基于后向喇曼散射分布式光纤测温系统温度解调方法研究

 讨论了喇曼和瑞利散射光的温度效应。通过具体的理论分析,指出反斯托克斯散射光比斯托克斯散射光的温度灵敏度高,是此类系统解调温度信息的首选对象。详细讨论了 2种解调方法。通过分析对比它们在系统温度灵敏度、相对温度灵敏度与波长关系上的差异,得到了一系列有意义的结论。针对实际测量过程中光纤损耗因素,利用最小二乘法给出了一种“校正”算法。系统实践证明,上述结论是正确、合理的,校正算法是简洁、有效的。     

大气湍流对APD直接检测接收机抗噪声性能影响

针对以往分析湍流信道对系统抗噪声性能影响的不足,给出了一种基于APD直接检测接收机的湍流噪声的处理方法.在APD直接检测接收机模型的基础上,推导了其信噪比和曼彻斯特编码系统的差错概率,并详细分析了湍流对接收机的抗噪声性能影响.结果表明,增大接收天线孔径可以减弱湍流的影响,但在天线孔径较小时,增加发射功率并不能有效地提高...     

基于小生境遗传算法的分布式OS-CFAR检测系统优化与性能分析

 利用小生境遗传算法,对不同检测窗长度和检测信噪比的三传感器分布式 OS-CFAR检测系统进行了优化设计,给出了一组针对不同检测环境与融合方式的搜索结果。分析表明,对于非一致环境下分布式 OS-CFAR检测系统,小生境遗传算法是一种良好的优化算法。利用搜索结果,研究了不同融合方式下环境变化对分布式 OS-CFAR检测系统的性能影响,结果表明,“或”融合对检测环境的非一致变化具有较强的鲁棒性,而“3选2”融合和“与”融合对检测环境的变化比较敏感。     

基于拉曼散射的分布式光纤温度传感技术的研究

论述了基于拉曼散射的分布式光纤温度传感器的基本工作原理、结构、系统特点及信号处理方法。该结构及信号处理方法具有一定的空问分辨率，保证了系统的实用性。将分布式光纤传感器与传统的复用温度光纤传感器阵列进行了比较。通过使用分布式光纤温度传感器信号处理系统和信号处理软件相结合进行实验，得出结论。     

量化对GPS接收机捕获性能影响的研究

由于接收机输入端的信噪比对接收机的捕获性能具有很重要的意义,所以要尽量减少接收机输入端信噪比的损失。本文首先给出了含高斯白噪声的GPS信号经过不同量化位数和量化电平的量化器后的输出信噪比计算公式;然后,在此基础上分析其对接收机捕获性能的影响;最后,仿真实验表明,接收机可以在不影响捕获性能的情况下,尽量选择合适的量化位数和量化门限。实验结果也为量化器的设计提供了重要的技术参考。     

分布式光纤布里渊散射应变传感器参数计算

介绍了由布里渊散射机理构成的分布式光纤应变传感器,首次推导出了布里渊散射光相对于入射光的频移与光纤应变的关系及有关参数的理论计算公式。计算结果表明：光纤中由应变引起的布里渊频移变化主要是通过调制杨氏模量实现的;其布里渊频移为几十GHz,由应变引起的布里渊频移变化量为几十MHz.其理论与实验数据基本吻合。     

INS辅助GPS接收机及抗干扰能力的分析

针对高动态或低信噪比条件下GPS卫星信号容易失锁的特点,根据GPS接收机码／载波跟踪环特性,研究分析了惯性导航（INS）辅助GPS接收机原理及其抗干扰能力。在复杂电磁环境下,INS辅助GPS接收机（特别是紧耦合GPS/INS组合模式）是组合导航的发展方向。     

含能液滴微爆特性分析

借助高速摄影和热电偶测温系统研究了液体推进剂ＬＰ１８４６液滴在０．１ＭＰａ～１．０ＭＰａ,７００°Ｃ～８５０°Ｃ环境下的微爆特性。给出了液滴着火前微爆过程的序列照片,结合ＬＰ１８４６热分解试验结果分析了液滴微爆机理,认为水组份的过热是主要因素,而ＨＡＮ的微弱液相热分解是诱导因素。     

基于LEO辅助的北斗B1C高灵敏快速捕获算法

随着低轨(LEO)卫星数量的不断增加,利用LEO星座辅助增强GNSS导航性能已经成为一种新的趋势.针对低信噪比环境下B1C信号难以捕获的问题,提出了一种基于LEO辅助的B1C信号高灵敏快速捕获算法.首先对提升接收机捕获灵敏度进行了分析,对比了相干积分与非相干积分对于信号处理增益的影响,得出在低轨导航增强信号的辅助下采用增加相干积分时间的捕获算法对低信噪比条件下B1C信号的捕获更有效.然后提出了一种基于LEO辅助的B1C高灵敏快速捕获算法,从理论分析和实验仿真两方面,对比验证了在LEO辅助下可以显著提高B1C信号的捕获灵敏度,缩短捕获时间,提高捕获效率.     

