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来自海洋潮汐的磁信号:新的卫星观测与应用

Magnetic signals from oceanic tides: new satellite observations and applications.

作者信息

Grayver Alexander, Finlay Christopher C, Olsen Nils

机构信息

Institute of Geophysics and Meteorology, University of Cologne, Cologne, Germany.

DTU Space, Technical University of Denmark, Lyngby, Hovedstaden, Denmark.

出版信息

Philos Trans A Math Phys Eng Sci. 2024 Dec 23;382(2286):20240078. doi: 10.1098/rsta.2024.0078. Epub 2024 Dec 2.

DOI:10.1098/rsta.2024.0078
PMID:39617039
Abstract

The tidal flow of seawater across the Earth's magnetic field induces electric currents and magnetic fields within the ocean and solid Earth. The amplitude and phase of the induced fields depend on the electrical properties of both seawater and the solid Earth, and thus can be used as proxies to study the seabed properties or potentially for monitoring long-term trends in the global ocean climatology. This article presents new global oceanic tidal magnetic field models and their uncertainties for four tidal constituents, including [Formula: see text] and even [Formula: see text], which was not reliably retrieved previously. Models are obtained through a robust least-squares analysis of magnetic field observations from the and CHAMP satellites using a specially designed data selection scheme. We compare the retrieved magnetic signals with several alternative models reported in the literature. Additionally, we validate them using a series of high-resolution global three-dimensional (3D) electromagnetic simulations and place constraints on the conductivity of the sub-oceanic mantle for all tidal constituents, revealing an excellent agreement between all tidal constituents and the oceanic upper mantle structure.This article is part of the theme issue 'Magnetometric remote sensing of Earth and planetary oceans'.

摘要

海水穿过地球磁场的潮流动在海洋和固体地球内部感应出电流和磁场。感应场的振幅和相位取决于海水和固体地球的电学性质,因此可以用作研究海底性质的代理指标,或者潜在地用于监测全球海洋气候学的长期趋势。本文给出了新的全球海洋潮汐磁场模型及其针对四个潮汐成分的不确定性,包括[公式:见正文]甚至[公式:见正文],后者此前未能可靠获取。模型是通过使用专门设计的数据选择方案对来自[卫星名称]和CHAMP卫星的磁场观测数据进行稳健的最小二乘分析得到的。我们将检索到的磁信号与文献中报道的几种替代模型进行了比较。此外,我们使用一系列高分辨率的全球三维(3D)电磁模拟对它们进行了验证,并对所有潮汐成分的洋下地幔电导率施加了约束,揭示了所有潮汐成分与海洋上地幔结构之间的极佳一致性。本文是主题为“地球和行星海洋的磁力遥感”的一部分。

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1
Magnetic signals from oceanic tides: new satellite observations and applications.来自海洋潮汐的磁信号:新的卫星观测与应用
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引用本文的文献

1
Physical oceanographic factors controlling the ocean circulation-induced magnetic field.控制海洋环流感应磁场的物理海洋学因素。
Philos Trans A Math Phys Eng Sci. 2024 Dec 23;382(2286):20240076. doi: 10.1098/rsta.2024.0076. Epub 2024 Dec 2.
2
Magnetometric remote sensing of Earth and planetary oceans.地球和行星海洋的磁力遥感
Philos Trans A Math Phys Eng Sci. 2024 Dec 23;382(2286):20240089. doi: 10.1098/rsta.2024.0089. Epub 2024 Dec 2.
3
Satellite monitoring of long period ocean-induced magnetic field variations.
长期海洋诱发磁场变化的卫星监测
Philos Trans A Math Phys Eng Sci. 2024 Dec 23;382(2286):20240077. doi: 10.1098/rsta.2024.0077. Epub 2024 Dec 2.