Maxwell方程的高阶间断有限元数值解法

采用高精度方法求解时域Maxwell方程,方程的空间离散采用基于计算流体力学(Computational fluid dynamics,CFD)领域的高阶间断有限元格式,非定常时间迭代采用四步龙格-库塔格式。为了提高计算效率,本文采用了Quadrature-free implementation和网格分区并行技术。数值结果表明,采用高阶格式的情况下,采用稀疏网格便可以得到高精度数值解。另外由于本文的方法基于非结构网格,因此非常适合计算复杂外形的情况。     

一种基于量化力矩的静密封面缺陷补偿方法

在某次阀门静密封连接处漏气问题归零过程中,提出了一种基于量化力矩方法,用来弥补静密封面缺陷,以提高产品的静密封可靠性。     

基于协调权的案例学习群决策分类方法

基于案例学习的决策方法具有易于理解、贴近 实际决策过程的优点,成为当前决策领域的一个研究热点。文中针对如何有效地集成不同决 策专家提供的案例信息,提出了一种基于协调权的案例学习群决策模型用以解决多属性分类 决策问题。该方法首先针对各决策者给出不同案例数据,通过构建混合整数规划模型,识别 出具有一致案例信息重要度最大化的典型案例集。然后设计了分类阈值远离程度最大化模型 ,以此确定兼容各个决策者案例信息的指标权重（协调权）和最优分类阈值,由此构建一致 性的效用函数并应用获得的阈值进行分类决策。最后通过案例研究以及与其他模型的比较分 析,验证了方法的可行性。     

Dynamics of Planetary Waves in the Ionosphere as Observed from GPS Satellites

The GPS satellite data are used to study the dynamics of the ionospheric total electron content (TEC) over Central Europe in the summer season from June 23 to September 30, 1996. The TEC variations within the range of periods typical of the planetary waves were found to be nearly synchronous with the neutral wind variations in the mesosphere and with the variations in the occurrence of ionospheric sporadic layers. The observed TEC variations were interpreted as the result of penetration of energy carried by nonstationary Rossby waves to the upper atmospheric altitudes.     

微型惯导系统在余度配置时的转动标定技术研究

余度技术是提高惯性导航系统性能的一种重要手段。对微小型惯性组合导航系统中的惯性传感器多余度配置技术进行了研究,开发了MEMS惯性器件构成的微型余度配置惯导系统,分析了微小型惯性组合导航系统的特点和误差特性,并经过测试分析,建立了惯性传感器的误差模型。针对余度配置系统静态标定精度低的问题,提出了六位置转动标定算法,该算法只需要一个单轴速率转台就可以标定出IMU误差参数,并对采用低精度陀螺的惯性系统标定具有通用性。经过实际系统测试分析,误差补偿后的微型余度配置惯导系统的系统导航精度明显提高,验证了算法的有效性。     

