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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/42EDFAS
Repositorysid.inpe.br/mtc-m21c/2020/05.05.11.55   (restricted access)
Last Update2020:05.05.11.55.37 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2020/05.05.11.55.37
Metadata Last Update2022:01.04.01.35.07 (UTC) administrator
DOI10.1016/j.asr.2019.09.009
ISSN0273-1177
1879-1948
Citation KeyFrancoFränEcheBolz:2020:WaAnLo
TitleWavelet analysis of low frequency plasma oscillations in the magnetosheath of Mars
Year2020
Monthmay
Access Date2024, May 16
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size1959 KiB
2. Context
Author1 Franco, Adriane Marques de Souza
2 Fränz, M.
3 Echer, Ezequiel
4 Bolzan, M. J. A.
Resume Identifier1
2
3 8JMKD3MGP5W/3C9JH3D
Group1 YYY-CGCEA-INPE-MCTIC-GOV-BR
2
3 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Max Planck Institute for Solar System Research
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Universidade Federal de Jataí
Author e-Mail Address1 drianemarquesds@gmail.com
2
3 ezequiel.echer@inpe.br
JournalAdvances in Space Research
Volume65
Number9
Pages2090-2098
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)2020-05-05 11:55:37 :: simone -> administrator ::
2020-05-05 11:55:37 :: administrator -> simone :: 2020
2020-05-05 11:56:23 :: simone -> administrator :: 2020
2022-01-04 01:35:07 :: administrator -> simone :: 2020
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsInduced magnetosphere of Mars
ULF waves
Wavelet transform
AbstractWavelet analysis was employed to identify the major frequencies present in the plasma oscillations in the Martian magnetosheath. We have selected magnetosheath crossings and applied the Morlet wavelet transform to the electron density and temperature data, obtained from the Analyzer of Space Plasmas and Energetic Atoms experiment (ASPERA-3), onboard the Mars Express (MEX). In a study of 9667 magnetosheath crossings observed from 2005 to 2016, we have found 22,912 frequencies with high wave power between 5 and 60 mHz for the electron density data, For about 2/3 of the high wave power periods (63.3%), the most energetic frequencies were identified in the range 520 mHz. The analysis of the electron temperature data led to similar results, with 61.9% of the highest power frequencies in the 520 mHz range. No significant influence of the solar cycle on the frequencies of ULF waves has been observed in our analysis. The frequencies obtained here are near the O+ gyrofrequency. The main fact that controls the ion gyroradius is the interplanetary magnetic field that is compressed around the planet.
AreaCEA
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4. Conditions of access and use
Languageen
Target Filefranco-wavelet.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/4467GD8
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.45.47 5
sid.inpe.br/bibdigital/2013/10.01.22.11 3
sid.inpe.br/bibdigital/2021/02.11.01.58 2
DisseminationWEBSCI; PORTALCAPES; COMPENDEX; SCOPUS.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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