Citation: | Li Kejun, Bai Jinming, Xiang Fuyuan. Preliminary Exploration of the Mathematical Method for Fitting Line Profiles[J]. Publications of the Yunnan Observatory, 1993, (1): 5-9. |
[1] | YU Xiao-xia. Hα Line Profile Asymmetry in Chromospheric Flare [J]. Astronomical Research and Technology, 2005, 2(4): 218-231. |
[2] | Wolfram Kollatschny. Structure and Kinematics of Emission Line Regions in AGN [J]. Astronomical Research and Technology, 2003, 0(S1): 32-41. |
[3] | LI Ke-jun, GU Xiao-ma, LI Qiu-sha, LI Jian-yong. Spectral Analysis of the D3 Emission Lines of a Mound Prominence II-Physical Properties of the Active Edge and the Mound Prominence [J]. Publications of the Yunnan Observatory, 2000, 0(1): 27-34. |
[4] | LI Ke-jun, GU Xiao-ma, LI Qiu-sha, LI Jian-yong. Spectral Analysis of the D3 Emission Lines of a Mound Prominence I-Characteristics and Calculations of the D3 Lines [J]. Publications of the Yunnan Observatory, 2000, 0(1): 20-26. |
[5] | Xu D. W.. Is There a Link Between Emission-Line Widths and X-Ray Continuum Slopes in Narrow Line Seyfert 1 Galaxies? [J]. Publications of the Yunnan Observatory, 1999, 0(S1): 314-317. |
[6] | Li Kejun, Zhong Shuhua, Bai Jinming. The Source Function Changed within Layers and the Self-Reverse of Prominence Line [J]. Publications of the Yunnan Observatory, 1995, 0(2): 12-18. |
[7] | Li Kejun, Bai Jinming. Analysis of the Line Spectrum of A Prominence by Means of the Dimension Descending Method [J]. Publications of the Yunnan Observatory, 1993, 0(2): 20-25. |
[8] | Li Kejun. An Analytical Method of the Spectra of the Active Bodies with the Three-Layer Radiative Structure on the Solar Disk and at the Solar Limb [J]. Publications of the Yunnan Observatory, 1992, 0(2): 20-27. |
[9] | Li Kejun, Bai Jingming. Analyses of the Self-Reversal Lines of the Prominence of 1984 February 18 [J]. Publications of the Yunnan Observatory, 1992, 0(2): 14-19. |
[10] | Wu Guanqian. On the Theoretical Calculation of Line Formation [J]. Publications of the Yunnan Observatory, 1991, 0(4): 46-54. |