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Modeling nightglow in atomic oxygen red and green lines under moderate disturbed geomagnetic conditions at midlatitudes

机译:在中纬度中度扰动的地磁条件下模拟原子氧红线和绿线中的夜光

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We present results of a study of mid-latitude auroras. The study is based on optical measurements and theoretical modeling. The modeling shows that precipitation can indirectly generate airglow in red and green lines of atomic oxygen by increasing rates of ion formation and heating of thermal electrons. This causes an increase in the rate of dissociative recombination and thermal-electron-collision excitation of the 1D and 1S levels.
机译:我们提出了中纬度极光研究的结果。该研究基于光学测量和理论建模。该模型表明,降水可以通过增加离子形成速率和加热热电子间接在原子氧的红线和绿线中产生气辉。这导致1D和1S能级的解离重组和热电子碰撞激发速率增加。

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