2000
DOI: 10.1080/01431160050121294
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Automatic computation of speckle standard deviation in SAR images

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Cited by 8 publications
(4 citation statements)
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“…Since the value of the noise variance is an essential part of SDC, it should first be estimated from the image. Different solutions to the noise variance estimation problem in image had been published, such as the autoregressive model [26], the least-squares [27] and the wavelet decomposition [28].…”
Section: Resultsmentioning
confidence: 99%
See 1 more Smart Citation
“…Since the value of the noise variance is an essential part of SDC, it should first be estimated from the image. Different solutions to the noise variance estimation problem in image had been published, such as the autoregressive model [26], the least-squares [27] and the wavelet decomposition [28].…”
Section: Resultsmentioning
confidence: 99%
“…The spectral-domain constrained subspace method is implemented using spectral constraint α i given in (27). The implementation steps are as follows, 1) Apply the homomorphic transformation to the noisy image, G = W N. …”
Section: Implementation Of Signal Subspace Approach For Multiplicamentioning
confidence: 99%
“…We adopt an automatic procedure to estimate speckle standard deviation from SAR images as in Frulla et al [24], which observed that the CV should be equal to the theoretical speckle standard deviation according to the number of looks of the SAR image for fully developed speckled images. However, the coefficient of variation measured over homogeneous regions on the images may differ from theoretical values due to several reasons such as the inherent image variations and the size of the selected sample.…”
Section: Speckle Statistics and Image Modelmentioning
confidence: 99%
“…Therefore we decided to implement Lee's polarimetric filter [5]. The speckle standard deviation is estimated according to Frulla [4]. to achieve some independency from the data and assist the less experienced user.…”
Section: Hv Absmentioning
confidence: 99%