Model of infrared emission from sprites

被引:7
作者
Milikh, GM [1 ]
Usikov, DA
Valdivia, JA
机构
[1] Univ Maryland, Dept Phys, College Pk, MD 20742 USA
[2] Univ Maryland, Dept Astron, College Pk, MD 20742 USA
基金
美国国家科学基金会;
关键词
D O I
10.1016/S1364-6826(98)80009-6
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 model of the 4.26 mu m infrared emission due to red sprites is presented. The model considers the generation of nitrogen 'vibrons' due to the collisions of the nitrogen molecules with the electrons energized by the electric field from lightning, followed by the transition of the nitrogen vibrons to the CO2(001) vibrational level, with a lifetime much shorter than that of nitrogen. The infrared photons of wavelength lambda = 4.26 mu m radiated by the CO2(001) propagate through the optically thick atmosphere; therefore, this emission could best be observed from space. The model computes the infrared radiance of sprites, as well as the energy collected by a state-of-the-art space infrared detector, and estimates the signal to background ratio. (C) 1998 Elsevier Science Ltd. All rights reserved.
引用
收藏
页码:895 / 905
页数:11
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