Studying nighttime nitric oxide emission at 5.3 μm during the geomagnetic storm in the Earth's ionosphere

被引：1

作者：

Bouziane, Abdelaaziz ^{[1
]}

Amin Ferdi, Mohammed ^{[1
]}

Djebli, Mourad ^{[1
]}

机构：

[1] USTHB, Fac Phys, Theoret Phys Lab, BP 32 Bab Ezzouar, Algiers 16079, Algeria

来源：

ASTROPHYSICS AND SPACE SCIENCE | 2022年 / 367卷 / 01期

关键词：

Ionosphere; Geomagnetic storm; NO vibrational emission; FLUX; ENERGY;

D O I：

10.1007/s10509-021-04037-y

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The nighttime NO 5.3 mu m emission at Irkutsk location is studied during the November 20, 2003, geomagnetic storm by using a coupled 1-D Boltzmann kinetic-fluid model, to calculate densities of the major ions: O-2(+); N-2(+); NO+; O+, nitrogen atoms: N(S-4); N(D-2), and vibrationally excited levels: NO (v <= 7), in the thermosphere between 100 and 200 km. By considering chemical reactions of neutrals and ions species in addition to molecular diffusion and an updated reaction rate coefficients, a good agreement is seen between numerical simulation and SABER (Sounding of the Atmosphere using Broadband Emission Radiometry) measurements of NO 5.3 mu m volume emission rate, compared to models based on photochemical equilibrium assumption.

引用

页数：10

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