Predicting sunspot number from topological features in spectral images I: Machine learning approach
This study presents an advanced machine learning approach to predict the number of sunspots using a comprehensive dataset derived from solar images provided by the Solar and Heliospheric Observatory (SOHO). The dataset encompasses various spectral bands, capturing the complex dynamics of solar activ...
- Autores:
-
Sierra Porta, David
Tarazona Alvarado, Miguel
Herrera Acevedo, Daniel
- Tipo de recurso:
- Fecha de publicación:
- 2024
- Institución:
- Universidad Tecnológica de Bolívar
- Repositorio:
- Repositorio Institucional UTB
- Idioma:
- eng
- OAI Identifier:
- oai:repositorio.utb.edu.co:20.500.12585/12701
- Acceso en línea:
- https://hdl.handle.net/20.500.12585/12701
- Palabra clave:
- Machine learning
Sunspots prediction
Spectral images
Sun’s dynamics
Fractal features
LEMB
- Rights
- openAccess
- License
- http://creativecommons.org/publicdomain/zero/1.0/
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dc.title.spa.fl_str_mv |
Predicting sunspot number from topological features in spectral images I: Machine learning approach |
title |
Predicting sunspot number from topological features in spectral images I: Machine learning approach |
spellingShingle |
Predicting sunspot number from topological features in spectral images I: Machine learning approach Machine learning Sunspots prediction Spectral images Sun’s dynamics Fractal features LEMB |
title_short |
Predicting sunspot number from topological features in spectral images I: Machine learning approach |
title_full |
Predicting sunspot number from topological features in spectral images I: Machine learning approach |
title_fullStr |
Predicting sunspot number from topological features in spectral images I: Machine learning approach |
title_full_unstemmed |
Predicting sunspot number from topological features in spectral images I: Machine learning approach |
title_sort |
Predicting sunspot number from topological features in spectral images I: Machine learning approach |
dc.creator.fl_str_mv |
Sierra Porta, David Tarazona Alvarado, Miguel Herrera Acevedo, Daniel |
dc.contributor.author.none.fl_str_mv |
Sierra Porta, David Tarazona Alvarado, Miguel Herrera Acevedo, Daniel |
dc.subject.keywords.spa.fl_str_mv |
Machine learning Sunspots prediction Spectral images Sun’s dynamics Fractal features |
topic |
Machine learning Sunspots prediction Spectral images Sun’s dynamics Fractal features LEMB |
dc.subject.armarc.none.fl_str_mv |
LEMB |
description |
This study presents an advanced machine learning approach to predict the number of sunspots using a comprehensive dataset derived from solar images provided by the Solar and Heliospheric Observatory (SOHO). The dataset encompasses various spectral bands, capturing the complex dynamics of solar activity and facilitating interdisciplinary analyses with other solar phenomena. We employed five machine learning models: Random Forest Regressor, Gradient Boosting Regressor, Extra Trees Regressor, Ada Boost Regressor, and Hist Gradient Boosting Regressor, to predict sunspot numbers. These models utilized four key heliospheric variables — Proton Density, Temperature, Bulk Flow Speed and Interplanetary Magnetic Field (IMF) — alongside 14 newly introduced topological variables. These topological features were extracted from solar images using different filters, including HMIIGR, HMIMAG, EIT171, EIT195, EIT284, and EIT304. In total, 60 models were constructed, both incorporating and excluding the topological variables. Our analysis reveals that models incorporating the topological variables achieved significantly higher accuracy, with the r2-score improving from approximately 0.30 to 0.93 on average. The Extra Trees Regressor (ET) emerged as the best-performing model, demonstrating superior predictive capabilities across all datasets. These results underscore the potential of combining machine learning models with additional topological features from spectral analysis, offering deeper insights into the complex dynamics of solar activity and enhancing the precision of sunspot number predictions. This approach provides a novel methodology for improving space weather forecasting and contributes to a more comprehensive understanding of solar-terrestrial interactions. |
publishDate |
2024 |
dc.date.accessioned.none.fl_str_mv |
2024-07-29T16:52:06Z |
dc.date.available.none.fl_str_mv |
2024-07-29T16:52:06Z |
dc.date.issued.none.fl_str_mv |
2024-07-19 |
dc.date.submitted.none.fl_str_mv |
2024-07-29 |
dc.type.coarversion.fl_str_mv |
http://purl.org/coar/version/c_970fb48d4fbd8a85 |
dc.type.driver.spa.fl_str_mv |
info:eu-repo/semantics/article |
dc.type.hasversion.spa.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.spa.spa.fl_str_mv |
http://purl.org/coar/resource_type/c_2df8fbb1 |
status_str |
publishedVersion |
dc.identifier.citation.spa.fl_str_mv |
Sierra-Porta, D., Tarazona-Alvarado, M., & Acevedo, D. H. (2024). Predicting sunspot number from topological features in spectral images I: Machine learning approach. Astronomy and Computing, 100857. https://doi.org/10.1016/j.ascom.2024.100857 |
dc.identifier.uri.none.fl_str_mv |
https://hdl.handle.net/20.500.12585/12701 |
dc.identifier.doi.none.fl_str_mv |
10.1016/j.ascom.2024.100857 |
dc.identifier.instname.spa.fl_str_mv |
Universidad Tecnológica de Bolívar |
dc.identifier.reponame.spa.fl_str_mv |
Repositorio Universidad Tecnológica de Bolívar |
