Long-term solar variability deduced from changes in the atmospheric 14C production rate
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Resumen
Un análisis espectral de la producción de 14C en la atmósfera (300-1900 d.C) evidencia la existencia de oscilaciones superseculares en la actividad solar. Se somete a prueba la significación y estabilidad de estas oscilaciones mediante la reproducción del registro histórico. La extensión de este registro hacia el futuro muestra que una nueva oscilación del tipo Sporer, similar a la ocurrida durante el siglo XV, es muy probable que ocurra de nuevo alrededor del año 2300.
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