Modified high definition reconstruction algorithm of astronomical speckle images
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Modified high definition reconstruction algorithm of astronomical speckle images
Optics and Precision EngineeringVol. 15, Issue 7, Pages: 1151-1156(2007)
作者机构:
解放军信息工程大学 测绘学院,河南 郑州,450052
作者简介:
基金信息:
DOI:
CLC:TP391.4
Received:05 October 2006,
Revised:21 March 2007,
Published Online:30 July 2007,
Published:30 July 2007
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GENG Ze-xun, WANG Zhen-guo. Modified high definition reconstruction algorithm of astronomical speckle images[J]. Optics and precision engineering, 2007, 15(7): 1151-1156.
DOI:
GENG Ze-xun, WANG Zhen-guo. Modified high definition reconstruction algorithm of astronomical speckle images[J]. Optics and precision engineering, 2007, 15(7): 1151-1156.DOI:
Modified high definition reconstruction algorithm of astronomical speckle images
the performance of high resolution imaging of large optical instruments is severely limited. Speckle imaging is one of ways to eliminate atmospheric blur based on recording series of images with short exposure to freeze the turbulence to obtain restoration image for reconstruction. By incorporating dynamic shrinkage of support region
a modified maximum likelihood blind deconvolution algorithm is proposed in this paper. The algorithm is applied to the restorations of short-exposure images of astronomical point source star
images of astronomical extended object and adaptive optics long exposure images of point source star. Experimental results prove that this algorithm works well not only for short exposure images of point source star
but also for images of astronomical extended object and adaptive optics long exposure images. The PSNR of reconstruction images is raised by over 10 percent. The novelty of this algorithm is that the support region of astronomical object can be contracted adaptively according to the threshold in reconstruction iterations.