4.2 Article

Re-parameterisations of the Cole-Cole model for improved spectral inversion of induced polarization data

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NEAR SURFACE GEOPHYSICS
卷 16, 期 4, 页码 385-399

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EUROPEAN ASSOC GEOSCIENTISTS & ENGINEERS
DOI: 10.3997/1873-0604.2017065

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The induced polarization phenomenon, both in time domain and frequency domain, is often parameterised using the empirical Cole-Cole model. To improve the resolution of model parameters and to decrease the parameter correlations in the inversion process of induced polarization data, we suggest here three re-parameterisations of the Cole-Cole model, namely the maximum phase angle Cole-Cole model, the maximum imaginary conductivity Cole-Cole model, and the minimum imaginary resistivity Cole-Cole model. The maximum phase angle Cole-Cole model uses the maximum phase phi(max) and the inverse of the phase peak frequency, tau(phi), instead of the intrinsic charge-ability m(0) and the time constant adopted in the classic Cole-Cole model. The maximum imaginary conductivity Cole-Cole model uses the maximum imaginary conductivity sigma max instead of m(0) and the time constant (sigma) of the Cole-Cole model in its conductivity form. The minimum imaginary resistivity Cole-Cole model uses the minimum imaginary resistivity sigma(max)'' min instead of m(0) and the time constant tau(sigma) of the Cole-Cole model in its resistivity form. The effects of the three re-parameterisations have been tested on synthetic time-domain and frequency-domain data using a Markov chain Monte Carlo inversion method, which allows for easy quantification of parameter uncertainty, and on field data using 2D gradient-based inversion. In comparison with the classic Cole-Cole model, it was found that for all the three re-parameterisations, the model parameters are less correlated with each other and, consequently, better resolved for both time-domain and frequency-domain data. The increase in model resolution is particularly significant for models that are poorly resolved using the classic Cole-Cole parameterisation, for instance, for low values of the frequency exponent or with low signal-to-noise ratio. In general, this leads to a significantly deeper depth of investigation for the phi '' max,sigma '' max, and rho '' min parameters, when compared with the classic m(0) parameter, which is shown with a field example. We believe that the use of re-parameterisations for inverting field data will contribute to narrow the gap between induced polarization theory, laboratory findings, and field applications.

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