A roadmap to cave dwelling on the Moon and Mars

Habitat in lava tubes recently discovered on the Moon and Mars, should become a unifying concept for occupancy. Basic motivations and specifications for such a habitat are briefly reviewed.     

空气动压探头的动态响应研究

本文采用动力类比法对用于核爆炸测量的空气动压探头的动态响应进行了理论分析,并对探头的三个压力量程计算了总压边和静压边进气管道中的阻尼孔直径和动压波形的上升时间。分析计算表明,在探头的三个系统中,电学系统对动态响应的影响可忽略不计;力学系统的影响也是较小的;对动态响应起主要作用的是声学系统(即管道空腔系统)。在直径为130mm 激波管中进行了全尺寸探头的动态响应实验。实验表明,阻尼孔直径和波形上升时间的实验值与计算值符合较好。此探头曾多次用于我国大气层核试验测试中。从核爆炸和激波管实验中测得的空气动压波形可看出,它们的前沿都是很好的,这反映出此探头具有良好的动态响应特性。     

SuperDARN cross polar cap potential dependence on the solar wind conditions and comparisons with models

In this study SuperDARN Cross Polar Cap Potentials (CPCPs), collected over the year 2000, are investigated with a goal to statistically assess its relationship with various parameters of the solar wind and Interplanetary Magnetic Field (IMF). We show that SuperDARN CPCPs tend to cluster around discrete values, prescribed by the statistical model, unless the amount of points on each convection map is above ∼300. By selecting CPCP data obtained with radar coverage of >300 points, we investigate the CPCP relationship with IMF B_z and B_y, IMF clock angle, solar wind speed and dynamic pressure, Alfven velocity, Alfven–Mach number, and interplanetary electric field. Some reported tendencies, such as dependence upon IMF B_z, were found to be consistent with measurements by other instruments. We demonstrate that SuperDARN CPCPs show consistency with several theories/empirical models (predicting the CPCP) in terms of a linear trend but, on average, the slopes of the dependencies are at least two times smaller. We also determine the coupling function, out of those published in literature, best correlating with SuperDARN CPCPs.     

宽带信号角跟踪和四通道单脉冲方案

分析了宽带信号角跟踪的特殊问题及其实现方案。基于互相关函数的角误差检测方法,推导出了在非相关噪声及相关噪声背景下差路信号的输出信噪比及其角度随机误差的数学表达式,进而给出了带宽增益和最佳带宽的概念,以及提高输出信噪比的方法。为了在低载噪比（C/N）时获得角捕获所需要的和路信号以及差路的归一化信号,提出了四通道单脉冲方案。最后归纳出了低C/N时宽带信号角捕获和角跟踪的几种方法并提出了建议。     

飞机机头气动补偿空速管的设计

针对某飞机需要在机头配置空速管的设计要求,提出了采用机头气动补偿空速管的设计方法并给出了设计思路.通过数值计算得到了该飞机的机头位置误差,由此给出了一种气动补偿空速管外形;对给出的空速管的气动补偿特性进行了计算,并通过风洞试验对比验证了模型和数值计算方法的正确性,得到了该空速管的补偿曲线和补偿区的最佳静压开孔位置;在此...     

螺旋形纳米碳纤维的电磁波吸收特性分析

根据手征材料的本构方程,讨论了螺旋形手征纳米气相生长碳纤维(VGCF)手征参数ξ与电磁参数ε,μ的关系,并分析螺旋形VGCF几何结构产生的手征特性,与电磁波相互作用时产生电磁交叉极化的耦合吸收电磁波的机理,研究了改善手征材料ξ和性能的方法。结果表明,取螺旋形VGCF半径与螺距比为0.23左右,增加手征体含量可改善手征介质的手征参数,手征体的含量适当、螺旋形VGCF的尺寸与电磁波的波长接近能提高材料的吸波能力。     

纵向加速流场中风速管系数的理论修正

基于理想不可压轴对称位流理论，求得一任意椭球在纵向加速流场中绕流的精确解。并以一根细长的棉球近似模拟风速管，求得均匀流中风速管系数理论值，以及在纵向加速流中它的相对偏差值。以两个长细比各为32和250的椭球为算例，得知在一般风洞实验段内存在的速度梯度下，风速管系数的相对偏差量很小。文中表1、表2所列不同加速下风速管系数的相对偏差值，可近似用来修正实际风速管，或根据流场加速程度选择合适的风速管外径的大小。     

Formability enhancement in hot spinning of titanium alloy thin-walled tube via prediction and control of ductile fracture

The damage and fracture in hot spinning of titanium alloy is a very complex process under the combined effects of microstructure evolution and stress state. In this study, their dependences on processing parameters were investigated by an integrated FE model considering microstructure and damage evolution, and revealing the effects of microstructure and stress states on damage evolution. The results show that the inner surface of workpiece with the largest voids volume fraction is the place with...     

承压管道壁厚自动化检测系统研制

研制一套自动化超声检测系统,对1~2 mm壁厚承压管道的均匀性进行检测,获得承压管道全壁厚信息,为航天系统中的承压管道可靠性和安全性设计提供依据。超声检测系统采用六点矩阵控制方法,获取承压管道周向的全壁厚信息。文中研制的系统包括超声硬件系统;机械执行系统,实现超声换能器的夹持与运动;超声软件系统,搭建数据算法,对检测信号进行分析处理。试验结果表明该自动化超声检测系统对承压管道全壁厚信息的检测精度不低于0.02 mm。该超声检测系统对其它无损检测研究和系统开发具有很好的参考价值。     

The bistatic radar capabilities of the Medicina radiotelescopes in space debris detection and tracking

An accurate measurement of the position and trajectory of the space debris fragments is of primary importance for the characterization of the orbital debris environment. The Medicina Radioastronomical Station is a radio observation facility that is here proposed as receiving part of a ground-based space surveillance system for detecting and tracking space debris at different orbital regions (from Low Earth Orbits up to Geostationary Earth Orbits). The proposed system consists of two bistatic radars formed by the existing Medicina receiving antennas coupled with appropriate transmitters. This paper focuses on the current features and future technical development of the receiving part of the observational setup. Outlines of possible transmitting systems will also be given together with the evaluation of the observation strategies achievable with the proposed facilities.