融入非平稳随机场正则化的可控源音频大地电磁法约束反演方法

A method integrating a non-stationary random field for constrained inversion of CSAMT data

  • 摘要:
    目的 可控源音频大地电磁法反演的计算效率和分辨率问题始终是该领域的关键议题。为解决可控源音频大地电磁法反演中计算效率和分辨率不足的问题,特别是传统正则化方法对复杂地质结构估计的过度平滑现象,提出了一种改进的正则化反演方法,旨在更真实地反映地下物性参数的空间分布特性。
    方法 采用基于Matérn函数随机偏微分方程的构建法,通过引入矢量场及变程“椭圆”的形状参数,充分考虑地层的倾斜变化和物性分布的非平稳性,构建出满足非平稳假设的模型协方差矩阵,并以此作为正则化约束条件进行反演。通过从反演结果、残差值、视电阻率相对残差及不确定度这4个维度,对比分析了传统最平滑约束方法、基于平稳假设的协方差约束方法以及非平稳协方差约束方法的效果。此外,为验证方法的实际应用效果,将其应用于新疆哈巴河县也尔克曼−金坝金矿勘探的实测数据处理中。
    结果 理论模型结果表明,非平稳假设约束下4组试验的残差值介于20.47%~21.29%,优于平稳假设约束(残差值分别为21.25%及22.83%),优于传统最平滑约束方法(残差值为32.46%),且能更真实地反映地质构造特征,以及更清晰地识别地质边界。实测数据结果表明,非平稳假设约束方法在成像效果方面明显优于传统Occam平滑约束方法,数据拟合残差提升达51.47%,显著增强对复杂地质结构的分辨能力,并在一定程度上降低深部区域反演的不确定性,从而有效提升了整体反演结果的可靠性。
    结论 基于非平稳假设的Matérn函数正则化反演方法为解决可控源音频大地电磁法反演中的计算效率和分辨率问题提供了一种新的技术手段,对推动地球物理反演技术的发展具有重要意义。

     

    Abstract:
    Objective The inversion of controlled-source audio-frequency magnetotelluric (CSAMT) data remains challenging due to two key issues: computational efficiency and resolution. To tackle these two issues, especially the over-smoothing effect caused by traditional regularization methods in estimating complex geological structures, this study proposed an improved regularization inversion method to reflect the spatial distribution characteristics of subsurface physical property parameters more accurately.
    Methods The proposed method was developed using the method for establishing the stochastic partial differential equation (SPDE) based on the Matérn covariance function. By introducing vector fields and the shape parameters of a range ellipse, this method fully considered both variations in the inclination of strata and the non-stationary nature of physical property distribution. Accordingly, this study developed a model covariance matrix meeting the non-stationary assumption. Then, inversion was conducted using the model covariance matrix as the regularization constraint. From the perspective of inversion results, residuals, relative residuals of apparent resistivity, and uncertainty, this study compared the proposed method with traditional maximum smoothness-constrained inversion and covariance-constrained inversion based on the stationary assumption. In addition, the proposed method was applied to measured data from the exploration of the Ye’erkeman-Jinba gold deposit in Habahe County, Xinjiang to validate its practical application effects.
    Results The results from the theoretical model indicate that the four experiments with the non-stationary constraint yielded residuals ranging from 20.47% to 21.29%, which were lower than those of experiments with the stationary constraint (21.25% and 22.83%) and those of experiments using traditional maximum smoothness-constrained inversion (32.46%). Furthermore, the proposed method could characterize geological structures more accurately and delineate geological boundaries more distinctly. The results from measured data show that the covariance-constrained CSAMT inversion based on the non-stationary assumption delivered significantly higher imaging performance than the conventional Occam-type (smoothness constrained) inversion, achieving a 51.47% reduction in data fitting residuals. The proposed method exhibited a remarkably enhanced capacity to identify complex geological structures and reduced the uncertainty in the inversion results of deep areas, thereby effectively improving the overall reliability of inversion results.
    Conclusions The non-stationary assumption-based inversion method with the Matérn covariance function as the regularization constraint provides a novel technical solution for addressing the issues of the insufficient computational efficiency and resolution of CSAMT inversion. This method holds great significance for advancing geophysical inversion technology.

     

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