Killeen T L, Hays P B
Appl Opt. 1981 Oct 1;20(19):3314-7. doi: 10.1364/AO.20.003314.
Generalized composite nonthermal line profiles are calculated for the thermospheric nighttime emission from O((1)S) metastable atoms based on an extension to the simple relaxation model of Hays and Walker. It is shown that the Dynamics Explorer Fabry-Perot interferometer will enable accurate values to be obtained for the branching ratio of the O((1)S) production reaction and for the excitation exchange collision frequency.
基于对海斯和沃克简单弛豫模型的扩展,计算了热层夜间O((1)S)亚稳态原子发射的广义复合非热谱线轮廓。结果表明,动力学探测器法布里-珀罗干涉仪将能够获得O((1)S)产生反应的分支比和激发交换碰撞频率的精确值。