Filesolar and interplanetary.pdf
User Groupadministrator
banon
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; 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
7. Description control
e-Mail (login)marciana
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