identifier_str_mv |
Sierra-Porta, D., Tarazona-Alvarado, M., & Acevedo, D. H. (2024). Predicting sunspot number from topological features in spectral images I: Machine learning approach. Astronomy and Computing, 100857. https://doi.org/10.1016/j.ascom.2024.100857 10.1016/j.ascom.2024.100857 Universidad Tecnológica de Bolívar Repositorio Universidad Tecnológica de Bolívar |
url |
https://hdl.handle.net/20.500.12585/12701 |
dc.language.iso.spa.fl_str_mv |
eng |
language |
eng |
dc.rights.coar.fl_str_mv |
http://purl.org/coar/access_right/c_abf2 |
dc.rights.uri.*.fl_str_mv |
http://creativecommons.org/publicdomain/zero/1.0/ |
dc.rights.accessrights.spa.fl_str_mv |
info:eu-repo/semantics/openAccess |
dc.rights.cc.*.fl_str_mv |
CC0 1.0 Universal |
rights_invalid_str_mv |
http://creativecommons.org/publicdomain/zero/1.0/ CC0 1.0 Universal http://purl.org/coar/access_right/c_abf2 |
eu_rights_str_mv |
openAccess |
dc.format.extent.none.fl_str_mv |
10 páginas |
dc.format.mimetype.spa.fl_str_mv |
application/pdf |
dc.publisher.place.spa.fl_str_mv |
Cartagena de Indias |
dc.source.spa.fl_str_mv |
Astronomy and Computing |
institution |
Universidad Tecnológica de Bolívar |
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Sierra Porta, David88a81b30-0b54-4821-b432-affefb13412bTarazona Alvarado, Miguelef024c8f-0c62-47e6-90e1-9de2e2566b23Herrera Acevedo, Daniel2f2e14ba-6e9b-4697-a7f7-312414a61c762024-07-29T16:52:06Z2024-07-29T16:52:06Z2024-07-192024-07-29Sierra-Porta, D., Tarazona-Alvarado, M., & Acevedo, D. H. (2024). Predicting sunspot number from topological features in spectral images I: Machine learning approach. Astronomy and Computing, 100857. https://doi.org/10.1016/j.ascom.2024.100857https://hdl.handle.net/20.500.12585/1270110.1016/j.ascom.2024.100857Universidad Tecnológica de BolívarRepositorio Universidad Tecnológica de BolívarThis study presents an advanced machine learning approach to predict the number of sunspots using a comprehensive dataset derived from solar images provided by the Solar and Heliospheric Observatory (SOHO). The dataset encompasses various spectral bands, capturing the complex dynamics of solar activity and facilitating interdisciplinary analyses with other solar phenomena. We employed five machine learning models: Random Forest Regressor, Gradient Boosting Regressor, Extra Trees Regressor, Ada Boost Regressor, and Hist Gradient Boosting Regressor, to predict sunspot numbers. These models utilized four key heliospheric variables — Proton Density, Temperature, Bulk Flow Speed and Interplanetary Magnetic Field (IMF) — alongside 14 newly introduced topological variables. These topological features were extracted from solar images using different filters, including HMIIGR, HMIMAG, EIT171, EIT195, EIT284, and EIT304. In total, 60 models were constructed, both incorporating and excluding the topological variables. Our analysis reveals that models incorporating the topological variables achieved significantly higher accuracy, with the r2-score improving from approximately 0.30 to 0.93 on average. The Extra Trees Regressor (ET) emerged as the best-performing model, demonstrating superior predictive capabilities across all datasets. These results underscore the potential of combining machine learning models with additional topological features from spectral analysis, offering deeper insights into the complex dynamics of solar activity and enhancing the precision of sunspot number predictions. This approach provides a novel methodology for improving space weather forecasting and contributes to a more comprehensive understanding of solar-terrestrial interactions.10 páginasapplication/pdfenghttp://creativecommons.org/publicdomain/zero/1.0/info:eu-repo/semantics/openAccessCC0 1.0 Universalhttp://purl.org/coar/access_right/c_abf2Astronomy and ComputingPredicting sunspot number from topological features in spectral images I: Machine learning approachinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_2df8fbb1http://purl.org/coar/version/c_970fb48d4fbd8a85Machine learningSunspots predictionSpectral imagesSun’s dynamicsFractal featuresLEMBCartagena de IndiasPúblico generalAggarwal, A., Kumar, M., 2021. Image surface texture analysis and classification using deep learning. Multimedia Tools Appl. 80 (1), 1289–1309. doi:10.1007/s11042- 020-09520-2Alexakis, P., Mavromichalaki, H., 2019. 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Earth Planetary Sci. 8, 1–102. doi:10.1186/s40645-021-00426-7.http://purl.org/coar/resource_type/c_2df8fbb1ORIGINALPredicting sunspot number from topological features in spectral images I_ Machine learning approach.pdfPredicting sunspot number from topological features in spectral images I_ Machine learning approach.pdfArtículo principalapplication/pdf2598683https://repositorio.utb.edu.co/bitstream/20.500.12585/12701/1/Predicting%20sunspot%20number%20from%20topological%20features%20in%20spectral%20images%20I_%20Machine%20learning%20approach.pdf3120f240687c7becff7ed0457468006aMD51CC-LICENSElicense_rdflicense_rdfapplication/rdf+xml; charset=utf-8701https://repositorio.utb.edu.co/bitstream/20.500.12585/12701/2/license_rdf42fd4ad1e89814f5e4a476b409eb708cMD52LICENSElicense.txtlicense.txttext/plain; charset=utf-83182https://repositorio.utb.edu.co/bitstream/20.500.12585/12701/3/license.txte20ad307a1c5f3f25af9304a7a7c86b6MD53TEXTPredicting sunspot number from topological features in spectral 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