基于立体视觉的孔探分析系统及其应用

孔探分析在现代航空发动机故障诊断中一直发挥着重要的作用，开发基于立体视觉的孔探分析系统，对提高故障诊断水平和预测准确度，节约发动机维护成本有着重要的现实意义，系统利用立体视觉技术以及图像处理技术，完成了对双目视觉左右图像的标定和匹配，实现了对实体表面的三维测量和立体重建，本文介绍了基于立体视觉的孔探分析系统的基本原理与主要功能，并结合应用实例验证了系统的有效性。     

金属载体上线天线阻抗与辐射特性的矩量法研究

用线网格模拟金属载体表面，应用矩量法求出天线及载体网格上的电流分布，据此研究在该金属载体影响下的天线特性，在计算阻抗矩阵元素时，利用了非对称正弦偶极子辐射场的精确表达式，并采用了直接复数积分，简化了计算公式，本文给出了几种金属载体上线天线的阻抗与辐射特性的计算结果，它们与有关文献上的数据或实验结果一致，最后计算了一种舰船简单模型上两根线天线的远区辐射场及它们的自阻抗与互阻抗。     

飞机主起落架的光弹性应力分析

讨论了用光弹性嵌片法（一种新的模型试验方法）进行飞机主起落架的实验应力分析。采用该方法解决了传统光弹性贴片法中的贴片增强效应问题，避免了在贴片边界，因泊松比不匹配引起的误差，从而提高了测试灵敏度。实验应力分析选用了与实物尺寸相同的模型试件，克服了模型制作过程中遇到的许多困难。该方法在一套试验模型上能够直观地进行多种载荷状态下主起落架表面应力场的分析比较，为主起落架结构优化设计方案提供了试验依据，故具有广泛的应用前景．测试数据的计算校核表明，试验结果是可信的，可作为主起落架结构减重修型的重要试验依据。关键词     

生物组织光学参数：优化散射系数（μ’s）的实时在位测定

利用了一套特殊设计光纤探头组成的稳定态光纤光谱仪测试生物组织的光学参数，从悬乳液(Intralpid)与模拟胶(Phantom)实验推导出优化散射系数(Reduced scattering coeffcient：μ’s)近红外谱测量经验公式。测量反射系数就可以计算出优化散射系数谱。计算结果用模拟胶作了验证，并对大鼠脑组织μ’s进行了实时在位测量，从而得到了一种μ’s在位测量的有效方法。     

基于BP网络的热工过程模型辨识方法

主要研究了人工神经网络在辨识火电厂热工过程模型中的应用，利用Visual C^ 语言构造BP神经网络,提出了把BP网络权值转换为传递函数的方法，针对火电厂常见的热工过程，不用人为加入特殊的激励信号，只利用现场生产中自然存在的扰动信号进行辨识试验，试验结果准确可靠。     

关于精密度、正确度、准确度和精度

讨论指出以词义相近的名词精密度、正确度、准确度来定义不同的概念值得商榷；认为精密度和正确度在实际中极少应用，我国文件将精密度译为ｐｒｅｃｉｓｉｏｎ的合理性值得探讨；详细阐述了名词精度在国内的应用发展情况及其在实际使用中的不成文的约定概念；认为我国计量名词应与国际一致，对我国名词精密度等提出了修改意见：建议从我国计量名词中删去精密度和正确度，将ａｅｃｕｒａｃｙ译为精度（准确度），即精度和准确度等同使用。此外，就目前如何翻译ｐｒｅｃｉｓｉｏｎ提出了想法。     

Energetic ion emission for active spacecraft control

Future space missions aiming at the accurate measurement of cold plasmas and DC to very low frequency electric fields will require that the potential of their conductive surfaces be actively controlled to be near the ambient plasma potential. In the near-Earth space these spacecraft are usually solar-cell powered; consequently, parts of their surface are most of the time exposed to solar photons. Outside the plasmasphere, a positive surface potential due the dominance of surface-emitted photoelectrons over ambient plasma electrons is to be expected. Photo- and ambient electrons largely determine the potential and positive values between a few Volts up to 100 V have been observed. Active ion emission is the obvious solution of this problem. A liquid metal ion emitter and a saddle field ion emitter are nearing the stage of flight unit fabrication. We will attempt to clamp the spacecraft potential to values close to the plasma potential. We present first results from vacuum chamber tests and describe the emission behaviour and characteristics of emitters producing, respectively, In⁺ and N₂⁺ beams with an energy of ≥ 5 keV.     

The detection of energetic cometary and solar particles by the EPONA instrument on the Giotto mission

EPONA is an energetic particle detector system incorporating totally depleted silicon surface barrier layer detectors. Active and passive background shielding will be employed and, by applying various techniques, particles of different species, including electrons, protons, alpha particles and pick-up ions of cometary origin may be detected over a wide spectrum of energies extending from the tens of KeV into the MeV range.

The instrument can operate in two modes namely (a) in a cruise phase or storage mode and (b) in a real time mode. During the real time mode, observations at high spatial (octosectoring) and temporal (0.5s) resolution in the cometary environment permit studies to be made of accelerated particles at the bow shock and/or in the tail of the comet. In conjunction with magnetic field measurements on board Giotto, observations of energetic electrons and their anisotropies can determine whether the magnetic field lines in the cometary tail are open or closed. Further, the absorption of low energy solar particles in the cometary atmosphere can be measured and such data would provide an integral value of the pertaining gas and dust distribution. Solar particle background measurements during encounter may also be used to correct the measurements of other spacecraft borne instruments potentially vulnerable to such radiation.

Solar particle flux measurements, obtained during the cruise phase will, when combined with simultaneous observations made by other spacecraft at different heliographic longitudes, provide information concerning solar particle propagation in the corona and in interplanetary space.     

符合CCSDS标准的RS(255,223)码译码器的FPGA实现及其性能测试

RS（Reed-Solomon)码是差错控制领域中一种性能优异的非二进制分组循环码，由于它具有很强的随机错误和突发错误的纠错能力，被CCSDS，NASA，ESA等空间组织接受，广泛应用于深空探测中．本文采用改进的Berlekamp算法，用FPGA实现了符合CCSDS标准的RS(255，223)码译码器；介绍了该译码器的实现流程、性能测试方法和基于PCI总线接口的测试平台；给出了测试结果，并且对理论上RS(255，223)译码器的误码性能与实际测试的误码率结果进行了比较和分析．验证结果证明该译码器能工作在400Mbps以上的码率，使用FPGA资源180000门，译码效果与理论上译码效果一致．     

The characteristics of sharp (small-scale) boundaries of solar wind plasma and magnetic field structures

We investigate properties of large (>20%) and sharp (<10 min) solar wind ion flux changes using INTERBALL-1 and WIND plasma and magnetic field measurements from 1996 to 1999. These ion flux changes are the boundaries of small-scale and middle-scale solar wind structures. We describe the behavior of the solar wind velocity, temperature and interplanetary magnetic field (IMF) during these sudden flux changes. Many of the largest ion flux changes occur during periods when the solar wind velocity is nearly constant, so these are mainly plasma density changes. The IMF magnitude and direction changes at these events can be either large or small. For about 55% of the ion flux changes, the sum of the thermal and magnetic pressure are in balance across the boundary. In many of the other cases, the thermal pressure change is significantly more than the magnetic pressure change. We also attempted to classify the types of discontinuities observed.