航空发动机轴承腔热状态分析模型及温度场计算

分析了轴承腔的主要热源。建立了轴承及石墨密封摩擦热的计算模型、密封热泄漏量的计算模型、对流换热系数的计算模型及温度场的计算模型。用热网络法建立了轴承腔的热平衡方程组,并采用拟牛顿法求解了该方程组。获得了10种不同工况下的温度场计算结果,该结果与本文的测试结果基本吻合。      

Range Correction Computations for Weapons Dropped from Aircraft

A general set of equations is developed from which the effects of initial condition perturbations upon weapon impact point are readily evaluated. Data are presented to illustrate the accuracy with which predictions can be made. Results obtained from the actual ballistic equations, from the time-varying perturbation equations, and from a time-invariant approximation of the perturbation equations are compared. It is shown that reasonable impact point predictive accuracy can be provited for fairly large changes in initial conditions.     

Current Status of Turbulent Dynamo Theory

Several recent advances in turbulent dynamo theory are reviewed. High resolution simulations of small-scale and large-scale dynamo action in periodic domains are compared with each other and contrasted with similar results at low magnetic Prandtl numbers. It is argued that all the different cases show similarities at intermediate length scales. On the other hand, in the presence of helicity of the turbulence, power develops on large scales, which is not present in non-helical small-scale turbulent dynamos. At small length scales, differences occur in connection with the dissipation cutoff scales associated with the respective value of the magnetic Prandtl number. These differences are found to be independent of whether or not there is large-scale dynamo action. However, large-scale dynamos in homogeneous systems are shown to suffer from resistive slow-down even at intermediate length scales. The results from simulations are connected to mean field theory and its applications. Recent work on magnetic helicity fluxes to alleviate large-scale dynamo quenching, shear dynamos, nonlocal effects and magnetic structures from strong density stratification are highlighted. Several insights which arise from analytic considerations of small-scale dynamos are discussed.     

计算机数控系统中的干扰源及抗干扰技术

分析了数控系统自身和工作环境中存在的各种干扰因素,具有针对性的从硬件／软件。从设计到生产采用了一系列实用的抗干扰技术,从而提高了数控系统的抗干扰能力和可靠性．     

考虑辐射的化学平衡流驻点线解

本文用数值方法求解了化学平衡的高超声速粘性激波层驻点线流场。考虑了辐射和质量引射对流场的影响。辐射模型采用线和连续谱模型。文中讨论了引射率、头部半径、来流速度对壁面传热的影响。与有关文献结果比较表明,本文的方法是可行的。     

Characterizing wood by microwaves

Common properties of raw wood can be determined by measuring the microwave propagation in the media. Unlike early designs from the 1970s and 1980s, simple constructions with phase and attenuation recording are now possible, if optimal frequencies are selected. At K-band, most quality impairments can be detected from basic group delay measurements, e.g., knots or insect holes smaller than 5 mm are observable. Impairments can be detected from a non-parallel viewing direction     

商用飞机驾驶舱造型设计特征研究

介绍了国内外商用飞机驾驶舱设计的历史及现状,在分析多类飞机驾驶舱造型设计图片资料的基础上,探讨主要飞机制造商驾驶舱造型设计的特征。依据驾驶舱造型的相似性,对国际上12家商用飞机制造商的66款机型的驾驶舱进行聚类分析和多维尺度分析,挑选出10款有代表性的驾驶舱。在提取代表性驾驶舱造型特征线后,分析主要飞机制造商的驾驶舱造型设计特点及差异,为新型飞机驾驶舱造型设计提供参考。     

Sco X-1

The physical properties of X-ray, optical and radio emissions from Sco X-1 are reviewed. Sco X-1 is a typical X-ray source which has an optically thick hot plasma. The observational spectra of X-ray and optical emissions are consistent with theoretical ones from the hot plasma, but the radio emission shows a non-thermal feature. The restrictive conditions for the model of Sco X-1 are discussed from the observational facts. In spite of numerous observational facts on Sco X-1 further detailed and elaborate studies are necessary to understand this object and general compact X-ray sources comprehensively.     

