Ionospheric response modeling under eclipse conditions: Evaluation of 14 December 2020, total solar eclipse prediction over the South American sector
- Autores
- Bravo, M. A.; Molina, Maria Graciela; Martínez Ledesma, Miguel; de Haro Barbás, Blas Federico; Urra, B.; Elias, Ana Georgina; Souza, J.; Villalobos, C.; Namour, Jorge Habib; Ovalle, E.; Venchiarutti, José Valentín; Blunier, S.; Valdés Abreu, J.C.; Guillermo, Eduardo Daniel; Rojo, E.; de Pasquale, Lorenzo; Carrasco, E.; Leiva, R.; Castillo Rivera, C.; Foppiano, A.; Milla, M.; Muñoz, P. R.; Stepanova, M.; Valdivia, J. A.; Cabrera, Miguel Angel
- Año de publicación
- 2022
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- 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.
Fil: Bravo, M. A.. Universidad de Concepción; Chile. Universidad Adventista de Chile; Chile
Fil: Molina, Maria Graciela. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Tucumán; Argentina. Istituto Nazionale di Geofisica e Vulcanologia; Italia. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología; Argentina
Fil: Martínez Ledesma, Miguel. Universidad de Concepción; Chile
Fil: de Haro Barbás, Blas Federico. Universidad Nacional de Tucumán; Argentina
Fil: Urra, B.. Universidad Adventista de Chile; Chile
Fil: Elias, Ana Georgina. Universidad Nacional de Tucumán. Instituto de Física del Noroeste Argentino. - Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet Noa Sur. Instituto de Física del Noroeste Argentino; Argentina
Fil: Souza, J.. Centro de Previsao de Tempo e Estudos Climáticos. Instituto Nacional de Pesquisas Espaciais; Brasil
Fil: Villalobos, C.. Universidad Adventista de Chile; Chile
Fil: Namour, Jorge Habib. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología; Argentina
Fil: Ovalle, E.. Universidad de Concepción; Chile
Fil: Venchiarutti, José Valentín. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Tucumán; Argentina
Fil: Blunier, S.. Universidad de Chile; Chile
Fil: Valdés Abreu, J.C.. Universidad de Chile; Chile
Fil: Guillermo, Eduardo Daniel. Universidad Tecnológica Nacional; Argentina
Fil: Rojo, E.. Universidad Adventista de Chile; Chile
Fil: de Pasquale, Lorenzo. Universidad Tecnológica Nacional; Argentina
Fil: Carrasco, E.. Universidad Adventista de Chile; Chile
Fil: Leiva, R.. Universidad Adventista de Chile; Chile
Fil: Castillo Rivera, C.. Universidad de Concepción; Chile
Fil: Foppiano, A.. Universidad de Concepción; Chile
Fil: Milla, M.. Pontificia Universidad Católica de Perú; Perú
Fil: Muñoz, P. R.. Universidad de La Serena; Chile
Fil: Stepanova, M.. Universidad de Santiago de Chile; Chile
Fil: Valdivia, J. A.. Universidad de Chile; Chile
Fil: Cabrera, Miguel Angel. Universidad Nacional de Tucumán; Argentina - Materia
-
ECLIPSE CONDITION
IONOSPHERIC MODELING AND PREDICTION
IONOSPHERIC RESPONSE
SOUTH AMERICAN SECTOR
TOTAL SOLAR ECLIPSE - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/218285
Ver los metadatos del registro completo
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Ionospheric response modeling under eclipse conditions: Evaluation of 14 December 2020, total solar eclipse prediction over the South American sectorBravo, M. A.Molina, Maria GracielaMartínez Ledesma, Miguelde Haro Barbás, Blas FedericoUrra, B.Elias, Ana GeorginaSouza, J.Villalobos, C.Namour, Jorge HabibOvalle, E.Venchiarutti, José ValentínBlunier, S.Valdés Abreu, J.C.Guillermo, Eduardo DanielRojo, E.de Pasquale, LorenzoCarrasco, E.Leiva, R.Castillo Rivera, C.Foppiano, A.Milla, M.Muñoz, P. R.Stepanova, M.Valdivia, J. A.Cabrera, Miguel AngelECLIPSE CONDITIONIONOSPHERIC MODELING AND PREDICTIONIONOSPHERIC RESPONSESOUTH AMERICAN SECTORTOTAL SOLAR ECLIPSEhttps://purl.org/becyt/ford/1.5https://purl.org/becyt/ford/1In 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.Fil: Bravo, M. A.. Universidad de Concepción; Chile. Universidad Adventista de Chile; ChileFil: Molina, Maria Graciela. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Tucumán; Argentina. Istituto Nazionale di Geofisica e Vulcanologia; Italia. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología; ArgentinaFil: Martínez Ledesma, Miguel. Universidad de Concepción; ChileFil: de Haro Barbás, Blas Federico. Universidad Nacional de Tucumán; ArgentinaFil: Urra, B.. Universidad Adventista de Chile; ChileFil: Elias, Ana Georgina. Universidad Nacional de Tucumán. Instituto de Física del Noroeste Argentino. - Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet Noa Sur. Instituto de Física del Noroeste Argentino; ArgentinaFil: Souza, J.. Centro de Previsao de Tempo e Estudos Climáticos. Instituto Nacional de Pesquisas Espaciais; BrasilFil: Villalobos, C.. Universidad Adventista de Chile; ChileFil: Namour, Jorge Habib. