The numerical simulation of the growth rate of electron-cyclotron maser  

作　　者：金声震 赵仁扬 

机构地区：[1]Beijing Astronomical Observatory, Chinese Academy of Sciences Beijing 100080, China

出　　处：《Chinese Science Bulletin》1996年第1期49-54,共6页

基　　金：Project supported by the National Natural Science Foundation of China amd Astronomical Committee of Chinese Academy of Sciences

摘　　要：The spike radiation in the microwave region has been known for a long time as a special radiation which comes from the interaction of waves and nonthermal electron beams in the source region of corona. Many solar radio astronomers, such as Melrose and Dulk, Zhao and Shi, have studied the physical reason of spike radiation. It is generall believed that the lose cone distribution of the nonthermal electrons in a flaring loop is unstable, and if the beam particle distribution develops a positive gradient, i.e. (?)f/(?)p】0, some electron-magnetic waves are excited.

关 键 词：SPIKE electron-cyclotron MASER simulation. 

分 类 号：P412[天文地球—大气科学及气象学]