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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3UHFUG5
Repositorysid.inpe.br/mtc-m21c/2019/12.10.10.35
Last Update2021:02.19.12.35.32 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2019/12.10.10.35.15
Metadata Last Update2021:02.19.12.35.32 (UTC) simone
Secondary KeyINPE--PRE/
Citation KeyJauerWSAPMASLLGVDECD:2019:CoInRe
TitleA Global Magnetohydrodynamic Simulation Study of Ultra-Low Frequency Waves Activity in the Inner Magnetosphere: Corotating Interaction Region + Alfvénic Fluctuation
Year2019
Access Date2024, May 16
Secondary TypePRE CI
Number of Files1
Size83 KiB
2. Context
Author 1 Jauer, Paulo Ricardo
 2 Wang, Chi
 3 Souza, Vitor Moura Cardoso e Silva
 4 Alves, Maria Virgínia
 5 Paula, Marcelo Banik de
 6 Marchezi, José Paulo
 7 Alves, Livia Ribeiro
 8 Silva, Lígia Alves da
 9 Li, Hui
10 Liu, Zhengkuan
11 Gonzalez Alarcon, Walter Demétrio
12 Vieira, Luís Eduardo Antunes
13 Dal Lago, Alisson
14 Echer, Ezequiel
15 Medeiro
16 Costa, Joaquim Eduardo Rezende
17 Denardin, Clezio Marcos
Resume Identifier 1
 2
 3
 4 8JMKD3MGP5W/3C9JHRS
 5
 6
 7
 8
 9
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11 8JMKD3MGP5W/3C9JJC4
12
13 8JMKD3MGP5W/3C9JGH3
14 8JMKD3MGP5W/3C9JH3D
15
16 8JMKD3MGP5W/3C9JHF8
Group 1 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
 2
 3 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
 4 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
 5 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
 6 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
 7 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
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13 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
14 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
15 COCRC-COCRC-INPE-MCTIC-GOV-BR
16 DIDAS-CGCEA-INPE-MCTIC-GOV-BR
17 DIDAS-CGCEA-INPE-MCTIC-GOV-BR
Affiliation 1 Instituto Nacional de Pesquisas Espaciais (INPE)
 2 CSSAR, CAS
 3 Instituto Nacional de Pesquisas Espaciais (INPE)
 4 Instituto Nacional de Pesquisas Espaciais (INPE)
 5 Instituto Nacional de Pesquisas Espaciais (INPE)
 6 Instituto Nacional de Pesquisas Espaciais (INPE)
 7 Instituto Nacional de Pesquisas Espaciais (INPE)
 8 Instituto Nacional de Pesquisas Espaciais (INPE)
 9 NSSC National Space Science Center, CAS
10 NSSC National Space Science Center, CAS
11 Instituto Nacional de Pesquisas Espaciais (INPE)
12 Instituto Nacional de Pesquisas Espaciais (INPE)
13 Instituto Nacional de Pesquisas Espaciais (INPE)
14 Instituto Nacional de Pesquisas Espaciais (INPE)
15 Instituto Nacional de Pesquisas Espaciais (INPE)
16 Instituto Nacional de Pesquisas Espaciais (INPE)
17 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address 1 paulo.jauer@inpe.br
 2
 3 vitor.souza@inpe.br
 4 mvirginia.alves@inpe.br
 5 marcelo.banik@inpe.br
 6 jose.marchezi@inpe.br
 7 livia.alves@inpe.br
 8 ligia.silva@inpe.br
 9
10
11 walter.alarcon@inpe.br
12 luis.vieira@inpe.br
13 alisson.dalago@inpe.br
14 ezequiel.echer@inpe.br
15 claudia.medeiros@inpe.br
16 joaquim.costa@inpe.br
17 clezio.denardin@inpe.br
Conference NameAGU Fall Meeting
Conference LocationSan Francisco, CA
Date09-13 dec.
History (UTC)2019-12-10 10:35:15 :: simone -> administrator ::
2019-12-13 22:11:59 :: administrator -> simone :: 2019
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Abstractcomprised of a Corotating Interaction Region (CIR) followed by solar wind Alfvénic fluctuations it is not straightforward to decisively say which solar wind parameters or which combinations thereof are most effective in causing disturbances in the inner magnetosphere, or how each part of the complex interplanetary structure influences the most the temporal evolution of the magnetosphere. Using global magnetohydrodynamic (MHD) simulations we perform a study which address some of these questions. Firstly, we use the magnetic field and plasma parameters of a real CIR+Alfvénic fluctuations event as input to the SWMF/BATS-R-US code. The model outputs are used to calculate the convection electric field's power spectral density (PSD) integrated in the ultra-low frequency (ULF) waves frequency range in the equatorial, nightside magnetosphere region. Then, we separate the real event into its constituent parts by building up synthetic magnetic field and plasma profiles based on the physical parameters which characterize each of these parts. The MHD code is then fed with each new synthetic profile containing Alfvénic fluctuations with two driving frequencies, namely 0.833 and 1.66 mHz. Our preliminary results show that the toroidal electric field (Er) component fluctuations are related with both driving frequencies, specially at farther out locations near the flanks of the modeled magnetopause. The poloidal (Ef) component fluctuations do respond differently to the driving frequencies in terms of both spatial structure and integrated power intensities.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > A Global Magnetohydrodynamic...
Arrangement 2urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > A Global Magnetohydrodynamic...
Arrangement 3urlib.net > BDMCI > Fonds > Produção anterior à 2021 > COCRC > A Global Magnetohydrodynamic...
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source Directory Contentthere are no files
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W34R/3UHFUG5
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34R/3UHFUG5
Languageen
Target Filejauer_global.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Update Permissionnot transferred
5. Allied materials
Mirror Repositoryurlib.net/www/2017/11.22.19.04.03
Next Higher Units8JMKD3MGPCW/3ETR8EH
8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/3F3PAJE
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.55.54 6
sid.inpe.br/mtc-m21/2012/07.13.14.45.47 5
sid.inpe.br/mtc-m21/2012/07.13.14.39.46 2
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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