高速滚子轴承运动特性的动态模拟

在高速轻载的工况下 ,滚子轴承的打滑蹭伤及由于滚子歪斜引起的滚子端面磨损已成为滚子轴承的主要失效原因。本文根据牛顿运动定律 ,建立了滚子的动力学模型 ,并对滚子轴承径向载荷分布和油膜拖动力的计算进行了详细讨论。利用本文所编制的软件 ,对滚子和保持架的打滑以及滚子的歪斜运动进行了动态模拟 ,得到与实际相符的结果 ,可用为实际轴承设计。     

鸟撞击叶片时的载荷模型

为了预估叶片的鸟撞击响应 ,首先要建立鸟撞击载荷模型。为此 ,开展了以下研究工作 :运用高速冲击动力学理论分析鸟撞击的物理过程 ;进行鸟撞击载荷试验 ;采用计算机数值模拟分析鸟撞击载荷的各种因素对叶片响应的影响。在综合运用上述研究结果的基础上 ,本文从鸟撞击载荷的冲量与加载持续时间的确定、力—时间函数的选择以及载荷空间因素的确定三个方面论述了有关的方法与原则 ,供建立鸟撞击载荷模型时参照使用     

AC/DC converter topologies for the Space Station

A new class of AC/DC converter topologies (Type-1 converters) is described, suitable for use in an advanced single-phase sine-wave voltage, high-frequency power distribution system, of the type that was proposed for a 20 kHz Space Station primary electrical power distribution system. The converter comprises a transformer, a resonant network, a current controller, a diode rectifier, and an output filter. The input AC voltage source is converted into a sinusoidal current source using the resonant network. The output of this current source is rectified by the diode rectifier and is controlled by the current controller. The controlled rectified current is then filtered by the output filter to obtain a constant voltage across the load. Three distinct converter topologies, Type-1A, Type-1B, and Type 1-C, are described, and their performance characteristics are presented. All three types have a close-to-unity rated power factor (greater than 0.98), low total harmonic distortion in input current (less than 5%), and high conversion efficiency (greater than 96%)     

The Galileo Dust Detector

The Galileo Dust Detector is intended to provide direct observations of dust grains with masses between 10^-19 and 10^-9 kg in interplanetary space and in the Jovian system, to investigate their physical and dynamical properties as functions of the distances to the Sun, to Jupiter and to its satellites, to study its interaction with the Galilean satellites and the Jovian magnetosphere. Surface phenomena of the satellites (like albedo variations), which might be effects of meteoroid impacts will be compared with the dust environment. Electric charges of particulate matter in the magnetosphere and its consequences will be studied; e.g., the effects of the magnetic field on the trajectories of dust particles and fragmentation of particles due to electrostatic disruption. The investigation is performed with an instrument that measures the mass, speed, flight direction and electric charge of individual dust particles. It is a multicoincidence detector with a mass sensitivity 10⁶ times higher than that of previous in-situ experiments which measured dust in the outer solar system. The instrument weighs 4.2 kg, consumes 2.4 W, and has a normal data transmission rate of 24 bits s^-1 in nominal spacecraft tracking mode. On December 29, 1989 the instrument was switched-on. After the instrument had been configured to flight conditions cruise science data collection started immediately. In the period to May 18, 1990 at least 168 dust impacts have been recorded. For 81 of these dust grains masses and impact speeds have been determined. First flux values are given.     

离散事件系统的Petri网图仿真

1.前言 离散事件动态系统DEDS(Discrete Event Dynamic System)的传统分析方法——应用排队论和随机过程理论为离散事件动态系统建立排队网络模型,在很多情况下已不适用。新的理论和研究方法相继提出。其中之一是“皮特里网”(Petri Nets)理论。另一种比较成熟的方法是仿真法,但是,仿真法要以高昂的计算机设备的大量计算时间为代     

硅基内衬喷管扩张段烧蚀和温度场的耦合计算方法

本文叙述固体火箭喷管扩张段硅基内衬烧蚀和温度场的耦合计算方法.烧蚀采用非定常的液体层烧蚀模型;温度场计算采用圆柱坐标系下的一维径向瞬态导热模型,考虑材料在高温下形成的炭化层和热解层,而由烧蚀产生的边界移动问题用坐标变换的方法处理.利用烧蚀和导热计算方程组中二者的结合部,通过充分耦合,获得了更准确的预示计算结果.     

Venus lightning

Although it is not unanimously accepted, many independent observations lead to the conclusion that lightning is prevalent on Venus. The electromagnetic signals detected by all 4 Venera landers are most readily explained as generation by lightning. The Venera 9 spectrometer appears to have observed a lightning storm on one occasion. The Pioneer Venus plasma wave instrument detects waves both below the electron gyrofrequency that may be due to lightning and signals above the electron gyrofrequency but at very low altitudes that may be due to the near field of the lightning. The VLF observations suggest that Venus lightning must be an intra-cloud phenomenon which is most frequent in the afternoon and evening sector. The occurrence rate is likely to be greater than on Earth.     

State Estimation and Divergence Analysis

A growing memory discrete dynamic model for performing temporal extrapolations along a predetermined path in a random field is presented. This dynamic model is used to drive a linear system that is itself driven by discrete white noise. The coupled system is used to derive a state estimation scheme that recursively processes noisy measurements of the system. In addition, using the aforementioned dynamic model as a reference (truth) model, the authors develop a covariance analysis to measure the estimation errors that occur when the dynamics along the path through the field are modeled as a Markov linear model and state estimation is performed using discrete Kalman filtering. The performance evaluation of an inertial navigation system influenced by the Earth's gravity field aboard a maneuvering ship is provided as a specific illustrative example.     

高负荷跨音速复合气冷涡轮叶片的试验研究

在燃气涡轮研究所 ( GTE)的涡轮叶片综合冷却效果试验器上对四套大载荷跨音速复合式气冷涡轮叶片 (多种气膜孔方案 ) ,成功地进行了 2 90小时试验。试验结果表明 ,导叶在 2 - 8% ,动叶在 1- 6%宽广的冷气流量比范围内 ,具有良好的冷却特性。此外还分析了叶片参数对冷却效果的影响     

Parallel resonant converter with LLC-type commutation

It is shown that by using a proper transformation of state variables, the third-order system of the parallel resonant converter (PRC) with LLC-type commutation can be analyzed by means of a two-dimensional state-plane diagram. A set of characteristic curves which can be used for the converter design is derived from the analysis. It is shown from these curves that the converter possesses more desirable features than the conventional PRC