首页> 外文期刊>Optik: Zeitschrift fur Licht- und Elektronenoptik: = Journal for Light-and Electronoptic >High noise astronomical image denoising via 2G-bandelet denoising compressed sensing
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High noise astronomical image denoising via 2G-bandelet denoising compressed sensing

机译:高噪声天文图像去噪通过2g-candelet denoising压缩传感

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摘要

In deep space exploration, high resolution astronomical image captured is often contaminated by various cosmic noise signals during its shooting and long distance transmission, which has brought inconvenience to astronomical image analysis. The famous compressed sensing (CS) proposed by Candes et al. can successfully solve the problem of high resolution astronomical image compression and low noise reconstruction. In this paper, we further concern how to reconstruct a high quality image from a high resolution and high noise astronomical image. A 2G-bandelet denoising compressed sensing (BDCS) is first proposed based on the advantage of CS in image denoising and the superior ability of 2G-bandelet in sparse representation of astronomical images, then iterative bandelet thresholding (IBT-BTCS) algorithm based on BDCS is proposed for high resolution and high noise astronomical image reconstruction. Firstly, an iterative bandelet thresholding method is designed to obtain optimal approximation of original image; Secondly, to further improve the reconstructed image quality, group sparse total variation with stepsize constraints (GSTV-SC) method is proposed to adjust the reconstructed astronomical image in each iteration. The simulation results show that the proposed algorithm can quickly reconstruct a high quality astronomical image only using a few observations, preserve more astronomical image details and effectively solve high noise astronomical image denoising problem.
机译:在深度空间探索中,捕获的高分辨率天文图像通常被各种宇宙噪声信号污染,并且在其拍摄期间和长距离传输,这给了天文图像分析带来了不便。 Candes等人提出的着名压缩传感(CS)。可以成功解决高分辨率天文图像压缩和低噪声重建问题。在本文中,我们进一步涉及如何从高分辨率和高噪声天文图像重建高质量的图像。首先基于在天文图像的稀疏表示中的图像去噪和2G-Candelet中的优势的优点,基于COMOROMICAL图像的稀疏表示的优势,基于BDC的疏远BANDLETET阈值(IBT-BTCS)算法,首先提出了一种2G-BANDETENT压缩感应(BDC)。建议高分辨率和高噪声天文图像重建。首先,设计迭代Bandelet阈值方法以获得原始图像的最佳近似;其次,为了进一步提高重建的图像质量,提出了通过步骤限制(GSTV-SC)方法的组稀疏总变化(GSTV-SC)方法来调整每个迭代中的重建天文图像。仿真结果表明,该算法只能使用少数观察来快速重建高质量的天文图像,保持更多天文图像细节,并有效地解决高噪声天文图像去噪问题。

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