Abstract
In the paper (Kushnir et al., Int J Geomath 4(2):201–225, 2013) we offered the mathematically rigorous justification of the adaptive algorithm for statistical estimation of parameters of micro-earthquake source based on data recorded by a surface array of seismic receivers. The algorithm exploits the popular statistical Maximum Likelihood approach for determination of unknown parameters of probability distribution of a multichannel data generated by micro-earthquake source and registered by the surface array in the presence of strong noise. In this paper we consider unique properties of the mentioned adaptive maximum-likelihood estimator (AMLE) in conditions when the noise affecting the surface array receivers contains strong time-spatially correlated (coherent) component of man-made origin. These conditions are typical when AMLE algorithm is implemented for location of the micro-earthquakes caused by the medium hydraulic fracturing at hydrocarbon deposit sites. In the mentioned conditions AMLE algorithm demonstrates capability to suppress coherent noise component and hence to significantly improve the accuracy of determination of the coordinates of micro-earthquake sources. In the paper we theoretically investigate the signal-to-noise ratio (SNR) of AMLE statistic and show that this SNR tends to infinity while seismic noise becomes purely coherent. We have undertaken also the computer simulation of the micro-earthquake location with the help of AMLE algorithm using deployment of the 150 seismic receivers which corresponds geometry of a real USA surface seismic array. For this array we computed the model multidimensional realizations of the micro-earthquake signal, the coherent man-made noise component and the natural noise component. The results of this computer simulation have shown that in conditions when the power of the coherent man-made component of the modeled noise significantly exceeds the power of the natural component of this noise the errors of micro-earthquake source position determination become negligible.
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Appendices
Appendix 1
Let us consider a m-dimensional random stationary regular time series \(\varvec{v}_t =\left( {v_{1,t} ,\ldots ,v_{m,t} } \right) ^{T}, t\in {\mathbb {Z}}\) and its truncation \(\varvec{v}_{t,N} \) at the discrete time interval \(t\in \overline{1,N} \): \(\varvec{v}_{t,N} =\varvec{v}_t , t\in \overline{1,N} ; \varvec{v}_{t,N} \equiv 0, t\notin \overline{1,N} \). The Finite Discrete Fourier Transform (DFFT) of the time sequence \(\varvec{v}_{t,N} \) exists for any length N of the discrete time interval \(t\in \overline{1,N} \) and has the form
Designate as \(\varvec{F}_N \left( {\lambda _j } \right) =E\left\{ {\varvec{u}_N \left( {\lambda _j } \right) \varvec{u}_N^*\left( {\lambda _j } \right) } \right\} \) the mean square matrix of the random complex vectors \(\varvec{u}_N \left( {\lambda _j } \right) \).
The our goal is to derive conditions for which the matrix function \(\varvec{F}_N \left( {\lambda _j } \right) =\left[ {F_{N, k,l} \left( {\lambda _j } \right) ; k,l\in \overline{1,m} } \right] \) converge to the matrix power spectral density
of the time series \(\varvec{v}_t , t\in {\mathbb {Z}}\), (where \(\varvec{R}\left( \tau \right) =E\left\{ {\varvec{v}_t \varvec{v}_{t+\tau }^*} \right\} , t,\tau \in {\mathbb {Z}}\) is the matrix autocovariance function of the time series \(\varvec{v}_t , t\in {\mathbb {Z}})\) and this conversion have the rate \(\mathbf{O}\left( {N^{-\varepsilon }} \right) \) where \(\varepsilon \ge 1\).
The matrix function \(\varvec{F}_N \left( {\lambda _j } \right) \) can be written in the form
Let us assign \(\tau =t-r\in \overline{-N+1,N-1} \). Because the time series \(\varvec{v}_t , t\in {\mathbb {Z}}\) is stationary we have:
Using Eq. (6.3) we can write Eq. (6.2) in the form:
The double sum at the right side of Eq. (6.4) means summation of the square \(m\times m\) blocks \(\varvec{B}_{t,r} =\varvec{R}\left( {t-r} \right) exp \left\{ {-i\lambda _j \left( {t-r} \right) } \right\} \) of the matrix \(\varvec{Q}_N =\left[ {\varvec{B}_{t,r} ; t,r\in \overline{1,N} }\, \right] \) over its columns (\(t\in \overline{1,N} )\) and rows (\(r\in \overline{1,N} )\). But the value of this double sum can be calculated by consequent summation of the blocks \(\varvec{B}_{t,r} \) located on each block diagonal of the matrix \(\varvec{Q}_N \). This is convenient because at each block diagonal of the matrix \(\varvec{Q}_N \) the blocks \(\varvec{B}_{t,r} =\varvec{R}\left( {t-r} \right) \) are identical. The blocks \(\varvec{B}_{t,r} \) vary only from one diagonal to another due to changing the value \(\tau =t-r\) in the interval \(\left[ {-N+1, N-1} \right] \) .
