模式大气
The variation of Chapman's function in a realistic model atmosphere due to high temperature gradient, molecular and eddy diffusion transport, gravity field as well as solar activity is computed and discussed for the lower thermosphere.
计算并讨论了低热层高温度梯度、分子与湍流扩散、重力场及太阳活动对Ch(z p,χ)的影响。
After analyzing the 11-yr, 27 days and diurnal variation of upper atmosphere caused by solar activity, a calculation method for MET model atmosphere density is presented in which solar activity is taken into account.
该文分析了高层大气与太阳活动有关的11周年变化、27天变化以及周日变化,讨论了考虑太阳活动的MET模式大气密度计算途径,并且介绍了卫星大气阻力加速度模型。
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