Abstract

This study explores improvements obtained in microseismic data processing through the application of inversion techniques that utilize sparse and non-linear constraints. Specifically, we present a method for de-noising microseismic traces and a method for the automatic time picking of microseismic events. The de-noising method is based on a sparsity constrained time-frequency transform which is obtained by finding a sparse representation of the input data in terms of a dictionary of complex Ricker wavelets. The utilization of a complex wavelet dictionary possesses the advantage that signals with arbitrary phase can be represented with enhanced sparsity. The automatic time picking method consists in the recovery of a blocky version of the short-termaveraging/ long-term-averaging (STA/LTA) curve through inversion using a non-linear constraint. Examples of the implementation of both methods are presented using synthetic and real microseismic data.

Introduction

In oil and gas wells, microseismicity induced during hydraulic injections is characterized for its small magnitude (Maxwell, 2005; Shemeta and Anderson, 2010). This important reason is why microseismic records often display a low signal-to-noise ratio (SNR). Accuracy and reliability of the location and other event attributes derived from microseismic traces are influenced by this strong noise content (Maxwell, 2009). The relatively recent growth of interest in microseismicity analysis in the petroleum industry opens an area of opportunity to apply the vast amount of signal processing knowledge previously developed in signal analysis and imaging processing. In this study, we give a step into this area of opportunity by implementing methods for de-noising and automatic time picking using inverse regularization approaches taken from other areas of geophysics and engineering. The de-noising method is based on a spectral decomposition technique originally developed for seismic data interpretation. Following the exposition by Bonar and Sacchi (2010), we seek a sparse representation of the microseismic signal in terms of a dictionary of complex Ricker wavelets. By imposing sparsity and misfit constraints to the decomposition process, we find a de-noised version of the original signal (Chen et al., 1998, Vera Rodriguez et al., 2011). The automatic time picking algorithm is based upon the recovery of the standard short-term-averaging/long-termaveraging (STA/LTA) (Allen, 1978) curve using an inversion with a constraint that results in a non-linear system of equations. In this case, the selection of the constraint is directed towards the recovery of blocky versions of the STA/LTA curve (Sabbione and Velis, 2010). Such a constraint has also been used to invert for the earth’s relative impedance profile (Walker and Ulrych, 1983) and medical imaging applications (Charbonnier et al., 1997).

De-noising method

The decomposition of a discrete seismic trace s[n] in terms of dilations and translations of a reference complex wavelet w[n] is given by (Bonar and Sacchi, 2010)

Formula 01

where the indexes i and k are related, respectively, to the translations and dilations of w[n], and the complex coefficients ak[i] control the amplitude and phase of the wavelets. In matrix-vector notation, equation (1) is written as the convolution of a set of complex coefficient vectors {ak} with a set of dilated versions of the reference wavelet {wk}, this is

Formula 02

where Wk is the convolution matrix of the wavelet with dilation index k. In order to generalize this model, the convolution matrices of a set of N dilated versions of the reference wavelet can be incorporated to create a redundant dictionary R (Mallat, 2008),

Formula 03

Equation (3) is an under-determined system that accepts an infinite number of solutions. In other words, there are multiple possible representations of s in terms of linear combinations of the columns of R. One alternative solution that presents advantages for de-noising purposes entails using an 1 regularization term. In other words, we will impose sparsity on the coefficients needed to represent the seismogram. This is accomplished by solving

Formula 04

The trade-off parameter λ balances the fidelity of fit versus the amount of sparsity in the solution vector. Sparse solutions in this study are estimated using the Fast Iterative Soft Thresholding Algorithm (FISTA) (Beck and Teboulle, 2009). Other methods that could also be used to solve (4) are Basis Pursuit (BP) (Chen et al., 1998) and Orthogonal Matching Pursuit (OMP) (Pati et al., 1993). The de-noised seismic trace can then be obtained from the sparse solution â via

Formula 05

Automatic time picking

An efficient algorithm for automatic time picking is the shortterm- averaging/long-term-averaging (STA/LTA) filter. Changing the previous notation such that s[n] = sn, the STA/LTA curve is defined by

Formula 06

Time picks are often determined through amplitude thresholding of the STA/LTA curve. Inaccurate time picks are commonly the result of the slow build up of the STA/LTA curve from the time of the wave arrival until the time where the curve surpasses the user defined threshold. An alternative method to reduce the inaccuracy of the time picks is through the recovery of blocky STA/LTA curves from inversion. This is obtained by the minimization of the cost function

Formula 07

where the vectors xSTA, xLTA and ySTA/LTA are the time series given by equations (6a), (6b) and (6c), respectively. The scalar α is a trade-off parameter, D is the first derivative matrix, and R(x) is a non-linear norm. One possibility for R(x) is

Formula 08

where δ is a stabilization factor. The solution to the minimization of (7) is obtained through iterative schemes such as Iterative Reweighted Least Squares (IRLS).

