2018
DOI: 10.1016/j.optcom.2018.05.004
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Reduction of speckle noise in digital holography by combination of averaging several reconstructed images and modified nonlocal means filtering

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Cited by 10 publications
(13 citation statements)
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“…And it is also a difficult noise to deal with. [51][52][53][54] The parameters of the relevant physical quantities are set as follows: the wavelength of the light source is λ = 0.6328 μm. The distance z between the simulated object and the CCD is z = 1000 mm.…”
Section: Simulation Resultsmentioning
confidence: 99%
“…And it is also a difficult noise to deal with. [51][52][53][54] The parameters of the relevant physical quantities are set as follows: the wavelength of the light source is λ = 0.6328 μm. The distance z between the simulated object and the CCD is z = 1000 mm.…”
Section: Simulation Resultsmentioning
confidence: 99%
“…where k => 8000 r is the correlation coefficient. The greatest standard deviation estimate is received when r value is close to zero, then σ r ≈ 0.011 where r ≈ 0.5 we have σ r ≈ 0.007 [29][30][31][32][33][34][35][36][37][38][39][40][41].…”
Section: Covariance Model Of Vibration Signal Parametersmentioning
confidence: 94%
“…where γ > 0 is a descent parameter and prox γR D denotes the proximity operator of the functional R D . Here, we follow the plug-andplay prior philosophy [23][24][25] and replace prox γR D in (11) by the Algorithm 1 Proposed algorithm to solve (9) Require:…”
Section: Final Reconstruction Using the Learnt Dictionarymentioning
confidence: 99%
“…Put simply, the ODT lateral resolution is better than its axial resolution. Finally, the measured fields contain optical aberrations or speckle noise [8,9] which are usually unknown and constitute a source of model mismatch. To mitigate these problems, former works added prior knowledge in the reconstruction process using regularization [4,7,10,11].…”
Section: Introductionmentioning
confidence: 99%