一种基于分组截短PN码的SOFDM信道估计方法

基于PN序列的信道估计方法的特点是计算过程简明,已被广泛应用在地面无线局域网系统中。在卫星正交频分多路复用传输体制(SOFDM)系统中引入传统PN序列信道估计方法的主要问题在于卫星信道的多径延时远大于SOFDM数据符号的持续时间,信道特性比较复杂,使得传统方法的估计精度严重下降。提出了一种改进的方法,根据信道的近似周期特性对数据帧进行合理的等长度分组,并把长PN序列改为短PN码来跟踪信道局部特性的变化,再对分组后的数据子帧分别进行信道估计。对该方法的设计思想进行了理论分析,并通过仿真验证了该方法的估计精度比传统方法至少提高了10倍。     

Prospects in the orbital and rotational dynamics of the Moon with the advent of sub-centimeter lunar laser ranging

Lunar laser ranging (LLR) measurements are crucial for advanced exploration of the laws of fundamental gravitational physics and geophysics as well as for future human and robotic missions to the Moon. The corner-cube reflectors (CCR) currently on the Moon require no power and still work perfectly since their installation during the project Apollo era. Current LLR technology allows us to measure distances to the Moon with a precision approaching 1 mm. As NASA pursues the vision of taking humans back to the Moon, new, more precise laser ranging applications will be demanded, including continuous tracking from more sites on Earth, placing new CCR arrays on the Moon, and possibly installing other devices such as transponders, etc. for multiple scientific and technical purposes. Since this effort involves humans in space, then in all situations the accuracy, fidelity, and robustness of the measurements, their adequate interpretation, and any products based on them, are of utmost importance. Successful achievement of this goal strongly demands further significant improvement of the theoretical model of the orbital and rotational dynamics of the Earth–Moon system. This model should inevitably be based on the theory of general relativity, fully incorporate the relevant geophysical processes, lunar librations, tides, and should rely upon the most recent standards and recommendations of the IAU for data analysis. This paper discusses methods and problems in developing such a mathematical model. The model will take into account all the classical and relativistic effects in the orbital and rotational motion of the Moon and Earth at the sub-centimeter level. The model is supposed to be implemented as a part of the computer code underlying NASA Goddard’s orbital analysis and geophysical parameter estimation package GEODYN and the ephemeris package PMOE 2003 of the Purple Mountain Observatory. The new model will allow us to navigate a spacecraft precisely to a location on the Moon. It will also greatly improve our understanding of the structure of the lunar interior and the nature of the physical interaction at the core–mantle interface layer. The new theory and upcoming millimeter LLR will give us the means to perform one of the most precise fundamental tests of general relativity in the solar system.     

亚像素条纹边缘提取技术在型面测量上的应用

三维型面非接触测量在工业领域有着广泛的应用前景.双目视觉是一种有效获取三维轮廓信息的方法,其中对大密度的黑白相间条纹进行精确定位和提取,是基于投影光栅图像的光学三维型面测量的关键技术和难点.利用空间编码技术将被测空间划分为若干区域,每个区域对应一个二进制码.条纹落在区域上与唯一的二进制码相对应,就可以对条纹精确定位.利用边缘提取算法获得像素级条纹后,再利用亚像素技术可以进一步对条纹进行高精度提取.介绍了基于灰度矩的和基于多项式拟合的亚像素边缘检测算法.将空间编码和亚像素条纹提取技术相结合,对光栅条纹进行亚像素级定位和提取的技术,与像素级的定位技术相比,能提高图像的定位精度,有效地改善测量系统的性能.      

