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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34P/3MPPUN2
Repositorysid.inpe.br/mtc-m21b/2016/11.11.15.27
Last Update2016:11.11.15.27.15 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21b/2016/11.11.15.27.15
Metadata Last Update2021:07.28.22.15.56 (UTC) administrator
DOI10.1002/2015JA021835
ISSN2169-9402
Citation KeyHajraTsuEchGonGje:2016:MaStSo
TitleSupersubstorms (SML <-2500nT): magnetic storm and solar cycle dependences
Year2016
MonthAug.
Access Date2024, May 17
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size837 KiB
2. Context
Author1 Hajra, Rakjumar
2 Tsurutani, Bruce T.
3 Echer, Ezequiel
4 Gonzalez Alarcon, Walter Demétrio
5 Gjerloev, Jesper W.
Resume Identifier1
2
3 8JMKD3MGP5W/3C9JH3D
4 8JMKD3MGP5W/3C9JJC4
Group1 GES-CEA-SPG-INPE-MCTI-GOV-BR
2
3 DGE-CEA-INPE-MCTI-GOV-BR
4 DGE-CEA-INPE-MCTI-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Jet Propulsion Laboratory
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
5 The Johns Hopkins University Applied Physics Laboratory
Author e-Mail Address1 rajkumarhajra@yahoo.co.in
2
3 eecher@dge.inpe.br
4 walter.alarcon@inpe.br
JournalJournal of Geophysical Research: Space Physics
Volume121
Number8
Pages7805-7816
History (UTC)2016-11-11 15:27:15 :: simone -> administrator ::
2016-11-11 15:27:15 :: administrator -> simone :: 2016
2016-11-11 15:28:01 :: simone -> administrator :: 2016
2016-11-12 13:39:45 :: administrator -> simone :: 2016
2016-12-21 12:05:49 :: simone -> administrator :: 2016
2021-07-28 22:15:56 :: administrator -> simone :: 2016
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractWe study extremely intense substorms with SuperMAG AL (SML) peak intensities < -2500 nT ("supersubstorms"/SSSs) for the period from 1981 to 2012. The SSS events were often found to be isolated SML peaks and not statistical fluctuations of the indices. The SSSs occur during all phases of the solar cycle with the highest occurrence (3.8 year(-1)) in the descending phase. The SSSs exhibited an annual variation with equinoctial maximum altering between spring in solar cycle 22 and fall in solar cycle 23. The occurrence rate and strength of the SSSs did not show any strong relationship with the intensity of the associated geomagnetic storms. All SSS events were associated with strong southward interplanetary magnetic field B-s component. The B-s fields were part of interplanetary magnetic clouds in 46% and of interplanetary sheath fields in 54% of the cases. About 77% of the SSSs were associated with small regions of very high density solar wind plasma parcels or pressure pulses impinging upon the magnetosphere. Comments on how SSS events may cause power outages at Earth are discussed at the end of the paper.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Supersubstorms (SML <-2500nT):...
Arrangement 2urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > GES > Supersubstorms (SML <-2500nT):...
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4. Conditions of access and use
data URLhttp://mtc-m21b.sid.inpe.br/ibi/8JMKD3MGP3W34P/3MPPUN2
zipped data URLhttp://mtc-m21b.sid.inpe.br/zip/8JMKD3MGP3W34P/3MPPUN2
Languageen
Target Filehajra-subt.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policydenypublisher6 allowfinaldraft
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
Mirror Repositoryurlib.net/www/2011/03.29.20.55
Next Higher Units8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/3F2PBEE
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.45.47 5
sid.inpe.br/bibdigital/2013/10.12.21.02 3
sid.inpe.br/bibdigital/2013/10.01.22.11 2
DisseminationWEBSCI; PORTALCAPES; COMPENDEX; SCOPUS.
Host Collectionsid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notes
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