毫米波/红外复合制导半实物仿真关键技术研究

对毫米波/红外复合制导的半实物仿真进行了研究,给出了仿真系统的总体方案,引入毫米波/红外双波束合成器以实现真正意义的复合制导仿真.对毫米波目标的模拟仿真、红外目标的模拟仿真以及双波束合成器等系统关键技术进行了重点分析和阐述,提出了利用分形频率选择表面实现双波束合成器的方法,给出了具体设计实例,仿真和实测结果表明该波束合成器对毫米波信号的透射性能稳定,对长波红外信号的反射率平均保持在85%,并对8mm和3mm毫米波/红外复合制导体制均适用.     

模拟旋转内冷通道中压力测量的实验研究

在旋转内冷通道中,用压力传感器测量垂直于旋转轴的矩形管道充动气体的压力分布,实验结果表明：（１）在同一半径处,转速增加引起压差减少,（２）在转速较低时随着半径增大,压差减小,但转速较大,总的压差反而随着半径增大而增大,（３）流体管道中的扰流柱起着增另气流紊流的作用,导致压力损失增大,压降增大。     

Proton lateral broadening distribution comparisons between GRNTRN,MCNPX, and laboratory beam measurements

Recent developments in NASA’s deterministic High charge (Z) and Energy TRaNsport (HZETRN) code have included lateral broadening of primary ion beams due to small-angle multiple Coulomb scattering, and coupling of the ion-nuclear scattering interactions with energy loss and straggling. This new version of HZETRN is based on Green function methods, called GRNTRN, and is suitable for modeling transport with both space environment and laboratory boundary conditions. Multiple scattering processes are a necessary extension to GRNTRN in order to accurately model ion beam experiments, to simulate the physical and biological-effective radiation dose, and to develop new methods and strategies for light-ion radiation therapy. In this paper we compare GRNTRN simulations of proton lateral broadening distributions with beam measurements taken at Loma Linda University Proton Therapy Facility. The simulated and measured lateral broadening distributions are compared for a 250 MeV proton beam on aluminum, polyethylene, polystyrene, bone substitute, iron, and lead target materials. The GRNTRN results are also compared to simulations from the Monte Carlo MCNPX code for the same projectile-target combinations described above.     

异形光斑的高精度光束偏转角度测量

大气湍流通常会造成激光光斑畸变为不规则的异形光斑,针对目前四象限探测器(QD)对空间光通信中不规则光斑偏转角度测量精度不足的问题,提出了一种基于多源信息融合的高精度光束偏转角度测量方法.该方法通过对QD及电荷耦合元件(CCD)的数据信息进行融合分析,在保持QD高分辨率和高响应速度的基础上,提高QD对不规则光斑偏转角的测...     

快响SAR卫星零多普勒波束中心姿态机动策略研究

传统偏航牵引方法采用惯性系下卫星轨道6要素推导得出姿态机动参数,在此方法中仅控制卫星主轴方向多普勒频率为0Hz,无法补偿SAR天线安装偏差和波束在天线内的方位距离向离轴角引起的斜距偏差和多普勒频率偏移,不能满足SAR系统时序设计需求和快响SAR卫星在轨实时处理器性能要求。因此,提出了地心固定坐标系中SAR天线波束指向零多普勒面内目标方向的姿态机动策略,使快响SAR卫星在轨实际波束中心多普勒频率为0Hz。该策略首先计算了基于场景目标的SAR总体设计的精确时序参数和观测参数,然后在地心固定坐标系中建立了波束中心多普勒频率为0Hz的SAR天线波束三轴指向模型,推导得出卫星三轴指向和姿态机动参数,并通过Matlab对该策略进行了仿真验证。结果表明,该策略可将多普勒频率由地球自转引起的29kHz、天线与卫星安装偏差引起的360Hz和波束方位向离轴角引起的3950Hz补偿至0Hz,同时将由天线与卫星安装偏差和波束距离向离轴角综合引起的波束中心偏离目标的斜距偏差6.28km补偿至米的量级。     

