Full Vector Inversion of Magnetic Microscopy Images Using Euler Deconvolution as Prior Information

IF 2.9 2区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Gelson F. Souza-Junior, Leonardo Uieda, Ricardo I. F. Trindade, Janine Carmo, Roger Fu
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Abstract

Paleomagnetic data is collected from bulk samples, containing a mixture of stable and unstable magnetic particles. Recently, magnetic microscopy techniques have allowed the examination of individual magnetic grains. However, accurately determining the magnetic moments of these grains is difficult and time-consuming due to the inherent ambiguity of the data and the large number of grains in each image. Here we introduce a fast and semi-automated algorithm that estimates the position and magnetization of dipolar sources solely based on the magnetic microscopy data. The algorithm follows a three-step process: (a) employ image processing techniques to identify and isolate data windows for each magnetic source; (b) use Euler Deconvolution to estimate the position of each source; (c) solve a linear inverse problem to estimate the dipole moment of each source. To validate the algorithm, we conducted synthetic data tests, including varying particle concentrations and non-dipolarity. The tests show that our method is able to accurately recover the position and dipole moment of particles that are at least 15 μm apart for a source-sensor separation of 5 μm. For grain concentrations of 6,250 grains/mm3, our method is able to detect over 60% of the particles present in the data. We applied the method to real data of a speleothem sample, where it accurately retrieved the expected directions induced in the sample. The semi-automated nature of our algorithm, combined with its low processing cost and ability to determine the magnetic moments of numerous particles, represents a significant advancement in facilitating paleomagnetic applications of magnetic microscopy.

Abstract Image

利用欧拉解卷积作为先验信息对磁显微图像进行全矢量反演
古地磁数据是从含有稳定和不稳定磁性颗粒混合物的块状样本中收集的。最近,磁显微镜技术允许对单个磁性颗粒进行检查。然而,由于数据固有的模糊性和每幅图像中的大量磁粒,准确确定这些磁粒的磁矩既困难又耗时。在此,我们介绍一种半自动化的快速算法,该算法可完全根据磁显微镜数据估算偶极源的位置和磁化。该算法分为三个步骤:(a) 使用图像处理技术识别和分离每个磁源的数据窗口;(b) 使用欧拉解卷积估算每个磁源的位置;(c) 解决线性逆问题以估算每个磁源的偶极矩。为了验证算法,我们进行了合成数据测试,包括不同的粒子浓度和非偶极性。测试结果表明,我们的方法能够准确地恢复相距至少 15 μm 的粒子的位置和偶极矩,而源与传感器之间的距离为 5 μm。在颗粒浓度为 6,250 粒/立方毫米时,我们的方法能够检测到数据中超过 60% 的颗粒。我们将该方法应用于岩浆样本的真实数据中,它准确地检索出了样本中诱导的预期方向。我们的算法具有半自动化的特点,而且处理成本低,能够确定大量颗粒的磁矩,这在促进磁显微镜的古地磁应用方面是一个重大进步。
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来源期刊
Geochemistry Geophysics Geosystems
Geochemistry Geophysics Geosystems 地学-地球化学与地球物理
CiteScore
5.90
自引率
11.40%
发文量
252
审稿时长
1 months
期刊介绍: Geochemistry, Geophysics, Geosystems (G3) publishes research papers on Earth and planetary processes with a focus on understanding the Earth as a system. Observational, experimental, and theoretical investigations of the solid Earth, hydrosphere, atmosphere, biosphere, and solar system at all spatial and temporal scales are welcome. Articles should be of broad interest, and interdisciplinary approaches are encouraged. Areas of interest for this peer-reviewed journal include, but are not limited to: The physics and chemistry of the Earth, including its structure, composition, physical properties, dynamics, and evolution Principles and applications of geochemical proxies to studies of Earth history The physical properties, composition, and temporal evolution of the Earth''s major reservoirs and the coupling between them The dynamics of geochemical and biogeochemical cycles at all spatial and temporal scales Physical and cosmochemical constraints on the composition, origin, and evolution of the Earth and other terrestrial planets The chemistry and physics of solar system materials that are relevant to the formation, evolution, and current state of the Earth and the planets Advances in modeling, observation, and experimentation that are of widespread interest in the geosciences.
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