共查询到20条相似文献,搜索用时 781 毫秒
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众所周知,水下声信道是相干多途信道,信号在信道中的多径传播使得接收信号序列复杂化,因而极大地增加了信号处理的难度。对于水下目标跟踪系统,从带有干扰的接收数据中挑选出直达脉冲是系统正常工作的必要前提。本文着重介绍了系统软件的核心部分——专家系统,它用于实时跟踪系统的数据预处理,负责在多途干扰背景中提取定位解算所需的有效信息。通过计算机仿真、松花湖试验和海上试验的验证,专家系统可以准确地挑选出直达脉冲和最佳解算阵元,因而确保了系统的定位精度与测深精度。 相似文献
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This Letter presents two synchronization schemes between two different chaotic systems. Active control synchronization and adaptive synchronization between Chen system and Genesio system are studied, different controllers are designed to synchronize the drive and response systems, active control synchronization is used when system parameters are known; adaptive synchronization is employed when system parameters are unknown or uncertain. Simulation results show the effectiveness of the proposed schemes. 相似文献
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鉴于复杂大气条件下的红外系统作用距离难以精确、实时地计算,提出一种建立红外系统作用距离实时计算系统的方法。通过将MODTRAN软件与基于光谱等分法建立的红外系统作用距离模型有机地结合起来,实现对于MODTRAN软件自动写入配置及调用计算,简化了大气模型的配置方法,并能够自动读取MODTRAN生成的结果输出文件。对某探测目标在不同海拔高度(1 km~6 km)及不同降雨强度(0 mm/h~4 mm/h)下红外系统作用距离进行计算,结果表明:探测高度的变化对于红外系统作用距离有比较明显的影响,其中在1 km~3 km探测高度范围内,探测距离变化尤为明显。降雨对于红外系统作用距离影响巨大。降雨强度为1 mm/h时,红外系统作用距离衰减为无降雨时的50%。当降雨强度大于3 mm/h时,作用距离趋于稳定。 相似文献
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The Forschungszentrum Dresden-Rossendorf provides an intense pulsed 40 MeV electron beam with high brilliance and low emittance (ELBE). The pulse has a length of 1-10 ps and a repetition time of 77 ns, or in slow mode 616 ns. The EPOS system (ELBE Positron Source) generates by pair production on a tungsten converter and a tungsten moderator an intense pulsed beam of mono-energetic positrons. To transport the positrons to the laboratory (12 m) we constructed a magnetic beam guidance system with a longitudinal magnetic field of 75 G. In the laboratory outside the cave, the positron beam is chopped and bunched according to the time structure, because the very sharp bunch structure of the electron pulses is broadened for the positron beam due to transport and moderation. 相似文献
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A basic state and parameter estimation scheme for an extended excitable system is presented, where time series from a spatial grid of sampling points are used to drive and synchronize corresponding model equations. Model parameters are estimated by minimizing the synchronization error. This estimation scheme is demonstrated using data from generic models of excitable media exhibiting spiral wave dynamics and chaotic spiral break-up that are implemented on a graphics processing unit. 相似文献
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M. Lakshmanan 《Physics letters. A》1977,61(1):53-54
The continuum limit of a one-dimensional classical spins with nearest neighbour Heisenberg interaction is shown to be an exactly solvable system and that its dynamics describable by the nonlinear Schrödinger equation. N-soliton solutions for the energy density exist. 相似文献
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高速双光谱遥感图像传输系统 总被引:2,自引:0,他引:2
提出并设计了一种高速舣光谱遥感图像传输系统.对该系统所采用的传输策略,传输帧结构以及时序恢复等问题进行了深入的研究.首先,将双探测器一行数据中有效部分提取后传输,采用行有效标志中断发送的方式在接收端恢复时序,保证了系统输入输出数据、时序的完全一致;接着,采用发送与接收缓存机制,利用时分复用打法将双探测器的数据在单根光纤... 相似文献
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平流层飞艇通信系统载荷舱热控设计 总被引:1,自引:0,他引:1
分析了平流层飞艇通信系统的工作热环境.提出了以被动热控为主,主动热控为辅的载荷舱热控系统设计思路,给出了隔热、等温化、加热和液体循环回路等热控手段的具体设计方法. 相似文献
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干涉仪系统传递函数能有效地表征系统相位成像的性能。通过假设干涉成像系统是复振幅的线性平移不变系统,模拟计算正弦相位光栅和相位台阶这两类标准相位物体的成像,确定干涉仪系统传递函数。数值分析结果表明:系统传递函数随着波像差的增加而减小;干涉成像系统对小幅度相位(远小于1 rad)成像是近似线性的,而对大幅度相位(大于0.5 rad)成像则是明显非线性的。当正弦相位的幅度为1时,系统传递函数在1/2和1/3截止频率处出现明显的急剧下降。高度为/2的相位台阶成像时,系统传递函数随着空间频率的增加而缓慢地降低。 The performance of phase imaging in interferometric imaging system is well characterized by the system transfer function (STF). The STF of the interferometric imaging system is analyzed numerically by assuming that the system is linear and shift-invariant for the complex field. Two standard phase objects, sinusoidal phase grating and phase step, are employed and simulated to determine the STF. Numerical simulation results show that the STF decreases as the wavefront aberration of interferometric imaging system increases. It also shows that the interferometric imaging system is approximately linear for small phase (far less than 1 rad) but explicitly nonlinear for large phase (larger than 0.5 rad). The STF has a visible drop at one half or one third of the cut-off frequency of the imaging system when the amplitude of sinusoidal phase is 1 rad. For a phase step with a height of /2 rad, the STF has no visible drop but decreases slowly with the increasing of spatial frequency. The results provide a useful guidance to the design of interferometer and the measurement of STF and power spectrum density in experiment. 相似文献