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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/45HFJUP
Repositorysid.inpe.br/mtc-m21d/2021/10.04.15.53
Last Update2021:10.04.15.53.44 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21d/2021/10.04.15.53.44
Metadata Last Update2022:04.03.22.39.31 (UTC) administrator
DOI10.1029/2021JA029416
ISSN2169-9402
Citation KeyResendeZDBSMCCSAMFCPWL:2021:NeFiSp
TitleNew Findings of the Sporadic E (Es) Layer Development Around the Magnetic Equator During a High-Speed Solar (HSS) Wind Stream Event
Year2021
MonthSept.
Access Date2024, May 18
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size3819 KiB
2. Context
Author 1 Resende, Laysa Cristina Araújo
 2 Zhu, Y.
 3 Denardini, Clezio Marcos
 4 Batista, Inez Staciarini
 5 Shi, J.
 6 Moro, Juliano
 7 Chen, Sony Su
 8 Conceição Santos, F.
 9 Silva, Ligia Alves da
10 Andrioli, Vânia Fátima
11 Muella, Marcio Tadeu de Assis Honorato
12 Fagundes, P. R.
13 Carrasco, A. J.
14 Pillat, V. G.
15 Wang, C.
16 Liu, Z.
Resume Identifier 1
 2
 3
 4 8JMKD3MGP5W/3C9JHDA
ORCID 1 0000-0001-6968-6184
 2
 3 0000-0002-3624-2461
 4 0000-0001-5385-4112
 5 0000-0002-8008-0527
 6 0000-0003-4078-2222
 7 0000-0001-6307-7484
 8 0000-0002-4987-7132
 9 0000-0002-8822-5030
10 0000-0001-9065-2122
11 0000-0003-3408-6861
12 0000-0003-3764-2202
13 0000-0002-6182-8077
14 0000-0002-5849-0597
15 0000-0001-6991-9398
Group 1 DICEP-CGCE-INPE-MCTI-GOV-BR
 2
 3 DICEP-CGCE-INPE-MCTI-GOV-BR
 4 DICEP-CGCE-INPE-MCTI-GOV-BR
 5
 6 COESU-CGGO-INPE-MCTI-GOV-BR
 7 GESAST-CEA-DIPGR-INPE-MCTI-GOV-BR
 8
 9 DIHPA-CGCE-INPE-MCTI-GOV-BR
10 CGCE-CGCE-INPE-MCTI-GOV-BR
Affiliation 1 Instituto Nacional de Pesquisas Espaciais (INPE)
 2 State Key Laboratory of Space Weather
 3 Instituto Nacional de Pesquisas Espaciais (INPE)
 4 Instituto Nacional de Pesquisas Espaciais (INPE)
 5 State Key Laboratory of Space Weather
 6 Instituto Nacional de Pesquisas Espaciais (INPE)
 7 Instituto Nacional de Pesquisas Espaciais (INPE)
 8 Universidade do Vale do Paraíba (UNIVAP)
 9 Instituto Nacional de Pesquisas Espaciais (INPE)
10 Instituto Nacional de Pesquisas Espaciais (INPE)
11 Universidade do Vale do Paraíba (UNIVAP)
12 Universidade do Vale do Paraíba (UNIVAP)
13 Universidad de Los Andes
14 Universidade do Vale do Paraíba (UNIVAP)
15 State Key Laboratory of Space Weather
16 State Key Laboratory of Space Weather
Author e-Mail Address 1 laysa.resende@gmail.com
 2
 3 clezio.denarnin@inpe.br
 4
 5
 6 juliano.moro@inpe.br
 7 sony.chen@inpe.br
 8
 9 ligia.alves01@gmail.com
10 vaniafatima@gmail.com
JournalJournal of Geophysical Research: Space Physics
Volume126
Number9
Pagese2021JA029416
History (UTC)2021-10-04 15:53:44 :: simone -> administrator ::
2021-10-04 15:53:45 :: administrator -> simone :: 2021
2021-10-04 15:56:02 :: simone -> administrator :: 2021
2022-04-03 22:39:31 :: administrator -> simone :: 2021
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordsequatorial sporadic layers
gradient drift instability
sporadic layers simulation
AbstractThe equatorial (Esq) and blanketing (Esb) sporadic (Es) layers occur due to the Equatorial Electrojet Current (EEJ) plasma instabilities and tidal wind components, respectively. Both Esq and Esb layers can appear concurrently over some Brazilian equatorial regions due to the peculiar geomagnetic field configuration in this sector. Previous works indicate that the inclination angle limit for the Esq occurrence in ionograms is 7°. However, we found evidence that regions more distant can also experience such equatorial dynamics during disturbed periods. In this context, we deeply investigated this EEJ influence expansion effect by analyzing the Esq layers in regions not so close to the magnetic equator during a high-speed solar wind stream event that occurred on May 05 and 06, 2018. To explain these atypical Esq layer occurrences, we considered the Es layer parameters obtained from digital ionosondes over the Brazilian regions, São Luís (dip: 9.5°), and Araguatins (dip: 10.5°). We use magnetometer data and a model named MIRE (E Region Ionospheric Model) to validate this mechanism. The results show that the eastward electric field of the Gradient Drift instability in the EEJ is effective during the magnetic storm main phase in the boundary equatorial magnetic sites, creating the Esq layers. Thus, the EEJ plasma irregularity superimposes the wind shear mechanism, changing the Es layer dynamics during disturbed periods over the magnetic equator boundary sites. Therefore, this work establishes new findings of the EEJ influence expansion dynamics in the Es layer formation over the Brazilian regions, which was considered in MIRE for the first time.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > GES > New Findings of...
Arrangement 2urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > New Findings of...
Arrangement 3urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGGO > New Findings of...
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data URLhttp://urlib.net/ibi/8JMKD3MGP3W34T/45HFJUP
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34T/45HFJUP
Languageen
Target Fileresende_new.pdf
User Groupsimone
Visibilityshown
Archiving Policydenypublisher6 allowfinaldraft
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3F2PBEE
8JMKD3MGPCW/46KTFK8
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Citing Item Listsid.inpe.br/bibdigital/2022/04.03.22.35 8
sid.inpe.br/bibdigital/2013/10.12.21.02 1
sid.inpe.br/mtc-m21/2012/07.13.14.50.14 1
DisseminationWEBSCI; AGU; MGA; COMPENDEX.
Host Collectionurlib.net/www/2021/06.04.03.40
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