Please use this identifier to cite or link to this item: https://ir.swu.ac.th/jspui/handle/123456789/29275
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dc.contributor.authorTausiesakul B.
dc.contributor.authorAsavaskulkiet K.
dc.contributor.otherSrinakharinwirot University
dc.date.accessioned2023-11-15T02:08:14Z-
dc.date.available2023-11-15T02:08:14Z-
dc.date.issued2023
dc.identifier.urihttps://www.scopus.com/inward/record.uri?eid=2-s2.0-85165629485&doi=10.1016%2fj.ymssp.2023.110459&partnerID=40&md5=a76527b9ad557a792c09c7e30c9a93ac
dc.identifier.urihttps://ir.swu.ac.th/jspui/handle/123456789/29275-
dc.description.abstractA computation technique, known as inverse perturbation-fractional norm regularization (IP-FNR), is proposed in this wok for a sparse signal recovery problem. The objective function of this method is derived using a general ℓp norm, when p is a positive fractional number. Numerical examples are conducted for both noiseless and noisy cases. Performance of the proposed approach in terms of root-mean-square relative error (RMSRE), mean normalized squared error, standard deviation mean, occupied memory during the computation, and computational time is compared to several previous methods. It is found that in the noiseless case, the IP-FNR method significantly outperforms the former fixed-point algorithms for a certain range of the norm exponent p, provided that the perturbation parameter and the regularization multiplier are properly chosen. In the noisy case, at the expense of computational time, the IP-FNR approach provides noticeably lower RMSRE when the signal-to-noise ratio or the sparsity ratio is high and the compression ratio is quite low. © 2023 Elsevier Ltd
dc.publisherAcademic Press
dc.subjectCompressive sensing
dc.subjectFractional norm
dc.subjectRegularization
dc.titleFractional norm regularization using inverse perturbation
dc.typeArticle
dc.rights.holderScopus
dc.identifier.bibliograpycitationMechanical Systems and Signal Processing. Vol 199, No. (2023)
dc.identifier.doi10.1016/j.ymssp.2023.110459
Appears in Collections:Scopus 2023

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