Empirical model of variations in the helium 1083 nm emission. 2. Temperature

被引：1
|
作者：
Shefov, N. N. [1 ]
Semenov, A. I. [1 ]
Yurchenko, O. T. [1 ]
机构：
[1] Russian Acad Sci, Obukhov Inst Atmospher Phys, Moscow 109017, Russia
来源：
GEOMAGNETISM AND AERONOMY | 2009年 / 49卷 / 05期
基金：
俄罗斯基础研究基金会;
关键词：
TOPSIDE IONOSPHERE; ATOMS; HE+;
D O I：
10.1134/S0016793209050144
中图分类号：
P3 [地球物理学]; P59 [地球化学];
学科分类号：
0708 ; 070902 ;
摘要：
Based on the measurements of the ortho helium 1083 nm emission intensity during twilights and on the calculation of its variations depending on the solar zenith angle, the method for determining the atmospheric temperature at heights of 300-1000 km during the nighttime period of day has been developed, taking into account the diurnal and seasonal conditions.
引用
收藏
页码：670 / 678
页数：9
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