紫外光通信调制方式的对比研究

分析了启闭键控调制(OOK)、脉冲位置调制(PPM)、差分脉冲位置调制(DPPM)和数字脉冲间隔调制(DPIM)的编码结构,然后从带宽需求、平均发射功率、传输容量和差错性能等方面对各种调制方式进行了仿真对比。结果表明,DPIM调制比PPM具有更高的传输容量和更少的带宽需求,并且解调对同步要求较低,实现更简易,并结合紫外LED阵列将作为今后实用化紫外光源的发展趋势,DPIM调制在未来紫外光通信系统的应用中将具有更大的优势。     

光通信 其他

TN929.132006010667空间光通信PPM信号的软解调及其性能=Soft demodu-lation&performance of PPMinfree-space optical commu-nications[刊,中]/张江鑫(浙江工业大学信息学院,浙江省光纤通信技术重点研究实验室.浙江,杭州(310032)),胡宏飞∥光电子技术与信息.—2005,18(4).—42-46对光PPM信号的解调进行了分析,提出了PPM信号的软解调而不对脉冲位置作先期判决,并对软解调及其性能进行了分析,最后利用计算机对用APD接收且存在热噪下的空间光通信PPM信号的解调进行了模拟仿真。仿真结果说明软解调由于充分利用了光电探测器计数软信息…     

S/X波段低损耗波导真空窗技术研究

低损耗波导真空窗具有优异的微波特性和真空密封性能,是高灵敏度致冷接收机的关键部件.文中介绍了波导真空窗的工作原理和应用场合,给出了详细的设计模型和性能指标.     

光通信数字接收中位同步信号的智能提取

在光通信数字接收机中,为了达到系统的位同步,结合数字锁相环的基本原理,采用现场可编程技术,设计了位同步信号的时序逻辑电路,并用FPGA芯片实现了整个位同步电路.通过单片机实时控制FPGA,进行频带宽度和中心频率的实时调节,实现了位同步信号的智能提取.仿真分析和实际测试表明,该系统具有实时跟踪,提取快速且稳定,抗干扰能力强,升级方便等特点.     

大气弱湍流下星地光链路衰落特性影响因素分析

研究了弱湍流条件下星地光通信链路的衰落概率、平均衰落次数以及平均衰落时间3个重要参数的统计特性,并通过数值仿真分析了链路天顶角、光波长以及接收机海拔高度对链路衰落特性的影响。结果表明:减小天顶角和提高接收机探测灵敏度可以改善链路的衰落特性;1.55 m激光较0.85 m、1.06 m激光更适合于星地光通信;地面接收机应尽量建在2 000 m以上的高海拔地区。     

大气湍流光PPM通信系统中LDPC码的置信传播译码

对大气弱湍流光PPM通信系统中LDPC码的BP 解码算法进行了研究,提出了相应系统模型下的解码算法.通过理论分析和大量计算机仿真,结果表明:采用LDPC的大气弱湍流光PPM通信系统比未编码的大气弱湍流光PPM通信系统的性能好,但是系统的BER性能随着PPM的时隙数的增加而增大.     

基于扩展卡尔曼的PDM-16QAM偏振态和载波相位快速跟踪

在偏振复用(PDM)高速光通信系统的相干检测中,需要实现信号偏振态和载波相位的快速跟踪。将扩展卡尔曼滤波器用在偏振复用16进制正交振幅调制(PDM-16QAM)光调制信号相干接收机中,成功实现了偏振态和载波相位的快速精确跟踪。在单信道112Gb/s PDM-16QAM传输系统中,数值仿真发现,扩展卡尔曼滤波器所能跟踪的最大偏振态旋转速率可达级联多模算法的100倍,而且具有很好的收敛精度,其收敛速度和精度可以通过调优参量控制。使用扩展卡尔曼滤波器跟踪100kHz线宽18 Mrad/s偏振态旋转信号时,10-3误码率(BER)对应的接收机灵敏度代价仅为0.2dB。研究了应用于长距离传输光通信系统的扩展卡尔曼相干接收的性能。     

多调制方式下的强度叠加编码多发多收大气光通信系统性能分析

对开关键控(OOK)、脉冲位置调制(PPM)、差分脉冲位置调制(DPPM)和数字脉冲间隔调制(DPIM)下强度叠加编码多发多收(MIMO)光通信系统的性能进行了比较分析。研究表明:随着调制阶数的提高,后三种调制在平均发射功率需求方面较OOK调制有很大优势,但是相应的传输容量却有所下降。在差错性能方面,OOK调制在接收功率较低时误包率相对其它三种调制要小,当接收功率提高到一定程度时,PPM,DPPM和DPIM调制相对OOK调制均体现出了3～10dB的误包率优势。     

