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卫星振动对星间光码分多址系统性能的影响 总被引:2,自引:2,他引:0
卫星振动是影响星间光CDMA通信系统性能的一个重要因素.考虑多用户干扰、背景光噪音、热噪音、接收机噪音和卫星振动,给出了基于PPM信号格式的星间二维光CDMA通信系统的系统模型.采用数值分析的方法,详细分析了卫星振动对该系统误码率性能的影响.结果表明,码速率、通信波长和卫星振动都会影响星间二维光CDMA通信系统的误码率性能.当卫星振动标准偏差σ≤4×10-7时,卫星振动对系统误码率性能的影响较小;当卫星振动标准偏差σ≥1.2×10-6,卫星振动对系统误码率性能的影响很大,得到的误码率难以满足系统的通信要求,需要采用卫星振动抑制或补偿等技术提高星间二维光CDMA通信系统的误码率性能. 相似文献
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Influence of satellite vibration on optical communication performance for intersatellite laser links
For intersatellite laser links, vibration-induced pointing jitter severely influences the communication quality as a result
of intensity fluctuation. In this paper the probability density function of normalized intensity at the receiver is derived
in the presence of pointing jitter taking consideration of bias error. Accordingly, the scintillation index is developed to
identify the impact of bias error on intensity fluctuation. Furthermore the bit error rate (BER) is obtained as a function
of the beam divergence angle and vibration variance. Qualitative analysis is also given, and the numerical simulation is carried
out for demonstration. Results suggested that bias error has a significant detrimental impact on optical terminals which should
be considered in system design. This work can benefit the intersatellite optical system design. 相似文献
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在恒星辐照度谱模型的基础上,根据卫星轨道理论及恒星数据库建立仿真实验系统,对低轨卫星与中继卫星间(LEO_GEO)、中继卫星间(GEO_GEO)、低轨卫星间(LEO_LEO)三种典型的星间激光链路进行了仿真研究,深入分析了恒星背景噪声对卫星光通信终端跟瞄子系统的影响规律、背景光功率等特性。仿真结果表明:对于视场较大的LEO终端,恒星进入视场的概率约为7%~10%,而对于视场较小的GEO终端,恒星进入视场的概率仅为0.05%,恒星背景光功率约为10-13~10-11W。该项工作对星间激光链路设计、光通信系统参数优化等工作具有一定指导意义。 相似文献
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In this paper, we analyze the outage probability of the radio over intersatellite optical wireless communication system in the presence of satellite vibration with bias error. The lower-based Mach–Zehnder modulator, optical booster amplifier and optical preamplifier are employed. First, the models of the proposed system and channel are given. Then the outage probability for a given bit error ratio (BER) of a quadrature phase shift keying signal is obtained in the presence of satellite vibration with bias error. Numerical results of outage probability with different bias error and average BER are given. Results indicate that the outage probability is obviously influenced by the pointing error and the optimum telescope diameter to minimize the outage probability exists. With the same pointing error condition, the value of the optimal telescope diameter will increase with the reduction of the given average BER. 相似文献
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1 Introduction Forveryhighdatarates,intersatelliteopticalcommunications (IOC)holdapotentialperformanceedgeovermicrowave (RF )communicationsintermsofhigherdatarates,smallerantennasandlow probabilityofjammingandintercept[1] .WiththewidedevelopmentofIOCtechnol… 相似文献
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In this paper, a theoretical model of the acquisition in intersatellite optical communications (IOC) is founded with the assumption that beacon pointing errors could be modeled as Gaussian random variables. An optimal scan method should be chosen according to the average acquisition time under a certain acquisition probability. With analysis of the most common scan methods during the establishment of IOC, the raster-spiral scanning can substitute the spiral scanning is found. The raster scanning and raster-spiral scanning are simulated using Monte Carlo method and the result shows the first one is optimal for acquisition in IOC. 相似文献
