Comparison of histogram-curve fitting-based and global threshold methods for cloud detection

MakaleYalnız künyeScopus SJRQ1

Özet

The goal of this research is fit the best curve to the image histogram using polynomial (i.e., linear, quadratic, cubic, and quartic), Fourier and Gaussian with two different term numbers, and Bezier functions, and then compare their performance with nine automatic state-of-the-art thresholding methods: Shanbhag, Triangle, Huang, Intermode, IsoData, Li's, Maximum entropy, Moment, and Otsu. The visible bands of the Landsat-9, Landsat-8, and Sentinel 2 satellite images are averaged to create an index map, which was used to perform the cloud detection. Since many satellites system only has visible bands, the average index map was used. Three different images which include various cloud types were clipped from each satellite imaging. Thresholding methods were evaluated using statistical tools such as structural similarity index measure (SSIM), peak signal-to-noise ratio (PSNR), and universal image quality index (UIQI), accuracy, Cohen's kappa, precision, recall, F-Measure, and G-Mean. The histogram-based approaches that performed the best after Li's method were Bezier (96.71% accuracy and 99.83% SSIM), 2nd Gaussian (97.62% precision), Quartic (80.56% kappa, 16.16% PSNR, 82.45% F-Measure, and 89.52%), and 2nd Fourier (81.08% recall and 89.27% G-Mean), according to the average statistics of all images. Additionally, methods other than Shanbhag yielded favorable results (more than 90% accuracy).

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https://rdlopen.rawdatalibrary.net/r/gumushane/12763Resmi atıflarda kullanılan kalıcı adres
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https://doi.org/10.1007/s13762-023-05379-6Yayıncı resmi DOI adresi
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dc.contributor.authorGünen, M. Akif
dc.date.accessioned2026-10-22T10:20:30.960156810Z
dc.date.available2026-10-22T10:20:30.960156810Z
dc.date.issued2024
dc.description.abstractThe goal of this research is fit the best curve to the image histogram using polynomial (i.e., linear, quadratic, cubic, and quartic), Fourier and Gaussian with two different term numbers, and Bezier functions, and then compare their performance with nine automatic state-of-the-art thresholding methods: Shanbhag, Triangle, Huang, Intermode, IsoData, Li's, Maximum entropy, Moment, and Otsu. The visible bands of the Landsat-9, Landsat-8, and Sentinel 2 satellite images are averaged to create an index map, which was used to perform the cloud detection. Since many satellites system only has visible bands, the average index map was used. Three different images which include various cloud types were clipped from each satellite imaging. Thresholding methods were evaluated using statistical tools such as structural similarity index measure (SSIM), peak signal-to-noise ratio (PSNR), and universal image quality index (UIQI), accuracy, Cohen's kappa, precision, recall, F-Measure, and G-Mean. The histogram-based approaches that performed the best after Li's method were Bezier (96.71% accuracy and 99.83% SSIM), 2nd Gaussian (97.62% precision), Quartic (80.56% kappa, 16.16% PSNR, 82.45% F-Measure, and 89.52%), and 2nd Fourier (81.08% recall and 89.27% G-Mean), according to the average statistics of all images. Additionally, methods other than Shanbhag yielded favorable results (more than 90% accuracy).
dc.identifier.doi10.1007/s13762-023-05379-6
dc.identifier.eissn1735-2630
dc.identifier.endpage5848
dc.identifier.issn1735-1472
dc.identifier.issue6
dc.identifier.scopus2-s2.0-85179302628
dc.identifier.startpage5823
dc.identifier.urihttps://rdlopen.rawdatalibrary.net/r/gumushane/12763
dc.identifier.volume21
dc.identifier.wosWOS:001122759600002
dc.language.isoen
dc.publisherInstitute for Ionics
dc.relation.ispartofInternational Journal of Environmental Science and Technology
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.subjectBezier
dc.subjectCloud detection
dc.subjectFourier
dc.subjectGaussian
dc.subjectHistogram fit
dc.subjectPolynomial
dc.subjectThreshold
dc.subject.classificationEnvironmental Sciences
dc.subject.classificationEnvironmental Sciences & Ecology
dc.subject.otherCurve fitting
dc.subject.otherFourier transforms
dc.subject.otherGaussian distribution
dc.subject.otherInterpolation
dc.subject.otherMaps
dc.subject.otherMaximum entropy methods
dc.subject.otherSignal to noise ratio
dc.subject.otherStatistical mechanics
dc.subject.otherBezy
dc.subject.otherCloud detection
dc.subject.otherFourier
dc.subject.otherGaussians
dc.subject.otherHistogram fit
dc.subject.otherIndex maps
dc.subject.otherLANDSAT
dc.subject.otherThreshold
dc.subject.otherThresholding methods
dc.subject.otherVisible band
dc.subject.otheraccuracy assessment
dc.subject.othercomparative study
dc.subject.otherdetection method
dc.subject.otherFourier transform
dc.subject.otherGaussian method
dc.subject.otherhistogram
dc.subject.otherimage analysis
dc.subject.othersatellite altimetry
dc.subject.otherSentinel
dc.subject.othersignal-to-noise ratio
dc.subject.othersimilarity index
dc.titleComparison of histogram-curve fitting-based and global threshold methods for cloud detection
dc.typeArticle
rdl.citation.openalex19
rdl.citation.scopus19
rdl.citation.wos16
rdl.oa.statusclosed
rdl.scopus.quartileQ1
rdl.source.indexSCOPUS
rdl.source.indexWOS
rdl.wos.indexScience Citation Index Expanded (SCI-EXPANDED)