Seasonal variations of O2 atmospheric and OH(6-2) airglow and temperature at mid-latitudes from SATI observations

被引：41
|
作者：
López-González, MJ
Rodríguez, E
Wiens, RH
Shepherd, GG
Sargoytchev, S
Brown, S
Shepherd, MG
Aushev, VM
López-Moreno, JJ
Rodrigo, R
Cho, YM
机构：
[1] CSIC, Inst Astrofis Andalucia, E-18080 Granada, Spain
[2] Univ Asmara, Dept Phys, Asmera, Eritrea
[3] York Univ, Ctr Res Earth & Space Sci, Toronto, ON M3J 1P3, Canada
[4] Minist Educ & Sci, Inst Ionosphere, Alma Ata 480020, Kazakhstan
来源：
ANNALES GEOPHYSICAE | 2004年 / 22卷 / 03期
关键词：
atmospheric composition and structure; airglow and aurora; pressure density and temperature; instruments and techniques;
D O I：
10.5194/angeo-22-819-2004
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
More than 3 years of airglow observations with a Spectral Airglow Temperature Imager (SATI) installed at the Sierra Nevada Observatory (37.06degrees N, 3.38degrees W) at 2900 m height have been analyzed. Values of the column emission rate and vertically averaged temperature of the 02 atmospheric (0-1) band and of the OH Meinel (6-2) band from 1998 to 2002 have been presented. From these observations a clear seasonal variation of both emission rates and rotational temperatures is inferred at this latitude. It is found that the annual variation of the temperatures is larger than the semiannual variation, while for the emission rates the amplitudes are comparable.
引用
收藏
页码：819 / 828
页数：10
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