收稿日期: 2002-12-10
修回日期: 2003-04-28
网络出版日期: 2004-01-10
基金资助
中国科学院、科技部973项目(G2000078403)和自然科学基金项目(19973008;19833050;10225313)共同资助
Pattern Recognition and Parameter Statistics of Fine Structures in the Solar Radio Bursts
Received date: 2002-12-10
Revised date: 2003-04-28
Online published: 2004-01-10
张丽丽 , 颜毅华 , 宋国乡 . 太阳射电爆发精细结构的特征提取和参数统计[J]. 中国科学院大学学报, 2004 , 21(1) : 33 -39 . DOI: 10.7523/j.issn.2095-6134.2004.1.005
Being advantageous to pattern-enhancement and noise-suppression,wavelet transform is applied to extract the frequency band of fibril and zebrapat ternfine structure and remove noise to get their clear characteristics.Then,a pattern recognition algorithm is presented to determine all fine structures in the whole burst regime.Finally the parameters of fine structures is calculated and analyzed so as to understand the physics of solar radio burst .
Key words: solar radio burst; fine structure; wavelet transform
[1] St arck J L, Bijaoui A, Lopez B, Perrier C. Image reconstruct ion by t he wavelet t ransform applied to apert ure synt hesis. Ast ronomy andAst rophysi cs, 1994, 283( 1) : 349-360
[2] Y ihua Yan, Bo Peng. D-e noising w it h wavelet s in image restorat ion f or radio aperture synt hesis. Chi nese Journal of Radi o Sci ence. PI-CRS, China, 1995 ( S. I. ) : 276-279
[3] Y ihua Y an, Bo Peng, X izhen Zhang. N oise suppression w it h w avelets in image reconst ruct ion for apert ure synt hesis. In: G eorge H Jacoby,Jeannet t e Barnes. Ast ronomical dat a analysis sof tw are and syst ems V. A SPCS, A merica, 1995. 101: 223-226
[4] M sz rosov H, Jiricka K, K arlick M. Fourier an d w avelet analysis of type 42 S ER and 41 F solar radio burst s. Ast ronomy and Ast ro-physics, 1999, 348: 1005-1011
[5] M essm er P, Benz A O. The minimum bandw idt h of narrow band spikes in solar flare decimetric radio w aves. Ast ronomy and Ast rophysi cs,2000, 354: 287-295
[6] R obert A Sych, Y-i Hua Y an. Wavelet cleaning of solar dynamic radio spect rograms. Chin J. A stron. A st rop hys., 2002, 2( 2) : 183-192
[7] 颜毅华, 谭程明, 徐 龙, 等. 太阳射电爆发的非线性相对定标方法与数据处理. 中国科学( A 辑), 2001, 31( 增刊) : 73-79
[8] Fu Q, Q in Z, Ji H, et al. A broadband spect rometer f or decimet er and microw ave radio bursts. S ol ar Physi cs, 1995, 160: 97-103
[9] 赵仁扬, 金声震, 傅其骏. 太阳射电微波爆发. 北京: 科学出版社, 1997
[10] 姬慧荣, 傅其俊, 刘玉英, 等. 2. 6-3. 8 GH z 太阳射电动态频谱仪. 天体物理学报, 2000, 20( 2) : 209-215
[11] Caroubalos, et al. A rt emis IV radio observat ions of t he 14 July 2000 large solar event. Solar Physics. 2001, 204: 167-179
[12] St ephane M allat, W en Liang Hw ang. S ingularit y det ection and processing w ith w avelet s. IEEE Tr an. on I. T., 1992, 38( 2) : 617-643
[13] St ephane M allat, Sif en Zhong. Wavelet maxima represent at ion. In: Y M eyer. Wavelet s and A pplicat ions. PICM, Fran ce, 1989. 1992.207-284
[14] 杨福生. 小波变换的工程分析与应用. 北京: 科学出版社, 2000
[15] M ario A T Figueirdo, Robert D N ow ak. Wavelet-based image estimation: an empirical bayes approach using jef freys 'noninformat ive Pri-or. IEEE Tra n. on I. P. 2001, 10( 9) : 1322-1331
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