旋转爆震发动机燃烧室壁面烧蚀热防护研究

为了研究碳化烧蚀材料对旋转爆震燃烧室的被动热防护作用效果,建立了旋转爆震燃烧室热环境计算模型和多层复合壁一维烧蚀热响应分析模型。基于旋转爆震燃烧过程的数值模拟,确定了沿燃烧室轴向的壁面平均温度与热流的分布特征;针对典型的壁面热负荷输入条件,采用动边界隐式差分格式,对碳化型烧蚀材料的烧蚀过程和传热过程进行了耦合计算,分析了碳化层剥蚀、热解热、热解气体质量流率、材料厚度等因素对燃烧室壁面热防护效果的影响。研究结果表明,旋转爆震燃烧室温度和热流密度分布不均匀,斜激波扫掠区域热负荷更为剧烈;碳化层剥蚀后会使烧蚀材料的烧蚀率增加,壁面温度迅速上升;增大热解热及热解气体质量流率都有利于延长工作时间、降低壁面温度; 旋转爆震燃烧室不同区域的烧蚀有一定差异,增加烧蚀材料厚度无疑有利于壁面热防护,但是在实际应用中应综合考虑壁面重量和空间尺寸。     

柔性梁结构的时滞主动控制

对考虑时滞影响的柔性悬臂梁的离散最优控制进行了研究。首先采用独立模态空间方法给出包含有时滞项的控制模态方程，然后将之离散化并通过状态变量增广转化成不含时滞的标准离散形式。离散形式的性能指标也转化成增广形式。则离散时滞最优控制律可以针对增广的系统进行设计。因在最初的系统动力方程中就考虑了时滞项，且在推导离散模态控制律的过程中无近似处理，因而所给控制方法易于保证控制系统的稳定性。另外，文中还给出了从实际测量中提取模态坐标和将模态控制力转换成实际控制力的方法。最后通过数值仿真对本文所提控制方法的可行性和效果进行了验证。仿真结果显示，采用本文所提控制方法能够有效地抑制结构的振动。若在控制设计中忽略时滞，有可能引起动力失稳。     

基于ANSYS电子束焊接高压电源倍压整流电路仿真设计

采用ANSYS对电子束焊接用高压电源的倍压整流电路进行仿真,结果表明采用全波倍压整流电路比常规倍压整流电路输出波形稳定性好,纹波系数小且电路所需的电容值小;进行输入波形振荡对输出波形影响性的分析,结果表明输入波形发生振荡会在一定程度上影响输出电压值。根据仿真结果设计了倍压整流电路并测试其输出波形,测试结果表明,所设计的电路满足要求。     

"神舟四号"飞船微波辐射计天线的主波束效率

参照反射面天线主波束效率估计的简易计算公式,对“神舟四号”(SZ-4)飞船辐射计天线的主波束效率进行了具体估算,给出了计算流程和计算结果．计算表明,该辐射计天线在6．6GHz,19．35GHz,23．8GHz和37GHz 4个频段上的波束效率分别为89％,91．24％,92．91％和94．87％,并经过了在轨飞行验证．     

Evolution of an electron beam pulse influenced by coulomb collision effects in the solar corona

Electrons accelerated in the corona during solar activity give rise to radio emission events that can be observed over a wide range of frequencies. Among different finer-scale structures in the dynamic spectra observed in the radio range, fast transients with extents of some milliseconds known as solar radio spikes are observed accompaning the background continuum emission. Fundamental to the generation of radio spikes is a propagating electron beam and following its evolution allows us to understand the physical processes occurring in the solar corona. With the use of a numerical Fokker–Planck code we follow a previous numerical study to simulate the propagation of an electron beam pulse injected in a small region at the top of a magnetic field and outwards the solar corona under typical flare conditions. It was found that in large ambient densities of ${10}^{10}$ cm⁻³ at the injection point, Coulomb collision effects have an important effect on the propagation of the electrons, causing that the injected electrons thermalize faster in a time of $0.1$ and $0.4$ s for an electron distribution with a low-energy cut off of 16 and 7 keV respectively and a spectral index of 3. For a tenous ambient medium of density ${10}^9$ cm⁻³ thermalization occurs only for an electron distribution with smaller low-energy cut off (7 keV) with a duration of $\approx$1.5 s, while for a larger low-energy cut off (16 keV) the loss of accelerated electrons is very slow, regardles of the spectral index ($3,7$). The electron loss time by Coulomb collisions, which depends on the low boundary ambient density, might be an important parameter that influences the generation of radio spikes due to the formation of instabilities in the corona.