Abstract
The twelve pulsation events recorded by the solar radio synchronous observation system at four frequencies (1420, 2000, 2840 and 4000 MHz) with high time resolution of Yunnan Observatory in the period 1989 December-1994 January are investigated in this paper. Several characteristics of the microwave pulsations are found, including long-period (about 50s) and short-period (tens of ms) pulsations. The morphology, period and bandwidth of the pulsations are analysed and discussed.
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