The Complete Linearization Method for Computing Non-LTE Model Stellar Atmosphere

Han Zhanwen

PDF
Cite
Share

facebook

twitter

google

linkedin

Publications of the Yunnan Observatory > 1989 > 0(1): 45-50.

Han Zhanwen. The Complete Linearization Method for Computing Non-LTE Model Stellar Atmosphere[J]. Publications of the Yunnan Observatory, 1989, (1): 45-50.

Citation:

Han Zhanwen. The Complete Linearization Method for Computing Non-LTE Model Stellar Atmosphere[J]. Publications of the Yunnan Observatory, 1989, (1): 45-50.

Citation:

Han Zhanwen. The Complete Linearization Method for Computing Non-LTE Model Stellar Atmosphere[J]. Publications of the Yunnan Observatory, 1989, (1): 45-50.

PDF (356 KB)

The Complete Linearization Method for Computing Non-LTE Model Stellar Atmosphere

Han Zhanwen

More Information

Received Date: July 19, 1987
Published Date: January 14, 1989

Graphical Abstract

Abstract

Abstract

In this paper, the computational process and programming of the complete linearization method for calculating the non-LTE model stellar atmosphere is dercribed and the computed results are also discussed.

FullText(HTML)

References (0)

Articles Related

[1]	Jia Jingyi, Ma Guanyi, Fan Jiangtao, Lu Weijun, Li Qi. A Test of GNSS Positioning Error Model of Non-uniform Pseudorange Error [J]. Astronomical Research and Technology, 2019, 16(4): 437-446.
[2]	ZHANG Han-wei, LI Bin-hua, YANG Lei, TIE Qiong-xian, MAO Wei. Atmospheric Distribution Model [J]. Astronomical Research and Technology, 2005, 2(4): 278-284.
[3]	JIANG Hu, HUANG Cheng. DTM94 Atmosphere Model and Its Application [J]. Publications of the Yunnan Observatory, 1999, 0(4): 30-37.
[4]	Xiong Guanzhu, Chen Jianbao. Linearization Method for Fitting the Infrared Spectrum of the Late Type Stars [J]. Publications of the Yunnan Observatory, 1995, 0(2): 36-41.
[5]	Wu Guanqian. An Effective Method for Treating the Blanketing Effect of A Non-LTE Line [J]. Publications of the Yunnan Observatory, 1990, 0(2): 44-50.
[6]	Jia Guibin. An Approach to the Determination of the Order of the MEM Power Spectrum in the Non-Linear Process [J]. Publications of the Yunnan Observatory, 1989, 0(4): 33-40.
[7]	Li Renxiang. A Computing Method for Restoring the Linear Degradation Image Model [J]. Publications of the Yunnan Observatory, 1988, 0(4): 86-92.
[8]	Han Zhanwen. Applications of Model Stellar Atmospheres [J]. Publications of the Yunnan Observatory, 1988, 0(3): 76-87.
[9]	Han Zhanwen. Computational Methods for the non-LTE Atmospheric Model [J]. Publications of the Yunnan Observatory, 1988, 0(2): 29-39.
[10]	Xia Canying. A Computation Formula for the Satellite Atmospheric Drag Coefficient [J]. Publications of the Yunnan Observatory, 1982, 0(1): 81-91.