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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/48R8TS8
Repositorysid.inpe.br/mtc-m21d/2023/04.03.13.49   (restricted access)
Last Update2023:04.03.13.49.25 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2023/04.03.13.49.25
Metadata Last Update2024:01.02.17.16.41 (UTC) administrator
DOI10.1016/j.asr.2022.12.022
ISSN0273-1177
1879-1948
Citation KeyEcherFraMagBolHaj:2023:StNeDa
TitleStudy of Neptune dayside magnetosheath fluctuations during Voyager-2 flyby
Year2023
MonthApr.
Access Date2024, May 17
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size1480 KiB
2. Context
Author1 Echer, Ezequiel
2 Franco, Adriane Marques de Souza
3 Magalhães, Fabiola Pinho
4 Bolzan, Mauricio J. A.
5 Hajra, Rajkumar
Resume Identifier1 8JMKD3MGP5W/3C9JH3D
Group1 DIHPA-CGCE-INPE-MCTI-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Universidade Federal do Sul e Sudoeste do Pará
3 Pesquisador independente
4 Instituto Federal de Jataí
5 Indian Institute of Technology Indore
Author e-Mail Address1 ezequiel.echer@gmail.com
JournalAdvances in Space Research
Volume71
Number8
Pages3468-3478
Secondary MarkB1_INTERDISCIPLINAR B1_GEOCIÊNCIAS B1_ENGENHARIAS_IV B1_ENGENHARIAS_III B1_BIODIVERSIDADE B3_CIÊNCIA_DA_COMPUTAÇÃO B4_ASTRONOMIA_/_FÍSICA C_CIÊNCIAS_BIOLÓGICAS_I
History (UTC)2023-04-03 13:49:25 :: simone -> administrator ::
2023-04-03 13:49:26 :: administrator -> simone :: 2023
2023-04-03 13:50:25 :: simone -> administrator :: 2023
2024-01-02 17:16:41 :: administrator -> simone :: 2023
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsNeptune
Voyager
Solar wind
Waves
Turbulence
Magnetosheath
AbstractTurbulence in the outer planetary magnetospheres has been relatively less studied than in the Earth's magnetosphere, especially for the ice giants which have been visited only by the Voyager-2 spacecraft so far. The aim of this work is to study the turbulence in Nep-tune's dayside magnetosheath. Voyager-2 magnetometer 3-s averaged magnetic field data were analyzed with several data analysis tech-niques. It was found that most of the magnetosheath magnetic field is aligned in the BT direction. The BR-component spectrum showed the predominance of short-period (5 minutes) oscillations, while the BT- and BN- components showed the occurrence of longer-period (20-50 minutes) oscillations. The Fourier spectrum of the magnetic field showed a breakpoint near 0.00165 Hz. The lower frequency por-tion showed index (absolute values) smaller than 1.0. The higher frequency portion showed a much steeper spectrum, with power law values varying from about 2.0 to 2.4. The statistical kurtosis parameters for BR and BN are higher than 3 in almost all scales, while the BT component (main field direction) has a more Gaussian or sub-Gaussian behavior, specially in scales higher than 20 minutes. The kurtosis is very high at the low frequency spectral power of 40 minutes for the BN-component, indicating asymmetric or non -Gaussian magnetic field distribution in the magnetosheath. The multifractal spectrum is well spread in the magnetosheath revealing a rich and dynamic activity in this region. Overall, the Neptune's magnetosheath is found to have a strong turbulence activity that is com-parable to that of other planetary magnetosheaths.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Study of Neptune...
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Languageen
Target File1-s2.0-S0273117722011309-main.pdf
User Groupsimone
Reader Groupadministrator
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Visibilityshown
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Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/46KTFK8
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.45.47 5
DisseminationWEBSCI; PORTALCAPES; COMPENDEX; SCOPUS.
Host Collectionurlib.net/www/2021/06.04.03.40
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