地球富含铁的基本岩海洋的电和热导电性
Francis Dragulet1, Lars Stixrude1
1Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, CA 90095.
概括
地球的早期磁场可能是在深海的岩中形成的. 在这个海洋中丰富的铁可以维持动力发电机活动,在数十亿年内影响行星磁场的产生.
科学领域:
- 地质物理学 地质物理学
- 行星科学 行星科学
- 凝聚物质物理学 凝聚物质物理学
背景情况:
- 地球最早的磁场被假设起源于一个基底岩海洋.
- 在这种岩海洋中的电导率可能超过动力发电机活动的值.
- 由于地幔矿物学,预计基底岩海洋中的铁缩.
研究的目的:
- 为了研究铁丰富对酸盐动力发电机假设的影响.
- 为了确定在基底岩海洋条件下电导率如何随铁含量而变化.
- 为了评估铁丰富的基础岩海洋的对流动不稳定性.
主要方法:
- Ab-initio分子动力学的计算.
- 在相关的压力和温度下计算电导率.
- 电子导热率的计算.
主要成果:
- 酸盐液体的电导率在不同的铁缩下进行了分析.
- 评估了铁对动力发电机活动潜力的影响.
- 计算了导热率以评估对流动不稳定性.
结论:
- 铁的丰富显著影响了基底岩海洋的电导率.
- 在考虑现实的铁含量时,重新评估了酸盐发动机假设.
- 热和磁演变的建模为早期地球的地力学提供了洞察力.
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