For summation of the matrix \(\varvec{Q}_N \) elements though its block diagonals we change the summing variables in the double sum of Eq. (6.4). We will use the following variables: \(\tau \in \overline{-N+1,N-1} \) which numerates the block diagonals of the matrix \(\varvec{Q}_N \) and \(k\in \overline{1,N-\left| \tau \right| } \) which numerates the blocks at the diagonal with number \(\tau \). Thus we get the next convenient equation for calculation of the function \(\varvec{F}_N \left( {\lambda _j } \right) \):
Theorem 1
Let the elements \(R_{k,l} \left( \tau \right) \) of matrix autocovariance function
of a regular stationary time series \(\varvec{v}_t =\left( {v_{1,t} ,\ldots ,v_{m,t} } \right) ^{T} , t\in {\mathbb {Z}}\) satisfy the requirement
Than:
-
(1)
The elements
$$\begin{aligned} F_{k,l} \left( \lambda \right) =\sum _{\tau =-\infty }^\infty {R_{k,l} \left( \tau \right) } exp \left\{ {-i\lambda \tau } \right\} , k,l\in \overline{1,m} , \lambda \in \left( {0,2\pi } \right) \end{aligned}$$of the matrix power spectral density function \(\varvec{F}\left( \lambda \right) =\left[ {F_{k,l} \left( \lambda \right) , k,l\in \overline{1,m} } \right] \) for the time series \(\varvec{v}_t =\left( {v_{1,t} ,\ldots ,v_{m,t} } \right) ^{T}\) exist and have a derivative uniformly bounded in respect to \(\lambda \in \left( {0,2\pi } \right) \) :
$$\begin{aligned} \mathop {sup }\limits _{\lambda \in \left( {0,2\pi } \right) } \left| {\frac{\partial F_{k,l} \left( \lambda \right) }{\partial \lambda }} \right| <\infty \end{aligned}$$(6.7) -
(2)
For any sequence \(j_N \) such that \(\mathop {lim }_{N\rightarrow \infty } \lambda _{j_N } =\frac{2\pi j_N }{N}=\lambda \in \left( {0,2\pi } \right) \) the functions \(F_{N,k,l} \left( {\lambda _{j_N } } \right) , \lambda \in \left( {0,2\pi } \right) \) have the asymptotic representation:
where: the matrix \(\varvec{F}_N \left( {\lambda _j } \right) =\left[ {F_{N,k,l} \left( {\lambda _j } \right) , k,l\in \overline{1,m} } \right] \) is determined by Eq. (6.5); \(\mathop {\overline{lim } }_{N\rightarrow \infty } NO_{k,l,j_N } \left( {N^{-1}} \right) =c_\lambda ; NO_{k,l,j_N } \left( {N^{-1}} \right)<O\left( {N^{-1}} \right) ; \mathop {\overline{lim } }_{N\rightarrow \infty } N O\left( {N^{-1}} \right) =c<\infty ; c_\lambda , c\) are some constants.
Proof
-
(1)
Under requirement (6.6) the infinite functional series
(6.9)converge uniformly with respect \(\lambda \in \left( {0,2\pi } \right) \) according to Weierstrass theorem (Rudin 1991).
-
(2)
Accordingly with Eq. (6.5) we have to prove that the left side of Eq. (6.6):
$$\begin{aligned} F_{N,k,l} \left( {\lambda _{j_N } } \right) -F_{k,l} \left( \lambda \right)= & {} -\left( \sum _{\tau =-\infty }^\infty {R_{k,l} } \left( \tau \right) exp \left\{ {-i\lambda \tau } \right\} \right. \nonumber \\&\left. -\sum _{\tau =-N}^N {R_{k,l} } \left( \tau \right) exp \left\{ {-i\lambda _{j_N } \tau } \right\} \right) \nonumber \\&+\frac{1}{N}\sum _{\tau =-N+1}^{N-1} {\left| \tau \right| R_{k,l} } \left( \tau \right) exp \left\{ {-i\lambda _{j_N } \tau } \right\} \nonumber \\= & {} O_{k,l,j_N } \left( {N^{-1}} \right) \end{aligned}$$(6.10)The condition (6.6) of the Theorem T1 implies that
$$\begin{aligned} \left| {\frac{1}{N}\sum _{\tau =-N+1}^{N-1} {\left| \tau \right| R_{k,l} } \left( \tau \right) exp \left\{ {-i\lambda _{j_N } \tau } \right\} } \right|\le & {} \frac{1}{N}\sum _{\tau =-N+1}^{N-1} {\left| \tau \right| } \left| {R_{k,l} \left( \tau \right) } \right| \nonumber \\= & {} O_{k,l} \left( {N^{-1}} \right) \end{aligned}$$(6.11)It follows also from Eq. (6.6) that
$$\begin{aligned}&\left| {\sum _{\tau =-\infty }^\infty {R_{k,l} } \left( \tau \right) exp \left\{ {-i\lambda \tau } \right\} -\sum _{\tau =-N}^N {R_{k,l} } \left( \tau \right) exp \left\{ {-i\lambda _{j_N } \tau } \right\} } \right| \nonumber \\&\quad \le \sum _{\left| \tau \right| =N}^\infty {\left| {R_{k.l} \left( \tau \right) } \right| } \rightarrow 0\; \hbox {while}\; N\rightarrow \infty . \end{aligned}$$(6.12)Let us calculate the rate of convergence to zero of the left side of Eq. (6.12).