Far ultraviolet imaging from the IMAGE spacecraft. 2. Wideband FUV imaging

The Far Ultraviolet Wideband Imaging Camera (WIC) complements the magnetospheric images taken by the IMAGE satellite instruments with simultaneous global maps of the terrestrial aurora. Thus, a primary requirement of WIC is to image the total intensity of the aurora in wavelength regions most representative of the auroral source and least contaminated by dayglow, have sufficient field of view to cover the entire polar region from spacecraft apogee and have resolution that is sufficient to resolve auroras on a scale of 1 to 2 latitude degrees. The instrument is sensitive in the spectral region from 140–190 nm. The WIC is mounted on the rotating IMAGE spacecraft viewing radially outward and has a field of view of 17° in the direction parallel to the spacecraft spin axis. Its field of view is 30° in the direction perpendicular to the spin axis, although only a 17°×17° image of the Earth is recorded. The optics was an all-reflective, inverted Cassegrain Burch camera using concentric optics with a small convex primary and a large concave secondary mirror. The mirrors were coated by a special multi-layer coating, which has low reflectivity in the visible and near UV region. The detector consists of a MCP-intensified CCD. The MCP is curved to accommodate the focal surface of the concentric optics. The phosphor of the image intensifier is deposited on a concave fiberoptic window, which is then coupled to the CCD with a fiberoptic taper. The camera head operates in a fast frame transfer mode with the CCD being read approximately 30 full frames (512×256 pixel) per second with an exposure time of 0.033 s. The image motion due to the satellite spin is minimal during such a short exposure. Each image is electronically distortion corrected using the look up table scheme. An offset is added to each memory address that is proportional to the image shift due to satellite rotation, and the charge signal is digitally summed in memory. On orbit, approximately 300 frames will be added to produce one WIC image in memory. The advantage of the electronic motion compensation and distortion correction is that it is extremely flexible, permitting several kinds of corrections including motions parallel and perpendicular to the predicted axis of rotation. The instrument was calibrated by applying ultraviolet light through a vacuum monochromator and measuring the absolute responsivity of the instrument. To obtain the data for the distortion look up table, the camera was turned through various angles and the input angles corresponding to a pixel matrix were recorded. It was found that the spectral response peaked at 150 nm and fell off in either direction. The equivalent aperture of the camera, including mirror reflectivities and effective photocathode quantum efficiency, is about 0.04 cm². Thus, a 100 Rayleigh aurora is expected to produce 23 equivalent counts per pixel per 10 s exposure at the peak of instrument response.     

The Extreme Ultraviolet Imager Investigation for the IMAGE Mission

The Extreme Ultraviolet Imager (EUV) of the IMAGE Mission will study the distribution of He⁺ in Earth's plasmasphere by detecting its resonantly-scattered emission at 30.4 nm. It will record the structure and dynamics of the cold plasma in Earth's plasmasphere on a global scale. The 30.4-nm feature is relatively easy to measure because it is the brightest ion emission from the plasmasphere, it is spectrally isolated, and the background at that wavelength is negligible. Measurements are easy to interpret because the plasmaspheric He⁺ emission is optically thin, so its brightness is directly proportional to the He⁺ column abundance. Effective imaging of the plasmaspheric He⁺ requires global `snapshots in which the high apogee and the wide field of view of EUV provide in a single exposure a map of the entire plasmasphere. EUV consists of three identical sensor heads, each having a field of view 30° in diameter. These sensors are tilted relative to one another to cover a fan-shaped field of 84°×30°, which is swept across the plasmasphere by the spin of the satellite. EUVs spatial resolution is 0.6° or 0.1 R _E in the equatorial plane seen from apogee. The sensitivity is 1.9 count s^–1 Rayleigh^–1, sufficient to map the position of the plasmapause with a time resolution of 10 min.     

数字人感系统的研究

随着飞机模拟器技术的发展,电机伺服系统在人感系统中也得到了广泛的应用。本文着重讨论 了以DSP芯片为核心的数字人感系统组成和工作原理,并分析了系统的特点及功能。     

法兰环缝局部真空电子束焊机的研制

对所研制的法兰环缝局部真空电子束焊机作了简要介绍，对焊机的微机控制系统和电子 枪极坐标行走的控制、二次电子焊缝对中、焊接轨迹的示教再现、真空系统和焊接工艺的微机控制等关键技术作了较为详细的阐述。通过焊接工艺试验，用法兰环缝局部真空电子束焊机焊接出了成形良好、焊缝内部质量符合GJB1718－93Ⅰ级标准的铝合金法兰环缝典型工艺件。     

真空感应钎焊单层金刚石砂轮的实验研究

在真空条件下用Ni-Cr合金做钎料进行了钎焊单层金刚石砂轮的实验研究，实现了金刚石与钢基体间的牢固化学冶金结合。通过扫描电镜X射线能谱，结合X射线衍射结构分析，发现Ni-Cr合金中的Cr原子与金刚石表面的碳原子反应生成稳定连续的Cr3C2膜，在钢基体结合界面上生成（FexCry）C，这是实现合金层与金刚石及钢基体之间都有较高结合强度的主要因素。通过磨削实验验证了金刚石确实有较高的把持强度。