Method of monitoring atomic oxygen and molecular nitrogen composition in the upper atmosphere on XUV images of the Sun

被引：1
|
作者：
Mordovskaya, V. G. [1 ]
Ignat'ev, A. P. [2 ]
Boldyrev, S. I. [1 ]
Gorbunov, S. A. [1 ]
Ivanov-Kholodnyi, G. S. [1 ]
Kolomiitsev, O. P. [1 ]
机构：
[1] Russian Acad Sci, Inst Terr Magnetism Ionosphere & Radiowave Propag, Troitsk, Moscow Oblast, Russia
[2] Russian Acad Sci, Lebedev Inst Phys, Moscow, Russia
来源：
GEOMAGNETISM AND AERONOMY | 2010年 / 50卷 / 05期
基金：
俄罗斯基础研究基金会;
关键词：
EARTHS UPPER-ATMOSPHERE; SOLAR EUV; THERMOSPHERIC O/N-2; RADIATION; SATELLITE; ABSORPTION; ONBOARD;
D O I：
10.1134/S0016793210050154
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：
A method for determining the basic atmosphere O/N-2 based on the solar observations is described. It is shown that, on XUV images of the Sun received by transillumination of the atmosphere, it is possible to observe its state controlling the O/N-2 ratio. The method allows local inhomogeneities of the upper atmosphere to be studied. Its abilities were demonstrated according to the SPIRIT complex on board the Coronas-F satellite.
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页码：679 / 685
页数：7
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