Infrared auroral emissions driven by resonant electron impact excitation of NO molecules

被引:25
作者
Campbell, L
Brunger, MJ
Petrovic, ZL
Jelisavcic, M
Panajotovic, R
Buckman, SJ
机构
[1] Flinders Univ S Australia, Sch Chem Phys & Earth Sci, Adelaide, SA 5001, Australia
[2] Inst Phys, YU-11001 Belgrade, Serbia Monteneg, Serbia
[3] Australian Natl Univ, Res Sch Phys Sci & Engn, Atom & Mol Phys Labs, Canberra, ACT, Australia
关键词
D O I
10.1029/2003GL019151
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Although only a minor constituent of the earth's upper atmosphere, nitric oxide (NO) plays a major role in infrared auroral emissions due to radiation from vibrationally excited (NO*) states. The main process leading to the production of these excited molecules was thought to be chemiluminescence, whereby excited nitrogen atoms interact with oxygen molecules to form vibrationally excited nitric oxide (NO*) and atomic oxygen. Here we show evidence that a different production mechanism for NO*, due to low energy electron impact excitation of NO molecules, is responsible for more than 30% of the NO auroral emission near 5 mum.
引用
收藏
页码:L101031 / 4
页数:4
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