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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/46G6H38
Repositorysid.inpe.br/mtc-m21d/2022/03.11.12.28   (restricted access)
Last Update2022:03.11.12.28.18 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2022/03.11.12.28.18
Metadata Last Update2023:01.03.23.10.54 (UTC) simone
DOI10.1016/j.jastp.2022.105842
ISSN1364-6826
Citation KeyBolzanEcheFranHajr:2022:IdPlMa
TitleIdentification of the planetary magnetosphere boundaries with the wavelet multi-resolution analysis
Year2022
MonthApr.
Access Date2024, May 14
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size14283 KiB
2. Context
Author1 Bolzan, Maurício José Alves
2 Echer, Ezequiel
3 Franco, Adriane Marques de Souza
4 Hajra, Rajkumar
Resume Identifier1
2 8JMKD3MGP5W/3C9JH3D
Group1
2 DIHPA-CGCE-INPE-MCTI-GOV-BR
3 YYY-CGCE-INPE-MCTI-GOV-BR
Affiliation1 Universidade Federal do Jataí (UFJ) 
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE) 
4 Indian Institute of Technology Indore
Author e-Mail Address1 mauricio_bolzam@ufg.br 
2 ezequiel.echer@gmail.com
JournalJournal of Atmospheric and Solar-Terrestrial Physics
Volume230
Pagese105842
Secondary MarkA1_ENGENHARIAS_I A2_GEOCIÊNCIAS A2_ENGENHARIAS_III B1_INTERDISCIPLINAR B1_ENGENHARIAS_IV B1_BIODIVERSIDADE B2_ASTRONOMIA_/_FÍSICA C_CIÊNCIAS_BIOLÓGICAS_I
History (UTC)2022-03-11 12:28:18 :: simone -> administrator ::
2022-03-11 12:28:19 :: administrator -> simone :: 2022
2022-03-11 12:29:10 :: simone -> administrator :: 2022
2023-01-03 16:46:02 :: administrator -> simone :: 2022
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsHaar wavelet
Planetary bow shocks
Planetary magnetopauses
Planetary magnetosphere
Solar wind
Wavelet analysis
AbstractThe study of the properties and variations of planetary boundaries such as magnetosheaths and bow shocks is an important subject for magnetospheric dynamics and interaction with solar wind. The identification of these boundaries is important for those studies. Thus, the Haar wavelet decomposition technique is used to detect the planetary magnetosphere boundaries and discontinuities. We use the magnetometer data from the CASSINI and MESSENGER spacecraft to identify the abrupt changes in the magnetic field when the spacecraft crossed the magnetospheric bow shocks and magnetopauses of Saturn and Mercury, respectively. The methodology based on variance obtained by scale and edge identifications was shown to be a simple tool to perform this task. The results confirm that the Haar transform can efficiently identify the planetary magnetosphere boundaries characterized by the abrupt magnetic field changes. Due to this wavelet function to be a discrete function it promotes the abrupt and sharp identification of the boundaries. It is suggested that this technique can be applied to detect the planetary boundaries as well as the discontinuities such as the shock waves in the interplanetary space.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Identification of the...
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agreement Directory Content
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4. Conditions of access and use
Languageen
Target Filebolzan_2022_identification.pdf
User Groupself-uploading-INPE-MCTI-GOV-BR
simone
Reader Groupadministrator
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Visibilityshown
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
LinkingTrabalho não Vinculado à Tese/Dissertação
Next Higher Units8JMKD3MGPCW/46KTFK8
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.45.47 7
sid.inpe.br/bibdigital/2022/04.03.17.52 1
DisseminationWEBSCI; PORTALCAPES; AGU; COMPENDEX; SCOPUS.
Host Collectionurlib.net/www/2021/06.04.03.40
6. Notes
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