Spectral Moment Estimates from Correlated Pulse Pairs

Estimates statistics of the first two power spectrum moments from the pulse pair covariance are analyzed. The input signal is assumed to be colored Gaussian and the noise, white Gaussian. Perturbation formulas for the standard deviation of both mean frequency and spectrum width are applied to a Gaussian shaped power spectrum, and so is a perturbation formula for the bias in the width estimate. Mean frequency estimation from interlaced pulse pairs is presented. Throughout this study, estimators from independent, spaced, and contiguous pulse pairs are compared to provide a continuum of statistics from equispaced tightly correlated to statistically independent pulse pairs.     

双三角翼前缘剖面形状对涡运动的影响

采用数值模拟和理论分析相结合的方法,研究了前缘剖面形状对双三角翼涡运动的影响,分析了前缘剖面形状对三角翼、双三角翼涡运动影响的不同机理 :对三角翼,尖前缘可以形成组织最好的涡结构,但对于双三角翼,圆前缘生成的旋涡结构较靠近翼面,涡结构紧密,诱导能力较强,可以形成有利的涡涡干扰,使内翼涡通过剪切层向外翼涡输入涡量更加容易,合并涡变得更加稳定,推迟了涡破裂,而且由于涡较靠近翼面,因而可以产生较高的非线性涡升力,这同传统的认识是不一致的。     

Nuclear processes and accelerated particles in solar flares

Nuclear processes and particle acceleration in solar flares are reviewed. The theory of gamma-ray and neutron production is discussed and results of calculations are compared to gamma-ray, neutron, and charged-particle observations from solar flares. The implications of these comparisons on particle energy spectra, total numbers, anisotropies, electron-to-proton ratios, as well as on acceleration mechanisms and the interaction site, are presented. The information on elemental and isotopic abundances derived from gamma-ray observations is compared to abundances obtained from escaping accelerated particles and other sources.NAS/NRC Resident Research Associate.     

用微元法建立单刚体动力学的虚加速度原理和虚力原理

本文首先从刚体动力学方程出发,利用变积法推得其虚加速度原理和虚力原理,然后用微元法思想由质点系动力学的虚加速度原理、虚力原理推得刚体动力学的虚加速度原理与虚力原理,并对两种方法本身进行了比较。由于本文的推导方法是从连续介质力学的观点进行的,故这种方法对进一步建立单柔体、多柔体动力学的虚加速度原理和虚力原理具有重要应用价值,进而对现在热点之一的柔性飞行器动力学的研究有潜在的意义。     

Review of unsteady transonic aerodynamics: Theory and applications

Unsteady transonic flow theory is reviewed and classical results from the nonlinear asymptotic theory are combined with new results from computational fluid dynamics. The emphasis is on applications to the field of aeroelasticity and on clarifying the limitations of linearized theories in problems involving mixed subsonic-supersonic flows. The inherent differences between nonlinear transonic aerodynamics and linear subsonic and supersonic aerodynamics are considered from a theoretical and computational standpoint, and the practical implications of these differences in formulating suitable aerodynamic models for aeroelastic stability calculations are discussed. Transonic similarity principles are reviewed and their relevance in understanding flutter, divergence, and control reversal phenomena of transonic aircraft is illustrated through practical examples.     

基于超高速碰撞仿真的卫星碰撞解体碎片分析

使用超高速碰撞数值仿真技术,结合自主开发的碎片识别统计方法,以Iridium33与Cosmos2251卫星在轨撞击解体事件为例,进行了在轨卫星碰撞解体碎片分析.通过有限元方法(FEM)与光滑粒子流体动力学(SPH)的复合算法,从图形角度识别出碎片云中的大碎片,然后利用二值图转换与二值图连通域的快速统计,提取出了碎片数目...     

