利用双向滤波去除太阳图像中的柱状固定模式噪声

IF 1.8 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
Hao Lin, Xianyong Bai, Song Feng, Bo Liang, Wenda Cao, Ding Yuan, Wei Dai, Yangfan Guo
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引用次数: 0

摘要

太阳图像对于研究太阳活动和特征至关重要。如今,许多天文台依靠 CMOS 传感器获取这些图像。然而,这些传感器经常会引入列固定模式噪声(CFPN),严重影响图像质量。因此,我们提出了一种去除 CFPN 的双向滤波算法。首先,在水平方向上,我们使用一维全局加权最小二乘法滤波器和高效双边滤波器获得粗去噪图像。然后,我们利用垂直方向上的加权导向滤波器来估计 CFPN 成分,从而获得干净的太阳图像。我们选择了三幅不同的太阳观测图像,将我们的结果与三种比较方法获得的结果进行比较和评估。这些图像是由 SATech-01 卫星上的太阳上过渡区成像仪观测到的。此外,我们还进一步使用了两个量化指标,即光反应不均匀性和平均相对偏差,来量化去噪结果。结果表明,我们提出的方法能更好地去除 CFPN,并以更均衡的方式保留图像特征。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Column fixed-pattern noise removal in solar images using two-way filtering

Column fixed-pattern noise removal in solar images using two-way filtering

Solar images are critically important for studying solar activities and features. Today, many observatories rely on CMOS sensors to acquire these images. However, these sensors often introduce column fixed-pattern noise (CFPN), seriously affecting image quality. Therefore, we proposed a two-way filtering algorithm to remove CFPN. Firstly, in the horizontal direction, we used the one-dimensional global weighted least squares filter and the efficient bilateral filter to obtain a coarse denoised image. Then, we utilized the weighted guided filter in the vertical direction to estimate the CFPN components, thereby obtaining a clean solar image. We selected three different solar observation images to compare and evaluate our results to those obtained by three comparative methods. The images are observed by the Solar Upper Transition Region Imager aboard the SATech-01 satellite. Additionally, we further used two quantitative metrics, photo response non-uniformity and mean relative deviation, to quantify the denoised results. The results demonstrate that our proposed method removes the CFPN better and preserves the image features in a more balanced way.

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来源期刊
Astrophysics and Space Science
Astrophysics and Space Science 地学天文-天文与天体物理
CiteScore
3.40
自引率
5.30%
发文量
106
审稿时长
2-4 weeks
期刊介绍: Astrophysics and Space Science publishes original contributions and invited reviews covering the entire range of astronomy, astrophysics, astrophysical cosmology, planetary and space science and the astrophysical aspects of astrobiology. This includes both observational and theoretical research, the techniques of astronomical instrumentation and data analysis and astronomical space instrumentation. We particularly welcome papers in the general fields of high-energy astrophysics, astrophysical and astrochemical studies of the interstellar medium including star formation, planetary astrophysics, the formation and evolution of galaxies and the evolution of large scale structure in the Universe. Papers in mathematical physics or in general relativity which do not establish clear astrophysical applications will no longer be considered. The journal also publishes topically selected special issues in research fields of particular scientific interest. These consist of both invited reviews and original research papers. Conference proceedings will not be considered. All papers published in the journal are subject to thorough and strict peer-reviewing. Astrophysics and Space Science features short publication times after acceptance and colour printing free of charge.
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