Rapid computation of gravity anomalies and gradients using sparse decomposition in the wavenumber domain

Abstract Conventional gravity anomaly forward methods in the spatial-domain are grounded in the theoretical foundation of full-spectrum response. However, widely used gravity field spherical harmonic models such as Earth Gravitational Model (EGM) and European Improved Gravity model of the Earth (EIGEN) are finite-degree spherical harmonic expansions, inherently possessing a band-limited nature. This theoretical mismatch between the full-spectrum forward assumption and the band-limited data leads to unavoidable truncation errors, thereby compromising the accuracy and reliability of subsequent inversion. To address the above issues, this study systematically elaborates a wavenumber-domain rapid forward method for 3D gravity anomalies and their gradient tensors. By decomposing the dense Green's function matrix into the product of three sparse matrices in the wavenumber-domain, the computation workflow is straightforward. The truncation error between the wavenumber-domain and spatial-domain forward can systematically decreases as the observation points increases. The elaborated forward approach replaces the layer-by-layer calculation process with efficient sparse matrix multiplication; compared with spatial-domain methods, computational efficiency is significantly improved. The advantage of this method lies in the consistency between its inherent finite-frequency characteristics and the degree limitation of spherical harmonic models in the wave-number domain. This forward framework is more theoretically compatible with the band-limited nature of finite-degree gravity data, thereby effectively avoiding the theoretical mismatch problem inherent in traditional spatial-domain methods between the full-spectrum model and band-limited data. Therefore, the wave-number domain forward method elaborated provides a computationally efficient, low-memory, and theoretically self-consistent technical solution for processing modelling satellite, aerial, and ground-based gravity and its gradient tensor data. Graphical Abstract

Authors

Publication Details

Journal
Earth Planets and Space
Published
2026-04-25
DOI
https://doi.org/10.1186/s40623-026-02416-9
Primary Topic
Geophysics and Gravity Measurements
Type
article
Field-Weighted Citation Impact
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article

Rapid computation of gravity anomalies and gradients using sparse decomposition in the wavenumber domain

Yiju Tang, Quan Lou, Sheng Liu, Songbai Xuan et al.
Earth Planets and Space
Geophysics and Gravity Measurements
article

Rapid computation of gravity anomalies and gradients using sparse decomposition in the wavenumber domain

Yiju Tang, Quan Lou, Sheng Liu, Songbai Xuan, Renjie Yu, Fangchao Lu, Zhanfeng Huang, Shi Chen
article en

Abstract

Abstract Conventional gravity anomaly forward methods in the spatial-domain are grounded in the theoretical foundation of full-spectrum response. However, widely used gravity field spherical harmonic models such as Earth Gravitational Model (EGM) and European Improved Gravity model of the Earth (EIGEN) are finite-degree spherical harmonic expansions, inherently possessing a band-limited nature. This theoretical mismatch between the full-spectrum forward assumption and the band-limited data leads to unavoidable truncation errors, thereby compromising the accuracy and reliability of subsequent inversion. To address the above issues, this study systematically elaborates a wavenumber-domain rapid forward method for 3D gravity anomalies and their gradient tensors. By decomposing the dense Green's function matrix into the product of three sparse matrices in the wavenumber-domain, the computation workflow is straightforward. The truncation error between the wavenumber-domain and spatial-domain forward can systematically decreases as the observation points increases. The elaborated forward approach replaces the layer-by-layer calculation process with efficient sparse matrix multiplication; compared with spatial-domain methods, computational efficiency is significantly improved. The advantage of this method lies in the consistency between its inherent finite-frequency characteristics and the degree limitation of spherical harmonic models in the wave-number domain. This forward framework is more theoretically compatible with the band-limited nature of finite-degree gravity data, thereby effectively avoiding the theoretical mismatch problem inherent in traditional spatial-domain methods between the full-spectrum model and band-limited data. Therefore, the wave-number domain forward method elaborated provides a computationally efficient, low-memory, and theoretically self-consistent technical solution for processing modelling satellite, aerial, and ground-based gravity and its gradient tensor data. Graphical Abstract

Earth Planets and SpaceVol. 78(1)
Openalex Percentile: Top 13%
Geophysics and Gravity Measurements
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