2017
DOI: 10.1016/j.neucom.2017.05.018
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Group sparsity based regularization model for remote sensing image stripe noise removal

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Cited by 72 publications
(54 citation statements)
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“…In this section, we conduct experiments on both simulated and real data to test the efficiency of the proposed method. Five state-of-the-art destriping methods were chosen for comparison: the filtering-based method [12] (WAFT), the statistics-based method [13] (SLD), and optimization-based methods such as the weighted UTV-based method [29] (WDSUV), the low-rank decomposition-based method [38] (LRSID), and the group sparsity regularization-based method [40] (GSUTV). In the simulated experiments, the original MODIS Image Band 32 of size 400 × 400, which is available at https:// ladsweb.nascom.nasa.gov/, and the IKONOS image of size 377 × 331, which can be downloaded from https://openremotesensing.net/, were used by adding synthetic stripe noises to the clean image.…”
Section: Methodsmentioning
confidence: 99%
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“…In this section, we conduct experiments on both simulated and real data to test the efficiency of the proposed method. Five state-of-the-art destriping methods were chosen for comparison: the filtering-based method [12] (WAFT), the statistics-based method [13] (SLD), and optimization-based methods such as the weighted UTV-based method [29] (WDSUV), the low-rank decomposition-based method [38] (LRSID), and the group sparsity regularization-based method [40] (GSUTV). In the simulated experiments, the original MODIS Image Band 32 of size 400 × 400, which is available at https:// ladsweb.nascom.nasa.gov/, and the IKONOS image of size 377 × 331, which can be downloaded from https://openremotesensing.net/, were used by adding synthetic stripe noises to the clean image.…”
Section: Methodsmentioning
confidence: 99%
“…After estimating the stripe S from (2), the ground-truth image U is obtained by F − S. We explain in detail the motivation of each term in our model. To illustrate the stripe properties appropriately, we use GSUTV [40], which achieves the destriping by estimating the stripe component, to remove stripes in the Terra MODIS image and explore the stripe properties in results. Figure 1a-c presents the degraded image, the destriping result, and the stripe component, respectively.…”
Section: The Proposed Modelmentioning
confidence: 99%
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“…Considering the characteristic of stripes, sparse representation and sparsity promoting priors have been utilized to remove the stripes in HSIs [15,16,32,33]. However, this sparsity characteristic has not been considered under a tensor framework.…”
Section: Introductionmentioning
confidence: 99%
“…In [22], the UV model was converted to a least square problem by an iteratively reweighted technique that was easy to implement. Regarding the destriping problem as an ill-posed inverse problem, the (column) sparsity property and low rank property of the stripe noise served as a regularization to improve the stripe estimation performance in [23][24][25]. Chen et al [26] combined the group sparsity constraint and total variation regularization to remove the stripe noise and preserve edge information.…”
Section: Introductionmentioning
confidence: 99%