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A Noise Reduction Method for Solar Radio Spectrum Based on Improved Guided Filter and Morphological Cascade
Luo, Gaifang1; Yuan, Guowu1,2; Li, Guoliang1; Wu, Hao1; Dong L(董亮)3; Luo, Gaifang4; Yuan, Guowu4,5; Li, Guoliang4; Wu, Hao4; Dong L(董亮)6
会议录名称Advances in Intelligent Systems and Computing - Advances in Natural Computation, Fuzzy Systems and Knowledge Discovery - Volume 2
2020
卷号1075
页码815-822
DOI10.1007/978-3-030-32591-6_88
产权排序第3完成单位
收录类别EI
会议名称15th International Conference on Natural Computation, Fuzzy Systems and Knowledge Discovery, ICNC-FSKD 2019, co-located with the 5th International Conference on Harmony Search, Soft Computing and Applications, ICHSA 2019
会议日期2019-07-20
会议地点Kunming, China
关键词Solar radio spectrum Noise reduction Guided filtering Morphological filtering
摘要

In solar radio observation, it is inevitable to be disturbed by noise, and the solar radio spectrum is affected. The solar radio spectrum with good quality can provide useful information in analyzing solar activities and improve the accuracy of automatic detection and classification of solar radio bursts. A noise reduction method for solar radio spectrum based on improved guided filter and morphological cascade is proposed in this paper. Firstly, the background noise of solar radio spectrum is subtracted, and the cross-fringe interference caused by channel effect is reduced. Secondly, the improved guided filtering is used to keep the edge of the solar radio burst as far as possible when filtering the burst region of the spectrum. Finally, more noise from other external factors is removed by morphological operation. The experimental results show that the proposed method is effective in removing noise from solar radio spectrum.

资助项目Natural Science Foundation of China[11663007] ; Natural Science Foundation of China[11703089] ; Natural Science Foundation of China[41764007] ; Natural Science Foundation of China[61802337] ; Natural Science Foundation of China[U1831201] ; Open Project of Key Laboratory of Celestial Structure and Evolution, Chinese Academy of Sciences [OP201510] ; Open Project of the Key Laboratory of Space Weather of China Meteorological Administration, Chinese Academy of Sciences "Western Light" Talent Development Program ; Action Plan of Yunnan University Serving for Yunnan.
项目资助者Natural Science Foundation of China[11663007, 11703089, 41764007, 61802337, U1831201] ; Open Project of Key Laboratory of Celestial Structure and Evolution, Chinese Academy of Sciences [OP201510] ; Open Project of the Key Laboratory of Space Weather of China Meteorological Administration, Chinese Academy of Sciences "Western Light" Talent Development Program ; Action Plan of Yunnan University Serving for Yunnan
语种英语
学科领域天文学 ; 射电天文学 ; 射电天文方法 ; 电子、通信与自动控制技术 ; 信息处理技术
文章类型Conference article (CA)
出版者Springer
ISBN号9783030325909
ISSN号2194-5357
URL查看原文
EI入藏号20195207923597
EI主题词Radio Communication
EI分类号716.1 Information Theory And Signal Processing - 716.3 Radio Systems And Equipment - 723 Computer Software, Data hAndling And Applications - 751.4 Acoustic Noise - 961 Systems Science
引用统计
文献类型会议论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/22556
专题射电天文研究组
通讯作者Yuan, Guowu; Yuan, Guowu
作者单位1.School of Information Science and Engineering, Yunnan University, Kunming, 650091, China
2.CAS Key Laboratory of Solar Activity, National Astronomical Observatories of Chinese Academy of Sciences, Beijing, 100012, China
3.Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650011, China
4.School of Information Science and Engineering, Yunnan University, Kunming, 650091, China
5.CAS Key Laboratory of Solar Activity, National Astronomical Observatories of Chinese Academy of Sciences, Beijing, 100012, China
6.Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650011, China
推荐引用方式
GB/T 7714
Luo, Gaifang,Yuan, Guowu,Li, Guoliang,et al. A Noise Reduction Method for Solar Radio Spectrum Based on Improved Guided Filter and Morphological Cascade[C]:Springer,2020:815-822.
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