2001
DOI: 10.1109/97.975873
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Blind phase recovery in cross QAM communication systems with eighth-order statistics

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Cited by 28 publications
(8 citation statements)
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“…Now, let us consider a magnitude weighed version of (4), namely (5) In (5) we have performed a tomographic projection of the magnitude weighed phase pdf ; we will refer to the function as the magnitude weighed tomographic projection (MWTP) of the magnitude/phase bidimensional pdf . From (5), we recognize that also the MWTP cyclically shifts of under a phase-offset , and that, in presence of additive noise, also the Dirac pulses in (5) become wider pulses whose shape depends on the SNR and the noise pdf; the analytical evaluation of (5) is reported in Appendix A.…”
Section: Discrete-time Signal Modelmentioning
confidence: 99%
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“…Now, let us consider a magnitude weighed version of (4), namely (5) In (5) we have performed a tomographic projection of the magnitude weighed phase pdf ; we will refer to the function as the magnitude weighed tomographic projection (MWTP) of the magnitude/phase bidimensional pdf . From (5), we recognize that also the MWTP cyclically shifts of under a phase-offset , and that, in presence of additive noise, also the Dirac pulses in (5) become wider pulses whose shape depends on the SNR and the noise pdf; the analytical evaluation of (5) is reported in Appendix A.…”
Section: Discrete-time Signal Modelmentioning
confidence: 99%
“…For comparison purposes, also results pertaining to other selected estimators are reported, namely the nonlinear least square (WA03) estimator [11], the concentration ellipse orientation (CEO) estimator [12], and the fourth-order (CW99) estimator [1] for square constellations or the eighth-order (CW01) estimator [5] for cross constellations. In particular, the WA03 estimator is obtained by evaluating the angular coordinate of the sample average of a suitable nonlinear transformation of the received signal samples; it is constellation dependent, and it requires knowledge of both SNR and gain.…”
Section: Numerical Experiments and Performance Comparisonmentioning
confidence: 99%
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“…These systems can be grouped into two areas -those that require established gain control and those that do not. The Fourth Power Phase Estimator [1]- [3], which is a special case of the Viterbi and Viterbi (V&V) monomial-based estimators [4], the Eighth-Order Estimator (EOE) [5], the Concentration Ellipse Orientation (CEO) [6], and more recently the iterative methods (DCA-a and DCA-b) of Alvarez-Diaz and Lopez-Valcarce [7] are systems in the latter category. Among the former category are the Reduced-Constellation Fourth Power Estimator [1], the two methods of Georghiades [1] which require finding the mode of the probability density of the phase, the rather complex Minimum Distance Estimator (MDE) [8], the TwoStage Conjugate (2SC) algorithm which according to Rice et al.…”
Section: Introductionmentioning
confidence: 99%
“…The performance of the fourth-power method applied to square QAM constellations is considered acceptable. Alternatives have been devised to improve phase detection for such constellations: the Eighth-Order Estimator (EOE) [3], the Concentration Ellipse Orientation (CEO) [4], and more recently the iterative methods (DCA-a and DCA-b) of Alvarez-Diaz and Lopez-Valcarce [5], Reduced-Constellation Fourth Power Estimator [2], the Two-Stage Conjugate (2SC) algorithm [6], the optimal method, proposed by Wang and Serpedin [7]. Those methods are so complicated for hardware implementation, their increased computational expense prevent their practical adoption even in experiments.…”
Section: Introductionmentioning
confidence: 99%