Solar irradiance during the Maunder minimum

Blanca Mendoza

doi:10.22201/igeof.00167169p.1996.35.2.858

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Publicado: abr 1, 1996

DOI: https://doi.org/10.22201/igeof.00167169p.1996.35.2.858

Palabras clave:

lrradiancia solar, mínimo de Maunder

Blanca Mendoza

Universidad Nacional Autónoma de México, Instituto de Geofísica, Departamento de Física Espacial, Ciudad Universitaria, Delegación Coyoacán, 04510, Mexico City, México

Resumen

Se calcula la irradiancia solar total durante el periodo del mínimo de Maunder (1645-1715) usando la rotación solar. Se encuentra que esta irradiancia fue en promedio 0.1 a 0.43 % menor que la actual. Estos resultados concuerdan con la existencia de un periodo global de enfriamiento terrestre durante la segunda mitad del siglo XVII. Nuestro modelo calcula mejor las razones de rotación y los flujos HK que los modelos basados en cambios aparentes del radio solar.

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Cómo citar

Mendoza, B. (1996). Solar irradiance during the Maunder minimum. Geofísica Internacional, 35(2), 161–167. https://doi.org/10.22201/igeof.00167169p.1996.35.2.858

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Vol. 35 Núm. 2 (1996): Abril 1, 1996

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Esta obra está bajo una licencia internacional Creative Commons Atribución-NoComercial-CompartirIgual 4.0.

Biografía del autor/a

Blanca Mendoza, Universidad Nacional Autónoma de México, Instituto de Geofísica, Departamento de Física Espacial, Ciudad Universitaria, Delegación Coyoacán, 04510, Mexico City, México

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