这是一个古磁场. 一个由单个晶记录的哈代到古老时代的地气模
John A Tarduno1, Rory D Cottrell2, William J Davis3
1Department of Earth and Environmental Sciences, University of Rochester, Rochester, NY 14627, USA. Department of Physics and Astronomy, University of Rochester, Rochester, NY 14627, USA. john.tarduno@rochester.edu.
概括
早期的地球
科学领域:
- 地质学
- 古磁论
- 星球科学
背景情况:
- 对于地球的进化来说, 了解地质气体的起源至关重要.
- 地磁场产生地球的磁场, 屏蔽大气层.
研究的目的:
- 使用古强度数据重建早期的地气动机历史.
- 调查哈迪地磁场所需要的条件.
主要方法:
- 在Hadean-Archean zircons中测量磁性包含的全向量古强度.
- 分析来自澳大利亚西部杰克希尔斯集团的石.
主要成果:
- 记录了33亿至42亿年前的磁场.
- 电场强度是近期赤道值的0.12到1.0倍.
- 有证据表明哈迪的地磁场.
结论:
- 一个哈迪地磁场意味着超-adiabatic核心-地幔热流.
- 这表明早期的板块构造或磁层热传输.
- 支持晚重轰炸前的磁场,影响了地球和火星的早期大气演变.
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