基于波长控制的光纤陀螺标度因数温度性能提高方法

光纤陀螺的标度因数与光纤环的长度、直径及光源的平均波长有关。在温度条件下,光纤环的长度、直径及光源的平均波长均会发生变化,进而导致光纤陀螺在高低温下的标度因数不同,影响温度环境下的光纤陀螺标度因数的重复性。提出了一种基于光纤陀螺波长控制的标度因数温度性能提高方法,该方法在光源驱动电路的桥式回路中增加了铂电阻组件,从而可自动调节光纤陀螺光源的管芯温度,进而控制光源平均波长的变化,以抵消光纤环有效面积因温度变化而对标度因数产生的影响,提高温度环境下光纤陀螺的标度因数重复性。试验表明,该方法将未补偿情况下光纤陀螺全温范围内的标度因数重复性(1σ)由271×10-6~280×10-6减小到了32.5×10-6~43.5×10-6,标度因数重复性误差减小了84%~88%,并验证了该方法的有效性。     

Detection Performance of the Cell Averaging LOG/CFAR Receiver

The cell averaging LOG/CFAR receiver is a special implementation of a constant-false-alarm-rate (CFAR) receiver in which the noise level estimate is derived from a set of contiguous time samples of the output of a logarithmic (LOG) detector as obtained from a tapped delay line. This CFAR receiver is capable of operating over a larger dynamic range of noise levels than a conventional cell averaging CFAR receiver, but with somewhat poorer detectability. The performance in stationary Gaussian noise of the cell averaging LOG/CFAR receiver with no post-detection integration is determined in this paper. For a small number of reference noise samples, results were obtained by a Monte Carlo simulation using the technique of importance sampling. For a large number of reference noise samples, a second moment analysis gave the desired results. Both these results can be summarized in the following simple formula, NLOG = 1.65NLIN - 0.65, which relates the number of reference samples required by each of the two receivers for equivalent performance. Thus, for the cell averaging LOG/CFAR receiver to give the same detection performance as the conventional cell averaging CFAR receiver, the number of reference noise samples has to be increased by up to 65 percent.     

北斗导航接收机高增益相干积分算法

近年来,针对弱信号的高灵敏度接收机已逐渐成为国内外的研究热点。加长相干积分时间可以提高信噪比,从而跟踪到更弱的信号。但是,北斗导航接收机跟踪环路并不可以无限加长相干积分时间,相干积分时间的长短和功效还受到卫星导航电文比特跳变的限制。为了消除导航电文比特跳变对相干积分的影响,提出了一种改进的基于最大似然估计的北斗信号位同步方法,完成位同步后再利用先猜后检的方法便可以实现长相干积分。利用软件接收机进行编程设计,仿真结果表明：该长相干积分算法能够稳定可靠地实现对弱信号的跟踪,20ms相干积分环路信噪比约提升12dB,40ms相干积分环路信噪比约提升15dB,80ms相干积分环路信噪比约提升17dB,提高了北斗导航接收机的灵敏度。     

Doppler visibility of coherent ultrawideband random noise radar systems

Random noise radar has recently been used in a variety of imaging and surveillance applications. These systems can be made phase coherent using the technique of heterodyne correlation. Phase coherence has been exploited to measure Doppler and thereby the velocity of moving targets. The Doppler visibility, i.e., the ability to extract Doppler information over the inherent clutter spectra, is constrained by system parameters, especially the phase noise generated by microwave components. Our paper proposes a new phase noise model for the heterodyne mixer as applicable for ultrawideband (UWB) random noise radar and for the local oscillator in the time domain. The Doppler spectra are simulated by including phase noise contamination effects and compared with our previous experimental results. A genetic algorithm (GA) optimization routine is applied to synthesize the effects of a variety of parameter combinations to derive a suitable empirical formula for estimating the Doppler visibility in dB. According to the phase noise analysis and the simulation results, the Doppler visibility of UWB random noise radar depends primarily on the following parameters: 1) the local oscillator (LO) drive level of the receiver heterodyne mixer, 2) the saturation current in the receiver heterodyne mixer, 3) the bandwidth of the transmit noise source, and 4) the target velocity. Other parameters such as the carrier frequency of the receiver LO and the loaded quality factor of the LO have a small effect over the range of applicability of the model and are therefore neglected in the model formulation. The Doppler visibility curves generated from this formula match the simulation results very well over the applicable parameter range within 1 dB. Our model may therefore be used to quickly estimate the Doppler visibility of random UWB noise radars for trade-off analysis     

