Primary Analysis of CMEs Associted with the Radio Emission During October 22 to November 03,2002

Based on data of eight solar radio emissions associated with the coronal mass ejection (CME) in the period of October 22, 2003 to November 3, 2003 observed with the solar radio broad band spectromter of National Astronomical Observatories of China (NAOC), and combined with image data obtained from Nobeyama Radioheliograph (NoRH) and Siberian Solar Radio Telescope (SSRT), spectral data from Culgoora and Waves/Wind, and the fixed frequency data from Nobeyama Radio Polarimeter (NoRP), characteristics of radio emission of these 8 radio bursts are analyzed primaryly in order to find the relationship between the CMEs and the radio emissions.