用于直升机现场计量的低频振动校准技术

本文面向直升机健康与使用监测系统(HUMS)的现场计量保障需求,针对其中振动传感器在低频段尚无法实现现场校准的现状,提出了基于直线电机驱动技术的便携式低频振动校准技术方案。该方案利用高精度直线电机构造低频标准振动源,采用稳定性高的石英挠性加速度计作为标准加速度计,具有体积小、精度高、现场环境适应性好的特点,非常适用直升机HUMS的现场计量保障。根据不确定度评估结果,该方案能够实现0.5Hz～20Hz频率范围,0.01m/s~2～20m/s~2加速度范围内不超过1%的校准不确定度(k=2)。     

某测试台谐波摇摆运动的控制

某测试台主要运动方式为三自由度正弦摇摆Asinωt,三次谐波摇摆。本文详细阐述了该设备三次谐波谱的精密运动控制、在线实时轨迹显示和静态FFT分析。     

三叉杆式万向联轴器采用调心轴承时的运动分析

分析了三叉杆式万向联轴器采用调心轴承时输出转角和输入转角之间的关系式,并得出这种联轴器为准等角速传动万向联轴器的结论;讨论了轴偏转角大小对输出输入转角差值的影响,分析表明,这种联轴器中转角差值的变化周期是输入轴自转周期的3倍。     

The Primordial Helium-4 Abundance from Observations of a Large Sample of Blue Compact Dwarf Galaxies

We use a sample of 45 low-metallicity H II regions in blue compact dwarf (BCD) galaxies to determine the primordial helium abundance YP with a precision better than 5%. We have carefully investigated the physical effects which may make the He I line intensities deviate from their recombination values such as collisional and fluorescent enhancements, underlying He I stellar absorption and absorption by Galactic interstellar Na I. By extrapolating the Y vs. O/H and Y vs. N/H linear regressions to O/H = N/H = 0, we obtain YP = 0.244±0.002 and 0.245±0.001, respectively, higher than previous determinations (YP = 0.230 - 0.234). Part of the difference comes from the fact that previous investigators have not taken into account underlying He I stellar absorption, especially in the NW component of the BCD I Zw 18 which, because of its extremely low metallicity plays a key role in the determination of YP. We derive a slope dY/dZ = 2.3±1.0, considerably smaller than those derived before. With this smaller slope and taking into account the errors, chemical evolution models with an outflow of well-mixed material can be built for star-forming dwarf galaxies which satisfy all the observational constraints. Our YP gives _bh ₅₀ ² = 0.058±0.007,f consistent with the lower limit set by dynamical measurements and X-ray observations of clusters of galaxies. It is also consistent, within the framework of standard big bang nucleosynthesis theory, with measurements of primordial 7Li in galactic halo stars and with the D/H abundance measured in absorption systems toward quasars by Burles and Tytler (1997).     

钯改性镍基高温合金铝化物涂层的组织和热腐蚀性能

以M38合金作基材，先电镀Pd-20wt%Ni合金，再采用传统低温高活性(LTHA)固渗铝工艺，用NaCl作活性剂渗铝制得Pd-Ni-Al涂层。XRD和EPMA分析结果表明，涂层为固溶Ni的β-PdAl单相结构；在900℃Na     

Particle simulation of grid system for krypton ion thrusters

The transport processes of plasmas in grid systems of krypton (Kr) ion thrusters at different acceleration voltages were simulated with a 3D-PIC model, and the result was compared with xenon (Xe) ion thrusters. The variation of the screen grid transparency, the accelerator grid current ratio and the divergence loss were explored. It is found that the screen grid transparency increases with the acceleration voltage and decreases with the beam current, while the accelerator grid current ratio and divergence loss decrease first and then increase with the beam current. This result is the same with Xe ion thrusters. Simulation results also show that Kr ion thrusters have more advantages than Xe ion thrusters, such as higher screen grid transparency, smaller accelerator grid current ratio, larger cut-off current threshold, and better divergence loss characteristic. These advantages mean that Kr ion thrusters have the ability of operating in a wide range of current. Through comprehensive analyses, it can be concluded that using Kr as propellant is very suitable for a multi-mode ion thruster design.     

西部地区高校国际交流与合作现状及思考

在经济全球化,教育国际化的大背景下,西部地区高校和西部大开发的强劲东风,积极拓展了教育国际间的交流与合作,有力地推动了西部地区高等教育国际化的进程。但又由于受地域偏远、交通不发达和经济发展缓慢的影响,西部地区高校国际交流与合作和我国东部发展地区相比,在广度和深度方面还有很大的差距,面临着很大的发展空间。     

应用模糊变权的启发式搜索进行飞行轨迹优化

回顾了军机轨迹优化问题的提出及研究历史，介绍了几种主要方法的特点，特别是启发式搜索算法应用于飞行轨迹优化问题时存在的主要问题。提出为了得到较好的近优路径而采取的模糊变权处理方法。通过计算不同加权下解的情况，说明模糊变权方法是使加权随具体情况作相应调整的有效手段，为提高飞行路径规划系统的有效性开辟了一个新思路。     

运用SSM探讨高校科研成果的产业化

软系统方法（ＳＳＭ）是一个学习系统，能帮助人们认识人类问题的复杂环境，为人们提供一种用系统的观点认识软问题的思想方法。运用软系统方法综合分析高校科研成果产业化所面临的形势及存在的问题，按照根定义建立概念模型，然后经过理想的概念模型与现实的比较，得出了一系列解决问题的方法与策略。对在新形势下如何促进高校科研成果产业化做了有益的探讨。     

Crew autonomy for deep space exploration: Lessons from the Antarctic Search for Meteorites

Future piloted missions to explore asteroids, Mars, and other targets beyond the Moon will experience strict limitations on communication between vehicles in space and control centers on Earth. These limitations will require crews to operate with greater autonomy than any past space mission has demonstrated. The Antarctic Search for Meteorites (ANSMET) project, which regularly sends small teams of researchers to remote parts of the southern continent, resembles a space mission in many ways but does not rely upon a control center. It provides a useful crew autonomy model for planners of future deep space exploration missions. In contrast to current space missions, ANSMET gives the crew the authority to adjust competing work priorities, task assignments, and daily schedules; allows the crew to be the primary monitor of mission progress; demands greater crew accountability for operational errors; requires the crew to make the most of limited communication bandwidth; adopts systems designed for simple operation and failure recovery; and grants the crew a leading role in the selection and stowage of their equipment.