2m量级高速风洞强迫振动动导数试验技术研究

为满足大型运输机、先进战斗机、推进与机体一体化布局等现代高性能飞行器动导数风洞试验研究的需求,基于小振幅强迫振动动导数试验原理,在中国空气动力研究与发展中心2 m 量级高速风洞(FL-26和 FL-28)建立了一套俯仰、滚转及偏航的三通道动导数试验技术。在试验系统研制过程中,首先采用强度高、刚性好的航空轻质铝材和复合材料解决了亚跨超声速条件下大尺度试验模型研制问题;其次,结合动力学和运动学仿真分析手段,实现并优化了大载荷试验装置传动机构设计以及α、β耦合双转轴支撑结构设计的难题;最后,在测控系统研制部分,通过电机选取、电磁干扰屏蔽、滤波器设计等技术手段进一步提高了测试系统的精度。试验系统设计技术指标Ma=0.4~4.25,迎角α=-35°~35°,侧滑角β=-15°~15°,传动机构法向承载载荷≤10000 N。SDM 标模的验证试验结果表明,直接阻尼导数与文献值一致性较好,重复性试验数据误差基本控制在10%以内。目前,该项试验技术已经成功应用于某大型飞机模型的动导数风洞试验。     

短距起飞/垂直降落发动机建模技术研究

参考常规双轴涡扇发动机数学模型,建立了适用于短距起飞/垂直降落(STOVL)飞机的变循环发动机部件级数学模型;通过特性外推,建立了轴驱动升力风扇数学模型;采用神经网络映射涵道总压损失的方法,建立了滚转喷管和外涵模型.根据STOVL发动机结构和部件变化特点,建立了稳态和动态共同工作方程.参照国外文献仿真数据进行设计点计算,并按照Bevilaqua提出方法开展了由常规涡轮风扇模式到悬停涡轮轴模式的过渡态仿真.仿真结果表明:建立的数学模型在悬停状态设计点和高空巡航点与国外文献数据相比误差均小于1.5%,推力达到悬停状态要求,符合STOVL发动机的设计特点,验证了该建模方法的有效性.      

Development of thermal sensors and drilling systems for lunar and planetary regoliths

We consider some novel concepts for thermal properties experiments aboard lunar landers or rovers, that may lead to an improved understanding of both the structure of the lunar near surface layers and the lunar thermal history. The new instruments could be developed using the experience and heritage from recently developed systems, like the Rosetta Lander thermal conductivity experiment MUPUS and existing designs used for terrestrial measurements of thermal conductivity. We describe shortly the working principle of such sensors and the main challenges faced when using them in the airless regolith layers of the Moon or other airless bodies. In addition new concepts to create appropriate drill holes for thermal and other measurements in the lunar regolith are discussed.     

流动显示的现状和发展

本文以第四届国际流动显示会议为主要内容,结合其它资料介绍流动显示的现状和发展。     

旋翼/机身组合模型试验台技术改进及验证

中国空气动力研究与发展中心研制的旋翼/机身组合模型试验台,具有阻塞度小、功率大、支架干扰小等优点.近年来,试验台通过配套研制标模系统、改进测量系统及旋翼操纵系统标定方法等工作,使试验台的水平和能力得到了进一步的提升.验证试验表明:该试验台技术先进、性能指标优良,安全稳定性好,试验数据精准度高,可作为直升机型号研制和课题研究可靠的试验平台.     

石墨渗铜喉衬材料的微观结构与抗热震性能

采用粗粒级高强石墨加压渗铜工艺，制备了石墨渗铜(CIG：copper-impregnated graphite)喉衬材料。对其微观结构与抗热震性能的关系进行了研究。结果表明，由于渗铜提高了原石墨的热导率及整体增韧的综合效果，使石墨渗铜材料比通用的5种石墨材料具有更好的抗热震性能，更好地适应了小型高性能战术导弹、航天飞行器高压强大流量SRM对喉衬材料的要求。     

A strategic “viewfinder” for SETI research

One of the most important reasons why unsuccessful results have been obtained so far by the SETI Project is due to the fact that no sure targets to aim at have been available up-to the present state of research. All-sky surveys, even if very accurate and complete, might result to be time-consuming. SETI needs at least one effective “viewfinder” in order that a true targeted research is carried out with a possible success. The best foundation to get this can be identified with the search for the evidence of extraterrestrial astro-engineering activity in form of the Dyson spheres predicted by theory. The existence of such stellar objects can be ascertained by finding the evidence of two main signatures in stars of solar spectral type: infrared excess and anomalous light curves due to transiting artificial objects. These are probably the most powerful viewfinders in order to allow SETI techniques for intelligent signal search to be aimed at more appropriate targets. This paper is not intended to be a research paper but rather a review paper whose goal is not to present calculations and/or operational research but rather to be a research proposal for a more focused research in SETI just using Dyson Spheres as crucial markers.     

基于一致性预处理技术的作业车间调度算法研究

为降低CSP调度算法的计算复杂度和减少搜索过程中回溯发生概率,采用一致性预处理技术来预先修剪和过滤搜索空间。仿真实验证明:两种方法的综合运用可以显著提高CSP调度算法的搜索效率,从而为CSP调度算法求解大规模作业车间调度问题提供可能。     

Near infrared studies of the massive X-ray binary 2S 0114+65

We present near-infrared spectroscopy of the massive X-ray binary 2S 0114+650. These observations covering the spectral range 1.08–2.35 μm span the region where Paschen and Brackett series recombination lines of hydrogen are expected to be seen, namely, Paβ , Brγ and Br 10–17 lines. The absence of any of these lines in emission supports earlier inferences that the optical component in 2S 0114+650 is unlikely to be a Be star but rather a B type supergiant. Near-IR photometry gives J = 8.78, H = 8.53 and K = 7.96; these values show marginal variations from earlier reported measurements.