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Article: Automatic Recognition of Space-Time Constellations by Learning on the Grassmann Manifold

TitleAutomatic Recognition of Space-Time Constellations by Learning on the Grassmann Manifold
Authors
KeywordsModulation
Manifolds
Signal processing algorithms
Clustering algorithms
MIMO communication
Issue Date2018
PublisherIEEE. The Journal's web site is located at http://ieeexplore.ieee.org/xpl/RecentIssue.jsp?punumber=78
Citation
IEEE Transactions on Signal Processing, 2018, v. 66 n. 22, p. 6031-6046 How to Cite?
AbstractRecent breakthroughs in machine learning shift the paradigm of wireless communication towards intelligence radios. One of their core operations is automatic modulation recognition (AMR). Existing research focuses on coherent modulation schemes such as QAM and FSK. The AMR of (noncoherent) space-time modulation remains an uncharted area despite its deployment in modern multiple-input-multiple-output (MIMO) systems. The scheme using a so-called Grassmann constellation enables rate enhancement. In this paper, we propose an AMR approach for Grassmann constellation based on data clustering, which differs from traditional AMR based on classification using a modulation database. The approach allows algorithms for clustering on the Grassmann manifold (or the Grassmannian), such as Grassmann K-means and depth-first search, to be applied to AMR. We further develop an analytical framework for studying and designing these algorithms in the context of AMR. First, the expectation-maximization algorithm for Grassmann constellation detection is proved to be equivalent to clustering (K-means) on the Grassmannian for a high SNR. Thereby, a well-known machine-learning result that was originally established only for the Euclidean space is rediscovered for the Grassmannian. Next, we tackle the challenge on theoretical analysis of data clustering by introducing probabilistic metrics for measuring the inter-cluster separability and intra-cluster connectivity of received space-time symbols and deriving them using tools from differential geometry. The results provide useful insights into the effects of various parameters ranging from the signal-to-noise ratio to constellation size, facilitating algorithmic design.
Persistent Identifierhttp://hdl.handle.net/10722/277222
ISSN
2023 Impact Factor: 4.6
2023 SCImago Journal Rankings: 2.520
ISI Accession Number ID

 

DC FieldValueLanguage
dc.contributor.authorDU, Y-
dc.contributor.authorZHU, G-
dc.contributor.authorZhang, J-
dc.contributor.authorHuang, K-
dc.date.accessioned2019-09-20T08:46:56Z-
dc.date.available2019-09-20T08:46:56Z-
dc.date.issued2018-
dc.identifier.citationIEEE Transactions on Signal Processing, 2018, v. 66 n. 22, p. 6031-6046-
dc.identifier.issn1053-587X-
dc.identifier.urihttp://hdl.handle.net/10722/277222-
dc.description.abstractRecent breakthroughs in machine learning shift the paradigm of wireless communication towards intelligence radios. One of their core operations is automatic modulation recognition (AMR). Existing research focuses on coherent modulation schemes such as QAM and FSK. The AMR of (noncoherent) space-time modulation remains an uncharted area despite its deployment in modern multiple-input-multiple-output (MIMO) systems. The scheme using a so-called Grassmann constellation enables rate enhancement. In this paper, we propose an AMR approach for Grassmann constellation based on data clustering, which differs from traditional AMR based on classification using a modulation database. The approach allows algorithms for clustering on the Grassmann manifold (or the Grassmannian), such as Grassmann K-means and depth-first search, to be applied to AMR. We further develop an analytical framework for studying and designing these algorithms in the context of AMR. First, the expectation-maximization algorithm for Grassmann constellation detection is proved to be equivalent to clustering (K-means) on the Grassmannian for a high SNR. Thereby, a well-known machine-learning result that was originally established only for the Euclidean space is rediscovered for the Grassmannian. Next, we tackle the challenge on theoretical analysis of data clustering by introducing probabilistic metrics for measuring the inter-cluster separability and intra-cluster connectivity of received space-time symbols and deriving them using tools from differential geometry. The results provide useful insights into the effects of various parameters ranging from the signal-to-noise ratio to constellation size, facilitating algorithmic design.-
dc.languageeng-
dc.publisherIEEE. The Journal's web site is located at http://ieeexplore.ieee.org/xpl/RecentIssue.jsp?punumber=78-
dc.relation.ispartofIEEE Transactions on Signal Processing-
dc.rightsIEEE Transactions on Signal Processing. Copyright © IEEE.-
dc.rights©20xx IEEE. Personal use of this material is permitted. Permission from IEEE must be obtained for all other uses, in any current or future media, including reprinting/republishing this material for advertising or promotional purposes, creating new collective works, for resale or redistribution to servers or lists, or reuse of any copyrighted component of this work in other works.-
dc.subjectModulation-
dc.subjectManifolds-
dc.subjectSignal processing algorithms-
dc.subjectClustering algorithms-
dc.subjectMIMO communication-
dc.titleAutomatic Recognition of Space-Time Constellations by Learning on the Grassmann Manifold-
dc.typeArticle-
dc.identifier.emailHuang, K: huangkb@eee.hku.hk-
dc.identifier.authorityHuang, K=rp01875-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1109/TSP.2018.2873542-
dc.identifier.scopuseid_2-s2.0-85054526961-
dc.identifier.hkuros305396-
dc.identifier.volume66-
dc.identifier.issue22-
dc.identifier.spage6031-
dc.identifier.epage6046-
dc.identifier.isiWOS:000447853700005-
dc.publisher.placeUnited States-
dc.identifier.issnl1053-587X-

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