全弹性稳态微小流量测量系统

介绍了一种采用质量测量法的液体微小流量测量系统的工作原理与工作过程.系统采用全弹性连接方法设计,避免了常规质量测量法流量测量装置中非弹性连接管路造成的测量误差.采用压力补偿方法,修正由于压强对增压气体密度的影响.并以酒精为测试液体,进行了5种工况下流量测量试验.试验结果表明,该套微小流量测量系统工作稳定、可靠,可以精确测量出液体稳态微小流量.      

超宽带脉冲无线电在近距编队中的应用研究

编队飞行航天器间可靠的实时通信和精确的定位是需要解决的关键技术之一。超宽带脉冲无线电技术具有抗多径干扰、传输速率高、结构简单且可进行通信和导航一体化设计等鲜明特点。本文首先介绍超宽带脉冲无线电的基本原理,分析其主要特点,在跟踪编队飞行无线链路现有技术的基础上,研究了超宽带技术在近距编队中的潜在应用,最后分析了超宽带技术在航天器近距编队应用中需要注意的问题。     

航空碳纤维树脂基复合材料加筋板压缩屈曲及后屈曲性能

开展了复合材料加筋板轴压稳定性实验,对加筋板的屈曲及后屈曲性能、破坏模式和后屈曲失效表征进行了研究.实验结果表明加筋板在轴压下具有良好后屈曲承载潜能,破坏载荷约为屈曲载荷的2.2倍;其屈曲模式为筋条间蒙皮首先发生屈曲失稳,筋条在整个承载过程中保持直线,起到“屈曲分隔”的作用.通过对加筋板屈曲及后屈曲性能的理论分析,得出的理论屈曲载荷和理论破坏载荷与实验结果相对误差均小于8%,并确定了在后屈曲过程中蒙皮中心挠度的变化规律和轴向载荷的面内分布特征.      

Effect of sodium tartrate concentrations on morphology and characteristics of anodic oxide film on titanium alloy Ti–10V–2Fe–3Al

The effect of sodium tartrate concentrations on morphology and characteristics of ano-dic oxide film on titanium alloy was investigated. The alloy substrates were anodized in different concentration solutions of sodium tartrate with the addition of PTFE emulsion and their morphol-ogy and characteristics were analyzed. The anodic oxide film presented a uniform petaloid drums and micro-cracks morphology. Additionally, micro-cracks dramatically swelled with the increase of the tartrate concentrations. The thickness of the anodic oxide film increased with the concentra-tions until the concentration reached 15 g/L. The results of Raman analysis illustrate that all sam-ples have similarity in the crystal structure, consisting of mainly amorphous TiO2, some anatase TiO2 and a small amount of rutile TiO2. And the ratios of anatase TiO2 and rutile TiO2 increase with the concentrations until it reaches 15 g/L. Furthermore, the intensity of the peaks increases with enhanced concentrations until the concentration reaches 15 g/L. The corrosion resistance of the anodic oxide film is increased by the sodium tartrate with higher concentrations before 15 g/L. The coefficient of friction of the anodic oxide film reduces with the concentrations until the concentration reaches 15 g/L, then the coefficient of friction of the anodic oxide film increases with the concentrations.     

(高)超声速流动试验技术及研究进展

近年来,与高速飞行器相关的(高)超声速流动受到了极大的关注。这类流动所具有的非定常性、强梯度和可压缩性对试验方法和风洞设计技术提出了挑战。超声速纳米示踪平面激光散射(NPLS)技术是由作者所在团队研发的非接触光学测试技术。它能够以较高的空间分辨率来揭示超声速三维流场的一个瞬态剖面的时间解析的流动结构。介绍了NPLS技术以及基于NPLS开发的密度场测量、雷诺应力测量和气动光学波前测量等方法,并回顾了这些技术在超声速边界层、超声速混合层、超声速压缩拐角、激波/边界层相互作用和光学头罩绕流等流动中的应用,清晰地再现了边界层、混合层、激波等典型流场结构及其时空演化特性。另外,为了模拟和研究高空大气条件下边界层自然转捩和超声速混合层的转捩特性,介绍了高超声速静风洞、超-超混合层风洞的设计技术以及层流化喷管的设计方法。     

