2017
DOI: 10.1007/s00024-017-1654-3
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3D Magnetization Vector Inversion of Magnetic Data: Improving and Comparing Methods

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Cited by 51 publications
(25 citation statements)
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“…These include 2-D approaches assuming a constant magnetization of a layer and solving for the thickness of the layer (Parker, 1972) or assuming a constant layer thickness and solving for magnetization (Parker & Huestis, 1974). Three-dimensional approaches include solving for the full 3-D distribution of magnetization (either susceptibility or magnetization; Li & Oldenburg, 1996;Lelièvre & Oldenburg, 2009;Liu et al, 2017). Volcanic geology is very three-dimensional, and realistic slope stability models require detailed 3-D information on altered rock volumes (Ball et al, 2018); hence, 3-D inversion of magnetic data is required to achieve this.…”
Section: Magnetic Modelingmentioning
confidence: 99%
See 1 more Smart Citation
“…These include 2-D approaches assuming a constant magnetization of a layer and solving for the thickness of the layer (Parker, 1972) or assuming a constant layer thickness and solving for magnetization (Parker & Huestis, 1974). Three-dimensional approaches include solving for the full 3-D distribution of magnetization (either susceptibility or magnetization; Li & Oldenburg, 1996;Lelièvre & Oldenburg, 2009;Liu et al, 2017). Volcanic geology is very three-dimensional, and realistic slope stability models require detailed 3-D information on altered rock volumes (Ball et al, 2018); hence, 3-D inversion of magnetic data is required to achieve this.…”
Section: Magnetic Modelingmentioning
confidence: 99%
“…To address possible issues with remanence, we use a three-dimensional MVI implemented in the open source package SimPEG (Cockett et al, 2015), to invert our TMI data. Our MVI algorithm (see Fournier, 2019;Fournier & Oldenburg, 2019, for full details) simultaneously solves for both the direction and amplitude of magnetization building on the approaches described by Lelièvre and Oldenburg (2009) and Liu et al (2017). In the inversion the magnetization amplitude, a, is recast as an apparent susceptibility parameter, ⃗, by dividing the magnetization components by the amplitude of the Earth's field H o .…”
Section: Magnetic Modelingmentioning
confidence: 99%
“…These techniques face great challenges when magnetic data are collected at low magnetic latitudes because RTP and component conversion in wavenumber domain are known to be unstable near the magnetic equator (Blakely, 1996; Pedersen, 1978). Researchers have also developed inversion‐based methods (Coleman, 2014; Ellis et al, 2012; Foss & McKenzie, 2011; Fournier, 2015; Fournier et al, 2020; Fullagar & Pears, 2015; Lelièvre & Oldenburg, 2009; Li & Sun, 2016; S. Liu et al, 2017; Pratt et al, 2012; Sun & Li, 2018, 2019) to estimate the magnetization directions. These methods all have their pros and cons and typically involve 3‐D inversions that are either procedurally or computationally complex.…”
Section: Introductionmentioning
confidence: 99%
“…In this paper, we extend the sequential inversion method from 2D to 3D and propose a fast iteration method (M-IDI) to estimate the magnetization direction and to implement the magnetization vector inversion (Liu et al, 2017). We compare it with previous important methods: the magnetization vector inversion in Cartesian framework (MMM) and spherical framework (MID) proposed �� Lelièvre and �lden�urg (2009).…”
Section: Introductionmentioning
confidence: 99%
“…Synthetic example. �o test and compare the methods, we set a s�nthetic model that is consisted of one vertical cu�oid (i.e., A) and two dipping prisms (i.e., B and C) (Liu et al, 2017). �he inclination and declination of Earth's magnetic field are I 0 = 45° (horizontal to downward) and D 0 = 90° (east to north).…”
Section: Introductionmentioning
confidence: 99%