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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/43MN54H
Repositorysid.inpe.br/mtc-m21c/2020/12.02.14.13
Last Update2020:12.02.14.13.25 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21c/2020/12.02.14.13.25
Metadata Last Update2022:01.04.01.35.40 (UTC) administrator
DOI10.1029/2020JA028625
ISSN2169-9402
Citation KeyMartínez-LedesmaBraUrrSouFop:2020:PrIoRe
TitlePrediction of the Ionospheric Response to the 14 December 2020 Total Solar Eclipse Using SUPIM-INPE
Year2020
MonthNov.
Access Date2024, June 17
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size3344 KiB
2. Context
Author1 Martínez-Ledesma, Miguel
2 Bravo Sepulveda, Manuel Alejandro
3 Urra, Benjamin
4 Souza, Jonas Rodrigues de
5 Foppiano, Alberto J.
Resume Identifier1
2
3
4 8JMKD3MGP5W/3C9JHFE
ORCID1 0000-0001-6932-1249
2 0000-0002-5648-429X
3 0000-0003-3645-818X
4 0000-0001-7725-7785
5 0000-0003-4374-538X
Group1
2
3
4 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 Universidad de Concepción
2 Universidad de Concepción
3 Universidad de Concepción
4 Instituto Nacional de Pesquisas Espaciais (INPE)
5 Universidad de Concepción
Author e-Mail Address1
2
3
4 jonas.souza@inpe.br
JournalJournal of Geophysical Research: Space Physics
Volume125
Number11
Pagese2020JA028625
History (UTC)2020-12-02 14:13:25 :: simone -> administrator ::
2020-12-02 14:13:26 :: administrator -> simone :: 2020
2020-12-02 14:14:20 :: simone -> administrator :: 2020
2022-01-04 01:35:40 :: administrator -> simone :: 2020
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractWe present the first prediction of the ionospheric response to the 14 December 2020 solar eclipse using the SUPIM‐INPE model. Simulations are made for all known ionosonde stations for which solar obscuration is significant. The found response is similar to that previously reported for other eclipses, but it also shows a modification of the equatorial fountain transport that will impact the low latitudes after the event. In addition to the large reduction of electron concentration along the totality path (~4.5 TECu, ~22%), a significant electron and oxygen ion temperature cooling is observed (up to ~400 K) followed by lasting temperature increases. Changes of up to ~1.5 TECu (~5%) are also expected at the conjugate hemisphere. These predictions may serve as a reference for eventual ionospheric measurements of multiple instruments and are leading to a better understanding of the ionospheric response to solar eclipses.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produçăo anterior ŕ 2021 > DIDAE > Prediction of the...
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4. Conditions of access and use
data URLhttp://mtc-m21c.sid.inpe.br/ibi/8JMKD3MGP3W34R/43MN54H
zipped data URLhttp://mtc-m21c.sid.inpe.br/zip/8JMKD3MGP3W34R/43MN54H
Languageen
Target Filemartinez_prediction.pdf
User Groupsimone
Visibilityshown
Archiving Policydenypublisher6 allowfinaldraft
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETL868
Citing Item Listsid.inpe.br/bibdigital/2013/09.29.20.43 4
sid.inpe.br/mtc-m21/2012/07.13.14.51.12 2
DisseminationWEBSCI; AGU; MGA; COMPENDEX.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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