Abstract

The luminescence-intensity profiles of the bands of the first and second positive systems of molecular nitrogen were calculated for the case of the precipitation of high-energy electrons with energies from 10 keV to 10 MeV into the atmosphere. The calculations showed that the contribution of the quenching of state B³Π_g N₂ increases during molecular collisions with an increase in the energy of electrons intruding into the atmosphere. This leads to a decrease in the ratio of the integrated intensities of the bands of the first and second positive systems with an increase in the energy of electrons that precipitate into the atmosphere.

中文翻译：

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高能电子沉淀过程中地球大气中分子氮带的发光

摘要

对于具有10 keV到10 MeV能量的高能电子沉淀到大气中的情况，计算了分子氮的第一和第二正系统的能带的发光强度分布。计算表明，状态淬火的贡献乙³ Π_克Ñ ₂增大时与增加的电子侵入到大气中的能量分子的碰撞。这导致第一和第二正系统的能带的积分强度之比的减小，而沉淀到大气中的电子的能量增加。