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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/4835LH5
Repositorysid.inpe.br/mtc-m21d/2022/11.18.12.14
Last Update2022:11.18.12.14.00 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21d/2022/11.18.12.14.01
Metadata Last Update2023:04.04.06.47.11 (UTC) administrator
DOI10.1029/2022JA030615
ISSN2169-9402
Citation KeyJauerWESSMAADLLHVGDMC:2022:EnCoUl
TitleGlobal Modeling of the Inner Magnetosphere Under the Influence of a Magnetic Cloud Associated With an Interplanetary Coronal Mass Ejection: Energy Conversion and Ultra-Low Frequency Wave Activity
Year2022
MonthOct.
Access Date2024, May 14
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size5301 KiB
2. Context
Author 1 Jauer, Paulo Ricardo
 2 Wang, C.
 3 Echer, Ezequiel
 4 Souza, Vitor Moura Cardoso e Silva
 5 Silva, Ligia Alves da
 6 Marchezi, José Paulo
 7 Alves, Livia Ribeiro
 8 Alves, Maria Virgínia
 9 Douglas, S.
10 Loesch, C.
11 Liu, Z.
12 Hui, L.
13 Vieira, Luís Eduardo Antunes
14 Gonzalez Alarcon, Walter Demetrio
15 Denardini, Clezio Marcos
16 Medeiros, Cláudia
17 Costa, Joaquim Eduardo Rezende
Resume Identifier 1
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14 8JMKD3MGP5W/3C9JJC4
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17 8JMKD3MGP5W/3C9JHF8
ORCID 1 0000-0002-8064-5030
 2
 3 0000-0002-8351-6779
 4 0000-0001-7294-7963
 5 0000-0002-8822-5030
 6 0000-0002-2904-6411
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Group 1 DICEP-CGCE-INPE-MCTI-GOV-BR
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Affiliation 1 Instituto Nacional de Pesquisas Espaciais (INPE)
 2 State Key Laboratory of Space Weather (NSSC)
 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 State Key Laboratory of Space Weather
10 Institute of Higher Education of Brasília
11 State Key Laboratory of Space Weather
12 State Key Laboratory of Space Weather
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
 3 ezequiel.echer@gmail.com
 4 vitormoura21@gmail.com
 5 ligia.alves01@gmail.com
 6 jpmarchezi@gmail.com
 7 livia.alves@inpe.br
 8
 9
10
11
12
13 luis.vieira71@googlemail.com
14 walterdgalarcon@yahoo.com
15 clezio.denardin@inpe.br
16 claudia.inpe@gmail.com
17 jercosta@gmail.com
JournalJournal of Geophysical Research: Space Physics
Volume127
Number10
Pagese2022JA030615
History (UTC)2022-11-18 12:14:01 :: simone -> administrator ::
2022-11-18 12:14:01 :: administrator -> simone :: 2022
2022-11-18 12:16:37 :: simone -> administrator :: 2022
2022-12-08 10:06:23 :: administrator -> simone :: 2022
2022-12-19 19:15:41 :: simone -> administrator :: 2022
2023-04-04 06:47:11 :: administrator -> simone :: 2022
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordsenergy conversion
MHD simulation
ULF waves
magnetic cloud
magnetospheric activity
AbstractThe interaction and response of the magnetic cloud-type structure with Earth's magnetosphere were modeled by the SWMF/BATS-R-US code. The conversion of magnetic (E-m), kinetic (E-k), and internal (E-i) energies was analyzed as well as the wave power integrated in the ultra-low frequency (ULF) range of the poloidal (E-phi) and toroidal (E-r) electric field components in the equatorial region of the magnetosphere, in seven 2-hr long intervals, namely, I1 through I7. The intensity of energy conversion and wave activity for I1 and I7 intervals was negligible. The energy conversion started in the I2 interval and extended to the I3, I4, and I5 intervals. The power of the E-phi and E-r components in the dayside and nightside regions is clearly observed. The I4 corresponds to interplanetary magnetic field (IMF) B-z mostly southward and the I5 has similar amplitudes of the B-z and B-y components, corresponding to the period of the high geomagnetic activity. The conversion rate for the I4 and I5 was similar, however, the integrated power spectral density (IPSD) of the E-phi and E-r components is more intense in I5. During the I6 interval, with predominant IMF B-y, the energy conversion rate is intensified mostly for inner radial distances R R-E, and the E-k component becomes close to zero for outer regions. The energy conversion regions are located spatially close to or overlapping with regions where the IPSD in the ULF range is intensified. The energy conversion in the inner magnetosphere occurred preferentially between E-m and E-i, with the E-k energy component always present but with lower intensities.
AreaCEA
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4. Conditions of access and use
data URLhttp://mtc-m21d.sid.inpe.br/ibi/8JMKD3MGP3W34T/4835LH5
zipped data URLhttp://mtc-m21d.sid.inpe.br/zip/8JMKD3MGP3W34T/4835LH5
Languageen
Target FileJGR Space Physics - 2022 - Jauer - Global Modeling of the Inner Magnetosphere Under the Influence of a Magnetic Cloud.pdf
User Groupsimone
Visibilityshown
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5. Allied materials
Next Higher Units8JMKD3MGPCW/46KTFK8
8JMKD3MGPCW/46KUES5
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.45.47 4
sid.inpe.br/mtc-m21/2012/07.13.15.01.50 3
sid.inpe.br/mtc-m21/2012/07.13.14.55.54 2
DisseminationWEBSCI; AGU; MGA; COMPENDEX.
Host Collectionurlib.net/www/2021/06.04.03.40
6. Notes
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