无筒空射运载火箭重力出舱机箭耦合动力学

研究了以运输机为平台的内装式空射运载火箭重力出舱载机-火箭两体动力学。根据火箭受力条件和相对运动自由度,将其出舱运动顺次分为5个阶段。给出了各阶段过渡的力学条件,基于牛顿-欧拉法分别建立了前4个阶段的机-箭两体动力学模型。定义了火箭出舱过程可能发生危险的多种异常情况,给出了发生异常的力学或几何条件。然后对火箭出舱全程作了数值仿真。若发射初始条件合理,仿真将顺次经历前4个或3个正常阶段,直至火箭离舱。如果异常情况的条件满足,火箭出舱将发生危险,仿真失去意义,故中止,需要调整发射初始条件后进一步仿真验证。本文给出的系统动力学模型和仿真数据可为工程部门设计空射型火箭的本体参数,以及设置空射初始条件提供参考。     

自动钻铆装备的激光测量系统法向误差研究

飞机装配中铆接部位的孔垂直度直接影响铆钉的连接质量和疲劳寿命,进而影响飞机的力学性能。为了保证飞机铆接垂直度要求,必须分析自动钻铆系统法向误差的影响因素。首先,确定了倾角误差、数学模型的线性误差与法向误差的关系。其次,给出了激光位移传感器安装参数的选取规律,并研究了其对位姿标定的影响。最后,实验验证了安装参数优化后的实际效果。研究结果可为法向测量装置的设计与分析提供理论指导,对于提升自动钻铆系统的法向精度,进而保证孔垂直度要求具有重要意义。     

软件测试用例生成与约简算法研究

对于参数多、状态多且状态转换关系复杂的软件,测试人员设计的测试用例往往难以保障测试覆盖率。针对该问题,提出了一种测试用例生成与约简算法。该方法定义了一种数据模型——测试路径控制阵列模型,将其与因果图法结合起来,可通过编程实现测试用例设计。该方法设计测试用例便捷、充分,避免了由于人工绘制因果图和检查判定表引入的错误。应用于实时系统软件的主副切换功能测试时,生成测试用例32个,对被测对象覆盖全面且有效。     

加筋壁板轴压载荷下稳定性有限元分析

使用有限元方法对组装壁板及整体壁板轴压载荷下的稳定性进行分析,计算轴压位移载荷情况下组装壁板及整体壁板的模态分布、应力分布及位移分布等,并对组装壁板进行了轴压试验,将试验结果与有限元结果进行了对比,表明有限元结果与试验结果吻合较好。最后对比组装壁板与整体壁板的分析结果发现,整体壁板的承载能力优于组装壁板。     

河北省产业集群研究

基于菱形模型来分析河北省目前产业集群的现状和存在的问题,在政府职能定位、创新、特色产业集群等角度试图探求集群升级的策略。     

Massive stars: Setting the stage

The paper gives a summary of the situation mid-1993 of theory and observations regarding massive stars. I describe: stellar mass loss and its implications, pre-main-sequence evolution, the main sequence, problems of atmospheric instability, Luminous Blue Supergiants, Yellow Hypergiants, Wolf-Rayet stars and supernovae.     

Detectors for infrared heterodyne mixing and detection

Conclusion For wavelengths < 50m fast and sensitive detectors are available. For wavelengths > 50m the available detectors are far from ideal. Research and development of far infrared detectors for the mixing purpose are highly recommended.     

Eye light flashes on the Mir space station

The phenomenon of light flashes (LF) in eyes for people in space has been investigated onboard Mir. Data on particles hitting the eye have been collected with the SilEye detectors, and correlated with human observations. It is found that a nucleus in the radiation environment of Mir has roughly a 1% probability to cause an LF, whereas the proton probability is almost three orders of magnitude less. As a function of LET, the LF probability increases above 10 keV/micrometer, reaching about 5% at around 50 keV/micrometer.     

Study of cosmic rays and light flashes on board Space Station MIR: the SilEye experiment.

The SilEye experiment aims to study the cause and processes related to the anomalous Light Flashes (LF) perceived by astronauts in orbit and their relation with Cosmic Rays. These observations will be also useful in the study of the long duration manned space flight environment. Two PC-driven silicon detector telescopes have been built and placed aboard Space Station MIR. SilEye-1 was launched in 1995 and provided particles track and LF information; the data gathered indicate a linear dependence of FLF(Hz) ( 4 2) 10(3) 5.3 1.7 10(4) Fpart(Hz) if South Atlantic Anomaly fluxes are not included. Even though higher statistic is required, this is an indication that heavy ion interactions with the eye are the main LF cause. To improve quality and quantity of measurements, a second apparatus, SilEye-2, was placed on MIR in 1997, and started work from August 1998. This instrument provides energetic information, which allows nuclear identification in selected energy ranges; we present preliminary measurements of the radiation field inside MIR performed with SilEye-2 detector in June 1998.