A method to calculate the ionospheric 83. 4nm dayglow emissions

	A method to calculate the ionospheric 83. 4nm dayglow emissions
	Liu, X. Y.; X. X. Zhang; F. He and B. Chen
	2017
发表期刊	Chinese Journal of Geophysics-Chinese Edition
卷号	60 期号:9
摘要	The 83. 4 nm emissions of oxygen atoms is one of the most intense emission signals in the ionosphere. It provides a powerful method for the monitoring of the upper atmosphere from space. This paper uses the MSISE-00 model of the atmosphere, using AURIC to calculate the initial emission rate, the ionospheric molecular nitrogen, oxygen, and oxygen atom density distribution, then using Chapman oxygen ion density distribution method to solve the integral equation of linear equations to calculate the resonance scattering emissions under the action of the resonance scattering, then calculate different emission intensities under different initial emission rate. And then, calculate the results and compare with Anderson's result. Finally, we point out that if the proportion of the initial volume emissions created by the photoelectron source increased by 16%, the total emission intensity increased by 30% at 350 km. The work of this paper provides theoretical support for the inversion of ionospheric electron density.
收录类别	sci ; ei
语种	英语
文献类型	期刊论文
条目标识符	http://ir.ciomp.ac.cn/handle/181722/59100
专题	中科院长春光机所知识产出
推荐引用方式 GB/T 7714	Liu, X. Y.,X. X. Zhang,F. He and B. Chen. A method to calculate the ionospheric 83. 4nm dayglow emissions[J]. Chinese Journal of Geophysics-Chinese Edition,2017,60(9).
APA	Liu, X. Y.,X. X. Zhang,&F. He and B. Chen.(2017).A method to calculate the ionospheric 83. 4nm dayglow emissions.Chinese Journal of Geophysics-Chinese Edition,60(9).
MLA	Liu, X. Y.,et al."A method to calculate the ionospheric 83. 4nm dayglow emissions".Chinese Journal of Geophysics-Chinese Edition 60.9(2017).

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