Examples

The application of the previously described methods is first demonstrated on a synthetic microseismic trace computed in a horizontally layered medium. Random noise is added to the synthetic trace using the relationship SNR = μsn, where μs is the expected signal value and σn the standard deviation of the noise. The SNR is set to a value of SNR = 3, and the resulting noisy data is de-noised using the sparse time-frequency transform (Figure 1). When compared against a low-pass filtered version of the noisy synthetic trace, the improvement of the sparse de-noising result is clear. Not only was more random noise eliminated, but also the frequency content of the arrivals of interest was preserved. Figure 2 presents the results of applying the standard and blocky STA/LTA filters to the previously described synthetic trace. The most straightforward method to set time picks in the STA/LTA curve is through amplitude thresholding. A visible difference in the maximum amplitude of the “boxes” that denote the arrivals of P and S waves in the STA/LTA curves is observed when the filters are applied over the noisy data. This means that if the thresholding level is set too high, the P arrivals could be missed. On the other hand, a thresholding level that is too low would produce multiple time picks that do not correspond to actual wave arrivals. Although the problem of false picks is partially alleviated using the blocky STA/LTA curve, improved results are obtained after de-noising the data. In the de-noised version of the data, the difference in the maximum amplitude between the P and S “boxes” is reduced. Furthermore, the blocky STA/LTA curve is cleaner than the standard STA/LTA curve before the first arrival.

Fig. 01
Figure 1. Synthetic microseismic trace de-noising example. (a) synthetic microseismic trace; (b) synthetic with random noise; (c) trace in (b) after low-pass filtering to about one third of its original frequency content; (d) de-noised trace using the sparse time-frequency transform; (e) time-frequency map for the trace in (d). The frequency axis in the time-frequency map denotes the central frequency of the corresponding complex Ricker wavelet in the dictionary. Red vertical lines indicate the approximate position of P and S arrivals in the original synthetic trace.
Fig. 02
Figure 2. From top to bottom: synthetic microseismic trace (s), synthetic with random noise (s + n), STA/LTA curve from noisy synthetic, blocky version of the STA/LTA curve from noisy synthetic, de-noised synthetic using the sparse timefrequency transform, STA/LTA curve for the de-noised trace, blocky version of the STA/LTA curve for the de-noised trace. Red vertical lines indicate the approximate position of P and S arrivals in the original synthetic trace.

The second data example corresponds to an actual microseismic record (Figure 3). In this trace a wave arrival is visible around 0.56 s with ambient noise affecting the entire record. The denoised result displays a visible improvement in SNR, while the pulse shape and time location of the arrival of interest is preserved. This suggests that the sparse transform has not substantially affected either the phase or frequency content of the arrival. The standard STA/LTA curves in both the raw and denoised traces display a slow build up at the position of the arrival which, as stated before, introduces error in the automatic time picking process whose amount depends on the threshold value selected by the user. The blocky behavior of the inverted STA/LTA curves helps to reduce this error.

Fig. 03
Figure 3. From top to bottom: real microseismic trace (raw), STA/LTA curve from raw trace, blocky version of the STA/LTA curve from raw trace, de-noised trace using the sparse time-frequency transform, STA/LTA curve for the de-noised trace, blocky version of the STA/LTA curve for the de-noised trace. The red vertical line denotes the approximate position of a wave arrival.

Conclusions

Processing of microseismicity records is a challenge due to, among other problems, the low signal-to-noise ratio displayed by the signals of interest. Application of techniques and processing tools developed in other knowledge areas can be of great advantage to deal with microseismicity records. For instance, in this work we applied inverse regularization techniques previously used for reflection seismology data processing and image processing. The results observed in synthetic and real data show the efficacy of the methods described to remove ambient noise without affecting the phase or frequency content of the signal of interest, and to improve the accuracy of automatic time picks.

End

Acknowledgements

This work was partially supported by the Signal Analysis and Imaging Group (SAIG) and Pinnacle/Halliburton. We also acknowledge Fairborne Energy Ltd. for providing the real data example.

About the Author(s)

Ismael Vera Rodriguez graduated from Universidad Nacional Autonoma de Mexico as a Geophysicist Engineer. After graduation he worked for four years in Schlumberger as Borehole Geophysicist. His work experience includes vertical seismic profile and microseismic processing. In 2008 Ismael started postgraduate studies at the University of Alberta where currently he is a PhD candidate. Since the summer of 2010, he is also working for Pinnacle/Halliburton as a student intern.

David Bonar received his B.Sc. in Geophysics with distinction from the University of Alberta in 2009 and is currently enrolled in the M.Sc. program in Geophysics. His current research interests include time-frequency analysis and de-noising and multiple attenuation strategies.

Mauricio D. Sacchi received a degree (Diploma) in geophysics from UNLP (Argentina) in 1983 and a PhD in Geophysics in 1993 from UBC. He has written some hard to read papers, one book and supervise students in the area of exploration Geophysics. He is now a full time professor at the UofA (Edmonton). He is also a member of SAIG (Signal Analysis and Imaging Group), a scientific consortium for seismic data processing, imaging and inversion.

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Appendices

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