Sensitivity of M<sub>2</sub>tidal magnetic signals to seasonal and spatial variations of ocean electric conductivity

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'.

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Publication Details

Journal
Philosophical Transactions of the Royal Society A Mathematical Physical and Engineering Sciences
Published
2024-12-02
DOI
https://doi.org/10.1098/rsta.2024.0079
Citations
3
Primary Topic
Geophysical and Geoelectrical Methods
Type
article
Field-Weighted Citation Impact
1.60

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article

Sensitivity of M2tidal magnetic signals to seasonal and spatial variations of ocean electric conductivity

Jakub Velı́mský, Libor Šachl
3 citations
Philosophical Transactions of the Royal Society A Mathematical Physical and Engineering Sciences
Geophysical and Geoelectrical Methods
1.60
article

Sensitivity of M2tidal magnetic signals to seasonal and spatial variations of ocean electric conductivity

Jakub Velı́mský, Libor Šachl
article en
3 citations

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'.

Philosophical Transactions of the Royal Society A Mathematical Physical and Engineering SciencesVol. 382(2286)
Charles University (CZ)
European Space Agency, Ministerstvo Školství, Mládeže a Tělovýchovy
Life below water
Openalex Percentile: Top 17%
Geophysical and Geoelectrical Methods
1.60
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