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本文利用瑞士Berne大学1988年1月-1989年12月发布的15个太阳微波脉冲事件的观测资料，分析其时间轮廓的3个主要特征：脉冲度、不对称性和半功率宽度频率响应．这些特性，可以定性地用非热电子的连续注入模，和不均匀的源模型给出较合理的解释．
In this paper, the observation data of 15 solar microwave pulse events published by Berne University in Switzerland from January 1988 to December 1989 are used to analyze three main characteristics of time profile: pulse, asymmetry and half-power frequency response. These properties can be qualitatively explained by a non-hot electron continuous injection mold and a non-uniform source model.