在公元前第一千年,用树环和放射性碳追踪古代太阳周期
Nicolas Brehm1,2, Charlotte L Pearson3, Marcus Christl4
1Laboratory of Tree Ring Research, University of Arizona, Bryant Bannister Tree-Ring Building, 1215 E. Lowell Street, Tucson, AZ, 85721-0045, USA. nbrehm@arizona.edu.
Nature communications
|January 6, 2025
概括
本研究介绍了公元前第一千年的详细14C树环记录. 它证实了11年的太阳周期,并且在此期间没有发现新的太阳能粒子 (SEP) 事件.
科学领域:
- 古气候学 古气候学
- 太阳物理 太阳物理
- 放射性约会方法 放射性约会方法
背景情况:
- 太阳的变化影响着地球的气候和农业,但直接太阳观测是有限的.
- 树环中的宇宙射线产生的放射性核酸,如碳-14 (C),扩展了我们对过去太阳活动的理解.
- 现有的记录往往缺乏研究短期太阳现象和太阳能粒子 (SEP) 事件的分辨率或跨度.
研究的目的:
- 重建一个高分辨率,连续的大气14C记录,跨越公元前一千年.
- 调查短期太阳现象,包括11年太阳周期和潜在的SEP事件.
- 为改善放射性碳校准和日期准确性提供数据集.
主要方法:
- 在树环中分析每年得到的14C度.
- 从公元前第一千年的大气14C水平的重建.
- 在C记录中识别和描述太阳周期和异常.
主要成果:
- 从公元前第一千年开始,建立了一个连续的,每年解决的大气14C记录.
- 11年的太阳周期是明确定义的,平均周期为10.5年,幅度约为0.4‰.
- 在此期间没有发现新的太阳能粒子 (SEP) 事件的证据.
结论:
- 呈现的14C记录提供了前所未有的关于太阳在长时间尺度上的行为细节.
- 结果为气候研究和太阳能危害减缓战略提供了宝贵的见解.
- 该数据集提高了这个历史时期的放射性碳校准和约会的准确性.
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