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Records of sunspots and aurora candidates in the Chinese official histories of the Yuán and Míng dynasties during 1261–1644

机译:在1261年至1644年间,中国元和明朝的官方历史上有黑子和极光的记录

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Records of observations of sunspots and auroras in pre-telescopic historical documents provide useful information about past solar activity both in long-term trends and short-term space weather events. In this study, we present the results of a comprehensive survey of the records of sunspots and aurora candidates in the Yuánsh? and Míngsh?, Chinese Official Histories spanning 1261–1368 and 1368–1644, based on continuous observations with well-formatted reportds conducted by contemporary professional astronomers. We then provide a brief comparison of these data with Total Solar Irradiance (TSI) as an indicator of the solar activity during the corresponding periods to show significant active phases between the 1350s–80s and 1610s–30s. We then compared the former with contemporary Russian reports concerning naked-eye sunspots and the latter with contemporary sunspot drawings based on Western telescopic observations. Especially some of the latter are consistent with nitrate signals preserved in ice cores. These results show us some insights on and beyond minima and maxima of solar activity during the 13th–17th centuries.
机译:在望远镜前的历史文献中对黑子和极光的观测记录提供了有关长期趋势和短期空间天气事件中过去太阳活动的有用信息。在这项研究中,我们提出了对Yuánsh?黑子和极光候选者的记录进行全面调查的结果。和Míngsh?,中国的官方历史跨越了1261–1368和1368–1644,是基于对当代专业天文学家进行的格式合理的报道的连续观察得出的。然后,我们将这些数据与总太阳辐照度(TSI)进行简要比较,以作为相应时期太阳活动的指标,以显示1350s–80s和1610s–30s之间的重要活动阶段。然后,我们将前者与当代俄罗斯关于裸眼黑子的报道进行了比较,而将后者与基于西方望远镜观测的当代黑子图进行了比较。特别是后者中的一些与保存在冰芯中的硝酸盐信号一致。这些结果向我们展示了在13至17世纪太阳活动的最小值和最大值之外的一些见解。

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