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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
IdentifierQABCDSTQQW/46AC7UB
Repositoryurlib.net/www/2022/02.03.21.42   (restricted access)
Last Update2022:02.03.21.42.27 (UTC) simone
Metadata Repositoryurlib.net/www/2022/02.03.21.42.27
Metadata Last Update2023:01.03.23.29.30 (UTC) simone
DOI10.26464/epp2022006
ISSN2096-3955
Citation KeyFrancoEcheBolzFrae:2022:MaExOb
TitleStudy of fluctuations in the Martian magnetosheath using a kurtosis technique: Mars Express observations
Year2022
Access Date2024, May 14
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size4071 KiB
2. Context
Author1 Franco, Adriane Marques de Souza
2 Echer, Ezequiel
3 Bolzan, M. J. A.
4 Fraenz, M.
Resume Identifier1
2 8JMKD3MGP5W/3C9JH3D
Group1
2 DIHPA-CGCE-INPE-MCTI-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE) 
2 Instituto Nacional de Pesquisas Espaciais (INPE) 
3 Universidade Federal de Jatai 
4 Mak Planck for Solar System Research
Author e-Mail Address1 adriane.marquesds@gmail.com 
2 ezequiel.echer@inpe.br
JournalEarth and Planetary Physics
Volume6
Number1
Pages28-41
History (UTC)2022-02-03 21:43:19 :: simone -> administrator :: 2022
2023-01-03 16:46:29 :: administrator -> simone :: 2022
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsMars magnetosheath
kurtosis
ULF waves
AbstractPlanetary magnetosheaths are characterized by high plasma wave and turbulence activity. The Martian magnetosheath is no exception; both upstream and locally generated plasma waves have been observed in the region between its bow shock and magnetic boundary layer, its induced magnetosphere. This statistical study of wave activity in the Martian magnetosheath is based on 12 years (2005-2016) of observations made during Mars Express (MEX) crossings of the planet's magnetosheath - in particular, data on electron density and temperature data collected by the electron spectrometer (ELS) of the plasma analyzer (ASPERA-3) experiment on board the MEX spacecraft. A kurtosis parameter has been calculated for these plasma parameters. This value indicates intermittent behavior in the data when it is higher than 3 (the value for a normal or Gaussian distribution). The variation of wave activity occurrence has been analyzed in relation to solar cycle, Martian orbit, and distance to the bow shock. Non-Gaussian properties are observed in the magnetosheath of Mars on all analyzed scales, especially in those near the proton gyrofrequency in the upstream region of the Martian magnetosphere. We also report that non-Gaussian behavior is most prominent at the smaller scales (higher frequencies). A significant influence of the solar cycle was also observed; the kurtosis parameter is higher during declining and solar maximum phases, when the presence of disturbed solar wind conditions, caused by large scale solar wind structures, increases. The kurtosis decreases with increasing distance from the bow shock, which indicates that the intermittence level is higher near the bow shock. In the electron temperature data the kurtosis is higher near the perihelion due to the higher incidence of EUV when the planet is closer to the Sun, which causes a more extended exosphere, and consequently increases the wave activity in the magnetosheath and its upstream region. The extended exosphere seems to play a lower effect in the electron density data.
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4. Conditions of access and use
Languageen
Target FileStudy+of+fluctuations+in+the+Martian+magnetosheath+using+a+kurtosis+technique_+Mars+Express+observations.pdf
User Groupself-uploading-INPE-MCTI-GOV-BR
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Reader Groupadministrator
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Visibilityshown
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
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Next Higher Units8JMKD3MGPCW/46KTFK8
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.45.47 5
sid.inpe.br/bibdigital/2022/04.03.17.52 2
DisseminationWEBSCI; SCOPUS.
Host Collectionurlib.net/www/2021/06.04.03.40
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