The Observation of Radio Fast Processes During the PartialSolar Eclipse on Marth 9,1997 in Kunming

Observational results of the partial solar eclipse on March 9, 1997 by using the synchronous observational system with high time resolution at 4 bands in Yunnan Observatory are presented in this paper. The process of electron acceleration in the slowly variable source in the corona are presumed by variable rate of radio fast fluctuations during eclipsing and appearing sunspots. The accelerations may contribute to the enhancement of the rate of radio fast fluctuations. 