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Simulation of tropospheric scintillation on LEO satellite link based on space-time channel modeling.

机译:基于时空信道建模的LEO卫星对流层闪烁仿真。

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摘要

Tropospheric scintillation effect is well modelled for Earth to satellite communication in clear air conditions. Statistical models are available for geostationary and nongeostationary satellites. Time series simulators have been developed for geostationary links and are not valid for spatial applications involving LEO satellites such as Earth Observation Satellites. A new scintillation model is proposed in order to take into account both the dynamic behaviour of the troposphere and the movement of the LEO satellite. This model takes advantages of the outputs generated by Weather Research and Forecasting software which simulates the space-time behaviour of the turbulent troposphere. From its outputs, the refractive index structure constant and the standard deviation of the signal logamplitude caused by the scintillation are computed and the time varying scintillation spectrum is defined by its two asymptotes. Finally, time series of clear air scintillation can be generated by filtering white noise with the spectrum obtained.
机译:对流层闪烁效应已很好地模拟了在晴朗空气条件下地球与卫星之间的通信。统计模型可用于对地静止和非对地静止卫星。时间序列模拟器是为对地静止链路开发的,不适用于涉及地球观测卫星等LEO卫星的空间应用。提出了一种新的闪烁模型,以考虑对流层的动态行为和LEO卫星的运动。该模型利用了Weather Research and Forecasts软件生成的输出的优势,该软件可模拟湍流对流层的时空行为。根据其输出,计算由闪烁引起的折射率结构常数和信号对数振幅的标准偏差,并通过其两个渐近线定义随时间变化的闪烁光谱。最后,通过用获得的频谱对白噪声进行滤波,可以生成清晰的空气闪烁时间序列。

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