亚、跨音速三维机翼气动外形反设计的控制理论方法

本文进行了基于控制论的气动外形反设计方法研究，根据给定的目标函数推导了在物理空间上描述的共轭及相应的边界条件，通过构造共轭方程耗散通量项，以及使用特征线理论处理远场边界等措施，研究了共轭方程的数值求解方法，使用Hicks-Henne函数来描述设计变量扰动对机翼表面外形的影响，通过网格扰动获得度量矩阵变分来获得目标函数对设计变量的敏感性导数，优化过程使用拟牛顿优化算法，通过对流场计算、共轭方程数值求解、敏感性导数求解和优化算法这四个方面的有效结合，成功地发展出了一种机翼气动外形反设计方法，进行了机翼气动外形反设计研究，结果表明该设计方法在设计理论及可实现性方面，特别在跨音速及复杂外形气动设计方面比以往设计方法具有更好的适用性和优越性，且设计结果较为可靠，在现有计算条件下是一个好的设计方法，时间花费也较少。     

Advanced Technologies Demonstrated by the Miniature Integrated Camera and Spectrometer (MICAS) Aboard Deep Space 1

MICAS is an integrated multi-channel instrument that includes an ultraviolet imaging spectrometer (80–185 nm), two high-resolution visible imagers (10–20 μrad/pixel, 400–900 nm), and a short-wavelength infrared imaging spectrometer (1250–2600 nm). The wavelength ranges were chosen to maximize the science data that could be collected using existing semiconductor technologies and avoiding the need for multi-octave spectrometers. It was flown on DS1 to validate technologies derived from the development of PICS (Planetary Imaging Camera Spectrometer). These technologies provided a novel systems approach enabling the miniaturization and integration of four instruments into one entity, spanning a wavelength range from the UV to IR, and from ambient to cryogenic temperatures with optical performance at a fraction of a wavelength. The specific technologies incorporated were: a built-in fly-by sequence; lightweight and ultra-stable, monolithic silicon-carbide construction, which enabled room-temperature alignment for cryogenic (85–140 K) performance, and provided superb optical performance and immunity to thermal distortion; diffraction-limited, shared optics operating from 80 to 2600 nm; advanced detector technologies for the UV, visible and short-wavelength IR; high-performance thermal radiators coupled directly to the short-wave infrared (SWIR) detector optical bench, providing an instrument with a mass less than 10 kg, instrument power less than 10 W, and total instrument cost of less than ten million dollars. The design allows the wavelength range to be extended by at least an octave at the short wavelength end and to ∼50 microns at the long wavelength end. Testing of the completed instrument demonstrated excellent optical performance down to 77 K, which would enable a greatly reduced background for longer wavelength detectors. During the Deep Space 1 Mission, MICAS successfully collected images and spectra for asteroid 9969 Braille, Mars, and comet 19/P Borrelly. The Borrelly encounter was a scientific hallmark providing the first clear, high resolution images and excellent, short-wavelength infrared spectra of the surface of an active comet’s nucleus.     

航空弧齿锥齿轮齿面接触应力计算与优化

本文在弧齿锥齿轮的轮齿接触分析 (TCA)和承载接触分析 (LTCA)的基础上 ,根据计算所得的齿面接触点附近的准确几何形状 ,一定载荷下的齿间载荷分配和齿面载荷分布状态 ,采用弹性力学中两个空间曲面弹性接触的计算公式 ,提出了航空弧齿锥齿轮齿面接触应力变化过程的计算方法 ,进一步结合齿轮的加工参数设计和齿面修正 ,对齿面接触强度进行了优化     

弹用涡喷发动机密封元件摩擦性能试验研究

从添加剂和表面改性两个方面，对某涡喷发动机密封部件摩擦副的摩擦性能进行了试验研究。结果表明FROMULA 4－10和PC－7000两种添加剂，以及磷化和刷镀铟铜合金两种密封环表面改性方法，能够改善密封元件的摩擦性能。     

Energetic particle transport coefficients in the heliosphere

It is the purpose of this review to summarize and discuss recent research done in the field of particle propagation in the heliosphere. Several lines of approach have been followed to treat this problem. As a starting point the different forms of the transport equation are discussed. Quasi-Linear Theory (QLT) relates the power contained in fluctuations of the Interplanetary Magnetic Field (IMF) to the transport coefficients of energetic particles, an outline of the basic results of this theory is presented followed by a discussion of subsequent corrections made to the original formulation with an emphasis in recent developments where the effects of wave polarization, its propagation respect to the solar wind and the dissipation of power at large frequencies have been taken into account. The numerical approach using test particle trajectory integrations to obtain transport coefficients based on in situ satellite measureents is also discussed. It is well known that the determination of the particles mean free path for solar particle events by alternative methods leads to conflicting results, corrections made to original QLT are attempts to bridge the gap. Determination of the transport parameters from different lines of approach in a comparative basis have been done recently by calculating power spectra of IMF measured at the time solar particles were detected on the same spaceprobe, and performing numerical simulations with equivalent IMF data. Some of the results of such studies point to the solution of the conflicting determinations of the mean free path which has existed for nearly 30 years. An assesment of the present situation in this respect is given. Numerical determinations of transport parameters in the outer heliosphere are also reviewed and its consequences for solar modulation of galactic cosmic rays discussed. Space Science Reviews 62: Printed in Belgium.     

基于AutoCAD几何建模的近场目标电磁散射计算技术

为了计算复杂目标的雷达散射截面（RCS），提出了一种基于AutoCAD几何建模的近场目标电磁散射计算技术，计算了单元体，组成体以及飞机的近场雷达散射截面，理论计算和实测结果较为吻合，为在微机上计算复杂目标近场RCS提供了一种理想的方法。