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首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Nonmigrating tidal impact on the CO_2 15 μminfrared cooling of the lower thermosphere during solar minimum conditions
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Nonmigrating tidal impact on the CO_2 15 μminfrared cooling of the lower thermosphere during solar minimum conditions

机译:在太阳能最小条件下,非迁移对CO_2 15微米的CO_2 15微米冷却冷却

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摘要

Carbon dioxide (CO_2) infrared emissions at 15 μm is the primary radiative cooling mechanism of the thermosphere in the altitude range of 100-135 km. This paper explores the role of two important diurnal nonmigrating tides, the DE2 and DE3, in the modulation of CO_2 15 μm emissions during the solar minimum year 2008 by (i) analyzing Sounding the Atmosphere using Broadband Emission Radiometry (SABER) CO_2 cooling rate data and (ii) photochemical modeling using dynamical tides from the empirical Climatological Tidal Model of the Thermosphere model. Tidal diagnostics of SABER data shows that the CO_2 cooling rate amplitudes for the DE2 and DE3 components are on the order of approximately 20-50% relative to the monthly means, and they maximize around the lower bound (100 km) of the analyzed height interval. The photochemical modeling reproduces the observed results, albeit with systematic amplitude differences which is likely related to the uncertainty in the model input backgrounds, especially atomic oxygen. The main tidal coupling mechanism is found to be the temperature dependence of the collisional excitation of the CO_2 v_2 vibrational state. However, neutral density becomes equally important above -110 km, thereby explaining observed evanescent DE2 and DE3 phases which are not present in temperature tides. The contribution of vertical tidal advection is comparatively small. The relative importance of the coupling mechanisms is the same at all latitudes/seasons. These results indicate that upward propagating nonmigrating tides forced by latent heat release in the lower atmosphere impact the thermospheric energy budget by modulating the longitudinal/local time behavior of the CO_2 infrared cooling.
机译:15μm的二氧化碳(CO_2)红外排放是热圈的主要辐射冷却机制100-135公里。本文探讨了两种重要的昼夜非迁移潮汐,DE2和DE3的作用,在太阳能最短的2008年的CO_215μm排放中的调制中(i)使用宽带发射辐射辐射测定(SABER)CO_2冷却速率数据进行分析(ii)采用动态潮汐从热圈模型的经验气候潮汐模型采用动态潮汐模型。 Sabre数据的潮汐诊断表明,DE2和DE3部件的CO_2冷却速度幅度相对于月度手段约为20-50%,并且它们围绕分析的高度间隔的下限(100km)最大化。光化学建模再现观察结果,尽管具有系统幅度差异,其可能与模型输入背景中的不确定性相关,尤其是原子氧。发现主潮汐耦合机构是CO_2V_2振动状态的碰撞激发的温度依赖性。然而,中性密度在-110km高于-110km以上同样重要,从而说明了在温度潮汐中不存在的观察到的蒸发器DE2和DE3相。垂直潮汐平流的贡献相对较小。耦合机构的相对重要性在所有纬度/季节都是相同的。这些结果表明,通过调节CO_2红外冷却的纵向/局部时间行为,通过较低大气中潜热释放的潜热释放的向上传播的非迁移潮汐冲击热散液。

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