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New methods of non-linear image restoration and reconstruction.

机译:非线性图像复原和重建的新方法。

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摘要

Integral logarithmic transforms are defined for both one-dimensional and two-dimensional input functions. These have the desirable properties of linearity and invariance to scale change of the input. Two-dimensional integral logarithmic transform is additionally invariant to rotation. The integral logarithmic transforms are conveniently inverted by simple differentiation. Second, a new approach is given for the problem of reconstruction of phase from modulus data. A set of Wiener-filter functions is formed that multiply, in turn, displaced versions of the modulus data in frequency space such that the sum is a minimum L₂-error norm solution for the object. The required statistics are power spectra of the signal and noise, and correlation between modulus data at a given frequencies and complex object spectral values at adjacent frequencies. Finally, a new technique is proposed to reconstruct a turbulent image from a superposition model. Imagery through random atmospheric turbulence is modeled as a stochastic superposition process. By this model, each short-exposure point spread function is a superposition of randomly weighted and displaced versions of one intensity profile. If we could somehow estimate the weights and displacements for a given image, then by the superposition model we would known the spread function, and consequently, could invert the imaging equation for the object.
机译:为一维和二维输入函数定义了积分对数变换。它们具有线性和不变的特性,可以随输入比例变化。二维积分对数变换对于旋转也不变。积分对数变换可通过简单的微分方便地反转。其次,针对从模量数据重建相位的问题给出了一种新方法。形成一组维纳滤波器函数,该函数依次将模数数据的位移版本在频率空间中相乘,以使该和成为对象的最小L 2误差范数解。所需的统计信息是信号和噪声的功率谱,以及给定频率下的模量数据与相邻频率下的复杂对象光谱值之间的相关性。最后,提出了一种从叠加模型中重建湍流图像的新技术。通过随机的大气湍流将图像建模为随机叠加过程。通过该模型,每个短曝光点扩展函数都是一个强度分布的随机加权和位移版本的叠加。如果我们能够以某种方式估计给定图像的权重和位移,则通过叠加模型,我们将知道扩散函数,因此可以将物体的成像方程式求逆。

著录项

  • 作者

    Oh Choonsuck.;

  • 作者单位
  • 年度 1992
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  • 原文格式 PDF
  • 正文语种 en
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