[1] Wang SJ,Yan YH,Fu QJ.Spikes in solar radio bursts at frequencies near 3 GHz.Solar Physics,2002,209 :185 ～ 193

[2] Benz AO,Kane SR.Electron acceleration in f lares inf erred from radio and hard X-ray emission.Solar Physics,1986,104 :179 ～ 185

[3] Benz AO.Millisecond radio spikes.Solar Physics,1986,99 ～ 100

[4] Csi llaghy A,Benz AO.The bandwidth of millionsecond radio spikes in solar flares.Astronomy &Astrophysics,1993,274 :487 ～ 496

[5] Messmer P,Benz AO.The minimum bandwidth of narrowband spikes in solar flare decimetric radio waves.Astronomy &Astrophysics,2000,354 :287 ～ 295

[6] Mallat SG.A theory formultiresolution signal decomposition :the wavelet representation.IEEE Transaction on Pattern Analysis and MachineIntelligence,1989,674～ 693

[7] Daubechies I.Orthonormal bases of compactly supportedwavelets.Communicat ions on Pure and Applied Mathematics,1988,XLI :909 ～ 996

[8] Feng XC,Gan XB,Song GX.Numeric Functional Analysis and Wavelet Theory.Xi' an :Xidian University Publishing House,2003(in Chinese)

[9] Hu CH,Zhang JB,Xia J,et al.Analysis and Design of System Based on Matlab.Xi' an :Xidian University Publishing House,1999(in Chinese)

[10] Bendjoya P,Petit JM,Spahn F.Wavelet analysis of the voyager data on planetarings.I.description of the method.Icarus,1993,105 :385 ～ 411

[11] Schwarz U,Kurths J,Kliem B,et al.Multiresolution analysis of solar mm-wave bursts.Astronomy &Astrophysics Supplement Series,1998,127 :309～ 318

[12] Aschwanden MJ,Kliem B.Wavelet analysis of solar flare hard X-rays.The Astrophysical Journal,1998,505 :941 ～ 956

[13] Zhao RY.Solar Radio Emission Theory.Beijing :Science Press,1999(in Chinese)

[8] 冯象初,甘小冰,宋国乡.数值泛函与小波理论.西安:西安电子科技大学出版社,2003

[9] 胡昌华,张军波,夏　军,等.基于Matlab 的系统分析和设计.西安:西安电子科技大学出版,1999

[13] 赵仁扬.太阳射电辐射理论.北京:科学出版社,1999