<p>As a convenient and efficient passive-source geophysical method, microtremor exploration is widely used. The traditional Extended Spatial Autocorrelation (ESPAC) method tends to generate high-frequency cross-artifacts with sparse arrays. Although the Modified ESPAC (M-ESPAC) method can eliminate these artifacts, its inversion depth (less than twice the array radius) is much lower than ESPAC’s 3–5 times. To resolve this contradiction, this paper proposes a Further Modified ESPAC (FM-ESPAC) method based on cross-correlation spectrum adaptive segmental fitting. First, it defines the first intersection frequency <i>f</i><sub>01</sub> between the cross-correlation curve and the frequency axis as the adaptive segmentation threshold. Then, adaptive segmental fitting is performed using <i>f</i><sub>01</sub>: the low-frequency band (<i>f</i> ≤ <i>f</i><sub>01</sub>) adopts ESPAC’s zero-order Bessel function J<sub>0</sub> fitting to retain low-frequency responses, while the high-frequency band (<i>f</i> &gt; <i>f</i><sub>01</sub>) uses M-ESPAC’s analytic signal and first-kind zero-order Hankel function H<sub>0</sub><sup>(1)</sup> fitting to eliminate cross-artifacts. Finally, the array-averaged dispersion spectrum is obtained via superposition and normalization. Simulation experiments (triangular/linear arrays) and practical cases (Enshi geothermal exploration, Antarctic ice sheet detection) verify that FM-ESPAC not only eliminates high-frequency cross-artifacts but also inherits ESPAC’s low-frequency information to ensure inversion depth, showing significant advantages in the case of sparse arrays and insufficient spatial sampling.</p>

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Improvement and application of ESPAC method based on cross-correlation spectrum adaptive segmental fitting technology

  • Mingming Wu,
  • Lianghong Zhang,
  • Hesheng Zeng,
  • Zhixian Gui,
  • Guixi Liu

摘要

As a convenient and efficient passive-source geophysical method, microtremor exploration is widely used. The traditional Extended Spatial Autocorrelation (ESPAC) method tends to generate high-frequency cross-artifacts with sparse arrays. Although the Modified ESPAC (M-ESPAC) method can eliminate these artifacts, its inversion depth (less than twice the array radius) is much lower than ESPAC’s 3–5 times. To resolve this contradiction, this paper proposes a Further Modified ESPAC (FM-ESPAC) method based on cross-correlation spectrum adaptive segmental fitting. First, it defines the first intersection frequency f01 between the cross-correlation curve and the frequency axis as the adaptive segmentation threshold. Then, adaptive segmental fitting is performed using f01: the low-frequency band (f ≤ f01) adopts ESPAC’s zero-order Bessel function J0 fitting to retain low-frequency responses, while the high-frequency band (f > f01) uses M-ESPAC’s analytic signal and first-kind zero-order Hankel function H0(1) fitting to eliminate cross-artifacts. Finally, the array-averaged dispersion spectrum is obtained via superposition and normalization. Simulation experiments (triangular/linear arrays) and practical cases (Enshi geothermal exploration, Antarctic ice sheet detection) verify that FM-ESPAC not only eliminates high-frequency cross-artifacts but also inherits ESPAC’s low-frequency information to ensure inversion depth, showing significant advantages in the case of sparse arrays and insufficient spatial sampling.