OH气辉对重力波响应的模式研究
OH AIRGLOW RESPONSE TO SHORT PERIOD GRAVITY WAVE
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摘要: 重力波是中间层大气的重要能量来源,气辉观测为研究中间层重力波特性提供了极好的方法。本文利用最新的 OH 气辉激发机制,建立了一个较完整的光化、动力模式来分析重力波传播对 OH 气辉的影响。结果表明,化学反应速率系数不定性对 Krassovsky 比振幅的影响较小,但淬灭过程的影响必须考虑。Krassovsky 比的振幅和相位均依赖于波周期,其振幅在2.1和10.3之间变化;这表明 OH 气辉亮度的相对变化大于温度的相对变化。一般情况下,重力波引起的温度扰动超前于气辉亮度的变化。与实测资料比较发现,两者变化趋势基本一致,在短周期波时吻合较好。Abstract: The gravity wave is an important energy source of mesosphere.The airglow measurements provide a good method to study gravity wave characteristics in the mesosphere.In this paper,a full photochemical-dynamical model for analyzing the effect of gravity waves on the OH airglow was established by adopting recent excitation mechanism for total OH airglow.The result shows that the effects of the uncertainty of rate constants in the chemical reaction is not larger than 10%,but the effects of quenching must be considered.The amplitude and phase angle of Krassovsky ratio 77 depend on wave period,the value of |η| is 2.1 to 10.3,which shows that the relative variation of OH airglow intensity is larger than that of atmospheric temperature.And the variation of the OH brightness is led by the temperature fluctuation of gravity wave.The theoretic model is consistent with the observations,especially for short period wave.
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Key words:
- OH airglow /
- Gravity wave /
- Photochemical-dynamical model /
- Mesospheric temperature /
- Short period wave.
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