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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3U9RRDB
Repositorysid.inpe.br/mtc-m21c/2019/10.24.11.39
Last Update2019:10.24.11.39.11 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2019/10.24.11.39.11
Metadata Last Update2021:02.11.02.00.14 (UTC) administrator
DOI10.5194/angeo-37-919-2019
ISSN0992-7689
Citation KeyFrancoEcheBolz:2019:WaAnMa
TitleWavelet analysis of the magnetotail response to solar wind fluctuations during HILDCAA events
Year2019
MonthOct.
Access Date2024, May 17
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size3185 KiB
2. Context
Author1 Franco, Adriane Marques de Souza
2 Echer, Ezequiel
3 Bolzan, Maurício José Alves
Resume Identifier1
2 8JMKD3MGP5W/3C9JH3D
Group1 YYY-CGCEA-INPE-MCTIC-GOV-BR
2 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Universidade Federal de Jataí
Author e-Mail Address1 adrianemarquesds@gmail.com
2 ezequiel.echer@inpe.br
JournalAnnales Geophysicae
Volume37
Number5
Pages919-929
Secondary MarkA2_INTERDISCIPLINAR A2_GEOCIÊNCIAS A2_ENGENHARIAS_I B2_CIÊNCIAS_BIOLÓGICAS_I B2_ASTRONOMIA_/_FÍSICA
History (UTC)2019-10-24 11:39:11 :: simone -> administrator ::
2019-10-24 11:39:12 :: administrator -> simone :: 2019
2019-10-24 11:39:46 :: simone -> administrator :: 2019
2021-02-11 02:00:14 :: administrator -> simone :: 2019
3. Content and structure
Is the master or a copy?is the master
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Content TypeExternal Contribution
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AbstractIn this work a study of the effects of the highintensity long-duration continuous AE activity (HILDCAAs) events in the magnetotail was conducted. The aim of this study was to search the main frequencies during HILDCAAs in the Bx component of the geomagnetic field in the magnetotail, as well as the main frequencies, at which the magnetotail responds to the solar wind during these events. In order to conduct this analysis the wavelet transform was employed during nine HILDCAA events that coincided with Cluster spacecraft mission crossing through the tail of the magnetosphere from 2003 to 2007. The most energetic periods for each event were identified. It was found that 76 % of them have periods ≤ 4 h. With the aim to search the periods that have the highest correlation between the IMF Bz (OMNI) component and the Cluster Bx geomagnetic field component, the cross wavelet analysis technique was also used in this study. The majority of correlation periods between the Bz (IMF) and Bx component of the geomagnetic field observed also were ≤ 4 h, with 62.9 % of the periods. Thus the magnetotail responds stronger to IMF fluctuations during HILDCCAS at 24 h scales, which are typical substorm periods. The results obtained in this work show that these scales are the ones on which the coupling of energy is stronger, as well as the modulation of the magnetotail by the solar wind during HILDCAA events.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Wavelet analysis of...
Arrangement 2urlib.net > BDMCI > Fonds > Produção anterior à 2021 > YYY-PCI-CGCEA > Wavelet analysis of...
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W34R/3U9RRDB
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34R/3U9RRDB
Languageen
Target Filefranco-wavelet.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policyallowpublisher allowfinaldraft
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/4467GD8
Citing Item Listsid.inpe.br/bibdigital/2021/02.11.01.58 6
sid.inpe.br/mtc-m21/2012/07.13.14.45.47 3
sid.inpe.br/bibdigital/2013/10.01.22.11 1
DisseminationWEBSCI; PORTALCAPES; COMPENDEX; SCOPUS.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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