Bandwidth maximization for satellite laser communication

Free space optical communication between satellites networked together can make possible high speed communication between different places on Earth. The basic free space optical communication network includes at least two satellites. In order to communicate between them, the transmitter satellite must track the beacon of the receiver satellite and point the information optical beam in its direction. The pointing systems for laser satellite communication suffer during tracking from vibration due to electronic noise, background radiation from interstellar objects such as Sun, Moon, Earth, and Stars in the tracking field of view, and mechanical impact from satellite internal and external sources. Due to vibrations the receiver receives less power. This effect limits the system bandwidth for given bit error rate (BER). In this research we derive an algorithm to maximize the communication system bandwidth using the transmitter telescope gain as a free variable based on the vibration statistics model and the system parameters. Our model makes it possible to adapt the bandwidth and transmitter gain to change of vibration amplitude. We also present an example of a practical satellite network which includes a direct detection receiver with an optical amplifier. A bandwidth improvement of three orders of magnitude is achieved in this example for certain conditions, as compared with an unoptimized system     

Medium frequency broadcast of differential GPS data

The broadcast performance of DGPS (differential global positioning systems)/radio beacons is studied. It is found that a combination of receiver limiting and forward error corrections is very effective against the atmospheric noise which characterizes the MF band. This combination significantly reduces the probability of bit error and the average time between differential updates. The authors compute the probability of link outage versus range, and find that forward error correction significantly increases DGPS/radio beacon coverage. It is found that groundwave/skywave interference slightly increases the probability of outage at moderate ranges. An estimate is made of the expected duration of outage for the DGPS/radio beacon signal. All results are based on analytical and experimental results     

脉冲干扰下交错与FEC编码扩频系统性能的研究

推导了在脉冲干扰下无人机扩频遥测系统的误码率公式。提出了用吉尔伯特信道 ( Gi信道 )描述脉冲干扰下无交错编码的扩频系统的信道,用离散无记忆信道 ( DMC)描述脉冲干扰下的有交错扩频系统的信道。对比分析了脉冲干扰下的扩频系统采用 FEC前向纠错和不采用 FEC,以及采用 FEC与交错技术相结合3种情况时的系统误码率性能。最后通过数值计算分析,得到了一些有用的结论。所得公式和结论同样适用于部分频带干扰。     

Optimum transmitter optics aperture for satellite opticalcommunication

An important aspect in satellite optical communication is to obtain minimum bit error rate (BER) using minimum power. This aim can be achieved with very small transmitter beam divergence angles. The disadvantages of too narrow divergence angle is that the transmitter beam may sometimes miss the receiver satellite, due to pointing vibrations. A mathematical model of communication and tracking systems that optimize the BER as function of the transmitter gain is derived     

桨扇近场噪声的FFT算法

Hanson的升力而理论是进行桨扇近场谐波噪声预测的最有效的方法,在Hanson的原始公式中,对波数的无穷积分非常复杂。本文介绍一种利用快速傅立叶变换(FFT)计算Hanson公式的方法,通过一次FFT就可以得到平行桨扇轴线任一表面上的噪声分布。本文详细讨论了FFT算法的计算公式和计算中的技术问题。通过对桨扇噪声的实际计算表明,这种方法非常适应于桨扇噪声分布场的计算和分析,计算结果与实验值相符。     

统计推算燃烧室出口热点温度的优化方法

根据统计学原理 ,采用优化方法 ,对燃烧室在某一状态下出口截面温度的多点测量值进行数据处理 ,确定其最佳的威布尔分布方程 ,并进而导出该状态下出口热点温度的推算公式。结果表明 ,燃烧室出口截面上最大概率的最高温度值总是高于多点测量中测到的最高值。因此 ,通常把后者视同真实最高值 (热点温度 )是不恰当的。认识这一事实具有理论上和实践上的重要意义。