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1. Identity statement
Reference TypeJournal Article
Siteplutao.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
IdentifierJ8LNKAN8RW/3AFLGA8
Repositorydpi.inpe.br/plutao/2011/09.22.19.40   (restricted access)
Last Update2011:12.06.17.27.21 (UTC) administrator
Metadata Repositorydpi.inpe.br/plutao/2011/09.22.19.40.14
Metadata Last Update2021:07.18.04.03.21 (UTC) administrator
DOI10.1016/j.jastp.2011.04.021
ISSN1364-6826
Labellattes: 3869820274542343 1 EcherGonzTsur:2011:StStGe
Citation KeyEcherGonzTsur:2011:StStGe
TitleStatistical studies of geomagnetic storms with peak Dst < -50 nT from 1957 to 2008
ProjectCNPq[PQ-300211/2008-2]; FAPESP[2007/52533-1]; FAPESP agency[2008/06650-9]
Year2011
Monthjuly
Access Date2024, May 05
Secondary TypePRE PI
Number of Files1
Size859 KiB
2. Context
Author1 Echer, Ezequiel
2 Gonzalez, W. D.
3 Tsurutani, B. T.
Resume Identifier1 8JMKD3MGP5W/3C9JH3D
Group1 DGE-CEA-INPE-MCT-BR
2 DGE-CEA-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Jet Propulsion Lab, Pasadena, CA
Author e-Mail Address1 eecher@dge.inpe.br
e-Mail Addresseecher@dge.inpe.br
JournalJournal of Atmospheric and Solar-Terrestrial Physics
Volume73
Number11-12
Pages1454-1459
Secondary MarkB2_ASTRONOMIA_/_FÍSICA B1_CIÊNCIAS_BIOLÓGICAS_I B1_ECOLOGIA_E_MEIO_AMBIENTE B1_ENGENHARIAS_IV B1_GEOCIÊNCIAS A2_INTERDISCIPLINAR
History (UTC)2011-09-23 14:11:21 :: lattes -> administrator :: 2011
2011-10-31 13:51:02 :: administrator -> secretaria.cpa@dir.inpe.br :: 2011
2011-11-01 11:21:21 :: secretaria.cpa@dir.inpe.br -> tereza@sid.inpe.br :: 2011
2011-12-06 17:27:21 :: tereza@sid.inpe.br -> administrator :: 2011
2021-07-18 04:03:21 :: administrator -> tereza@sid.inpe.br :: 2011
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsGeomagnetic storms
Ring current
Magnetosphere
Space weather
AbstractA catalog of 1377 geomagnetic storms with peak Dst (Dst(p)) <= -50 nT for the period 1957-2008 has been compiled. The dependence of Dst(p) on the solar cycle and annual variation are studied in this paper. It is found that geomagnetic storm peak intensity distribution can be described by an exponential form, P(Dst(p)) approximate to 1.2e(-Dstp/34) where P is the probability of geomagnetic storm occurrence with a given value Dstp. The updated solar cycle and annual distribution of geomagnetic storms have confirmed the expected behavior. For the solar cycle variation, geomagnetic storms display a two-peak distribution, with one peak close to solar maximum and the other a few years later in the beginning of the declining phase. Geomagnetic storms follow the well-known seasonal variation of geomagnetic activity. More intense storms show a peak in probability occurrence in July, confirming previous observations. These results are of practical importance for space weather applications.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Statistical studies of...
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4. Conditions of access and use
Languageen
Target FileEcher-JASTP-v73-n11-2-p1454-9.pdf
User Groupadministrator
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tereza@sid.inpe.br
Visibilityshown
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
DisseminationWEBSCI; PORTALCAPES; AGU; MGA; COMPENDEX.
Host Collectiondpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notes
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