一种实现陀螺马达准确制动方案的研究

在分析了几种传统的电机制动方案基础上,提出了一种适合陀螺马达的能耗制动方案,该方案依据马达逐渐停转时自身产生的微弱电信号,再经放大处理后作为能耗制动的控制信号,实现陀螺马达准确、可靠、平稳的停止,避免了不及时切断电源而烧坏定子绕组的情况.     

Stellar winds of massive stars in M31

We have obtained the first UV high resolution spectra of hot luminous stars in M31 with the FOS onHubble Space Telescope. The spectra, combined with optical spectroscopic and photometric observations, enable us to study their stellar winds and photospheric parameters. We derive mass-loss rates and velocity laws from the wind line profiles, with the SEI method, as well as information on abundances. The wind lines and photospheric spectra are compared with galactic stars of the same spectral type.The spectra analyzed so far indicate that the stars have mass-loss rates comparable or slightly lower than galactic stars of the same spectral type, but possibly different velocity laws in their winds. The spectra of two stars are discussed here.     

专用工作测力机不确定度评定

主要介绍了在JJF1134-2005<专用工作测力机校准规范>(以下简称规范)的不确定度评定过程中出现的若干问题.为了明确各个分量的定义及其公式的使用,我们对某些量的含义作了相应的解释并给出了具体的运算操作,对相关人员有参考价值.     

圆度仪被测工件的自动对中

对Ｙ９０２５—Ｂ型圆度仪中被测工件的自动对中部分作了较为详细的介绍，其中包括基本工作原理、数据采集、电机控制及有关的软件框图等。该系统能自动把被测工件的偏心调至微米级。     

Self-similar solutions to stellar winds with cosmic rays

A two-fluid model is used to study the time evolution of stellar winds including the dynamical effect of cosmic rays. Neglecting the diffusion of cosmic rays, we seek self-similar solutions to spherically symmetric winds with a termination shock. The velocity upstream of the shock is taken to be zero. Physical solutions are those that can connect the shock to the star with the velocity approaching zero at the star. Two parameters govern the behaviour of the solutions, namely, the ratio of the upstream sound speed to the shock speed (in an inertial frame) and the gravitation potential of the central star. In some parameter regimes, no physical solution is possible.     

舰载飞机自动着舰系统设计方法

研究了舰载飞机自动着舰系统（ACLS）的综合设计方法，其中包括油门系统、姿态控制、ACLS控制律、雷达噪声滤波和甲板运动补偿的设计方法。并对ACLS进行了仿真。     

飞机液压系统动态油温计算方法优化

分析了动态油温计算方法的不足,将此方法中的液压油箱计算模型加以优化得到改进的动态油温计算方法,基于功率损失法给出了飞机液压系统中四种典型液压附件的温度计算方程。以某航空液压泵地面试验系统为计算实例,将改进方法计算的结果与试验结果、改进前方法的计算结果进行对比分析,结果表明改进的动态油温计算方法相比改进前的方法具有更高的准确度。     

Energetic Hydrogen and Oxygen Atoms Observed on the Nightside of Mars

We present measurements of energetic hydrogen and oxygen atoms (ENAs) on the nightside of Mars detected by the neutral particle detector (NPD) of ASPERA-3 on Mars Express. We focus on the observations for which the field-of-view of NPD was directed at the nightside of Mars or at the region around the limb, thus monitoring the flow of ENAs towards the nightside of the planet. We derive energy spectra and total fluxes, and have compiled maps of hydrogen ENA outflow. The hydrogen ENA intensities reach 10⁵ cm⁻² sr⁻¹ s⁻¹, but no oxygen ENA signals above the detection threshold of 10⁴ cm⁻² sr⁻¹ s⁻¹ are observed. These intensities are considerably lower than most theoretical predictions. We explain the discrepancy as due to an overestimation of the charge-exchange processes in the models for which too high an exospheric density was assumed. Recent UV limb emission measurements (Galli et al., this issue) point to a hydrogen exobase density of 10¹⁰ m⁻³ and a very hot hydrogen component, whereas the models were based on a hydrogen exobase density of 10¹² m⁻³ and a temperature of 200 K predicted by Krasnopolsky and Gladstone (1996). Finally, we estimate the global atmospheric loss rate of hydrogen and oxygen due to the production of ENAs.     

一种弱场区无线传输系统

在铁路无线列调通信中存在弱场区和盲区,通信质量难以控制。设计了完整的方案,提高了原无线列调中存在的弱场区的场强,并增大场强覆盖率,使通话距离得到扩展,改善了话音质量。     

自动钻铆技术在波音737尾段项目中的应用

通过自动钻铆技术在波音737尾段中的应用,介绍了自动钻铆技术的特点及工艺.