Computer simulation of a method for object reconstruction from stellar speckle interferometry data.
Computer simulation of a method for object reconstruction from stellar speckle interferometry data.
复制标题
一种利用恒星散斑干涉测量数据重建物体的方法的计算机模拟。
DOI：
10.1364/ao.21.003132
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发表时间：
1982
期刊：
影响因子：
1.9
通讯作者：
J. G. Walker
中科院分区：
文献类型：
--
作者：
J. G. Walker
描述了一种由许多短曝光湍流退化图像组成的数据重建衍射限制图像的方法。给出了该方法的计算机仿真结果。这种方法对于从大型地球望远镜获得高角度分辨率的图像应该是有用的。仿真结果表明，该方法可以适用于微弱到11等的天体。
A method for reconstructing a diffraction-limited image from data consisting of many short-exposure turbulence degraded images is described. The results of a computer simulation of the method are presented. The method should prove useful for obtaining high-angular resolution images from large earth bound telescopes. The simulation indicates that the method may be applicable to astronomical objects as faint as approximately 11th magnitude.