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  2. Speckle (interference) - Wikipedia

    en.wikipedia.org/wiki/Speckle_(interference)

    The speckle can also represent some useful information, particularly when it is linked to the laser speckle and to the dynamic speckle phenomenon, where the changes of the spatial speckle pattern over time can be used as a measurement of the surface's activity, such as which is useful for measuring displacement fields via digital image correlation.

  3. Speckle imaging - Wikipedia

    en.wikipedia.org/wiki/Speckle_imaging

    The short exposure images are aligned by using the brightest speckle and averaged to give a single output image. [7] The method involves calculation of the differential shifts of the images. This is easily accomplished in astronomical images since they can be aligned with the stars. Once the images are aligned they are averaged together.

  4. Image noise - Wikipedia

    en.wikipedia.org/wiki/Image_noise

    Image noise can also originate in film grain and in the unavoidable shot noise of an ideal photon detector. Image noise is an undesirable by-product of image capture that obscures the desired information. Typically the term “image noise” is used to refer to noise in 2D images, not 3D images.

  5. Laser speckle contrast imaging - Wikipedia

    en.wikipedia.org/wiki/Laser_speckle_contrast_imaging

    The method to compute the contrast of speckle patterns can be classified into three categories: s-K (spatial), t-K (temporal), and st-K (Spatio-temporal). To compute the spatial contrast, raw images of laser speckle will be separated into small elements, and each element corresponds to a pixels.

  6. Lucky imaging - Wikipedia

    en.wikipedia.org/wiki/Lucky_imaging

    Lucky image of M15 core. Lucky imaging (also called lucky exposures) is one form of speckle imaging used for astrophotography.Speckle imaging techniques use a high-speed camera with exposure times short enough (100 ms or less) so that the changes in the Earth's atmosphere during the exposure are minimal.

  7. Multiplicative noise - Wikipedia

    en.wikipedia.org/wiki/Multiplicative_noise

    An important example is the speckle noise commonly observed in radar imagery. Examples of multiplicative noise affecting digital photographs are proper shadows due to undulations on the surface of the imaged objects, shadows cast by complex objects like foliage and Venetian blinds , dark spots caused by dust in the lens or image sensor, and ...

  8. Median filter - Wikipedia

    en.wikipedia.org/wiki/Median_filter

    However, its performance is not that much better than Gaussian blur for high levels of noise, whereas, for speckle noise and salt-and-pepper noise (impulsive noise), it is particularly effective. [6] Because of this, median filtering is very widely used in digital image processing .

  9. Shearography - Wikipedia

    en.wikipedia.org/wiki/Shearography

    Shearography or Speckle pattern shearing interferometry is a measuring and testing method similar to holographic interferometry. It uses coherent light or coherent soundwaves [ 1 ] to provide information about the quality of different materials in nondestructive testing , strain measurement, and vibration analysis.