NHDB关系数据库系统

本文介绍南航计算机系数据库小组研制的中文关系数据库系统NHDB,概述它的系统结构、功能和特点,并讨论在微机环境中解决内存容量有限的方法,然后将NHDB与dBASE作一比较。     

一种自学习Fuzzy控制器

为了提高Ｐｕｚｚｙ控制器的性能，适当调整Ｆｕｚｚｙ控制规则是很重要的。本文利用参考Ｆｕｚｚｙ集的概念给出了一种便于规则调整的Ｆｕｚｚｙ控制算法。由于这种算法避免了输入和输出数值域上的离散化，所以具有较强的灵活性。为了估计Ｆｕｚｚｙ控制器的性能，本文利用了参考模型。通过参考模型与被控对象输出的偏差来实时调整Ｆｕｚｚｙ控制规则，构成了自学习Ｆｕｚｚｙ控制器。仿真结果表明，自学习性能是令人满意的。     

激波风洞中三角翼体模型的大攻角气动力测量和局部方法的应用

在激波管风洞中,模型自由飞方法测量了两种不同迎风面三角翼体模型的大攻角气动力。应用局部方法以一种迎风面外形的实验结果为依据,估算了另一迎风面外形的气动特性,结果与实验值吻合较好。另外,本文还进一步估算了航天飞机外形的气动特性,与美国的 CALSPAN 公司48英寸(1.2米)激波风洞中的实验值相比,结果也令人满意。从而表明,局部方法和实验相结合。用于简捷快速估算任意外形的高超声速气动特性是一有效的工程预示方法。     

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.     

1990年7月30日太阳射电大爆发中的脉动现象

本文讨论了1990年7月30日伴随日面2B级双带光学耀斑发生的3.2cm波微波大爆发事件的观测特征,它呈现为显著的脉动形态。并对它进行了数据处理,发现射电爆发流量S与脉动的特征参量:平均重复率R,调制度△S/S和能量△E之间有良好的统计相关性。对此作了讨论和初步的解释。     

超音速喷流DPIV瞬时速度场实验测量

介绍了采用数字式互相关粒子图像测速系统(DPIV)在测量超音速喷流实验中的应用;实验给出了设计马赫数Ma=1.5的小型拉瓦尔喷管在不同总压和反压比条件下,喷流速度场、流线、涡量分布等定量信息.实验结果显示出流场中激波前后流体速度,涡量分布的明显变化,波系的结构和不同于一维管流的流动特性.     

应用ANSYS进行热接触弹塑性有限元分析

应用ANSYS对实际结构进行了热载荷下接触弹塑性有限元分析，建立了孔边接触弹性模型、孔边接触弹塑性模型和模拟弹性边界孔边接触弹塑性模型等三种不断改进的模型，分别模拟了结构的弹性和弹塑性以及固支边界和弹性边界。通过对计算结果的分析比较，表明弹性边界的弹塑性模型更为精确可靠。     

可靠性验证试验中的α、β计算方法探讨

介绍了系统可靠性验证试验中α、β风险值的计算方法,特别是当一个定时试验方案被用来验证含有冗余的系统的 MTBF 时,α、β风险值不仅取决于 MTBF,而且取决于系统内冗余百分比和被试系统数量。     

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.     

发动机进气总压动态畸变流场测试及影响因素分析

扼要介绍了发动机进气总压畸变流场的动态测试分析方法,并利用所获得的大量试验数据计算了进口畸变流场的总压脉动强度及其在流场中的周向分布,开展了动态测量方法及数据处理中滤波截止频率、取样分析时间等因素对总压脉动强度影响的研究,用统计方法分析了进口畸变流场的特点,进而总结了进气总压畸变试验动态流场数据的一些处理、分析技术。