共查询到20条相似文献,搜索用时 125 毫秒
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某类型可变相位中心天线的相位中心随频率和入射方位变化,而且受到天线阵架设环境的影响。因此需要在理想计算相位中心的基础上,在现场发射测试信号来修正各种误差引起的相位中心变化。提出一种现场校准方法,设计了校准天线的架设方法,推导出由测向基线相位差计算天线单元相位中心与阵中心距离的方程。仿真表明,天线单元相位中心经过校准后,空间谱测向算法的空间分辨力有明显提高。 相似文献
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卫星导航接收天线相位中心的测量 总被引:2,自引:0,他引:2
通常天线的相位中心与其几何中心是不一致的。为了确立天线相位中心与几何中心位置的相对偏差,提出了采用室内测量法和室外测量法对天线相位中心进行测量,描述了2种测量方法的测量原理。详细介绍了在测量过程中找出天线相位中心的方法步骤,并指出了2种测量方法的特点。 相似文献
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根据测地型高精度GPS天线相位中心检测的需要,本文研制了一种时间同步自动旋转装置,利用机械结构设计提高被测天线旋转的回转精度和指向精度,使用GPS授时芯片实现被测天线按GPS时序高频率自动旋转,从方法上提高了检测结果的准确性。该装置结构稳定、自动化程度高,天线相位中心检测精度可达亚毫米级,已在实际外业检测中取得良好的应用效果。 相似文献
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星间链路(ISL)是我国北斗三号克服区域布站、实现高精度服务的关键,其天线相位中心偏差(PCO)在设备出厂时会依据质量、设计姿态进行地面标定,但在卫星发射、入轨及在轨阶段,燃料消耗、天线展开姿态等均会引起卫星质量与姿态的变化,这将导致在轨的PCO与地面标定值不一致 ,该变化量会作为误差引入到测量值,进而影响卫星轨道确定精度。因此,该文研究了在轨卫星的星间链路天线相位中心偏差标定方法,联合星间、星地观测,建立了基于整网估计的星间链路天线相位中心偏差在轨估计方法,并利用两周的实测数据进行对北斗三号所有中轨卫星(MEO)进行验证,同时结合卫星生产商、轨道面进行在轨特性的详细分析,最后验证了其对轨道确定精度的影响。结果表明,该文方法可有效估计在轨卫星星间链路天线相位中心偏差,并发现,卫星在轨后大部分卫星的星间链路天线相位中心偏差基本与地面一致,但C36, C37, C41, C42卫星在Z方向与地面标定值存在15 cm左右的偏差,C25, C26, C43, C44在Y轴上存在符号相反的现象,且数值上有10 cm左右的偏差,C25, C26卫星在Z方向上存在近30 cm的偏差,正确标定在轨卫星星间链路天线相位中心偏差后,相比地面标定产品,轨道精度可提升15%。 相似文献
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研究了一种考虑地面影响时准确计算鱼骨天线相位中心的方法。由于相位方向图的准确计算是准确提取相位中心的前提,所以我们按照鱼骨天线的施工结构建模,并采用矩量法(MoM)进行计算,保证了相位方向图计算的准确性。地面的影响会导致主瓣上翘,为了减小相位中心计算的误差,选择包含主瓣最大辐射方向的两个正交平面内的相位方向图来进行处理。然后,采用最小二乘法计算了天线的相位中心,并验证了其准确性。最后,给出了一种鱼骨天线的相位中心位置随频率的变化曲线,结果表明该鱼骨天线的相位中心位置随着频率的变化较为明显。 相似文献
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Self-survey calibration of meteor radar antenna arrays 总被引:1,自引:0,他引:1
Valentic T.A. Avery J.P. Avery S.K. Livingston R.C. 《Geoscience and Remote Sensing, IEEE Transactions on》1997,35(3):524-531
This paper presents the self-surveying technique for calibrating the antenna spacing, orientation, and phase errors in multiple receiver radar antenna arrays. Utilizing a set of source transmitters placed at known locations in the far-field of the array and measurements of the phase present at each antenna, the array's relative antenna locations and phase errors can be determined. The advantage of this technique is that the radar is used in its normal operating mode, providing an end-to-end calibration under true operational conditions. A self-survey calibration was performed with a meteor radar located at Sondre Stromfjord, Greenland, successfully mapping the array. The antenna positions were relatively close the expected locations, although the baselines were rotated approximately 5° from the true cardinal directions. The majority of the phase error was introduced by the receivers 相似文献
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A rigorous method is presented for calibrating polarimetric backscatter measurements of distributed targets. By characterizing the radar distortions over the entire mainlobe of the antenna, the differential Mueller matrix is derived from the measured scattering matrices with a high degree of accuracy. It is shown that the radar distortions can be determined by measuring the polarimetric response of a metallic sphere over the main lobe of the antenna. The radar distortions are categorized as distortions caused by the active devices or distortions caused by the antenna structure (passive). Since passive distortions are immune to changes once they are determined, they can be used repeatedly. The active distortions can be obtained by measuring the sphere response only at boresight, reducing the time required for calibration under field conditions. The calibration algorithm was applied to backscatter data collected from a rough surface. The results indicate that removal of the radar distortions from the cross products of the scattering matrix elements cannot be accomplished with traditional calibration methods 相似文献
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监测站是卫星导航系统的核心部分,提供给主控站的原始测量数据精度决定着整个导航系统的定轨与时间同步精度,影响着系统的服务性能。多径和天线相位中心的变化是监测站高精度测距不可忽略的影响因素。采用一套基于高增益、抗多径面天线的多径检测和校正系统,定量地评估监测站的多径环境,并对接收机天线的相位中心和多径进行校正。通过多径检测与校正原型设施,开展阵列天线相心标校、多径检测与标校等试验,为监测站的天线相心与多径环境检测、抑制和校正提供一个完整的解决方案。 相似文献