MC-CDMA中的RLS-DRMTA算法

多载波码分多址(MC-CDMA)系统是将OFDM技术与CDMA技术结合起来的一种综合技术.MC-CDMA系统中同信道干扰仍然是影响系统性能的主要因素,这就需要使用智能天线来提高系统的性能.介绍一种适用于MC-CDMA系统的自适应阵的盲算法递推最小二乘解扩重扩多目标阵列(RLS-DRMTA)算法,利用扩频码的信息进行波束形成,不需要训练序列,节约了频谱资源;与LS-DRMTA算法相比,RLS-DRMTA算法节省了运算时间;另外仿真表明在正交频分复用(OFDM)解调后进行波束形成,提高了系统的性能;为了降低系统的复杂度,还用到了载波分组技术,但分组技术又会降低系统的性能,所以分组时考虑了系统性能和运算速度的折衷.仿真结果表明RLS-DRMTA算法能使方向图的主波束对准信号方向,而在干扰方向形成零陷,从而达到抑制干扰的目的.      

Influence of atmospheric turbulence on planetary transceiver laser ranging

In this paper we investigate the influence of atmospheric turbulence on the performance of the uplink of a planetary transceiver laser ranging system using a single photon detector. We numerically combine the influence of turbulence in the mean intensity profile variations, scintillation, beam-wander induced pointing errors and stochastic time-of-flight variations, using the Hufnagel–Valley turbulence profile to model the ground turbulence behavior. We map the intensity variations due to turbulence to variations in the probability distribution of the arrival time of the 1st photon in a laser pulse, which influences the range measurement error probability distribution. The turbulence models are applied to assess the influence on single-pass range accuracy and precision statistics, as well as the parameter estimation quality of a Phobos Laser Ranging (PLR) mission.     

基于广义相对论的轨道摄动下星间激光相位比对

针对纳米到皮米量级星间激光测距,在地心非旋转坐标系(GCRS)下,考虑卫星轨道摄动引起的广义相对论效应,建立了星间单向以及双向星间激光相位比对模型.通过仿真研究了地球主引力场范围内轨道摄动引起的广义相对论效应对星间激光相位比对误差的影响,并通过星间激光相位比对误差计算星间激光测距误差.不同轨道高度的卫星仿真结果表明,对...     

航天器C语言软件常见编程错误分析及检测方法研究

基于软件第三方评测发现的问题,梳理并详细分析了在航天器C语言软件中6种常见编程错误.针对其中的软件安全漏洞提出了使用代码分析技术的检测方法,针对编程语言使用错误提出了通过制定编程规则并使用代码分析方法进行检测的解决方法.采用上述方法可以有效检测出上述6种常见编程错误,并可以用于检测软件的其他严重错误.     

同时纠检错时某些线性分组码的不可检错误概率

研究同时纠错和检错时，线性分组码的不可检错误概率，证明了二元完备码及其扩展码是最佳纠检错码，而某些ＢＣＨ码不是最佳纠检错码。     

Estimation and analysis of GPS receiver differential code biases using KGN in Korean Peninsula

The total electron content (TEC) estimation by the Global Positioning System (GPS) can be seriously affected by the differential code biases (DCB), referred to as inter-frequency biases (IFB), of the satellite and receiver so that an accuracy of GPS–TEC value is dependent on the error of DCBs estimation. In this paper, we proposed the singular value decomposition (SVD) method to estimate the DCB of GPS satellites and receivers using the Korean GPS network (KGN) in South Korea. The receiver DCBs of about 49 GPS reference stations in KGN were determined for the accurate estimation of the regional ionospheric TEC. They obtained from the daily solution have large biases ranging from +5 to +27 ns for geomagnetic quiet days. The receiver DCB of SUWN reference station was compared with the estimates of IGS and JPL global ionosphere map (GIM). The results have shown comparatively good agreement at the level within 0.2 ns. After correction of receiver DCBs and knowing the satellite DCBs, the comparison between the behavior of the estimated TEC and that of GIMs was performed for consecutive three days. We showed that there is a good agreement between KASI model and GIMs.     

利用有限域上的辛几何构作一类Cartesian认证码

利用了有限域上的辛几何构造了一类Cartesian认证码，并且计算了其参数及模仿攻击成功的概率和替换攻击成功的概率．