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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/47A668B
Repositorysid.inpe.br/mtc-m21d/2022/07.18.14.21
Last Update2022:07.18.14.21.37 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2022/07.18.14.21.37
Metadata Last Update2023:01.03.16.46.10 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyJauerCWESSMGSVZLAARDC:2022:EnCoUL
TitleModeling of inner magnetosphere under the influence of a magnetic cloud associated with an ICME: energy conversion and ULF spectral density
FormatOn-line
Year2022
Access Date2024, May 13
Secondary TypePRE CI
Number of Files1
Size52 KiB
2. Context
Author 1 Jauer, Paulo Ricardo
 2 Costa, Joaquim Eduardo Rezende
 3 Wang, Chi
 4 Echer, Ezequiel
 5 Souza, Vitor Moura Cardoso e Silva
 6 Silva, Ligia Alves da
 7 Marchezi, José Paulo
 8 Gonzalez Alarcon, Walter Demetrio
 9 Silva, Douglas
10 Vieira, Luís Eduardo Antunes
11 Zhengkuan, Liu
12 Li, Hui
13 Alves, Maria Virgínia
14 Alves, Livia Ribeiro
15 Resende, Laysa Cristina Araújo
16 Denardini, Clezio Marcos
17 Costa, Joaquim Eduardo Rezende
Resume Identifier 1
 2 8JMKD3MGP5W/3C9JHF8
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17 8JMKD3MGP5W/3C9JHF8
Group 1 DICEP-CGCE-INPE-MCTI-GOV-BR
 2 DICEP-CGCE-INPE-MCTI-GOV-BR
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 4 DIHPA-CGCE-INPE-MCTI-GOV-BR
 5 DIHPA-CGCE-INPE-MCTI-GOV-BR
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Affiliation 1 Instituto Nacional de Pesquisas Espaciais (INPE)
 2 Instituto Nacional de Pesquisas Espaciais (INPE)
 3 Chinese Academy of Sciences (CAS)
 4 Instituto Nacional de Pesquisas Espaciais (INPE)
 5 Instituto Nacional de Pesquisas Espaciais (INPE)
 6 Instituto Nacional de Pesquisas Espaciais (INPE)
 7 Chinese Academy of Sciences (CAS)
 8 Instituto Nacional de Pesquisas Espaciais (INPE)
 9 Universidade Presbiteriana Mackenzie
10 Instituto Nacional de Pesquisas Espaciais (INPE)
11 Chinese Academy of Sciences (CAS)
12 Chinese Academy of Sciences (CAS)
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 pauloricardojauer@gmail.com
 2 joaquim.costa@inpe.br
 3 cw@spaceweather.ac.cn
 4 ezequiel.echer@gmail.com
 5 vitormoura21@gmail.com
 6 ligia.alves01@gmail.com
 7 jpmarchezi@gmail.com
 8 walterdgalarcon@yahoo.com
 9 douglas93f@gmail.com
10 luis.vieira71@googlemail.com
11 liuzhengkuan@nssc.ac.cn
12 hli@spaceweather.ac.cn
13 mvirginia.alves@inpe.br
14 liviarib@gmail.com
15 laysa.resende@gmail.com
16 clezio.denardin@inpe.br
17 jercosta@gmail.com
Conference NameCOSPAR Scientific Assembly, 44
Conference LocationAthens, Greece
Date16-24 July 2022
History (UTC)2022-07-18 14:21:37 :: simone -> administrator ::
2022-07-20 00:24:27 :: administrator -> simone :: 2022
2022-12-20 11:48:51 :: simone -> administrator :: 2022
2023-01-03 16:46:10 :: administrator -> simone :: 2022
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractThe objective of this work is to carry out a broad study of the coupling effects of a geoeffective interplanetary structure of the magnetic cloud (MC) type that occurred between May 27- 29, 2017 and promoted an intense impact on the global and inner magnetosphere in terms of energy conversion (magnetic, kinetic and internal) and the emergence of storm, substorm, intensification of electric and magnetic fields as well as the generation of electromagnetic waves in the ultralow frequency (ULF) range, specifically from 0.5 to 16.6 mHz. To carry out this study we fed the SWMF/BATSRUS global magnetohydrodynamic code with the MC solar wind data as obtained by the DISCOVERY satellite. SWMF/BATSRUS has been coupled with two other internal magnetosphere models, namely, Rice Convection Model and the ionospheric electrodynamics model in order to better describe the physical processes occurring in the inner magnetosphere. The regions of interest were both the dayside and nightside equatorial planes which spanned radial distances going from 3 to 9 Earth radii that encompasses the equatorial radiation belts regions. The global behavior of the energy conversion rate and the generation of disturbances in the ULF frequency range were analyzed for each phase of the MC in the aforementioned regions of interest. This study allows us to obtain physical information on the global distribution of the energy conversion rate and the intensification of ULF waves during different stages of the MC interaction with Earths magnetosphere.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Modeling of inner...
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data URLhttp://mtc-m21d.sid.inpe.br/ibi/8JMKD3MGP3W34T/47A668B
zipped data URLhttp://mtc-m21d.sid.inpe.br/zip/8JMKD3MGP3W34T/47A668B
Languageen
Target FileD3.1-0036-22-oral.pdf
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Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/46KTFK8
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.45.47 3
sid.inpe.br/mtc-m21/2012/07.13.15.01.50 2
sid.inpe.br/mtc-m21/2012/07.13.14.55.54 1
Host Collectionurlib.net/www/2021/06.04.03.40
6. Notes
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