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1. Identity statement
Reference TypeJournal Article
Siteplutao.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W/3UGCR85
Repositorysid.inpe.br/plutao/2019/12.03.13.53.27   (restricted access)
Last Update2019:12.06.14.24.40 (UTC) lattes
Metadata Repositorysid.inpe.br/plutao/2019/12.03.13.53.28
Metadata Last Update2022:03.18.22.12.57 (UTC) administrator
DOI10.26464/epp2019051
ISSN2096-3955
Labellattes: 7391173291748956 1 SouzaFränEcheBolz:2019:StStME
Citation KeySouzaFränEcheBolz:2019:StStME
TitleCorrelation length around Mars: a statistical study with MEX and MAVEN observations
Year2019
Access Date2024, May 17
Secondary TypePRE PI
Number of Files1
Size6388 KiB
2. Context
Author1 Souza, Adriane Marques de
2 Fränz, Markus
3 Echer, Ezequiel
4 Bolzan, Maurício José Alves
Resume Identifier1
2
3 8JMKD3MGP5W/3C9JH3D
Group1 GESAST-CEA-SESPG-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
2
3 ezequiel.echer@inpe.br
JournalEarth and Planetary Physics
Volume3
Pages1-10
History (UTC)2019-12-06 14:24:40 :: lattes -> administrator :: 2019
2022-03-18 22:12:57 :: administrator -> simone :: 2019
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsMars Magnetosphere
Correlation length
ULF waves
AbstractCorrelation lengths of ultra-low-frequency (ULF) waves around Mars were computed for the first time, using data from MEX (electron density from 2004 to 2015) and MAVEN (electron density and magnetic field from 2014 to 2016). Analysis of the MEX data found that, for the frequency range 8 to 50 mHz, correlation length in electron density varied between 13 and 17 seconds (temporal scale) and between 5.5 × 103 km and 6.8 × 103 km (spatial scale). For the MAVEN time interval, correlation length was found to vary between 11 and 16 seconds (temporal scale) and 2 × 103 4.5×103 km in spatial scale. In the magnetic field data, correlation lengths are observed to be between 815 seconds (temporal scale) and between 1 × 103 and 5 × 103 km (spatial scale) over the same frequency range. We observe that the cross sections of the plasma regions at the dayside of Mars are smaller than these correlation lengths in these regions in both analyses, where the correlation length derived from the MEX electron density data was between 5 and 25 times the size of the magnetosheath and the magnetic pile-up region (MPR), respectively. For MAVEN these ratios are about 4 (magnetosheath) and 11 (MPR) in electron density and between 1.5 and 5.5 for magnetic field data, respectively. These results indicate that waves at the magnetosheath/MPR can be related to oscillations in the upper ionosphere. In a local region, wave trains may cause resonance effects at the planetary ionopause, which consequently contributes to the enhanced ion escape from the atmosphere.
AreaCEA
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5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/3F2PBEE
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.45.47 2
sid.inpe.br/bibdigital/2013/10.01.22.11 1
DisseminationWEBSCI
Host Collectiondpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notes
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