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología; ArgentinaFil: Ovalle, E.. Universidad de Concepción; ChileFil: Venchiarutti, José Valentín. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Tucumán; ArgentinaFil: Blunier, S.. Universidad de Chile; ChileFil: Valdés Abreu, J.C.. Universidad de Chile; ChileFil: Guillermo, Eduardo Daniel. Universidad Tecnológica Nacional; ArgentinaFil: Rojo, E.. Universidad Adventista de Chile; ChileFil: de Pasquale, Lorenzo. Universidad Tecnológica Nacional; ArgentinaFil: Carrasco, E.. Universidad Adventista de Chile; ChileFil: Leiva, R.. Universidad Adventista de Chile; ChileFil: Castillo Rivera, C.. Universidad de Concepción; ChileFil: Foppiano, A.. Universidad de Concepción; ChileFil: Milla, M.. Pontificia Universidad Católica de Perú; PerúFil: Muñoz, P. R.. Universidad de La Serena; ChileFil: Stepanova, M.. Universidad de Santiago de Chile; ChileFil: Valdivia, J. A.. Universidad de Chile; ChileFil: Cabrera, Miguel Angel. Universidad Nacional de Tucumán; ArgentinaFrontiers Media2022-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/218285Bravo, M. A.; Molina, Maria Graciela; Martínez Ledesma, Miguel; de Haro Barbás, Blas Federico; Urra, B.; et al.; Ionospheric response modeling under eclipse conditions: Evaluation of 14 December 2020, total solar eclipse prediction over the South American sector; Frontiers Media; Frontiers in Astronomy and Space Sciences; 9; 1021910; 12-2022; 1-212296-987XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.3389/fspas.2022.1021910info:eu-repo/semantics/altIdentifier/url/https://www.frontiersin.org/articles/10.3389/fspas.2022.1021910/fullinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:22:30Zoai:ri.conicet.gov.ar:11336/218285instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:22:31.018CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
Ionospheric response modeling under eclipse conditions: Evaluation of 14 December 2020, total solar eclipse prediction over the South American sector |
| title |
Ionospheric response modeling under eclipse conditions: Evaluation of 14 December 2020, total solar eclipse prediction over the South American sector |
| spellingShingle |
Ionospheric response modeling under eclipse conditions: Evaluation of 14 December 2020, total solar eclipse prediction over the South American sector Bravo, M. A. ECLIPSE CONDITION IONOSPHERIC MODELING AND PREDICTION IONOSPHERIC RESPONSE SOUTH AMERICAN SECTOR TOTAL SOLAR ECLIPSE |
| title_short |
Ionospheric response modeling under eclipse conditions: Evaluation of 14 December 2020, total solar eclipse prediction over the South American sector |
| title_full |
Ionospheric response modeling under eclipse conditions: Evaluation of 14 December 2020, total solar eclipse prediction over the South American sector |
| title_fullStr |
Ionospheric response modeling under eclipse conditions: Evaluation of 14 December 2020, total solar eclipse prediction over the South American sector |
| title_full_unstemmed |
Ionospheric response modeling under eclipse conditions: Evaluation of 14 December 2020, total solar eclipse prediction over the South American sector |
| title_sort |
Ionospheric response modeling under eclipse conditions: Evaluation of 14 December 2020, total solar eclipse prediction over the South American sector |
| dc.creator.none.fl_str_mv |
Bravo, M. A. Molina, Maria Graciela Martínez Ledesma, Miguel de Haro Barbás, Blas Federico Urra, B. Elias, Ana Georgina Souza, J. Villalobos, C. Namour, Jorge Habib Ovalle, E. Venchiarutti, José Valentín Blunier, S. Valdés Abreu, J.C. Guillermo, Eduardo Daniel Rojo, E. de Pasquale, Lorenzo Carrasco, E. Leiva, R. Castillo Rivera, C. Foppiano, A. Milla, M. Muñoz, P. R. Stepanova, M. Valdivia, J. A. Cabrera, Miguel Angel |
| author |
Bravo, M. A. |
| author_facet |
Bravo, M. A. Molina, Maria Graciela Martínez Ledesma, Miguel de Haro Barbás, Blas Federico Urra, B. Elias, Ana Georgina Souza, J. Villalobos, C. Namour, Jorge Habib Ovalle, E. Venchiarutti, José Valentín Blunier, S. Valdés Abreu, J.C. Guillermo, Eduardo Daniel Rojo, E. de Pasquale, Lorenzo Carrasco, E. Leiva, R. Castillo Rivera, C. Foppiano, A. Milla, M. Muñoz, P. R. Stepanova, M. Valdivia, J. A. Cabrera, Miguel Angel |
| author_role |
author |
| author2 |
