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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/48BJ2KS
Repositorysid.inpe.br/mtc-m21d/2023/01.09.12.40   (restricted access)
Last Update2023:01.09.12.40.48 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2023/01.09.12.40.48
Metadata Last Update2023:01.10.17.38.30 (UTC) administrator
DOI10.3389/fspas.2022.1021910
ISSN2296-987X
Citation KeyBravoMMBUESVNOVBVGRPCLCFMMSVC:2022:Ev14De
TitleIonospheric response modeling under eclipse conditions: Evaluation of 14 December 2020, total solar eclipse prediction over the South American sector
Year2022
MonthDec.
Access Date2024, May 14
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size5493 KiB
2. Context
Author 1 Bravo, M. A.
 2 Molina, M. G.
 3 Martínez-Ledesma, M.
 4 Barbás, B. de Haro
 5 Urra, B.
 6 Elías, A.
 7 Souza, Jonas Rodrigues de
 8 Villalobos, C.
 9 Namour, J. H.
10 Ovalle, E.
11 Venchiarutti, J. V.
12 Blunier, S.
13 Valdés-Abreu, J. C.
14 Guillermo, E.
15 Rojo, E.
16 Pasquale, L. de
17 Carrasco, E.
18 Leiva, R.
19 Castillo Rivera, C.
20 Foppiano, A.
21 Milla, M.
22 Muñoz, P. R.
23 Stepanova, M.
24 Valdivia, J. A.
25 Cabrera, M.
Resume Identifier 1
 2
 3
 4
 5
 6
 7 8JMKD3MGP5W/3C9JHFE
Group 1
 2
 3
 4
 5
 6
 7 DIHPA-CGCE-INPE-MCTI-GOV-BR
Affiliation 1 Universidad Adventista de Chile
 2 Universidad Nacional de Tucumán
 3 Centro Interuniversitario de Física de la Alta Atmósfera
 4 FACET-UNT
 5 Universidad Adventista de Chile
 6 Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET)
 7 Instituto Nacional de Pesquisas Espaciais (INPE)
 8 Universidad Adventista de Chile
 9 Universidad Nacional de Tucumán
10 Universidad de Concepción
11 FACET-UNT
12 Universidad de Chile
13 Universidad de Chile
14 Universidad Tecnológica Nacional, Bahía Blanca
15 Universidad Adventista de Chile
16 Universidad Tecnológica Nacional, Bahía Blanca
17 Universidad Adventista de Chile
18 Centro Interuniversitario de Física de la Alta Atmósfera
19 Universidad de Concepción
20 Universidad de Concepción
21 Pontificia Universidad Católica del Perú
22 Centro Interuniversitario de Física de la Alta Atmósfera
23 Universidad de Santiago de Chile
24 Universidad de Chile
25 FACET-UNT
Author e-Mail Address 1 manuelbravo@unach.cl
 2
 3
 4
 5
 6
 7 jonas.souza63@gmail.com
JournalFrontiers in Astronomy and Space Sciences
Volume9
Pagese1021910
History (UTC)2023-01-09 12:51:01 :: simone -> administrator :: 2022
2023-01-10 17:38:30 :: administrator -> simone :: 2022
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordseclipse condition
ionospheric modeling and prediction
ionospheric response
south American sector
total solar eclipse
AbstractIn this work, we evaluate the SUPIM-INPE model prediction of the 14 December 2020, total solar eclipse over the South American continent. We compare the predictions with data from multiple instruments for monitoring the ionosphere and with different obscuration percentages (i.e., Jicamarca, 12.0°S, 76.8°W, 17%; Tucumán 26.9°S, 65.4° W, 49%; Chillán 36.6°S, 72.0°W; and Bahía Blanca, 38.7°S, 62.3°W, reach 95% obscuration) due to the eclipse. The analysis is done under total eclipse conditions and non-total eclipse conditions. Results obtained suggest that the model was able to reproduce with high accuracy both the daily variation and the eclipse impacts of E and F1 layers in the majority of the stations evaluated (except in Jicamarca station). The comparison at the F2 layer indicates small differences (<7.8%) between the predictions and observations at all stations during the eclipse periods. Additionally, statistical metrics reinforce the conclusion of a good performance of the model. Predicted and calibrated Total Electron Content (TEC, using 3 different techniques) are also compared. Results show that, although none of the selected TEC calibration methods have a good agreement with the SUPIM-INPE prediction, they exhibit similar trends in most of the cases. We also analyze data from the Jicamarca Incoherent Scatter Radar (ISR), and Swarm-A and GOLD missions. The electron temperature changes observed in ISR and Swarm-A are underestimated by the prediction. Also, important changes in the O/N2 ratio due to the eclipse, have been observed with GOLD mission data. Thus, future versions of the SUPIM-INPE model for eclipse conditions should consider effects on thermospheric winds and changes in composition, specifically in the O/N2 ratio.
AreaCEA
Arrangementurlib.net > CGCE > Ionospheric response modeling...
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4. Conditions of access and use
Languageen
Target Filefspas-09-1021910.pdf
User Groupsimone
Reader Groupadministrator
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Visibilityshown
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Mirror Repositoryurlib.net/www/2021/06.04.03.40.25
Next Higher Units8JMKD3MGPCW/46KTFK8
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.51.12 1
DisseminationWEBSCI; PORTALCAPES; SCOPUS.
Host Collectionurlib.net/www/2021/06.04.03.40
6. Notes
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