The scintillation index（SI） of a Gaussian–Schell model（GSM） beam in a moderate-to-strong anisotropic nonKolmogorov turbulent atmosphere is developed based on the extended Rytov theory. The on-axis SI in a marine ...The scintillation index（SI） of a Gaussian–Schell model（GSM） beam in a moderate-to-strong anisotropic nonKolmogorov turbulent atmosphere is developed based on the extended Rytov theory. The on-axis SI in a marine atmosphere is higher than that in a terrestrial atmosphere, but the off-axis SI exhibits the opposite trend. The on-axis SI first increases and then begins to decrease and saturate as the turbulence strength increases. Turbulence inner and outer scales have different effects on the on-axis SI in different turbulent fluctuation regions. The anisotropy characteristic of atmospheric turbulence leads to the decline in the on-axis SI, and the rise in the off-axis SI. The on-axis SI can be lowered by increasing the anisotropy of turbulence, wavelength, and source partial coherence before entering the saturation attenuation region. The developed model may be useful for evaluating ship-to-ship/shore free-space optical communication system performance.展开更多
The Fresnel approximation in phase screen model is discussed and the coherencefunction is derived for k】】k.The application condition for Rino’s results is obtained,and it is|▽R<sub>△N<sub>e</sub>...The Fresnel approximation in phase screen model is discussed and the coherencefunction is derived for k】】k.The application condition for Rino’s results is obtained,and it is|▽R<sub>△N<sub>e</sub></sub>|/R<sub>△n<sub>e</sub></sub>【【1.展开更多
电离层闪烁导致卫星导航信号在传播过程中幅度与相位发生随机波动,严重影响接收机的性能。为模拟真实的受电离层闪烁影响的卫星导航信号,以供接收机进行性能测试,提出了基于电离层总电子含量(Total Electron Content,TEC)数据的电离层...电离层闪烁导致卫星导航信号在传播过程中幅度与相位发生随机波动,严重影响接收机的性能。为模拟真实的受电离层闪烁影响的卫星导航信号,以供接收机进行性能测试,提出了基于电离层总电子含量(Total Electron Content,TEC)数据的电离层闪烁仿真方法。该方法通过输入卫星观测文件与导航电文获得电离层的TEC和仰角,利用TEC数据和各卫星仰角,估计出受电离层闪烁影响的各卫星导航信号幅度闪烁指数和相位闪烁指数,结合Cornell模型实现卫星导航信号模拟。该方法充分考虑了卫星导航信号闪烁指数获取困难,以及电离层闪烁对不同卫星导航信号的影响,能够高保真反演卫星导航信号。试验结果表明,该方法反演的电离层闪烁与实际发生的闪烁具有良好的一致性。展开更多
通过分析2010年至2017年期间的中国低纬地区海口站(20°N,110°E)特高频(ultra high frequency,UHF)电离层闪烁,发现绝大部分年份中春分前后电离层闪烁事件发生概率高于秋分前后,综合电离层垂测观测数据,认为主要原因是春秋分...通过分析2010年至2017年期间的中国低纬地区海口站(20°N,110°E)特高频(ultra high frequency,UHF)电离层闪烁,发现绝大部分年份中春分前后电离层闪烁事件发生概率高于秋分前后,综合电离层垂测观测数据,认为主要原因是春秋分背景电离层电子密度和h′F日落增强现象的不对称性.最后基于电离层闪烁月发生概率统计数据,及其与季节和太阳活动的相关性,建立了一种考虑春秋分不对称性的电离层闪烁发生概率季节变化统计模型.此模型能够较好地表征电离层闪烁发生概率的季节变化特性,具有重要应用价值.展开更多
基金Project supported by the Open Research Fund of State Key Laboratory of Pulsed Power Laser Technology(Grant No.SKL2016KF05)the Key Industrial Innovation Chain Project in Industrial Domain,China(Grant No.2017ZDCXL-GY-06-02)+1 种基金the Huawei Innovation Research Program,China(Grant No.HO2017050001AG)the Foundation for Innovative Research Groups of the National Natural Science Foundation of China(Grant No.61621005)
文摘The scintillation index（SI） of a Gaussian–Schell model（GSM） beam in a moderate-to-strong anisotropic nonKolmogorov turbulent atmosphere is developed based on the extended Rytov theory. The on-axis SI in a marine atmosphere is higher than that in a terrestrial atmosphere, but the off-axis SI exhibits the opposite trend. The on-axis SI first increases and then begins to decrease and saturate as the turbulence strength increases. Turbulence inner and outer scales have different effects on the on-axis SI in different turbulent fluctuation regions. The anisotropy characteristic of atmospheric turbulence leads to the decline in the on-axis SI, and the rise in the off-axis SI. The on-axis SI can be lowered by increasing the anisotropy of turbulence, wavelength, and source partial coherence before entering the saturation attenuation region. The developed model may be useful for evaluating ship-to-ship/shore free-space optical communication system performance.
文摘The Fresnel approximation in phase screen model is discussed and the coherencefunction is derived for k】】k.The application condition for Rino’s results is obtained,and it is|▽R<sub>△N<sub>e</sub></sub>|/R<sub>△n<sub>e</sub></sub>【【1.
文摘电离层闪烁导致卫星导航信号在传播过程中幅度与相位发生随机波动,严重影响接收机的性能。为模拟真实的受电离层闪烁影响的卫星导航信号,以供接收机进行性能测试,提出了基于电离层总电子含量(Total Electron Content,TEC)数据的电离层闪烁仿真方法。该方法通过输入卫星观测文件与导航电文获得电离层的TEC和仰角,利用TEC数据和各卫星仰角,估计出受电离层闪烁影响的各卫星导航信号幅度闪烁指数和相位闪烁指数,结合Cornell模型实现卫星导航信号模拟。该方法充分考虑了卫星导航信号闪烁指数获取困难,以及电离层闪烁对不同卫星导航信号的影响,能够高保真反演卫星导航信号。试验结果表明,该方法反演的电离层闪烁与实际发生的闪烁具有良好的一致性。
文摘通过分析2010年至2017年期间的中国低纬地区海口站(20°N,110°E)特高频(ultra high frequency,UHF)电离层闪烁,发现绝大部分年份中春分前后电离层闪烁事件发生概率高于秋分前后,综合电离层垂测观测数据,认为主要原因是春秋分背景电离层电子密度和h′F日落增强现象的不对称性.最后基于电离层闪烁月发生概率统计数据,及其与季节和太阳活动的相关性,建立了一种考虑春秋分不对称性的电离层闪烁发生概率季节变化统计模型.此模型能够较好地表征电离层闪烁发生概率的季节变化特性,具有重要应用价值.
