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http://hdl.handle.net/10662/21106
| Títulos: | Prediction of the maximum amplitude of solar cycle 25 using the ascending inflection point |
| Autores/as: | Pérez Aparicio, Alejandro Jesús Sánchez Carrasco, Víctor Manuel Vaquero Martínez, José M. |
| Palabras clave: | Número de mancha solar;Mancha solar;Ciclo solar;Observaciones;Sunspot number;Sunspots;Statistics;Solar cycle;Observations |
| Fecha de publicación: | 2023 |
| Editor/a: | Springer |
| Resumen: | In this work, we predict the maximum amplitude (using the 13-month smoothed Solar Influences Data Analysis Center (SILSO) Sunspot Number, version 2) of Solar Cycle 25 using as a predictor the slope of the inflection point during the ascending part of the cycle. After a description of the data and methodology employed in this work, we obtain a value of 131 ± 32 for the maximum amplitude of Solar Cycle 25. Finally, we discuss this result in the context of the current debate on the prediction of solar activity and compare it with other predictions of Solar Cycle 25 obtained by other methods. |
| URI: | http://hdl.handle.net/10662/21106 |
| DOI: | 10.1007/s11207-023-02194-7 |
| Colección: | DFSCA - Artículos IACYS - Artículos |
Archivos
| Archivo | Descripción | Tamaño | Formato | |
|---|---|---|---|---|
| s11207_023_02194_7.pdf | 1,05 MB | Adobe PDF | Descargar |
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