1. Identity statement | |
Reference Type | Journal Article |
Site | mtc-m21d.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 8JMKD3MGP3W34T/48BJ2KS |
Repository | sid.inpe.br/mtc-m21d/2023/01.09.12.40 (restricted access) |
Last Update | 2023:01.09.12.40.48 (UTC) simone |
Metadata Repository | sid.inpe.br/mtc-m21d/2023/01.09.12.40.48 |
Metadata Last Update | 2023:01.10.17.38.30 (UTC) administrator |
DOI | 10.3389/fspas.2022.1021910 |
ISSN | 2296-987X |
Citation Key | BravoMMBUESVNOVBVGRPCLCFMMSVC:2022:Ev14De |
Title | Ionospheric response modeling under eclipse conditions: Evaluation of 14 December 2020, total solar eclipse prediction over the South American sector |
Year | 2022 |
Month | Dec. |
Access Date | 2024, May 14 |
Type of Work | journal article |
Secondary Type | PRE PI |
Number of Files | 1 |
Size | 5493 KiB |
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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 |
Journal | Frontiers in Astronomy and Space Sciences |
Volume | 9 |
Pages | e1021910 |
History (UTC) | 2023-01-09 12:51:01 :: simone -> administrator :: 2022 2023-01-10 17:38:30 :: administrator -> simone :: 2022 |
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3. Content and structure | |
Is the master or a copy? | is the master |
Content Stage | completed |
Transferable | 1 |
Content Type | External Contribution |
Version Type | publisher |
Keywords | eclipse condition ionospheric modeling and prediction ionospheric response south American sector total solar eclipse |
Abstract | In 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. |
Area | CEA |
Arrangement | urlib.net > CGCE > Ionospheric response modeling... |
doc Directory Content | access |
source Directory Content | there are no files |
agreement Directory Content | |
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4. Conditions of access and use | |
Language | en |
Target File | fspas-09-1021910.pdf |
User Group | simone |
Reader Group | administrator simone |
Visibility | shown |
Read Permission | deny from all and allow from 150.163 |
Update Permission | not transferred |
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5. Allied materials | |
Mirror Repository | urlib.net/www/2021/06.04.03.40.25 |
Next Higher Units | 8JMKD3MGPCW/46KTFK8 |
Citing Item List | sid.inpe.br/mtc-m21/2012/07.13.14.51.12 1 |
Dissemination | WEBSCI; PORTALCAPES; SCOPUS. |
Host Collection | urlib.net/www/2021/06.04.03.40 |
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6. Notes | |
Empty Fields | alternatejournal archivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark nextedition notes number orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey secondarymark session shorttitle sponsor subject tertiarymark tertiarytype url |
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7. Description control | |
e-Mail (login) | simone |
update | |
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