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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/3E9B7NJ
Repositorysid.inpe.br/mtc-m19/2013/06.09.02.13.28   (restricted access)
Last Update2013:06.19.19.17.12 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m19/2013/06.09.02.13.29
Metadata Last Update2018:06.05.04.14.11 (UTC) administrator
DOI10.1016/j.asr.2012.10.029
ISSN0273-1177
Labelscopus
Citation KeyGonzalezGonz:2013:LoVaGe
TitleLocal-time variations of geomagnetic disturbances during intense geomagnetic storms and possible association with their interplanetary causes
ProjectFundo de Desenvolvimento Científico e Tecnológico e Conselho Nacional de Desenvolvimento Científico e Tecnológico (PQ-342734/2008-2 e PQ-300321/2005-8)
Year2013
Access Date2024, May 19
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size3869 KiB
2. Context
Author1 Gonzalez, Alicia Luisa Clua de
2 Gonzalez, Walter Demetrio
Resume Identifier1
2 8JMKD3MGP5W/3C9JJC4
Group1 DGE-CEA-INPE-MCTI-GOV-BR
2 DGE-CEA-INPE-MCTI-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 alicia@dge.inpe.br
2 gonzalez@dge.inpe.br
e-Mail Addressmarcelo.pazos@inpe.br
JournalAdvances in Space Research
Volume51
Number10
Pages1924-1933
Secondary MarkB1 B1 B1 B1 B2 B3 B4
History (UTC)2018-06-05 04:14:11 :: administrator -> marcelo.pazos@inpe.br :: 2013
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordsgeomagnetic disturbance
geomagnetic fields
geomagnetic indices
intense geomagnetic storms
mid-latitude station
relative intensity
solar-terrestrial relations
temporal evolution
solar energy
storms
geomagnetism
AbstractIn the present paper the local-time variations in the disturbance of the geomagnetic-field horizontal component (H) for eight intense geomagnetic storms that occurred during the descending phase of solar cycle 23 have been analyzed. The study was based on the plot of contour lines of the H-depletion intensity in the plane local time versus universal time (LT-UT maps) with the objective of observing how the morphology and evolution of the ring current is mapped into the surface of the Earth in presence of intense geomagnetic storms. The criterion for the selection of the events was a peak Dst below about-200 nT. The values of the horizontal geomagnetic field were obtained from six mid-latitude stations, with 1 min resolution, and the disturbances were computed by a process similar to that for obtaining the Sym-H geomagnetic index. By means of a cubic spline, the results were interpolated to all longitudes with 6 min in LT spacement. The observed contour maps show, as expected, that the region of largest depletion in H are situated around dusk, as a consequence of the formation of a partial ring current, mainly located in the noon-dusk-midnight hemisphere. However, H disturbances are also observed around midnight and, to a less extend, at the noon-dawn sector. In order to detect a prevalent pattern for the behavior of the geomagnetic-disturbance distribution, a statistical analysis was done by means of occurrence histograms, for different levels of the relative intensity of the storm as a function of local time. The relative intensity for each event was defined as a parameter varying between 0 and 1, with 0 (1) corresponding to the maximum (minimum) horizontal field disturbance during that particular event. Although this analysis does not show the temporal evolution of the disturbance, it confirms the above conclusions about its LT distribution. When only the main phases of the storms are considered in the statistics, the basic differences are the dawn peak is lightly shifted towards noon and that the noon-dawn contribution becomes larger. The observed distributions were tentatively associated with the corresponding interplanetary causes of the events. Since among the eight considered storms four are associated to magnetic cloud with a shock interplanetary structure (sMC) and three to sheath regions followed by a magnetic cloud (SH/MC), the statistical study was also performed for the two subsets of storms separately. For the first group (sMC) the LT distribution looks very similar to that of the whole set of storms. On the other hand, it was observed that for the last group (SH/MC) the peak around midnight was not present. This result might be a consequence that these type of storms are probably not associated to the presence of substorms.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Local-time variations of...
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4. Conditions of access and use
Languageen
Target File1-s2.0-S0273117712006801-main.pdf
User Groupadministrator
marcelo.pazos@inpe.br
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Reader Groupadministrator
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Visibilityshown
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Mirror Repositoryiconet.com.br/banon/2006/11.26.21.31
Next Higher Units8JMKD3MGPCW/3EU29DP
Citing Item Listsid.inpe.br/bibdigital/2013/10.01.22.11 2
sid.inpe.br/mtc-m21/2012/07.13.15.01.50 2
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX; SCOPUS.
Host Collectionsid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel format isbn lineage mark month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url
7. Description control
e-Mail (login)marcelo.pazos@inpe.br
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