如何做好雷达管制下航空器的飞行动态监控

一、前言在雷达管制空域,只要管制员发出“radar contact”或“radaridentified”这样的指令,就担负起了对该航空器的一切动态过程的监控责任。如果对该机的飞行动态监控不到位,造成的一切不安全后果,雷达管制员都将难辞其咎。近来在全国范围内发生的几起不安全事件,多是由于管     

关于平面空穴流动的截断误差减小方法(英文)

提出了一种新的截断误差减小方法。该方法是利用在粗网格 ( 2 h)上估算截断误差进而减小在原始网格( h)上的误差的迭代过程 ,最终目的是利用粗网格得出更精确的结果以及发展一种新的粗网格直接数值模拟方法     

均布压力作用各向异性矩形薄板大挠度问题

基于冯·卡门模型，选择中心挠度为摄动参数，利用摄动方法将正交异性矩形薄板大挠问题的非线性偏微分方程组逐级线性化，导出了各级摄动对应的几个线性偏微分方程组，然后再借助变分法求解，得到了均布载荷作用下正交异性矩形薄板的载荷-挠度曲线。     

转动旋翼模型动柔度的试验研究

介绍测定转动旋翼模型动柔度的试验方案、试验程序，综述以作者自行设计的旋翼模型进行试验所得到的结果及其与理论计算结果的比较。结果表明，试验方案与方法是可行的，理论计算公式是正确的。     

疲劳裂纹扩展速率试验数据的可靠性分析模型

以指定ΔＫ下的ｄａ／ｄＮ服从对数正态分布为基础，提出３种ｄａ／ｄＮ试验数据统计处理方法；依据一组４０ＣｒＮｉＭｏ材料的ＣＴ试样的试验数据处理结果，对３方法进行了分析对比。     

低轨卫星面阵凝视成像技术研究

文章介绍了面阵凝视成像的工作原理及特点，阐述了低轨卫星对地观测凝视成像面临的像移问题及其解决措施，对像移补偿装置与二维指向机构的结合做了初步探讨。     

星光折射航天器自主定轨方案比较

当星光透射大气发生折射时 ,用星光折射角精确地反映星光在大气中离地球表面的高度 ,并建立高度、航天器与地球的几何关系。通过对折射角进行观测 ,间接测得地平 ,从而改善了用地平仪直接测地平所造成的航天器自主导航精度低的不足。本文提出了几种利用星光折射的航天器自主定轨方案 ,并作了细致的仿真实验 ,对直接和间接两种测量地平方法以及几种星光折射自主定轨方案进行了分析比较。     

一种新型的橡塑复合半膜贮箱

橡塑复合半膜贮箱是为延长姿控发动机加注贮存期而研制的单组元推进剂贮箱。壳体采用钛合金材料,半膜采用双层复合形式,内层的氟塑料半膜与推进剂接触,外层的橡胶半膜对氟塑料半膜起保护作用。该贮箱利用钛合金及氟塑料对DT-3推进剂催化分解速率小的特性来实现长期加注贮存,加注贮存期可达5～10年。研制中,主要解决了橡塑复合半膜的粘合、复合半膜与推进剂的长期相容、赤道圆焊缝焊接时对复合半膜的热影响等关键技术问题,在液、气腔防堵防漏方面采取了独到的措施。三台试制贮箱已通过了各种力学环境试验及性能试验的考核。该贮箱可大大提高导弹的机动性、降低使用维护要求和全寿命周期成本。     

LISA — a study of the ESA cornerstone mission for observing gravitational waves

The primary objective of the Laser Interferometer Space Antenna (LISA) mission is to detect and observe gravitational waves from massive black holes and galactic binaries in the frequency range 10⁻⁴ to 10⁻¹ Hz. This low-frequency range is inaccessible to ground-based interferometers because of the unshieldable background of local gravitational noise and because ground-based interferometers are limited in length to a few km. LISA is an ESA cornerstone mission and recently had a system study (Ref. 1) carried out by a consortium led by Astrium, which confirmed the basic configuration for the payload with only minor changes, and provided detailed concepts for the spacecraft and mission design. The study confirmed the need for a drag-free technology demonstration mission to develop the inertial sensors for LISA, before embarking on the build of the flight sensors. With a technology demonstration flight in 2005, it would be possible to carry out LISA as a joint ESA-NASA mission with a launch by 2010 subject to the funding programmatics. The baseline for LISA is three disc-like spacecraft each of which consist of a science module which carries the laser interferometer payload (two in each science module) and a propulsion module containing an ion drive and the hydrazine thrusters of the AOCS. The propulsion module is used for the transfer from earth escape trajectory provided by the Delta II launch to the operational orbit. Once there the propulsion module is jettisoned to reduce disturbances on the payload. Detailed analysis of thermal and gravitational disturbances, a model of the drag-free control and of the interferometer operation confirm that the strain sensitivity of the interferometer will be achieved.