在南极冰层中,有3万年的宇宙尘埃
Gisela Winckler1, Hubertus Fischer
1Lamont-Doherty Earth Observatory (L-DEO), Earth Institute at Columbia University, Palisades, NY 10964, USA. winckler@ldeo.columbia.edu
概括
来自南极冰芯的宇宙尘埃记录显示,3万年来-3不断流动,排除它是冰川周期的驱动因素. 这支持-3作为一个稳定的古气候代理.
科学领域:
- 古气候学 古气候学
- 宇宙尘埃研究 宇宙尘埃研究
- 同位素地球化学 同位素地球化学
背景情况:
- 极地冰芯保留了历史上的宇宙尘埃涌入.
- 同位素 (3He和4He) 用作宇宙尘埃的代理物.
- 欧洲南极冰项目 (EPICA) 提供了有价值的冰芯数据.
研究的目的:
- 为了重建一个高分辨率的冰川到冰川间的宇宙尘埃记录.
- 为了研究-3 (3He) 流在普莱斯托纪晚期冰川周期中的作用.
- 为了确定冰川和冰川间时期之间的陆地尘埃来源的变化.
主要方法:
- 高分辨率的同位素分析 (3He和4He).
- 来自南极洲Dronning Maud陆地的EPICA冰芯的分析.
- 测量非海盐 (Ca2+),以评估陆地尘埃的贡献.
主要成果:
- 在过去的3万年里,观察到相对恒定的3He流.
- 发现3He流是独立于冰川-冰川间周期的.
- 从最后一个冰川时期到Holocene,检测到4He/非海盐Ca2+比率的变化.
结论:
- -3不是晚期普莱斯托时代冰川周期的起器.
- 在古气候研究中,-3作为可靠的恒流参数.
- 观察到的4He/非海盐Ca2+比率的变化表明,在气候转变期间,陆地尘埃来源发生了变化.
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