摘要
A study is made of the differences in the polarization distribution and other characteristics of microwave emission for several active regionswith high flare productivity. Conclusions are drawn about the magnetic field structure of these regions at coronal heights.
A study is made of the differences in the polarization distribution and other characteristics of microwave emission for several active regionswith high flare productivity. Conclusions are drawn about the magnetic field structure of these regions at coronal heights.
出处
《空间科学学报》
CAS
CSCD
北大核心
2005年第5期419-423,共5页
Chinese Journal of Space Science
基金
Supported by the Ministry of Industry and Science (No.477.2003,2)Russian Federal Program "Astronomy", and the China- Russia Joint Research Center on Space WeatheChinese Academy of Sciences
关键词
日光闪烁
微波散射
太阳活动
偏震现象
Microwave emission, Solar activity, Solar flare prediction
