Abstract
From January, 1988 to June, 1989 the solar radio synchronous observational system with high temporal resolution of the Yunnan Observatory was used to carry out observations at a decimetric wavelength (1420 MHz), and the data are analyzed in this paper. The result shows a relation between the millisecond spike radiation of the solar decimetric radio emission and the radio bursts recorded with a time constant of one second. It also reveals the coexistence of decimetric radio millisecond spike radiations and Hα flares, type III radio bursts as well as soft X-ray bursts. A solar activity event with abundant radio millisecond spike radiations is investigated preliminarily and the relation between the duration and flux of individual spikes is discussed.
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