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Paper: A new method for location sources of gravity and magnetic data using Euler's homogeneity equation

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compgeolab/euler-inversion

Euler inversion: Locating sources of potential-field data through inversion of Euler’s homogeneity equation

by Leonardo Uieda, Gelson Ferreira Souza-Junior, India Uppal, Vanderlei Coelho Oliveira Jr.

This repository contains the data and source code used to produce the results presented in:

Uieda, L., Souza-Junior, G. F., Uppal, I., Oliveira Jr., V. C. (2024). Euler inversion: Locating sources of potential-field data through inversion of Euler’s homogeneity equation. EarthArXiv. doi:10.31223/X5T41M.

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Version of record TBD (submitted to Geophysical Journal International)
Open-access version on EarthArXiv https://doi.org/10.31223/X5T41M
Archive of this repository https://doi.org/10.6084/m9.figshare.26384140
Reproducing our results REPRODUCING.md

About

The main idea for this paper came about during an potential-field methods class which Leo took in 2012 with his then PhD supervisor Prof. Valéria C. F. Barbosa. While learning about the Euler deconvolution method, which is a speciality of Valéria, Leo connected it with the geodetic network adjustment theory he had been taught by Prof. Spiros Pagiatakis during an exchange program at York University, Canada, in 2008. An initial prototype was developed in 2012 but there were still some rough edges and the project was shelved to make way for other more urgent projects at the time. Leo returned to this every few years, making slow progress, and involving Vanderlei in the planning and discussion of the theory. In 2024, co-authors Gelson, India, and Vanderlei joined Leo for a sprint to finish the method and produce this paper.

Abstract

Earth scientists can estimate the depth of certain rocks beneath Earth's surface by measuring the small disturbances that they cause in the Earth's gravity and magnetic fields. A popular method for this is Euler deconvolution, which is widely available in geoscience software and can be run quickly on a standard computer. Unfortunately, Euler deconvolution has some shortcomings: 1) the approximate shape of the rocks must be known, for example, a sphere or a wide flat slab, represented by the structural index 2) the depth of the rocks is not well estimated when there is noise in our data, which is a common occurrence. We propose a new method, Euler inversion, which fixes some of the shortcomings of Euler deconvolution by using more adequate (and complex) mathematics. Our method is less sensitive to noise in the data and is also able to determine the approximate shape of the source (the structural index). Euler inversion is also fast to execute on a standard computer, making it a practical alternative to Euler deconvolution on an Earth scientists toolbox.

Figure: Results of applying Euler inversion with a window size of 12 000 m and a window step of 2400 m to the aeromagnetic data from Rio de Janeiro, Brazil. Estimated source locations and structural indices obtained from Euler inversion are shown as triangles (𝜂 = 1), squares (𝜂 = 2), and circles (𝜂 = 3). The colour of each symbol represents the estimated depth below the surface of the Earth (topography). Also shown are the total-field anomaly flight-line data, the contours of the post-collisional magmatism and alkaline intrusions (solid black lines) and dykes (dashed lines). The purple squares highlight the A, B, C, and D anomalies that are discussed in the text.

License

All Python source code (including .py and .ipynb files) is made available under the MIT license. You can freely use and modify the code, without warranty, so long as you provide attribution to the authors. See LICENSE-MIT.txt for the full license text.

The manuscript text (including all LaTeX files), figures, and data/models produced as part of this research are available under the Creative Commons Attribution 4.0 License (CC-BY). See LICENSE-CC-BY.txt for the full license text.