环氧树脂电子束固化反应动力学研究

研究了以二芳基碘鎓盐为引发剂的电子束固化阳离子环氧树脂的固化反应动力学特征.研究表明:在反应初期,反应速率为质子酸数量所控制,反应速率随时间增加和环氧值的降低而加大;随反应的进行,反应速率的变化逐渐转化为环氧值所控制,反应速率达到一个极值点之后逐渐降低;当引发剂完全分解之后,反应速率只受环氧值所控制,呈一级反应动力学特征.     

模糊推理和证据理论融合的航空发动机故障诊断

提出了一种模糊推理与证据理论相结合的航空发动机故障诊断方法.首先,根据故障征兆信号,结合专家经验对发动机故障原因发生的可能进行模糊推理,解决故障诊断中的模糊性问题;其次,将模糊推理结果作为证据的基本置信度分配,确保赋值的准确性;最终,采用证据组合规则对多个证据进行融合决策,减小故障诊断的不确定性测度,并解决证据间的冲突问题,从而实现对故障源的精确定位.实验结果表明,该方法可行且有效.      

The Solar Energetic Particle Ionic Charge Analyzer (SEPICA) and the Data Processing Unit (S3DPU) for SWICS,SWIMS and SEPICA

The Solar Energetic Particle Ionic Charge Analyzer (SEPICA) is the main instrument on the Advanced Composition Explorer (ACE) to determine the ionic charge states of solar and interplanetary energetic particles in the energy range from ≈0.2 MeV nucl−1 to ≈5 MeV charge−1. The charge state of energetic ions contains key information to unravel source temperatures, acceleration, fractionation and transport processes for these particle populations. SEPICA will have the ability to resolve individual charge states and have a substantially larger geometric factor than its predecessor ULEZEQ on ISEE-1 and -3, on which SEPICA is based. To achieve these two requirements at the same time, SEPICA is composed of one high-charge resolution sensor section and two low- charge resolution, but large geometric factor sections. The charge resolution is achieved by the focusing of the incoming ions, through a multi-slit mechanical collimator, deflection in an electrostatic analyzer with a voltage up to 30 kV, and measurement of the impact position in the detector system. To determine the nuclear charge (element) and energy of the incoming ions, the combination of thin-window flow-through proportional counters with isobutane as counter gas and ion-implanted solid state detectors provide for 3 independent ΔE (energy loss) versus E (residual energy) telescopes. The multi-wire proportional counter simultaneously determines the energy loss ΔE and the impact position of the ions. Suppression of background from penetrating cosmic radiation is provided by an anti-coincidence system with a CsI scintillator and Si-photodiodes. The data are compressed and formatted in a data processing unit (S3DPU) that also handles the commanding and various automatted functions of the instrument. The S3DPU is shared with the Solar Wind Ion Charge Spectrometer (SWICS) and the Solar Wind Ion Mass Spectrometer (SWIMS) and thus provides the same services for three of the ACE instruments. It has evolved out of a long family of data processing units for particle spectrometers. This revised version was published online in June 2006 with corrections to the Cover Date.     

空气节流对超燃燃烧室流场结构与燃料混合影响的数值研究

实现高速气流的点火和稳定燃烧是超燃冲压发动机燃烧室设计面临的主要问题,空气节流通过在流场中产生激波串,减小主流气体的马赫数,提高当地的静温和静压,辅助发动机实现起动点火和稳定燃烧.为了研究空气节流的详细机理,通过求解三维N-S方程的方法研究了节流流量、节流位置对节流效果的影响,同时对比了有无节流存在对超燃冲压发动机燃烧室流场结构和掺混特性的影响,分析了节流促进燃料高效混合的机理.结果表明:在燃烧室入口马赫数2、静温517.7K、静压101342.2Pa的条件下,20％入口空气流量的节流流量是最合适的节流流量,本文研究的实例中最佳节流位置位于距燃烧室入口623mm处,同时证实了节流有效地促进了燃料的混合,提高了混合效率.     

