Comparison of the Third- order moving average and least square methods for estimating of shape and depth residual magnetic anomalies

IF 1 Q4 GEOSCIENCES, MULTIDISCIPLINARY Iranian Journal of Earth Sciences Pub Date : 2021-07-01 DOI:10.30495/IJES.2021.682866
M. Fouladi, Mirsattar Meshinchi Asl, M. Mehramuz, N. Nezafati
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Abstract

In the current study, we have developed a new method called the third- order moving average method to estimate the shape and depth of residual magnetic anomalies. This method, calculates a nonlinear relationship between depth and shape factor, at seven points with successive window length. It is based on the computing standard deviation at depths that are determined from all residual magnetic anomalies for each value of the shape factor. The method was applied to the synthetic model by geometrical shapes both as horizontal cylinder and combination of horizontal cylinder, sphere and thin sheet approaches, with and without noise. It was tested by real data in Geological Survey of Iran (GSI). In this study, least square methods were applied to interpret the magnetic field so that we can compare the results of this methods with the third- order moving average method. This method is applied to estimate the depth using second horizontal derivative anomalies obtained numerically from magnetic data with successive window lengths. This method utilizes the variance of the depths as a scale for calculation of the shape and depth. The results showed that the third- order moving average method is a powerful tool for estimating shape and depth of the synthetic models in the presence and absence of noise compared to least square method. Moreover, the results showed that this method is very accurate for real data while the least square method did not lead to feasible results. In this study, least square methods were applied to interpret the magnetic field so that we can compare the results of this methods with the third- order moving average method. This method is applied to estimate the depth using second horizontal derivative anomalies obtained numerically from magnetic data with successive window lengths. This method utilizes the variance of the depths as a scale for calculation of the shape and depth.The results showed that the third- order moving average method is a powerful tool for estimating shape and depth of the synthetic models in the presence and absence of noise compared to least square method. Moreover, the results showed that this method is very accurate for real data while the least square method did not lead to feasible results.
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三阶移动平均法与最小二乘法在形状和深度残磁异常估计中的比较
在目前的研究中,我们提出了一种新的方法,称为三阶移动平均法来估计残余磁异常的形状和深度。该方法计算深度和形状因子之间的非线性关系,在连续窗口长度的七个点。它基于深度的计算标准偏差,该标准偏差由形状因子的每个值的所有剩余磁异常确定。将该方法应用于有噪声和无噪声的水平圆柱体和水平圆柱体、球体和薄片组合几何形状的综合模型。并用伊朗地质调查局(GSI)的实际数据进行了验证。本研究采用最小二乘法来解释磁场,并将其结果与三阶移动平均法进行比较。该方法应用于利用连续窗长的磁资料数值计算得到的第二次水平导数异常来估计深度。该方法利用深度方差作为计算形状和深度的尺度。结果表明,与最小二乘法相比,三阶移动平均法是估计有噪声和无噪声情况下合成模型形状和深度的有力工具。结果表明,该方法对实际数据的拟合精度较高,而最小二乘法的拟合结果不可行。本研究采用最小二乘法来解释磁场,并将其结果与三阶移动平均法进行比较。该方法应用于利用连续窗长的磁资料数值计算得到的第二次水平导数异常来估计深度。该方法利用深度方差作为计算形状和深度的尺度。结果表明,与最小二乘法相比,三阶移动平均法是估计有噪声和无噪声情况下合成模型形状和深度的有力工具。结果表明,该方法对实际数据的拟合精度较高,而最小二乘法的拟合结果不可行。
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来源期刊
Iranian Journal of Earth Sciences
Iranian Journal of Earth Sciences GEOSCIENCES, MULTIDISCIPLINARY-
CiteScore
1.40
自引率
12.50%
发文量
0
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