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http://hdl.handle.net/10662/21093
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Campo DC | Valor | idioma |
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dc.contributor.author | Peguero Chamizo, Juan Carlos | - |
dc.contributor.author | Sánchez Carrasco, Víctor Manuel | - |
dc.date.accessioned | 2024-04-24T11:38:53Z | - |
dc.date.available | 2024-04-24T11:38:53Z | - |
dc.date.issued | 2023 | - |
dc.identifier.issn | 0038-0938 | - |
dc.identifier.uri | http://hdl.handle.net/10662/21093 | - |
dc.description | Open Access funding provided thanks to the CRUE-CSIC agreement with Springer Nature | es_ES |
dc.description.abstract | The sunspot number is the most used solar-activity index to study the behavior of solar activity. In this work, we reproduce the methodology of Coban, Raheem, and Cavus (Solar Phys. 296, 156, 2021) using a long short-term memory model with daily data from the American Association of Variable Star Observers (AAVSO) to predict the maximum amplitude of Solar Cycle 25. We have also used that same methodology with daily values from the official sunspot number (Version 2) of the Sunspot Index and Long-term Solar Observations (SILSO). The objective of this work is to analyze if the predictions obtained from that methodology agree with the observed values available for the current Solar Cycle 25. Thus, we conclude that the predictions are not reproducing well the behavior of the Solar Cycle 25 in its rising phase. Moreover, contrary to the previous prediction, no minor peak occurred in February 2022, and we also conclude that it seems unlikely that the combination of the solar-activity level of Solar Cycle 24 and 25 constitutes a new Dalton-type Minimum, such as Coban, Raheem, and Cavus (2021) proposed. | es_ES |
dc.description.sponsorship | This research was supported by the Economy and Infrastructure Counselling of the Junta of Extremadura through project IB20080 (co-financed by the European Regional Development Fund). The authors acknowledge the sunspot observations provided by SILSO and AAVSO. The authors also thank José M. Vaquero for his helpful comments and wise advice. | es_ES |
dc.format.extent | 14 p. | es_ES |
dc.format.mimetype | application/pdf | en_US |
dc.language.iso | eng | es_ES |
dc.publisher | Springer | es_ES |
dc.rights | Attribution 4.0 International | * |
dc.rights.uri | http://creativecommons.org/licenses/by/4.0/ | * |
dc.subject | Solar activity | es_ES |
dc.subject | Dataset | es_ES |
dc.subject | Prediction | es_ES |
dc.subject | Neural network | es_ES |
dc.subject | Actividad Solar | es_ES |
dc.subject | Conjunto de datos | es_ES |
dc.subject | Predicción | es_ES |
dc.subject | Red neuronal | es_ES |
dc.subject | Sunspots | en_US |
dc.subject | Sunspot number | en_US |
dc.subject | Solar cycle | en_US |
dc.subject | Solar cycle 25 | en_US |
dc.subject | Solar activity forecast | en_US |
dc.subject | Deep learning | en_US |
dc.subject | Manchas solares | es_ES |
dc.subject | Número de manchas solares | es_ES |
dc.subject | Ciclo solar | es_ES |
dc.subject | Ciclo solar 25 | es_ES |
dc.subject | Previsión de actividad solar | es_ES |
dc.subject | Aprendizaje profundo | es_ES |
dc.title | A critical comment on “can solar cycle 25 be a new Dalton minimum?” | es_ES |
dc.type | article | es_ES |
dc.description.version | peerReviewed | es_ES |
europeana.type | TEXT | en_US |
dc.rights.accessRights | openAccess | es_ES |
dc.subject.unesco | 21 Astronomía y Astrofísica | es_ES |
dc.subject.unesco | 2106.01 Energía Solar | es_ES |
dc.subject.unesco | 2106.02 Física Solar | es_ES |
europeana.dataProvider | Universidad de Extremadura. España | es_ES |
dc.identifier.bibliographicCitation | Peguero, J.C., Carrasco, V.M.S.(2023) A Critical Comment on “Can Solar Cycle 25 Be a New Dalton Minimum?”. Sol Phys 298, 48. https://doi.org/10.1007/s11207-023-02140-7 | es_ES |
dc.type.version | publishedVersion | es_ES |
dc.contributor.affiliation | Universidad de Extremadura. Departamento de Física | es_ES |
dc.contributor.affiliation | Universidad de Extremadura. Departamento de Ingeniería Eléctrica, Electrónica y Automática | es_ES |
dc.contributor.affiliation | Universidad de Extremadura. Instituto Universitario de Investigación del Agua, Cambio Climático y Sostenibilidad (IACYS) | - |
dc.relation.publisherversion | https://link.springer.com/article/10.1007/s11207-023-02140-7 | es_ES |
dc.identifier.doi | 10.1007/s11207-023-02140-7 | - |
dc.identifier.publicationtitle | Solar Physics | es_ES |
dc.identifier.publicationfirstpage | 48-1 | es_ES |
dc.identifier.publicationlastpage | 48-14 | es_ES |
dc.identifier.publicationvolume | 298 | es_ES |
dc.identifier.e-issn | 1573-093X | - |
dc.identifier.orcid | 0000-0001-9358-1219 | es_ES |
dc.identifier.orcid | 0000-0002-3564-9876 | es_ES |
Colección: | DFSCA - Artículos DIEEA - Artículos IACYS - Artículos |
Archivos
Archivo | Descripción | Tamaño | Formato | |
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s11207-023-02140-7.pdf | 3,72 MB | Adobe PDF | Descargar |
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