2017 IEEE International Symposium on Dynamic Spectrum Access Networks (DySPAN) 2017
DOI: 10.1109/dyspan.2017.7920748
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USRP N210 demonstration of wideband sensing and blind hierarchical modulation classification

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Cited by 14 publications
(5 citation statements)
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“…In [21][22][23] several spectrum sensing algorithms, including those based on cyclostationary features, have been implemented and tested using GNU Radio/USRP. In [24] cyclostationary features are used to perform hierarchical modulation clas-sification, and the resulting algorithms are implemented in C++ and tested using GNU Radio/USRP. Recently, in [25] cyclostationary feature detectors for spectrum sensing are implemented in the GNU Radio/USRP environment, which are characterized by a reduced design complexity in comparison to other solutions in the literature.…”
Section: Introductionmentioning
confidence: 99%
“…In [21][22][23] several spectrum sensing algorithms, including those based on cyclostationary features, have been implemented and tested using GNU Radio/USRP. In [24] cyclostationary features are used to perform hierarchical modulation clas-sification, and the resulting algorithms are implemented in C++ and tested using GNU Radio/USRP. Recently, in [25] cyclostationary feature detectors for spectrum sensing are implemented in the GNU Radio/USRP environment, which are characterized by a reduced design complexity in comparison to other solutions in the literature.…”
Section: Introductionmentioning
confidence: 99%
“…Besides, the performances of classification of higher-order modulation schemes are mostly unsatisfactory at low signal-to-noise ratio (SNR) values [46,47]. A few hierarchical classifiers have been reported [48,49] however they seem to be impractical as they utilize many stages and classifiers which makes them highly complex. Considering the trade-off of the low complexity and high success, these types of structures generally remain insufficient despite their high accuracy.…”
Section: Introductionmentioning
confidence: 99%
“…The constellation identification of QAM over frequencyselective fading channels is essential in signal processing [6]. For the QAM constellation identification, [7] employed high-order cumulants and signal cyclostationarity to identify 4/16/64QAM. Reference [8] adopted the Wigner-Ville distribution (WVD) time-frequency to transform the incoming signal, calculate the signal's Renyi entropy, and then leverage the Dempster-Shafer theory to identify the QAM.…”
Section: Introductionmentioning
confidence: 99%