The generalization of upper atmospheric wind and temperature based on the Voigt line shape profile

被引：64

作者：

Zhang, Chunmin ^{[1
]}

He, Jian

机构：

[1] Xian Jiaotong Univ, Sch Sci, Xian 710049, Peoples R China

[2] Henan Univ Sci & Technol, Sch Sci, Luoyang 471003, Peoples R China

来源：

OPTICS EXPRESS | 2006年 / 14卷 / 26期

关键词：

D O I：

10.1364/OE.14.012561

中图分类号：

O43 [光学];

学科分类号：

070207 ; 0803 ;

摘要：

The principle of probing the upper atmospheric wind field, which is the Voigt profile spectral line shape, is presented for the first time. By the Fourier Transform of Voigt profile, with the Imaging Spectroscope and the Doppler effect of electromagnetic wave, the distribution and calculation formulae of the velocity field, temperature field, and pressure field of the upper atmosphere wind field are given. The probed source is the two major aurora emission lines originated from the metastable O(S-1) and O(D-1) at 557.7nm and 630.0nm. From computer simulation and error analysis, the Voigt profile, which is the correlation of the Gaussian profile and Lorentzian profile, is closest to the actual airglow emission lines. (C) 2006 Optical Society of America.

引用

页码：12561 / 12567

页数：7

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