The conversion of the series \(\mathop {\sum }_{\tau =-\infty }^\infty {\left| {R_{k.l} \left( \tau \right) } \right| } \) that follows from condition (6.6) implies that the following restriction on the “tails” of the functions \(R_{k.l} \left( \tau \right) \) is valid: there exist such a number \(L\in {\mathbb {Z}}^{+}\) for which the next inequalities are valid for \(\left| \tau \right| >L\):
where \(\varepsilon >1\).
By the restriction (6.13) the following inequality is valid for any \(N>L\)
By applying the Maclauren–Cauchy theorem (Knopp 1956) we get the for any \(N>L\):
Hence,
where \(\varepsilon >1\).
The statement (2) of the Theorem T1 follows immediately from equations (6.11), (6.12) and (6.16). \(\square \)
Appendix 2
Proof of Lemma 1.
Statement 1
Let \(\varvec{F}_0 \) is a nonsingular \(m\times m\) matrix, \(\varvec{U}_s \) is a \(m\times s\) matrix, and the \(m\times m\) matrix \(\varvec{F}\) is equal to \(\varvec{F}=\left[ {\varvec{\sigma } ^{2}\varvec{F}_0 +\varvec{U}_s \varvec{U}_s^*} \right] \). Then the following representation of the inverse matrix \(\varvec{F}^{-1}\) is valid:
Proof
Below the direct verification of the statement 1 is given, that it is shown that:
The matrix \(\varvec{X}\) can be transformed as following:
Introducing the notation: \(G_s =\varvec{F}_0^{-1/2} \varvec{U}_s \) we can rewrite \(\varvec{X}\) to more simple form:
Making multiplication of two expressions in the square brackets we get:
Making elementary algebraic transformations we get
The statement 1 is proven.\(\square \)
Statement 2
Representation (7.1) of the inverse matrix \(\varvec{F}^{-1}\) admits the following expansion in powers of the \(\sigma ^{2}\):
were:
\(\varvec{U}_s =\varvec{Q}_s \varvec{T}_s \), \(\varvec{T}_s \) is the \(s\times s\) diagonal matrix, \(\varvec{Q}_s \) is the \(s\times m\) matrix.
Proof
The next transformation of the expression (A.2.1) is trivial:
Substitution in Eq. (7.1) the following decomposition of the inverse matrix \(\left( \sigma ^{2}\varvec{I}_s +\varvec{U}_s^{*} \varvec{F}_0^{-1} \varvec{U}_s \right) ^{-1}\)(see Eq. (3.11)):
gives us the following equation
where
The statement 2 is proven.\(\square \)
Statement 3
If \(\varvec{U}_s \) is a \(m\times s\) matrix and \(\varvec{F}_0 \) is nonsingular \(m\times m\) matrix then the following asymptotic decomposition is valid for \(\sigma ^{2}\rightarrow 0\):
Proof
To simplify the calculations denote \(s\times s\) matrix \(\varvec{U}_s^{*} \varvec{F}_0^{-1} \varvec{U}_s =\varvec{A}\) and \(\sigma ^{2}=\varepsilon \). Then Eq. (7.3) can be rewritten in the form:
Let us apply the Taylor expansion of the matrix function \(\varvec{C}^{-1}\left( \varepsilon \right) \) in Eq. (7.4):
Using the well known formula for differentiation of the inverse matrix function depending on a numeric parameter we get:
The Eqs. (7.4)–(7.6) (in view of the notation for the matrix \(\varvec{A})\) imply that the Eq. (7.3) to be proved. \(\square \)
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Kushnir, A., Varypaev, A. Accuracy of adaptive maximum likelihood algorithm for determination of micro earthquake source coordinates using surface array data in condition of strong coherent noise. Int J Geomath 7, 203–237 (2016). https://doi.org/10.1007/s13137-016-0082-3
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DOI: https://doi.org/10.1007/s13137-016-0082-3
Keywords
- Multichannel signal processing
- Hydraulic fracturing
- Micro seismic source
- Adaptive maximum likelihood estimator
- Coherent noise suppression