基于DDES的有／无舱门腔体气动噪声仿真分析

采用延迟分离涡仿真（ DDES）的方法研究了空腔和带有舱门的腔体的气动噪声特性。仿真在自由来流M＝0．85下,长宽深比值为5：1：1的矩形开放腔体展开。空腔仿真的声压级幅值结果与试验数据相比误差在4％以内,频率位置的预测较好。 DDES方法对于气动噪声问题具有很好的仿真准确性。空腔仿真结果和带有舱门的结果对比后表明,舱门迫使剪切层气流更多的撞击后壁进入腔体内部,使腔体内部尤其是中部压强波动增大,声压级在低频部分增量显著,达到了5 dB左右。     

内压缩段构型对高超声速进气道自起动性能的影响

为了探寻内压缩段构型对高超声速进气道自起动性能的影响,对二元高超声速进气道折角型和曲线型两种内压缩段的自起动过程进行准定常数值仿真研究.对比了这两种构型进气道在不同唇罩起始压缩角下的自起动性能和自起动过程中分离区的变化规律,并分析了内通道压缩强度沿程分布对进气道自起动性能的影响.研究表明:①即使进气道内收缩段的内收缩比相同,不同的内压缩段构型和唇罩起始压缩角对高超声速进气道的自起动性能影响显著,曲线型内压缩段构型的自起动性能明显优于折角型;②内压缩段的总压缩强度及其沿流向分布都是影响高超声速进气道自起动性能的关键因素,并且压缩强度沿流向分布决定着进气道在自起动过程中处于临界状态下主分离包所停留的位置.      

考虑陀螺效应的转子动力学相似准则

针对考虑陀螺力矩的转子系统缩尺相似模型与原型是否满足动力学相似的问题,采用量纲分析法推导了考虑陀螺力矩的转子-简单支撑系统相似准则,得到了模型与原型各物理量相似比.通过求解不同相似比下Jeffcott转子系统临界转速的解析解,和利用有限元软件ANSYS对某转子系统临界转速和振型相似性进行了数值模拟,验证了所推导的考虑陀螺力矩转子系统相似准则的正确性.研究表明:考虑陀螺力矩、简单支撑和Rayleigh比例阻尼的转子系统,在相似转速下缩尺模型与原型的固有频率具有相似性,并且临界转速相似.      

Relativistic electron fluxes and dose rate variations during April–May 2010 geomagnetic disturbances in the R3DR data on ISS

Space radiation has been monitored successfully using the Radiation Risks Radiometer-Dosimeter (R3D) installed at the ESA EXPOSE-R (R3DR) facility outside of the Russian Zvezda module of the International Space Station (ISS) between March 2009 and January 2011. R3DR is a Liulin type spectrometer–dosimeter with a single Si PIN detector 2 cm² of area and 0.3 mm thick. The R3DR instrument accumulated about 2 million measurements of the absorbed dose rate and flux of 10 s resolution. The total external and internal shielding before the detector of R3DR device is 0.41 g cm⁻². The calculated stopping energy of normally incident particles to the detector is 0.78 MeV for electrons and 15.8 MeV for protons. After the Coronal Mass Ejection (CME) at 09:54 UTC on 3 April 2010, a shock was observed at the ACE spacecraft at 0756 UTC on 5 April, which led to a sudden impulse on Earth at 08:26 UTC. Nevertheless, while the magnetic substorms on 5 and 6 of April were moderate; the second largest in history of GOES fluence of electrons with energy >2 MeV was measured. The R3DR data show a relatively small amount of relativistic electrons on 5 April. The maximum dose rate of 2323 μGy day⁻¹ was reached on 7 April; by 9 April, a dose of 6600 μGy was accumulated. By the end of the period on 7 May 2010 a total dose of 11,587 μGy was absorbed. Our data were compared with AE-8 MIN, CRESS and ESA-SEE1 models using SPENVIS and with similar observations on American, Japanese and Russian satellites.     

组合航天器转动惯量在轨两步辨识标定

在轨辨识转动惯量参数是主动航天器与非合作空间目标构成组合体后实现高精度姿态控制的重要前提,文章提出了一种两步在轨辨识组合航天器转动惯量参数的方法。第一步以航天器本体坐标系滚动轴转动惯量为基准将转动惯量矩阵归一化,得到特殊的转动惯量比矩阵,建立与其相关的姿态动力学模型,提出了基于扩展卡尔曼滤波的在轨辨识算法,基于星上陀螺角速率测量信息在100s左右辨识出所有转动惯量比参数,克服了由于模型简单导致转动惯量信息辨识不完整的缺点;第二步基于第一步辨识得到的转动惯量比参数,采用最小二乘算法辨识得到滚动轴转动惯量值,计算量小,消耗能量少。最后给出仿真算例,辨识精度基本在1|之内,验证了方法的有效性。