无线光通信新型组合脉冲调制性能分析

调制技术是影响无线光通信质量的重要因素之一,探索合适的调制方式是无线光通信的内在需要,为此,全面深入分析不同新型组合脉冲调制的性能。详细地分析了脉冲位置调制(PPM)和数字脉冲间隔调制(DPIM)等传统调制方式,以及脉冲位置宽度调制(PPWM)、差分脉冲位置宽度调制(DPPWM)、双幅度脉冲位置调制(DAPPM)和双幅度脉冲间隔调制(DAPIM)等新型组合调制方式的符号结构;全面比较了以上调制方式的平均发射功率和带宽需求;在给定模型下分析了它们的差错性能。数值结果表明:DAPPM的功率利用率最好,DPPWM的功率效率最低。当二进制比特位M取一定值时,PPM的带宽利用率最低,DPPWM的带宽利用率最高;随着M的增加,DAPPM的带宽效率与DPIM的带宽效率非常接近。而从差错性能看,在相同的信噪比RSN条件下,当M取值一定时,DAPPM的误包率与PPM接近,均优于其他组合调制方式,随着M或RSN增大,系统误包率逐渐减少;同时,通过增大PPWM的r参数、减少DAPPM的α参数,可适当改善差错性能。因此,要根据实际系统的要求选择合适的调制方式。     

激光器自发辐射噪声对混沌光通信系统的影响

构建了基于外光反馈的混沌光通信系统模型, 通过引入Langevin噪声源, 建立了包含自发辐射噪声特性的主从式速率方程. 利用所得数学模型, 研究了系统中可能存在的两类同步:全混沌同步和普通注入锁模型混沌同步; 分析了两端激光器自发辐射噪声对此二类同步以及系统收发两端混沌信号的影响; 最后,以2.5Gb/s伪随机数字调制下的混沌掩蔽方式为例,介绍了系统的加/解密过程以及噪声对系统解码性能的影响. 关键词： 混沌光通信 外光反馈 光注入 混沌同步 自发辐射噪声     

基于UVC LED的小型化紫外无线通信技术

紫外光通信技术具有低窃听、低位辨、全方位、全天候、抗干扰等优点,而基于紫外光灯的通信系统存在光源体积大、易碎、调制困难、通信速率低、功耗大等问题。设计了一种基于紫外C波段(UVC)LED的小型化无线通信系统方案,并对系统性能进行了理论分析。系统光源采用UVC LED,探测器采用日盲光电倍增管(PMT)和窄带紫外滤光片,通信系统采用开关键控(OOK)和脉冲位置调制(PPM)调制方案。仿真结果表明所设计的紫外无线通信系统可在200mW发射光功率情况下实现直径200m范围内的非视距语音通信和100mW发射光功率情况下实现250m的64Kbps准视距通信。     

Analysis of telescope array receivers for deep-space inter-planetary optical communication link between Earth and Mars

Optical communication technology shows promising prospects to fulfill the large bandwidth communication requirements of future deep-space exploration missions that are launched by NASA and various other international space agencies. At Earth, a telescope with a large aperture diameter is required to capture very weak optical signals that are transmitted from distant planets and to support large bandwidth communication link. A single large telescope has the limitations of cost, single point failure in case of malfunction, difficulty in manufacturing high quality optics, maintenance, and trouble in providing communication operations when transmitting spacecraft is close to the Sun. An array of relatively smaller-sized telescopes electrically connected to form an aggregate aperture area equivalent to a single large telescope is a viable alternative to a monolithic gigantic aperture. In this paper, we present the design concept and analysis of telescope array receivers for an optical communication link between Earth and Mars. Pulse-position modulation (PPM) is used at the transmitter end and photon-counting detectors along with the direct-detection technique are employed at each telescope element in the array. We also present the optimization of various system parameters, such as detector size (i.e., receiver field of view), PPM slot width, and the PPM order M, to mitigate the atmospheric turbulence and background noise effects, and to maximize the communication system performance. The performance of different array architectures is evaluated through analytical techniques and Monte-Carlo simulations for a broad range of operational scenarios, such as, Earth-Mars conjunction, Earth-Mars opposition, and different background and turbulence conditions. It is shown that the performance of the telescope array-based receiver is equivalent to a single large telescope; and as compared to current RF technology, telescope array-based optical receivers can provide several orders of magnitude greater data rates for deep-space communication with Mars.     

