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IMAGE RESTORATION

Image Restoration

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image restoration, noise models

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  • IMAGE RESTORATION

  • Materialpresentedinthispdf filehasbeentakenfromreferencesgiventoyou.Thisisnothavinganycommercialvalueandistobeusedasreferenceforyourpaperee606

  • NOISE MODELS

  • Principle source of noise in images arise during imageacquisition (digitization) and/or transmission.Performance of imaging sensors is affected by number offactors ie

    environmental condition during image acquisitions quality of sensing elements

    In case of CCD camera, light levels and sensor temperatureare major factors affecting the noise.

    Frequency domain properties of noise are also very usefulinformation. For example Fourier spectrum of noise if isconstant, the noise is usually called white noise. Thisterminology is used for white light

  • (a)Gaussian noise or normal noise:A common noise model. PDF of Gaussian random variable,Z, is given by:

    z gray level mean average value of z std. deviation2 variance70% of values of Z will be in the range [(-), (+)]95% will be [(-2), (+2)]99.7% will be [(-3), (+3)]

    For 99.7% of the gray level, that are due to Gaussian noise,the average peak to peak gray level deviation about themean is Peak to peak = 6.

  • For, example if mean gray level of noise in an image is 128, ands.d. is 10. For 99.7% of the pixels within this image, the peak-to-peak gray level deviation will be 60 ie images gray levelvarying between 98 and 158 for 99.7% of pixels.

    Rayleigh Noise

    Mean and variance are:

  • Basic shape is skewed towards right.Quite useful for approximating skewed histogram.

    Erlang (Gamma) Noise

    a > 0, b is + ive integer, ! indicate factorial. =b/a, 2=b/a2

    Exponential noise

    Where, a > 0

  • This is a special case of Erlange PDF where b=1This appears in images acquired using laser asilluminating sources. This is also known as laserspeckle. In this mean and std deviation is same ie (1/a).Highest p.d.f is at (0,0).This function is defined beyond the dynamic range of thetypical digital image.

    Uniform noise

  • If b>a, gray level b will appear as a light dot in the image. Gaussian noise is normally due to electronic circuit noise

    & sensor noise, to poor illumination or high temp. Rayleigh noise is helpful in characterization of noise in

    range imaging. Exponential & gamma noise is common in laser images. Impulse is common in phenomena such as quick transient,

    faulty switching. Uniform noise is least descriptive of a practical

    phenomena but useful in generating numerous random functions.

    Salt & Peper noise (Impulse noise)

  • Image with sinusoidal noise and its spectrum

    Periodic Noise