摘要
基于云南天文台射电频谱仪的频率设置，第２３ 周太阳峰年期，我们作了下列观测研究选题：（１） 质子耀斑的初始能量释放过程及粒子加速研究。（２） 通过微波———分米波运动Ⅳ型爆发观测，开展日冕物质抛射研究。（３） 射电快速精细结构及微耀斑研究。（４） 通过频谱观测发展日冕磁场的诊断方法、反演磁场的拓朴结构。（５） 开展太阳灾变事件中的射电先兆研究。
In view of the frequency installation of radiospectrographs at Yunnan Observatory, the following radio subjects of observations and studies are suggested for the maximum phase of solar cycle 23: (1) The study on releasing course of initial energy of proton flares and particle acceleration. (2) The research of coronal mass ejection by observations of Type Ⅳ burst ranging from microwave up to decimetre wave bands. (3) The study of radio fast fine structures and microflares. (4) The diagnostic methods of coronal magnetic fields by radio spectral observations to deduce magnetic topotogy. (5) The study of radio indication of catastrophic solar events to supply solar activity and alarm of solar therrestrical environment.