SPC-II机器鱼平台及其自主航行实验

SPC-II型仿生机器鱼是利用尾鳍推进机理,实现机器鱼稳定、高速游动和验证机动性的一个实验平台.SPC-II不模仿某种特定鱼类的外形,而是把游动稳定性作为仿生水下航行器设计首要考虑的因素,有效克服艏摇的鱼体,使得尾鳍推进器的运动不受到干扰,同时也降低航行阻力.SPC-II长度约1.2?m,采用完全刚体耐压舱,内部安装了电池、GPS(Global Position System)和罗盘组合导航系统、2关节伺服电机推进系统,能在深度5?m内进行定深的自主航行,速度达到了2.8?kn,功耗小于250?W.对直线航行速度,转弯机动性进行了测试,并进行了长距离风浪条件下的海试.与国内外相关实验平台进行了对比,在外形、航行速度方面展现出优越性.     

用真实IMU/GPS数据进行机载SAR运动补偿处理

分析了机载SAR(Synthetic Aperture Radar)条带成像模式的运动补偿技术原理,通过对激光IMU/GPS(Inertial Measurement Units/Global Positioning System)组合提供的位置参数进行分析,表明Y12载机平台具有很大的运动误差,在此基础上利用高精度激光IMU/GPS组合提供的天线相位中心精确位置参数,结合距离-多普勒成像算法进行了机载SAR数据的运动补偿处理,试验表明利用此IMU/GPS提供的运动参数进行对具有很大运动误差的SAR数据运动补偿后,已不需要计算负担沉重的自聚焦类算法进行残留运动误差补偿,就能得到高质量的高分辨率SAR图像.     

连续粒径粉体在浆体中的堆积密度

采用测定相同流动度时浆体需水量的方法,试验证明了不同粒径分布的矿粉其堆积密度有显著的差异.将浆体中的粉体颗粒及其表面包裹着的一层水膜作为复合颗粒,从而将求浆体中粉体颗粒堆积密度的问题转化为求假想复合颗粒体系的堆积密度问题,在Stovall模型的基础上推导了浆体中连续粒径粉体的堆积密度计算公式;通过试验确定了该公式中的待定参数值,并对公式的适用性进行了验证,结果表明:用该公式可以根据粉体的粒径分布计算它在浆体中的堆积密度.      

锶原子冷却与光晶格装载

锶原子光钟冷却实验实现原子由一级宽带冷却到二级窄线宽冷却转移二级冷却后原子温度约为2μK;晶格激光在原子冷却过程中始终开启,实现原子边冷却边装载。     

飞行过程中座舱盖透明件温度计算分析

介绍了飞机座舱盖透明件飞行过程中温度效应的理论计算方法。通过温度载荷计算结果,分析了气动加热对座舱盖透明件产生热应力的影响,为飞机座舱盖透明件疲劳定寿中考虑其影响提供了思路和方法。     

Theoretical modeling for the stereo mission

We summarize the theory and modeling efforts for the STEREO mission, which will be used to interpret the data of both the remote-sensing (SECCHI, SWAVES) and in-situ instruments (IMPACT, PLASTIC). The modeling includes the coronal plasma, in both open and closed magnetic structures, and the solar wind and its expansion outwards from the Sun, which defines the heliosphere. Particular emphasis is given to modeling of dynamic phenomena associated with the initiation and propagation of coronal mass ejections (CMEs). The modeling of the CME initiation includes magnetic shearing, kink instability, filament eruption, and magnetic reconnection in the flaring lower corona. The modeling of CME propagation entails interplanetary shocks, interplanetary particle beams, solar energetic particles (SEPs), geoeffective connections, and space weather. This review describes mostly existing models of groups that have committed their work to the STEREO mission, but is by no means exhaustive or comprehensive regarding alternative theoretical approaches.