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海洋潮汐磁场信号对海洋电导率季节和空间变化的敏感性。

Sensitivity of M tidal magnetic signals to seasonal and spatial variations of ocean electric conductivity.

作者信息

Velímský J, Šachl L

机构信息

Faculty of Mathematics and Physics, Department of Geophysics, Charles University, V Holešovičkách 2, Praha 8 180 00, Czech Republic.

出版信息

Philos Trans A Math Phys Eng Sci. 2024 Dec 23;382(2286):20240079. doi: 10.1098/rsta.2024.0079. Epub 2024 Dec 2.

Abstract

Electrical conductivity of the Earth's oceans is an important oceanographic parameter related through its dependence on temperature and salinity to the state of the ocean. The tidally induced magnetic field then provides a directly and globally observable physical variable affected by the ocean conductivity spatial and temporal distribution. This contribution addresses two topics of the impact of the ocean conductivity variations on the principal lunar semi-diurnal magnetic signals. First, using high-resolution forward modelling, we investigate the sensitivity of the magnetic field to seasonal conductivity variations. Here, we find that the differences between magnetic signatures calculated for individual monthly conductivity climatologies are small, and localized to the marginal seas of the global ocean. Second, we formulate an inverse method to provide a constraint for the ocean conductivity in the upper 1000 m of the ocean, and test it using a synthetic dataset, demonstrating a proof-of-concept for such an approach.This article is part of the theme issue 'Magnetometric remote sensing of Earth and planetary oceans'.

摘要

地球海洋的电导率是一个重要的海洋学参数,它通过对温度和盐度的依赖关系与海洋状态相关。潮汐感应磁场则提供了一个受海洋电导率时空分布影响的、可直接在全球范围内观测的物理变量。本文探讨了海洋电导率变化对主要月球半日磁信号影响的两个主题。首先,利用高分辨率正演模拟,我们研究了磁场对季节性电导率变化的敏感性。在此,我们发现针对各个月电导率气候学计算出的磁特征差异很小,且局限于全球海洋的边缘海域。其次,我们制定了一种反演方法,为海洋上层1000米的电导率提供约束,并使用合成数据集对其进行测试,证明了这种方法的概念验证。本文是“地球和行星海洋的磁力遥感”主题特刊的一部分。

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