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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/44BF2HH
Repositorysid.inpe.br/mtc-m21c/2021/03.15.13.01
Last Update2021:03.15.13.01.58 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2021/03.15.13.01.58
Metadata Last Update2022:04.03.22.39.36 (UTC) administrator
DOI10.1029/2020JA028663
ISSN2169-9402
Citation KeyMoroXDRBSSCPCLYWS:2021:ReReCo
TitleFirst Look at a Geomagnetic Storm With Santa Maria Digisonde Data: F Region Responses and Comparisons Over the American Sector
Year2021
MonthJan.
Access Date2024, May 18
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size6685 KiB
2. Context
Author 1 Moro, Juliano
 2 Xu, J.
 3 Denardini, Clezio Marcos
 4 Resende, Laysa Cristina Araújo
 5 Barbosa Neto, Paulo França
 6 Silva, Ligia Alves da
 7 Silva, Régia Pereira da
 8 Chen, Sony Su
 9 Picanço, Giorgio Arlan da Silva
10 Carmo, Carolina de Sousa do
11 Liu, Zehngkuan
12 Yan, Chunxiao
13 Wang, Chi
14 Schuch, Nelson Jorge
Resume Identifier 1
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 4
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 8
 9
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14 8JMKD3MGP5W/3C9JHUD
ORCID 1 0000-0003-4078-2222
 2 0000-0003-2868-0055
 3 0000-0002-3624-2461
 4 0000-0001-6968-6184
 5 0000-0001-5733-3541
 6 0000-0002-8822-5030
 7 0000-0002-6900-0928
 8 0000-0001-6307-7484
 9 0000-0003-3926-396X
10 0000-0001-6321-1663
11 0000-0001-8034-5575
12 0000-0002-6138-308X
13 0000-0001-6991-9398
14 0000-0002-7720-6491
Group 1 COESU-CGGO-INPE-MCTI-GOV-BR
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 3 DICEP-CGCE-INPE-MCTI-GOV-BR
 4 DICEP-CGCE-INPE-MCTI-GOV-BR
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 6 DIHPA-CGCE-INPE-MCTI-GOV-BR
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10 DIHPA-CGCE-INPE-MCTI-GOV-BR
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14 COESU-CGGO-INPE-MCTI-GOV-BR
Affiliation 1 Instituto Nacional de Pesquisas Espaciais (INPE)
 2 State Key Laboratory of Space Weathe
 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 Instituto Nacional de Pesquisas Espaciais (INPE)
10 Instituto Nacional de Pesquisas Espaciais (INPE)
11 State Key Laboratory of Space Weather
12 State Key Laboratory of Space Weather
13 State Key Laboratory of Space Weathe
14 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address 1 julianopmoro@gmail.com
 2
 3 clezio.denardin@inpe.br
 4 laysa.resende@gmail.com
 5
 6 ligia.alves01@gmail.com
 7 regiapereira@gmail.com
 8 sony.chen@inpe.br
 9 giorgiopicanco@gmail.com
10 carolina_kta25@hotmail.com
11
12
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14 njschuch@gmail.com
JournalJournal of Geophysical Research: Space Physics
Volume126
Number1
Pagese2020JA028663
History (UTC)2021-03-15 13:01:58 :: simone -> administrator ::
2021-03-15 13:01:59 :: administrator -> simone :: 2021
2021-03-15 13:03:45 :: simone -> administrator :: 2021
2021-06-22 19:11:14 :: administrator -> simone :: 2021
2021-06-22 20:57:41 :: simone -> administrator :: 2021
2021-07-29 11:54:20 :: administrator -> simone :: 2021
2021-12-16 18:26:20 :: simone -> administrator :: 2021
2022-04-03 22:39:36 :: administrator -> simone :: 2021
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractSanta Maria Digisonde data are used for the first time to investigate the F region behavior during a geomagnetic storm. The August 25, 2018 storm is considered complex due to the incidence of two Interplanetary Coronal Mass Ejections and a High-Speed Solar Wind Stream (HSS). The F 2 layer critical frequency (f o F 2) and its peak height (h m F 2) collected over Santa Maria, near the center of the South American Magnetic Anomaly (SAMA), are compared with data collected from Digisondes installed in the Northern (NH) and Southern (SH) Hemispheres in the American sector. The deviation of f o F 2 (Df o F 2) and h m F 2 (Dh m F 2) are used to quantify the ionospheric storm effects. Different F region responses were observed during the main phase (August 2526), which is attributed to the traveling ionospheric disturbances and disturbed eastward electric field during nighttime. The F region responses became highly asymmetric between the NH and SH at the early recovery phase (RP, August 26) due to a combination of physical mechanisms. The observed asymmetries are interpreted as caused by modifications in the thermospheric composition and a rapid electrodynamic mechanism. The persistent enhanced thermospheric [O]/[N2] ratio observed from August 27 to 29 combined with the increased solar wind speed induced by the HSS and IMF B z fluctuations seem to be effective in causing the positive ionospheric storm effects and the shift of the Equatorial Ionization Anomaly crest to higher than typical latitudes. Consequently, the most dramatic positive ionospheric storm during the RP occurred over Santa Maria (∼120%).
AreaCEA
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Languageen
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Next Higher Units8JMKD3MGPCW/46KTFK8
8JMKD3MGPCW/46KUBT5
Citing Item Listsid.inpe.br/bibdigital/2022/04.03.22.35 8
sid.inpe.br/mtc-m21/2012/07.13.14.57.02 2
DisseminationWEBSCI; AGU; MGA; COMPENDEX.
Host Collectionurlib.net/www/2017/11.22.19.04
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