A SOLAR MICROWAVE BURST SPECTROMETER

In the paper the solar radio specrtometer in 1.0—2.0GHz and 2.6—3.8GHz which are working and the 5.2—7.6 GHz spectrometer which will come into operation in 1999, are introduced. They are the key observation facilities of solar physicscommunity in China for the coming 23rd solar active maximum years. 171 and 146 bursts of different types in 1.0—2.0 GHz and 2.6—3.8 GHz, respectively, with awealth of fine structure in time and frequency has been registered. The solar radiobursts at different frequencies reflect the evolving processes of solar flares in timeand heigh, and provide useful data for the study of solar flares.