排序方式: 共有1条查询结果,搜索用时 15 毫秒
1
1.
Bromage B.J.J. Alexander D. Breen A. Clegg J.R. Del Zanna G. DeForest C. Dobrzycka D. Gopalswamy N. Thompson B. Browning P.K. 《Solar physics》2000,193(1-2):181-193
Coronal holes on the Sun are the source of high-speed solar wind streams that produce magnetic disturbances at the Earth. A series of multi-wavelength, multi-instrument observations obtained during the 1996 Whole Sun Month campaign examined a large coronal hole in greater detail than ever before. It appeared on the Sun in August, and extended from the north pole to a large active region in the southern hemisphere. Its physical and magnetic structure and subsequent evolution are described. 相似文献
1