Observational studies of gamma-rays and neutrons from solar flares

Gamma-ray observations from HINOTORI satellite and possible neutron observations from the Tokyo neutron monitor are reviewed. Time histories of gamma-ray and X-ray emissions for both typical impulsive and gradual flares are discussed in connection with the particle acceleration time. The gamma-ray spectral hardening observed around 400 keV is explained from superimposition of two different electron bremsstrahlung spectra. Proton-energy spectra derived from the gamma-ray observations are compared with the solar energetic particle spectra in interplanetary space. The weak correlation between the gamma-ray fluence and the proton flux is discussed in connection with the particle trapping and escaping in the flare region. The limb darkening of the 2.22 MeV line resulting from neutron-proton capture is interpreted in terms of the attenuation by the Compton scattering in the photosphere. Possible solar neutron events recorded by the Tokyo neutron monitor are presented and the correlation between the gamma-ray fluence and the neutron fluence are described.     

The origin of tektites

The tektites called Muong Nong type by V. Barnes apparently represent the parent material from which other types are derived. In these tektites are found clues (coesite, angular voids) which indicate that they have not been substantially remelted since the event which detached them from the planet or satellite on which they were formed.From the nickel-iron spherules and the coesite it is deduced that the tektites were detached by meteorite impact. From the absence of cosmogenic isotopes and the distribution over the earth it is deduced that the source was either the earth or the moon. Calculations of rates of diffusion in silicates indicate that tektites could not have been produced from terrestrial sedimentary rocks; it has long been remarked that they are different from terrestrial igneous rocks. A lunar origin is therefore considered likely, in agreement with aerodynamic evidence. Contrary indications from the geochemical likeness of tektites to terrestrial materials, especially at the Ries Kessel and the Bosumtwi crater are noted, but these indications are considered to be outweighed by the difficulties of giving a physical account of a terrestrial origin.Interpreted as lunar materials, the tektites suggest that large portions of the lunar surface are covered with ash-flow tuff of a peculiar type, remarkably free of water and other volatiles. They also give evidence concerning the origin of the moon.     

Electric Fields and Magnetic Fields in the Plasmasphere: A Perspective From CLUSTER and IMAGE

The electric field and magnetic field are basic quantities in the plasmasphere measured since the 1960s. In this review, we first recall conventional wisdom and remaining problems from ground-based whistler measurements. Then we show scientific results from Cluster and Image, which are specifically made possible by newly introduced features on these spacecraft, as follows. 1. In situ electric field measurements using artificial electron beams are successfully used to identify electric fields originating from various sources. 2. Global electric fields are derived from sequences of plasmaspheric images, revealing how the inner magnetospheric electric field responds to the southward interplanetary magnetic fields and storms/substorms. 3. Understanding of sub-auroral polarization stream (SAPS) or sub-auroral ion drifts (SAID) are advanced through analysis of a combination of magnetospheric and ionospheric measurements from Cluster, Image, and DMSP. 4. Data from multiple spacecraft have been used to estimate magnetic gradients for the first time.     

氢氧喷注器面板温度场的三维模型及计算分析

本文推导了热传导的三维不等距网格差分公式,对氢氧发动机喷注器面板进行了通用的传热数值分析,得出了现行结构结冰是不可避免的.并且预测了一种新结构面板的温度场,它可以避免结冰.这种分析不仅对燃气发生器,而且对燃烧室同样适用,为今后喷注器设计提供了一种有效的传热分析手段.     

激波管内膨胀气流导致汽—液瞬态相变的测量方法

建立激波管装置,用以产生一维非定常的膨胀气流。描述膨胀气流的流场分布以及由此导致的水蒸汽自发成核、相变、凝结的物理过程。实验装置中,设置两个通道探测瞬态相变的信息:动态压力传感器探测膨胀气流的压力变化和光电倍增管探测水蒸汽从成核直至生长成液滴(凝结)所产生的光散射辐射强度。两种信息都由FFT(CF-910)分析仪采集记录,得到膨胀气流的压力曲线,显永过饱和度的变化;得到散射光功率曲线,立定不同蒸汽分压下液滴的相对增长速率。