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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/42NRR6L
Repositorysid.inpe.br/mtc-m21c/2020/06.26.12.30
Last Update2020:06.26.12.30.09 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21c/2020/06.26.12.30.09
Metadata Last Update2022:03.18.22.11.33 (UTC) administrator
DOI10.1029/2019JA027519
ISSN2169-9402
Citation KeyResendeSDBNAAMSCBWL:2020:InDiDy
TitleThe influence of disturbance dynamo electric field in the formation of strong sporadic E layers over Boa Vista, a low‐latitude station in the American sector
Year2020
Access Date2024, May 15
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size6015 KiB
2. Context
Author 1 Resende, Laysa Cristina Araújo
 2 Shi, Jiankui K.
 3 Denardini, Clezio Marcos
 4 Batista, Inez Staciarini
 5 Nogueira, Paulo A. B.
 6 Arras, C.
 7 Andrioli, Vânia Fátima
 8 Moro, Juliano
 9 Silva, Ligia Alves da
10 Carrasco, A. J.
11 Barbosa Neto, Paulo França
12 Wang, Chi
13 Liu, Z.
Resume Identifier 1
 2
 3
 4 8JMKD3MGP5W/3C9JHDA
ORCID 1 0000-0001-6968-6184
 2 0000-0002-8008-0527
 3 0000-0002-3624-2461
 4 0000-0001-5385-4112
 5 0000-0003-0810-1044
 6
 7 0000-0001-9065-2122
 8 0000-0003-4078-2222
 9
10
11
12 0000-0001-6991-9398
Group 1 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
 2
 3 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
 4 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
 5
 6
 7 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
 8 CRCRS-COCRE-INPE-MCTIC-GOV-BR
 9 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
10
11 GESAST-CEA-SESPG-INPE-MCTIC-GOV-BR
Affiliation 1 Instituto Nacional de Pesquisas Espaciais (INPE)
 2 State Key Laboratory of Space Weather, NSSC/CAS
 3 Instituto Nacional de Pesquisas Espaciais (INPE)
 4 Instituto Nacional de Pesquisas Espaciais (INPE)
 5 Instituto Federal de Educação, Ciência e Tecnologia de São Paulo (IFSP)
 6 Helmholtz Centre Potsdam
 7 Instituto Nacional de Pesquisas Espaciais (INPE)
 8 Instituto Nacional de Pesquisas Espaciais (INPE)
 9 Instituto Nacional de Pesquisas Espaciais (INPE)
10 Universidad de Los Andes
11 Instituto Nacional de Pesquisas Espaciais (INPE)
12 State Key Laboratory of Space Weather, NSSC/CAS
13 State Key Laboratory of Space Weather, NSSC/CAS
Author e-Mail Address 1 laysa.resende@inpe.br
 2
 3 clezio.denardin@inpe.br
 4 inez.batista@inpe.br
 5
 6
 7 vania.andrioli@inpe.br
 8
 9
10
11 paulo.barbosa@inpe.br
JournalJournal of Geophysical Research: Space Physics
Volume102
Number9
History (UTC)2020-06-26 12:30:09 :: simone -> administrator ::
2020-06-26 12:30:10 :: administrator -> simone :: 2020
2020-06-26 12:34:06 :: simone -> administrator :: 2020
2020-06-26 13:35:31 :: administrator -> simone :: 2020
2020-06-26 13:47:34 :: simone -> administrator :: 2020
2020-06-27 12:29:46 :: administrator -> simone :: 2020
2020-12-14 13:58:32 :: simone -> administrator :: 2020
2022-03-18 22:11:33 :: administrator -> simone :: 2020
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractThis study analyzes strong sporadic E layer (Es) formation in Boa Vista (BV, 2.8°N, 60.7°W, dip: 18°), a low‐latitude region in the Brazilian sector, which occurred far after the onset of a magnetic storm recovery phase. Such occurrences were observed during seven magnetic storms with available data for BV. Thus, the ionospheric behavior on days around the magnetic storm that occurred on 20 January 2016 was investigated to search for possible explanations. This analysis indicated that the probable mechanism acting during the Es layer strengthening is the zonal westward electric field caused by a disturbance dynamo. The same evidence was also observed in two other magnetic storms at the same location. Hence, a numerical model of the E region dynamics, called MIRE (Portuguese acronym for E Region Ionospheric Model), was used to confirm whether the disturbance dynamo could cause the Es layer intensification. The inputs for the model were the electric field deduced from the vertical drift and the wind components provided by GSWM‐00 model. The simulations indicate that the Es layer density is significantly enhanced when the zonal electric field is present compared to the reference scenario with only the winds. Therefore, it is concluded that the disturbance dynamo electric field is the likely cause of the strong Es layers in the analyzed cases. Finally, the combined results from the model and observational data seem to contribute significantly to advance our understanding of the role of the electric fields in the Es layer formation at low latitudes.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > The influence of...
Arrangement 2urlib.net > BDMCI > Fonds > Produção anterior à 2021 > CRCRS > The influence of...
Arrangement 3urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > GES > The influence of...
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W34R/42NRR6L
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34R/42NRR6L
Languageen
Target FileResende_influence.pdf
User Groupsimone
Visibilityshown
Archiving Policydenypublisher6 allowfinaldraft
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETL868
8JMKD3MGPCW/3EUFCFP
8JMKD3MGPCW/3F2PBEE
Citing Item Listsid.inpe.br/bibdigital/2013/09.29.20.43 1
sid.inpe.br/mtc-m21/2012/07.13.14.50.14 1
sid.inpe.br/bibdigital/2013/10.12.21.02 1
DisseminationWEBSCI; AGU; MGA; COMPENDEX.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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