基于神经网络的激光陀螺误差测试与建模

用人工神经网络中的反向误差传播网络(BP网络)来建立温度补偿模型,通过训练后的BP网络对刻度因子误差以及随机漂移进行温度补偿。     

雷达信号处理MTI／MTD的性能分析和仿真研究

介绍了雷达信号处理技术中MTI/MTD的基本原理,对其性能进行了分析,研究了实现MTI/MTD的仿真方法,并在Simulink仿真平台上构建了MTI/MTD的仿真模型,最后给出了仿真结果。经分析可知,此仿真实现了雷达信号处理中的MTI/MTD,可为雷达系统建模仿真以及雷达信号处理技术和抗干扰技术的研究提供仿真支持。     

星载SAR多普勒频率计算与全零多普勒中心导引

讨论了在天线坐标系中多普勒频率的计算方法和全零多普勒中心的条件及其实现。证明对近圆轨道SAR卫星,采用与时间延迟积分-电荷耦合器件(TDI-CCD)空间相机相同的计算公式和偏流角补偿技术,能以偏航控制方式实现星载SAR的全零多普勒中心导引。由此可将回波多普勒中心频率的全球变化范围减至最小,显著降低了SAR成像处理的难度。研究具重要的应用价值。     

一种大频偏抗边带错锁的数字锁相环设计

在小卫星遥测系统中,地面站接收信号伴随着大多普勒频偏,副载波会落入主载波的多普勒频偏的范围之内,数字锁相环对主载波的跟踪必须避免边带错锁。提出一种新的数字锁相环结构,通过频谱分析辅助,初始频差和环路带宽被减小,副载波不会落入环路带宽之内;在环路中采用cic低通滤波下抽样滤除副载波分量,副载波对锁相环的影响得以消除。仿真结果表明,该锁相环在大频偏情况下能够很好地消除边带错锁。在实际的地面站遥测接收机中,该锁相环也能够很好地工作。     

星载ScanSAR天线指向稳定度对辐射校正的影响

基于均匀加权天线模型,推导星载ScanSAR天线指向不稳定引起的多普勒中心频率估计误差,建立多普勒中心频率估计误差与图像辐射校正精度之间的数学模型,进而提出星载ScanSAR辐射校正对天线指向稳定度的要求。最后,通过计算机仿真,验证了理论分析的正确性。     

利用BP网络校正跟踪接收机的相位漂移

针对跟踪接收机不同通道之间相位差的漂移问题,提出利用BP神经网络作为校正环节来消除此相位漂移。通过原理分析用数学方法描述跟踪接收机存在的相位漂移问题,介绍BP神经网络的网络模型和一种动态全参数自适应学习算法,进而提出基于BP神经网络的相位漂移校正算法。仿真结果表明,该方法的相位校正效果较好,不仅保证了系统的角跟踪精度,而且实现了高度的自动化。     

Using cross correlation to estimate Doppler frequency

Doppler frequency estimation with high accuracy is very important for precise orbit determination and scientific studies in deep space exploration. In this paper, we propose a new method which implements cross correlation of only received signals from one single station to estimate Doppler frequency. The algorithm is relatively simple and it can achieve high accuracy even when signal to noise ratio (SNR) is very low. Moreover, the accuracy can be further improved by implementing frequency compensation, especially when the frequency dynamic range is high. Simulations were performed and results proved the validity of this method. X-band observations on MEX (Mars Express) and Juno were performed by a 13 m telescope of Wuhan University, which was equipped by two back ends, i.e. CDAS (Chinese Data Acquisition System) and RSR (Radio Science Receiver). Raw data recorded by the CDAS were processed by using the proposed method, and the estimated frequencies were in good agreement with the real time frequency estimation values by the RSR. What’s more, the accuracy by using cross correlation was higher than the one of RSR.     

Integral inversion of GRAIL inter-satellite gravitational accelerations for regional recovery of the lunar gravitational field

We present an integral-based approach for high-resolution regional recovery of the gravitational field in this article. We derive rigorous remove-compute-restore integral estimators relating the line-of-sight gravitational acceleration to an arbitrary order radial derivative of the gravitational potential. The integral estimators are composed of three terms, i.e., the truncated integration, the low-frequency line-of-sight gravitational acceleration, and the high-frequency truncation error (effect of the distant zones). We test the accuracy of the integral transformations and of the integral estimators in a closed-loop simulation over the Montes Jura region on the nearside of the Moon. In this way, we determine optimal sizes of integration radii and grid discretisation. In addition, we investigate the performance of the regional integral inversion with synthetic and realistic GRAIL observations. We demonstrate that the regional inversion results of the disturbing gravitational potential and its first order radial derivative in the Montes Jura mountain range are less contaminated by high-frequency noise than the global spherical harmonic models.     

移位寄存器分析方法的研究

研究了串行输入 ,并行输出单向移位寄存器的功能。利用所提出的分析方法对移位寄存器进行的分析 ,揭示了移位寄存器内在的联系。     

Application of HF Doppler measurements for the investigation of internal atmospheric waves in the ionosphere

We present results of the spectral analysis of data series of Doppler frequency shifted signals reflected from the ionosphere, using experimental data received at Kazan University, Russia. Spectra of variations with periods from 1 min to 60 days have been calculated and analyzed for different scales of periods. The power spectral density for spring and winter differs by a factor of 3–4. Local maxima of variation amplitude are detected, which are statistically significant. The periods of these amplitude increases range from 6 to 12 min for winter, and from 24 to 48 min for autumn. Properties of spectra for variations with the periods of 1–72 h have been analyzed. The maximum of variation intensity for all seasons and frequencies corresponds to the period of 24 h. Spectra of variations with periods from 3 to 60 days have been calculated. The maxima periods of power spectral density have been detected by the MUSIC method for the high spectral resolution. The detected periods correspond to planetary wave periods. Analysis of spectra for days with different level of geomagnetic activity shows that the intensity of variations for days with a high level of geomagnetic activity is higher.