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Radio astronomy radio telescope plays the role of a linear operator, affecting the function that describes the object of research, formation of image of a monitored object. This paper presents methods for reconstruction and correction of solar radio images using the algorithm of rejections, the updated Weiner-filter, and the method CLEAN designed by Hegbomom (Pseudonym, 2009) for point sources. It is the process of numerical convolution in signal handling, an algorithm for separating weak-contrast formations on the solar which represents most points of the actual limb by using the ellipse equation. Consequently, the filling algorithm is applied by moving from the center to the ellipse points and filling each point by solar image data. Finally, a linear limb-darkening expression is used to remove the limb darkening. Different examples of the intermediate and final results are presented in addition to the developed algorithm.
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篇名 Adaptive Enhancement Techniques for Solar Images
来源期刊 信号与信息处理(英文) 学科 医学
关键词 IMAGE Processing SOLAR Imaging IMAGE Enhancement Linear Transformation Functions LIMB Darken-ing SOLAR DISK LIMB FITTING
年,卷(期) 2013,(4) 所属期刊栏目
研究方向 页码范围 359-363
页数 5页 分类号 R73
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研究主题发展历程
节点文献
IMAGE
Processing
SOLAR
Imaging
IMAGE
Enhancement
Linear
Transformation
Functions
LIMB
Darken-ing
SOLAR
DISK
LIMB
FITTING
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研究来源
研究分支
研究去脉
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期刊影响力
信号与信息处理(英文)
季刊
2159-4465
武汉市江夏区汤逊湖北路38号光谷总部空间
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301
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0
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