| Abstract: | In this paper the performances and the main observational results, including the identification of meterwave blips, 10 milliseconds coronal quasi-oscillations, the size distributions of the spikes' sources and the electron density determination of coronal condensation by the solar eclipse, by the solar radio meter-wave spectrograph at the Yunnan Observatory are introduced. This instrument is made based on the principle of the spectral analysis of the acousto-optic deflection. The spectral resolution is 0 25 MHz and the time resolution is promoted from 80 ms to l ms. |
