防静电白色热控涂层的耐空间环境及工艺性能

研究了防静电白色热控涂层（ACR-1）的耐空间环境性能及工艺性能。在模拟空间环境设施中研究了紫外辐照、电子辐照和质子辐照对涂层太阳吸收率（αs）的影响。结果表明ACR-1在地球静止轨道环境中具有较高的稳定性；经过3000当量太阳小时（ESH）的紫外光辐照后，△αs为0．02；质子辐照效应对涂层仅。的变化影响较大。另外，研究了涂层厚度对αs和其与基材结合力的影响，以及基材表面处理工艺对涂层在-196—150℃冷热交变循环试验中可靠性的影响。     

基于线性神经网络的滑油金属含量预测

利用神经网络方法对某型航空发动机滑油监控系统中需重点监控的金属元素含量建立了网络，并根据该模型对其含量变化趋势进行了预测分析。某部队通过对不同实测数据的检验证明，可根据该模型的预测结果预报金属含量是否超标。     

AD7714功能及应用

本文介绍了模数转换器AD7714的性能，特点及在压力测量方面应用。     

多线程控制技术在面向对象实时仿真中的应用

随着实时仿真复杂性的提高,单个的处理器不足以完成所有的必需仿真计算任务。希望能在不同的处理器上完成实时仿真的不同任务,对称多处理器的机制需要软件支持,以使每个处理器通过共享内存进行信息交换。利用多线程控制技术,可以在非全进程开销或不使用共享内存的条件下,使用多处理器。其理由在于线程本身就蕴涵有共享地址的概念。一个多线程的实时程序,利用其中的主线程控制其它的辅助线程,每个处理器用于完成一个辅助的实时计算线程,主线程负责实时时钟的监控,当时钟到达时,启动相应的辅助线程,辅助线程利用图形用户界面(GUI)来监控仿真的进行。     

直升机航姿信号仿真研究及其在电子特设系统综合模拟试验中的应用

本文介绍了某直升机电子特设系统综合模拟试验的直升机运动仿真模型,在此基础上着重对直升机航姿信号两种仿真方法进行了详细的阐述,并对两种方法的仿真试验结果进行了分析比较,指出了各自的优缺点。     

二维Euler方程的非结构网格再生成自适应方法

给出了提高二维Ｅｕｌｅｒ方程定常解质量的非结构网格自适应方法和模拟结果。流场算法为结点型有限体积法和Ｌａｘ－Ｗｅｎｄｒｏｆｆ格式，网格用阵面推进法生成，生成初始网格时使用均匀的直角坐标背景网格。     

三角翼低速动态大攻角气动特性试验研究

对后掠角分别为X=60°、70°和80°尖前缘平板三角翼模型和一个前缘后掠角为（76° 40°）的双三角翼模型在低速风洞中作大攻角俯仰摩波运动，振幅am=30°、60°和90°，缩减频率K=0.01～0.12，基于根弦长雷诺数Re=2.76×10^5～8.23×10^5。进行了六分量动态气动载荷测量，动态流动显示和70°三角翼上翼面非定常压力测量，并分别与对应的静态试验结果比较。分析了运动参数包括缩减频率、振幅和Re数、后掠角对气流动态迟滞特性的影响。     

500 – 3200 Å observations of the interacting binary stars V356 Sgr and β Lyr

In this paper we present new results from the Voyager ultraviolet spectrometers and the IUE spacecraft on V356 Sgr and β Lyr. The V356 Sgr observations cover, in detail, two eclipses and include one IUE high dispersion SWP image. During both eclipses the total strength of the UV emission lines were found to be invariant. Also, an uneclipsed UV continuum was detected at wavelengths shorter than 1600 Å. The IUE high dispersion SWP spectrum revealed that the emission lines are extremely broad, almost symmetrical lines with weak, slightly blue shifted absorption components. No evidence of carbon is seen in the emission or absorption spectrum of V356 Sgr in eclipse. A model for the origin of the circumstellar matter in this binary system is presented. The Voyager ultraviolet observations of β Lyr show a strong far-UV continuum that is detectable down to 912 Å The far-UV continuum flux level was variable on time scales shorter than the orbital period and displayed no obvious orbital modulation or eclipses. The spectral shape of the far-UV continuum closely resembles that of a UX UMa type cataclysmic variable. On 16 August 1985 an rapid brightening of the far-UV continuum was observed which was also reminiscent of cataclysmic variables. Analysis of the β Lyr data suggest that the central object must be small, with a radius on the order of 1 R_⊙ or less.     

Error Analysis of Space-Stable Inertial Navigation Systems

The error equations for a space-stable inertial navigation system are derived. This is done by directly perturbing the mechanization equations in the inertial frame and then transforming in open-loop fashion to the local-level frame. A rotating inertial platform and velocity and altitude damping are considered. The relations between errors in space-stable and local-level systems are noted. Numerical results are presented for certain random error sources.