摘要
In the first part of this paper, we propose that the term’ solar spectrum’should be generalized to Stokes (unpolarized and polarized) spectrum rather than the ordinary (unpolarized) one which is included in the former as the first component. The significance of Stokes (polarized) spectrum observation is emphasized. In the second part, a sample of recent Stokes spectrum observation carried out at Yunnann Observatory is shown and it signifies the beginning of such observation in China.
In the first part of this paper, we propose that the term' solar spectrum'should be generalized to Stokes (unpolarized and polarized) spectrum rather than the ordinary (unpolarized) one which is included in the former as the first component. The significance of Stokes (polarized) spectrum observation is emphasized. In the second part, a sample of recent Stokes spectrum observation carried out at Yunnann Observatory is shown and it signifies the beginning of such observation in China.
作者
Qu Z.Q. 1, 2 , Chen X.K. 1, Zhang X.Y. 1,Gu X.M. 1, Feng Y.M. 1, Zhong S.H. 1 1 (Yunnan Observatory, The Chinese Academy of Sciences, Kunming 650011, China) 2 (Beijing Astronomical Observatory, The Chinese Academy of Sciences, Beijing 100012, C
出处
《天文研究与技术》
CSCD
1999年第S1期279-282,共4页
Astronomical Research & Technology