大功率LED脉冲位置调制解调设计

脉冲位置调制是室内可见光通信的主要调制方式之一,它具有功率利用率高,频带利用率好,抗干扰性强的特点.为实现室内大功率白光LED照明通信,在分析PPM的原理基础上提出了一种改进的调制方式,给出了这种PPM符号的结构,并设计了大功率LED的驱动电路.其主要特点是由单片机直接输出帧同步信号加PPM信号,不设置保护时隙,其利用...     

All optical alternative approach of conducting NAND and NOR logic gates with phase encoding principle

All optical logic gates are the most important building blocks for conducting all optical digital and analog signal processing and computing. It has several uses in the high speed communication system. In last few years various non-linear properties of semiconductor optical amplifier have been utilized for realization of all optical logic gates exploiting different type's optical modulations. In such connection optical phase encoding technique drew more attention in last few years as it shows higher receiver sensitivity and extended tolerance limit in long-haul fiber transmission systems. In this communication the authors have proposed an alternative approach for conducting all optical logic gates with phase encoded inputs by the exploitation of the four wave mixing (FWM) property in semiconductor optical amplifier (SOA).     

二级级联式室内可见光通信光学接收天线设计

针对室内可见光通信系统的传统光学接收天线无法同时满足高增益和大视场的问题, 设计了一种二级级联式光学天线. 通过分析信噪比、通信速率与接收天线视场角的关系, 发现视场角为40°–60°的光学天线最适用于室内可见光通信系统. 通过光学仿真软件TracePro的模拟及计算, 给出了所设计的二级级联式光学天线的增益随信号光入射角的变化关系. 结果表明, 相较于传统接收天线, 二级级联式光学天线具有更好的光学性能, 视场角为菲涅耳透镜单独接收时的4 倍. 利用Matlab对二级级联式光学天线竖直向上时的接收功率分布进行仿真, 结果显示探测器接收到的信号功率提升效果明显, 平均值较直接探测时增大了7 dBm, 进一步证实该二级级联式光学天线适用于室内可见光通信系统.     

Noise performance of an InP/InGaAs superlattice avalanche photodiode

The noise performance of an InP/InGaAs Superlattice Avalanche Photodiode (SL-APD) has been studied theoretically to examine its suitability as a detector in optical receiver units. The results indicate that the device which has a very large gain-bandwidth product (450 GHz) provides a high receiver sensitivity compared to conventional APD. The device also exhibits a very low value of excess noise factor which results in a high value of signal-to-noise ratio. The SL-APD is expected to find useful applications as a high sensitivity photodetector in long-haul fibre optic communication systems. For a digital system, the device exhibits a very low value of bit-error rate (BER) even at moderate gain.     

A simplified approach to digital optical receiver design

A simplified theory for the performance of a digital optical receiver is developed. The receiver sensitivity is calculated in terms of circuit parameters, received and equalized pulse shapes, photodiode parameters and bit-rate. An excellent agreement between this theory and a more complicated analysis by Personick [4] is demonstrated. It is shown that the receiver sensitivity may be improved by launching reduced-width pulses into the fibre, particularly if fibre bandwidth is a significant limitation. Reduced-width pulses bring benefits in source power consumption and lifetime, and in timing recovery.     

室内可见光通信复合光学接收端设计与分析

本文提出了一种适用于室内可见光通信的新型光学接收端的设计.根据复合抛物面聚光器的聚光特性,将光电探测器与复合抛物面聚光器耦合作为接收子单元,并将这些接收子单元按照特定的几何关系嵌入一个半球面中,得到角度分集型的复合光学接收端,达到水平方向360°,垂直方向180°的大视场.对每个接收单元接收到的光能量,低传输数据时进行相加求和作为最终的接收功率,高数据速率时取各个子单元的最大值作为接收功率.在一个5 m×5 m×3 m的空旷房间中,通过MATLAB对室内可见光通信系统建模仿真.计算结果表明,采用这种复合型光学接收端后,两种不同处理算法下的接收功率相对于直接接收分别提高了11.85和7.47 dB,增益分别为15.31和5.98.信噪比较高,两种情况下的平均值分别为79.17和72.26 dB,且接收信噪比分布平缓,波动较小.这说明采用本文设计的光学接收端,不仅能够得到较大的接收端视场角,同时获得较高的增益和接收功率,以及稳定的接收信噪比,避免了室内可见光通信系统中通信盲区的存在,保证了室内通信性能的稳定性.