Molina, Maria Graciela Martínez Ledesma, Miguel de Haro Barbás, Blas Federico Urra, B. Elias, Ana Georgina Souza, J. Villalobos, C. Namour, Jorge Habib Ovalle, E. Venchiarutti, José Valentín Blunier, S. Valdés Abreu, J.C. Guillermo, Eduardo Daniel Rojo, E. de Pasquale, Lorenzo Carrasco, E. Leiva, R. Castillo Rivera, C. Foppiano, A. Milla, M. Muñoz, P. R. Stepanova, M. Valdivia, J. A. Cabrera, Miguel Angel |
| author2_role |
author author author author author author author author author author author author author author author author author author author author author author author author |
| dc.subject.none.fl_str_mv |
ECLIPSE CONDITION IONOSPHERIC MODELING AND PREDICTION IONOSPHERIC RESPONSE SOUTH AMERICAN SECTOR TOTAL SOLAR ECLIPSE |
| topic |
ECLIPSE CONDITION IONOSPHERIC MODELING AND PREDICTION IONOSPHERIC RESPONSE SOUTH AMERICAN SECTOR TOTAL SOLAR ECLIPSE |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.5 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
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. Fil: Bravo, M. A.. Universidad de Concepción; Chile. Universidad Adventista de Chile; Chile Fil: Molina, Maria Graciela. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Tucumán; Argentina. Istituto Nazionale di Geofisica e Vulcanologia; Italia. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología; Argentina Fil: Martínez Ledesma, Miguel. Universidad de Concepción; Chile Fil: de Haro Barbás, Blas Federico. Universidad Nacional de Tucumán; Argentina Fil: Urra, B.. Universidad Adventista de Chile; Chile Fil: Elias, Ana Georgina. Universidad Nacional de Tucumán. Instituto de Física del Noroeste Argentino. - Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet Noa Sur. Instituto de Física del Noroeste Argentino; Argentina Fil: Souza, J.. Centro de Previsao de Tempo e Estudos Climáticos. Instituto Nacional de Pesquisas Espaciais; Brasil Fil: Villalobos, C.. Universidad Adventista de Chile; Chile Fil: Namour, Jorge Habib. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología; Argentina Fil: Ovalle, E.. Universidad de Concepción; Chile Fil: Venchiarutti, José Valentín. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Tucumán; Argentina Fil: Blunier, S.. Universidad de Chile; Chile Fil: Valdés Abreu, J.C.. Universidad de Chile; Chile Fil: Guillermo, Eduardo Daniel. Universidad Tecnológica Nacional; Argentina Fil: Rojo, E.. Universidad Adventista de Chile; Chile Fil: de Pasquale, Lorenzo. Universidad Tecnológica Nacional; Argentina Fil: Carrasco, E.. Universidad Adventista de Chile; Chile Fil: Leiva, R.. Universidad Adventista de Chile; Chile Fil: Castillo Rivera, C.. Universidad de Concepción; Chile Fil: Foppiano, A.. Universidad de Concepción; Chile Fil: Milla, M.. Pontificia Universidad Católica de Perú; Perú Fil: Muñoz, P. R.. Universidad de La Serena; Chile Fil: Stepanova, M.. Universidad de Santiago de Chile; Chile Fil: Valdivia, J. A.. Universidad de Chile; Chile Fil: Cabrera, Miguel Angel. Universidad Nacional de Tucumán; Argentina |
| description |
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. |
| publishDate |
2022 |
| dc.date.none.fl_str_mv |
2022-12 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
| status_str |
publishedVersion |
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http://hdl.handle.net/11336/218285 Bravo, M. A.; Molina, Maria Graciela; Martínez Ledesma, Miguel; de Haro Barbás, Blas Federico; Urra, B.; et al.; Ionospheric response modeling under eclipse conditions: Evaluation of 14 December 2020, total solar eclipse prediction over the South American sector; Frontiers Media; Frontiers in Astronomy and Space Sciences; 9; 1021910; 12-2022; 1-21 2296-987X CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/218285 |
| identifier_str_mv |
Bravo, M. A.; Molina, Maria Graciela; Martínez Ledesma, Miguel; de Haro Barbás, Blas Federico; Urra, B.; et al.; Ionospheric response modeling under eclipse conditions: Evaluation of 14 December 2020, total solar eclipse prediction over the South American sector; Frontiers Media; Frontiers in Astronomy and Space Sciences; 9; 1021910; 12-2022; 1-21 2296-987X CONICET Digital CONICET |
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eng |
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eng |
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info:eu-repo/semantics/altIdentifier/doi/10.3389/fspas.2022.1021910 info:eu-repo/semantics/altIdentifier/url/https://www.frontiersin.org/articles/10.3389/fspas.2022.1021910/full |
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