金属热防护系统边缘热短路研究

研究了金属热防护系统(TPS)的缝隙辐射及支架两大热短路问题。通过数值计算分析了缝隙宽度和缝隙辐射率对热短路的影响,完成了整体样件以及阵列组合件的稳态传热实验测试,定量地研究了热短路的影响情况。实验结果显示:支架处热短路现象明显,实验中支架引发的热短路温差高达50K;在773K以下,缝隙传热引发的温升随着缝隙宽度的增加而线性增加;在773K以上,辐射热传导在缝隙宽度超过3mm时即成为内部传热的主导机制,这时缝隙传热引发的温升不再随宽度增加而线性递增。所提供的数值分析和实验方法可为金属热防护系统的分析与设计提供重要的参考价值。     

Ti-6Al-4V钛合金激光弯曲成形微观组织研究

以1mm厚Ti-6Al-4V合金薄板为对象,运用光学金相显微镜、电子探针、扫描电子显微镜、氮氢氧联合分析仪、显微维氏硬度计,研究了特定累积线能量下90°弯曲角弯折区显微组织。结果表明,弯折区组织与累积线能量输入有关,当累积线能量在适当范围时,材料堆积增厚,极表层出现轻微复熔铸态组织,上层为板条马氏体α′,中层为针状马氏体α′,底层为长大粗化的(α+β)组织;距表层约0.2mm范围吸收间隙元素强烈致使硬度急剧提高并呈明显梯度;累积线能量输入过大,弯折区出现大面积复熔铸态组织并伴有裂纹产生。     

Height of shock formation in the solar corona inferred from observations of type II radio bursts and coronal mass ejections

Employing coronagraphic and EUV observations close to the solar surface made by the Solar Terrestrial Relations Observatory (STEREO) mission, we determined the heliocentric distance of coronal mass ejections (CMEs) at the starting time of associated metric type II bursts. We used the wave diameter and leading edge methods and measured the CME heights for a set of 32 metric type II bursts from solar cycle 24. We minimized the projection effects by making the measurements from a view that is roughly orthogonal to the direction of the ejection. We also chose image frames close to the onset times of the type II bursts, so no extrapolation was necessary. We found that the CMEs were located in the heliocentric distance range from 1.20 to 1.93 solar radii (Rs), with mean and median values of 1.43 and 1.38 Rs, respectively. We conclusively find that the shock formation can occur at heights substantially below 1.5 Rs. In a few cases, the CME height at type II onset was close to 2 Rs. In these cases, the starting frequency of the type II bursts was very low, in the range 25–40 MHz, which confirms that the shock can also form at larger heights. The starting frequencies of metric type II bursts have a weak correlation with the measured CME/shock heights and are consistent with the rapid decline of density with height in the inner corona.     

同轴波导与开放式同轴谐振腔的比较研究

文章介绍了同轴波导内场分布的计算公式以及开放式同轴谐振腔的场分布、谐振频率和品质因数的计算公式。通过对同轴波导和开放式同轴谐振腔的比较研究发现,开放式同轴谐振腔实质上就是纵向剖面为缓变截面的同轴波导。     

民用飞机飞控系统副翼下垂浅析

在飞机起飞或着陆飞行阶段,当缝翼伸出襟翼放下时,副翼也随之对称地下偏一定偏度,这就增加了机翼的弯度,提高了机翼升力。从而减少了飞机起飞／着陆的速度和场长,改善了起飞和着陆性能。通过介绍X飞机与Y飞机的副翼下垂功能的历史发展、功能原理与功能实现,较详细地分析了副翼下垂功能的实现方式。     

一个用于目标跟踪的改进粒子滤波算法

简化UT（unscented transformation）转化参数，修改UKF（unscented Kalmanfilter）提议分布，提出了改进的粒子滤波算法。调节因子的增加使得能在线自适应估计，滤波性能提高，并形成一个自适应的算法。仅有角测量的目标跟踪仿真试验证实了改进的粒子滤波算法要优于其它滤波方式。     

双周期带涂层纤维压电复合材料反平面问题分析

 研究双周期带涂层纤维压电复合材料反平面问题。利用Eshelby等效夹杂原理引入特征应变和特征电场,并结合双准周期Riemann边值问题理论,获得了问题在反平面机械载荷和面内电载荷作用时的解析解。由本文解的特殊情形可以退化为已有结果。数值算例考察了复合材料内部应力和电场随复合材料各组分电弹参数的变化规律,研究了纤维排列方式和纤维体积分数对复合材料有效电弹系数的影响。带涂层纤维正六边形排列时的有效电弹系数与广义自洽方法的预测结果非常接近。结果对新型航空材料的设计和优化具有参考价值。     

Drag Reduction for an Airship with Proper Arrangement of Propellers

In this article, the flow field around an airship with propellers blowing is calculated on the basis of the Reynolds-averaged Navier-Stokes equations with SST turbulent models. Modeled each as an actuator disk, the propellers are arranged at different positions around the body of airship in the flow direction. The numerical results show that the blowing propellers produce open outer flows. They drive the separated vortexes off the body thus reducing the drag coefficients. The results also show that the position after leading sucking peak is the best place for a propeller to blow. When the propellers are positioned after sucking peak, the longer the area which the propellers work on, the more the profile drag coefficients can be reduced. If the working position of propeller moves from the sucking peak forward to the leading edge, the friction drag coefficient will increase. The bigger the diameter of the propellers and the stronger the pressure jump, the more the drag coefficient will be reduced. The results also reveal that for the design of circularly-positioned propellers with space intervals, the more drag coefficient reduction results, the smaller the space interval is specified.     

斜向弹性支撑飞船座椅缓冲性能

当出现具有较大水平速度的斜冲击着陆工况时,飞船座椅头盆向冲击过载可能危及航天员生命安全。在现有的胸背向着陆冲击过载缓冲机构的基础上,引入座椅斜向弹性支撑模型,建立了斜向弹性支撑座椅缓冲系统的动力学模型。对具有较大水平速度的斜冲击着陆工况的仿真结果表明,相比于现有的铰接支撑缓冲系统,适当参数组合下的斜向弹性支撑座椅缓冲系统能有效降低航天员头盆向冲击过载且不增加胸背向冲击过载;综合支撑角度、刚度和阻尼各个参数影响规律,可以得到优化的座椅设计方案。