[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 |