利用单站GNSS精密单点定位原理(Precise Point Positioning,PPP)解算天顶方向的对流层大气天顶延迟,并对其一天内的变化进行统计平均,结合经典的Kolmogorov-Obukhov"2/3"扰动理论和随机场理论,基于对流层天顶延迟与大气折射...利用单站GNSS精密单点定位原理(Precise Point Positioning,PPP)解算天顶方向的对流层大气天顶延迟,并对其一天内的变化进行统计平均,结合经典的Kolmogorov-Obukhov"2/3"扰动理论和随机场理论,基于对流层天顶延迟与大气折射率的时变相关性获得大气结构常数C_n,并分析了不同大气扰动强度下的二元天线阵大气相位误差.通过计算我国北京、上海、昆明、乌鲁木齐四个甚长基线干涉测量(Very Long Baseline Interferometry,VLBI)深空站处不同时间的C^2_n,评估各站点大气环境的扰动特性对X/Ka频段天线阵系统工作性能的影响,统计结果表明:除了北京、乌鲁木齐站在1月份的相位误差相对较小外,各站其他时间在Ka频段的相位误差大多数达到25°以上,北京的7月和上海的4月甚至高达50°以上,会严重降低天线阵信噪比合成性能,影响地面站与深空探测器之间的大容量通信.展开更多
Random fluctuations of turbulence bring random fluctuations of the refractive index, making the atmosphere a random fluctuation medium that destroys the coherence of light-waves. Research in atmospheric turbulence is ...Random fluctuations of turbulence bring random fluctuations of the refractive index, making the atmosphere a random fluctuation medium that destroys the coherence of light-waves. Research in atmospheric turbulence is actually the investigation of the atmospheric refractive index. The atmospheric structure constant of refractive index, C n 2 , is an important parameter denoting atmospheric turbulence. In this paper, C n 2 is measured during the day and at night and in all four seasons using a high sensitivity micro-thermal meter QHTP-2. The vertical profile of C n 2 in Hefei (0-30 km) is investigated by the analysis of experimental data. The average profile of C n 2 in Hefei exhibits conspicuous day and night differences with increased altitude. The distribution of log(C n 2 ) is nearly normal and has conspicuous seasonal differences.展开更多
在相距600 m 的两地进行了静态激光大气传输实验,并对接收到的光强和光束到达角起伏进行记录.以每10min 所记录的数据作为样本,计算出光强起伏方差和到达角起伏方差,并根据理论孔径平滑因子计算出点接收时的光强起伏方差,再分别根据光...在相距600 m 的两地进行了静态激光大气传输实验,并对接收到的光强和光束到达角起伏进行记录.以每10min 所记录的数据作为样本,计算出光强起伏方差和到达角起伏方差,并根据理论孔径平滑因子计算出点接收时的光强起伏方差,再分别根据光强起伏方差和到达角起伏方差计算出大气折射率结构常数.最后,得到一天之内大气折射率结构常数的变化曲线,并分析得出大气折射率结构常数在早晨和傍晚存在极小值.展开更多
文摘利用单站GNSS精密单点定位原理(Precise Point Positioning,PPP)解算天顶方向的对流层大气天顶延迟,并对其一天内的变化进行统计平均,结合经典的Kolmogorov-Obukhov"2/3"扰动理论和随机场理论,基于对流层天顶延迟与大气折射率的时变相关性获得大气结构常数C_n,并分析了不同大气扰动强度下的二元天线阵大气相位误差.通过计算我国北京、上海、昆明、乌鲁木齐四个甚长基线干涉测量(Very Long Baseline Interferometry,VLBI)深空站处不同时间的C^2_n,评估各站点大气环境的扰动特性对X/Ka频段天线阵系统工作性能的影响,统计结果表明:除了北京、乌鲁木齐站在1月份的相位误差相对较小外,各站其他时间在Ka频段的相位误差大多数达到25°以上,北京的7月和上海的4月甚至高达50°以上,会严重降低天线阵信噪比合成性能,影响地面站与深空探测器之间的大容量通信.
基金supported by the National High Technology Research and Development Program of China (GrantNo. 2011AA8061007)
文摘Random fluctuations of turbulence bring random fluctuations of the refractive index, making the atmosphere a random fluctuation medium that destroys the coherence of light-waves. Research in atmospheric turbulence is actually the investigation of the atmospheric refractive index. The atmospheric structure constant of refractive index, C n 2 , is an important parameter denoting atmospheric turbulence. In this paper, C n 2 is measured during the day and at night and in all four seasons using a high sensitivity micro-thermal meter QHTP-2. The vertical profile of C n 2 in Hefei (0-30 km) is investigated by the analysis of experimental data. The average profile of C n 2 in Hefei exhibits conspicuous day and night differences with increased altitude. The distribution of log(C n 2 ) is nearly normal and has conspicuous seasonal differences.
文摘在相距600 m 的两地进行了静态激光大气传输实验,并对接收到的光强和光束到达角起伏进行记录.以每10min 所记录的数据作为样本,计算出光强起伏方差和到达角起伏方差,并根据理论孔径平滑因子计算出点接收时的光强起伏方差,再分别根据光强起伏方差和到达角起伏方差计算出大气折射率结构常数.最后,得到一天之内大气折射率结构常数的变化曲线,并分析得出大气折射率结构常数在早晨和傍晚存在极小值.
