由于海洋潮流造成的磁场的卫星观测
Robert H Tyler1, Stefan Maus, Hermann Lühr
1Ocean Physics Department, Applied Physics Laboratory, University of Washington, 1013 NE 40th Street, Seattle, WA 98103, USA. tyler@apl.washington.edu
概括
海流会产生磁场,可被卫星探测到. 这项研究确定了来自海洋月球半日潮 (M2) 的磁信号,证明海洋磁场可以从远程清晰地观察到.
科学领域:
- 地质物理学 地质物理学
- 海洋学 海洋学 海洋学
- 太空科学 太空科学
背景情况:
- 地球上的海洋是导电流体.
- 海洋电流与地球磁场相互作用,产生二次磁场.
- 卫星技术现在使得这些磁场的遥感成为可能.
研究的目的:
- 为了研究由海洋月球半昼 (M2) 潮流产生的磁场.
- 在卫星观测中证明海洋磁场的可检测性.
主要方法:
- 对卫星磁场测量的分析.
- 模拟海洋潮流产生的磁场.
主要成果:
- 成功识别出源于海洋月球半日潮 (M2) 的磁场.
- 这些海洋磁信号在卫星数据中清晰可辨.
结论:
- 卫星观测可以有效地检测海洋潮产生的磁场.
- 这种能力为远程研究海洋动态开辟了新的途径.
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