2019 Sensor Signal Processing for Defence Conference (SSPD) 2019
DOI: 10.1109/sspd.2019.8751663
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Support Estimation of a Sample Space-Time Covariance Matrix

Abstract: The ensemble-optimum support for a sample spacetime covariance matrix can be determined from the ground truth space-time covariance, and the variance of the estimator. In this paper we provide approximations that permit the estimation of the sample-optimum support from the estimate itself, given a suitable detection threshold. In simulations, we provide some insight into the (in)sensitivity and dependencies of this threshold.

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Cited by 9 publications
(18 citation statements)
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“…For these, algorithmic efforts have been reviewed, with the main focus currently directed to extracting analytic eigenvalues and -vectors that afford lower-order polynomial approximations than the state-of-the-art in PEVD approaches with proven convergence. Important future developments also target the estimation of space-time covariance [63,64,65], since the statistics typically have to be estimated from finite data sets, and interesting new applications where the polynomial approach permits solutions that were previously unobtainable, such as in the area of impulse response modelling [66] or speech enhancement [67].…”
Section: Discussionmentioning
confidence: 99%
“…For these, algorithmic efforts have been reviewed, with the main focus currently directed to extracting analytic eigenvalues and -vectors that afford lower-order polynomial approximations than the state-of-the-art in PEVD approaches with proven convergence. Important future developments also target the estimation of space-time covariance [63,64,65], since the statistics typically have to be estimated from finite data sets, and interesting new applications where the polynomial approach permits solutions that were previously unobtainable, such as in the area of impulse response modelling [66] or speech enhancement [67].…”
Section: Discussionmentioning
confidence: 99%
“…Assuming that the first few frames contain only the interferer components, the space-time covariance matrix in (2) can be estimated using [24], [25]. After computing the PEVD of (2), the orthogonal complement subspace U ⊥ (z) is generated according to (5).…”
Section: A Polynomial Subspace Projectionmentioning
confidence: 99%
“…We assume that a number of L sources have been stationary for a period of time, over which a space-time covariance matrixR[τ ] has been estimated, using e.g. the procedures outlined in [32], [33] for the estimation and the optimum support length of this estimate. Using an approximation of the PhEVD in (4) by algorithms of the second order sequential best rotation (SBR2) [14], [17] or sequential matrix diagonalisation (SMD) [18] families to factoriseR(z) • • R[τ ], we establish the broadband signal-plus-noise subspace spanned by the columns of U (z) and its complement, the noise-only subspace, spanned by the columns of U ⊥ (z), as defined in (8) with R = L.…”
Section: A Approachmentioning
confidence: 99%