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Variations of thermospheric composition according to AE-C data and CTIP modelling

机译:根据AE-C数据和CTIP建模的热层成分变化

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摘要

Data from the Atmospheric Explorer C satellite, taken at middle and low latitudes in1975-1978, are used to study latitudinal and month-by-month variations of thermospheric composition. Theparameter used is the "compositional -parameter", related to the neutral atomic oxygen/molecularnitrogen concentration ratio. The midlatitude data show strong winter maxima of the atomic/molecular ratio,which account for the "seasonal anomaly" of the ionospheric F2-layer. When the AE-C data arecompared with the empirical MSIS model and the computational CTIP ionosphere-thermosphere model,broadly similar features are found, but the AE-C data give a more molecular thermosphere than do themodels, especially CTIP. In particular, CTIP badly overestimates the winter/summer change ofcomposition, more so in the south than in the north. The semiannual variations at the equator and insouthern latitudes, shown by CTIP and MSIS, appear more weakly in the AE-C data. Magnetic activityproduces a more molecular thermosphere at high latitudes, and at mid-latitudes in summer. Atmospheric composition and structure (thermosphere– composition and chemistry)
机译:1975-1978年中低纬度地区的Atmospheric Explorer C卫星的数据用于研究热层成分的纬度和逐月变化。所使用的参数是“组成参数”,与中性原子氧/分子氮浓度比有关。中纬度资料显示,冬季的原子/分子比极大,这是电离层F2层的“季节异常”。当将AE-C数据与经验MSIS模型和计算的CTIP电离层-热层模型进行比较时,发现的特征大致相同,但是AE-C数据比模型(尤其是CTIP)具有更多的分子热圈。特别是,CTIP严重高估了冬夏组成的变化,南部比北部更多。 CTIP和MSIS显示的赤道和南北纬度的半年变化在AE-C数据中显得较弱。磁活动在高纬度和夏季的中纬度产生了更多的分子热圈。大气成分和结构(热层–成分和化学)

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