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This work is motivated by the need to achieve the Shannon channel capacity for intersatellite optical communication with intensity modulation and direct detection. In this paper, we investigate the tradeoff between the channel capacity and the outage probability in the presence of random pointing jitter for intersatellite optical links. First, we derive an analytical expression of the outage probability in the absence of bias error, and then the bias error is taken into account. By minimizing the outage probability, we obtain analytically the optimum design of the beam half-width divergence angle $ w_0^{\text{opt}} $ for a given channel code rate. Furthermore, we discuss the tradeoff between the outage probability and the channel capacity and illustrate the results by adopting $ w_0^{\text{opt}} $ in the presence of random pointing jitter. The results obtained are useful for the parametric-estimation optimization of intersatellite optical communication systems. 相似文献
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空地激光通信跟踪精度主要外界影响因素研究 总被引:7,自引:5,他引:2
为了分析空地激光通信外界因素对跟踪精度的影响情况,将平台振动、大气湍流和背景光三个主要影响因素归结到对跟踪精度影响的统一框架下进行了研究。使用实际测量得到的平台振动数据,建立空地激光通信跟踪仿真系统,分析了不同条件下,三种外界因素对跟踪精度的综合影响情况。在文中假设基础上,分析可知:粗跟踪单元可以较好的抑制地面运动平台的振动,保证激光能够进入精跟踪视场;中强度的湍流使精跟踪残差标准差增大4倍左右,如果试验地点选择在高海拔地区,大气湍流使精跟踪残差标准差增大2倍左右。 相似文献
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空间光通信中基本振动对误码率的影响分析 总被引:1,自引:0,他引:1
在探讨卫星振动对空间光通信系统误码率所产生的影响时,有必要分析不同振动类型的影响问题。为了使讨论简单,本文主要侧重对正弦振动进行分析。分析结果表明,当振动持续时间为整周期时,误码率仅为振幅的函数,此时误码率随振幅的增加迅速上升,而与振动频率无关;当振动持续时间为非整周期时,误码率随时间的增加而波动,波动的起伏逐渐减小,误码率趋于仅与振幅有关的常数。该项工作为今后研究卫星复杂振动对空间光通信的影响打下了基础,同时也为研究对卫星振动影响的补偿分析提供了有意义的参考 相似文献
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光栅耦合结构的半导体激光器在自由空间光通信、卫星间通信、激光雷达测距、大气环境检测以及医学成像等领域有着广泛的应用前景。为了分析光栅耦合结构的半导体激光器的可靠性,本文基于拉曼光谱技术,对光栅耦合结构的半导体激光器在不同的制备阶段及其成品进行了检测。我们发现,对于未进行任何工艺加工的半导体激光器芯片,GaAs纵向(LO)光学光子模式的振动强而横向(TO)光学光子模式的振动弱;当在GaAs芯片表面生长一层SiO2膜后,LO模式向长波数方向移动,强度没有变化。当在生长SiO2膜的GaAs芯片上刻蚀100 μm的台面后,GaAs的LO模式的振动减弱而TO模式的振动加强,且峰出现宽化现象;在100 μm的台面上刻蚀光栅后,GaAs的LO模式的振动继续减弱而TO模式的变得更强,这说明在光栅耦合激光器的制备工艺过程中引入了缺陷。通过与无光栅的半导体激光器进行对比测试,光栅耦合结构半导体激光器无论出光面上有无缺陷,其拉曼光谱均有缺陷峰存在,进一步证明了在光栅结构的制备过程中,引入了应变或者缺陷,对其可靠性产生了影响,导致光栅耦合结构的半导体激光器可靠性降低。 相似文献
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Coupling a single-mode laser diode with 200 mW to a single-mode fiber (SMF) through an orthonormal aspherical cylindrical lens and a GRIN lens for the intersatellite optical communication system is proposed and demonstrated. We experimentally studied how the coupling efficiency changes with the SMF's position displacement and axial angle variation, and obtained 80 mW output power at the end of the SMF, which shows that the coupling units have satisfied the designed request. 相似文献
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The high precision calibration of optical trap stiffness is the foundation of the weak force measurement in an optical tweezers system. And the accuracy of the trap stiffness measurement is limited by the bandwidth of the acquisition system. In this article, such an influence is analyzed and discussed. The stiffness measuring process using an acquisition system with a finite acquisition time is numerically simulated by using Monte-Carlo method. Then the simulated results are analyzed by thermal motion analysis method to deduce the trap stiffness for different trapping system and for measuring systems with different acquisition time. As a comparison the power spectrum analysis method is used to study the thermal motion of the bead and to compute the trap stiffness for the same acquisition system, from which it is concluded that the bandwidth of the acquisition system is determined by its acquisition time, not the sampling frequency. The influence of the finite acquisition time or the limited bandwidth on the trap stiffness measurement is discussed. The numerical simulation shows that the measured position, which is here the average position within the acquisition time, shifts to the trap center due to the trapping force, which gives an alternative interpretation for the deviation of the measured stiffness from the true trap stiffness. 相似文献
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将激光信号与高帧频CCD结合,解决了光学系统中振动信号和激光信号之间的转换问题,不仅能够测量振动对系统光束指向稳定性的影响,而且能够得到振动信号本身的频率特性。利用该方法对振源为150 Hz和200 Hz两种条件下的光学系统受迫振动进行测量,得到了与输入信号相吻合的振动信号属性。通过实验与分析得知:时域振幅测量精度为6.25 m,频域分辨力为2 Hz,方法简便高效,测量结果准确,已应用于角多路准分子激光主振荡功率放大器系统打靶试验平台光束指向稳定性的研究中。 相似文献
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