概括
宇宙射线产生-10和-26同位素,这些同位素在古格陵兰岛的冰中发现. 它们在冰中的测量产量率与大气中的宇宙射线产量一致,这表明宇宙尘埃的贡献最小.
科学领域:
- 地质化学 地质化学
- 宇宙化学 宇宙化学
- 核物理 核物理 核物理
背景情况:
- -10 (Be-10) 和-26 (Al-26) 是宇宙生成的同位素.
- 冰芯为研究过去大气和外星物质沉积提供了宝贵的档案.
研究的目的:
- 测量度并计算古格陵兰冰中的Be-10和Al-26的生产率.
- 为了将这些速率与已知的宇宙射线大气产生的速率进行比较.
- 估计外星尘埃对冰中这些同位素存在的贡献.
主要方法:
- 对格陵兰岛200年老冰层中溶解的Be-10和Al-26活动的分析.
- 使用测量活动和冰沉降率计算同位素生产率.
- 对外星尘埃流入的上限估计.
主要成果:
- 溶解的Be-10活动:18.4 (+8.4, -4.8) x 10^-6dpm/L.
- 溶解的Al-26活动:3.2 +/- 0.9 x 10^-7dpm/L.
- 计算的产量速度与大气宇宙射线产量一致.
- 带有Al-26的宇宙尘埃流入的上限:每年3.2 x 10^5.
结论:
- 大气中由宇宙射线产生的Be-10和Al-26是研究格陵兰岛冰中的主要来源.
- 对于Al-26,外星尘埃的贡献可能是最小的.
- 颗粒物中的Be-10和Al-26的上限值不会改变主要的结论.
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