地外人工光合成装置研制与试验

原位资源利用技术是地外生命保障体系构建、实现人类地外生存的有效途径，是载人深空探索的核心技术。基于微通道技术的人工光合成反应器，采用流动反应器设计，用于低微重力等特殊环境条件下模拟人工光合作用，实现CO２向O２和含碳燃料的转化。微通道芯片通过气液剪切作用力使气体反应产物快速脱离电极表面并随反应介质排出反应器，理论上可以克服微重力条件对反应过程的影响，尚需进行微重力试验进行验证。同时，微通道结构可以通过精确控制反应气液的压力、流速、流量比等反应条件，获得优化的反应条件。通过地面试验，验证了该反应器将CO２还原为O２和含碳化合物的功能可行性。以Au和Ir/C作为阴极和阳极材料，3V电压条件下，O２产率可达11.74mL/h。此外，基于人工光合成反应器搭建了集反应模块、控制模块、流路驱动模块以及检测模块等于一体的地外人工光合成装置，形成原位反应、介质供给、精确控制、在线收集和检测等功能一体化的系统，并实现CO２有效转换和O２供给。为后续技术成熟度更高的反应装置研制、高产物选择性的含碳化合物转化以及人工光合成反应装置在轨试验奠定了理论和实践基础。     

Study of the rheological properties of water and Martian soil simulant mixtures for engineering applications on the red planet

The rheological properties of mixtures of water and the Martian soil simulant JSC-Mars-1A are investigated by preparing and testing samples at various solids concentrations. The results indicate that the dispersion is viscoelastic and, at small timescales (～0.1?s), reacts to sudden strain as an elastic solid. At longer timescales the dispersion behaves like a Bingham fluid and exhibits a yield stress. Hysteresis loops show that rapid step-changes (2?s duration) of shear-rate result in thixotropic behaviour, but slower changes (>10?s duration) can result in rheopexy. These observations are explained with the breakdown and recovery of the packing structure under stress. The rheological information is used to generate practical tools, such as the system curve and the Moody chart that can be used for designing piping systems, and calculating pump sizes and pressure requirements.     

A drilling tool design and in situ identification of planetary regolith mechanical parameters

The physical and mechanical properties as well as the heat flux of regolith are critical evidence in the study of planetary origin and evolution. Moreover, the mechanical properties of planetary regolith have great value for guiding future human planetary activities. For planetary subsurface exploration, an inchworm boring robot (IBR) has been proposed to penetrate the regolith, and the mechanical properties of the regolith are expected to be simultaneously investigated during the penetration process using the drilling tool on the IBR. This paper provides a preliminary study of an in situ method for measuring planetary regolith mechanical parameters using a drilling tool on a test bed. A conical-screw drilling tool was designed, and its drilling load characteristics were experimentally analyzed. Based on the drilling tool-regolith interaction model, two identification methods for determining the planetary regolith bearing and shearing parameters are proposed. The bearing and shearing parameters of lunar regolith simulant were successfully determined according to the pressure-sinkage tests and shear tests conducted on the test bed. The effects of the operating parameters on the identification results were also analyzed. The results indicate a feasible scheme for future planetary subsurface exploration.     

A参量在高频阻抗测量中的应用

根据微波网络理论提出了利用A参量求解高频阻抗的新方法,并将其应用于网络分析仪系统,对短波阻抗进行了测量。实践证明,该方法与传统的利用S参量的方法(利用反射系数)相比大大地拓宽了阻抗测量范围,在通用仪器上获得了比专用仪器高的测量精度,同时还解决了网络分析仪与非同轴网络的连接问题。     

直射式喷嘴喷雾特性的实验研究

用二维激光测速测粒仪,对直射式喷嘴在横向气流中所形成喷雾的粒度、平均和脉动速度,以及浓度进行了测量。研究了喷雾的结构,气流速度以及喷射方向对喷雾特性的影响,不同直径的粒子在横向的扩散。为两相流模型的研究以及数值计算结果的验证提供实验数据。      

螺桨飞机缩比模型表面声压预测的验证试验

介绍了在室外进行的螺浆飞机缩比模型的噪声测量试验,目的是验证改进的螺浆飞机声场模型,它可预测任意形状机身边界的表面声压分布。介绍了试验,噪声测量以及预测方法,预测和试验结果的比较表明得到了较满意的符合。      

Al－Al_3Ni自生复合材料的高周疲劳损伤断裂机制及其应力比的影响

实验观察和研究了Ａｌ－Ａｌ３Ｎｉ自生复合材料的高周疲劳损伤断裂行为以及应力比Ｒ的影响,结果显示在Ｒ＝－１疲劳过程中孔洞沿界面区基体的优先萌生、联接和扩展是其损伤断裂的主要机制;并且发现Ｒ对疲劳寿命及断裂过程有明显影响,当Ｒ＝０时滑移带裂纹生长相对容易,寿命减小,而Ｒ＝∞时,裂纹集中在类似于压缩变形的宏观形变带内发展,寿命很长     

高超音速后掠激波与边界层干扰流场特性

应用表面油流和液晶温度显示、表面热流率和压力测量四种测试技术,在Ma_∞=7.8、单位长度雷诺数尺Re_∞=3.5×10~7/m条件下,研究了30°迎角尖前缘翼面诱导激波和湍流边界层干扰流场特性。结果表明:表面流动是准锥型,在强相互作用下,流动发生了二次分离和再附,导致表面油流线的流向角、温度、热流率和压力分布均出现明显的凹坑。     

障碍物通道起爆过程高时空分辨化学发光测量研究

高时空分辨率的光学测量对认识障碍物通道中的火焰加速与起爆过程非常重要,通过自发光图像提取关键的火焰参数,可以深入地分析影响火焰加速的关键因素.为了研究障碍物对火焰加速与起爆过程的影响,采用高速化学发光测量手段,对障碍物通道中的火焰加速与起爆过程进行测量,测量的时间重复频率达到154kHz.在此基础上,提取燃烧强度、火焰...     

Dayside ionospheric uplift during strong geomagnetic storms as detected by the CHAMP,SAC-C,TOPEX and Jason-1 satellites

Ionosphere response to severe geomagnetic storms that occurred in 2001–2003 was analyzed using data of global ionosphere maps (GIM), altimeter data from the Jason-1 and TOPEX satellites, and data of GPS receivers on-board CHAMP and SAC-C satellites. This allowed us to study in detail ionosphere redistribution due to geomagnetic storms, dayside ionospheric uplift and overall dayside TEC increase. It is shown that after the interplanetary magnetic field turns southward and intensifies, the crests of the equatorial ionization anomaly (EIA) travel poleward and the TEC value within the EIA area increases significantly (up to ∼50%). GPS data from the SAC-C satellite show that during the main phase of geomagnetic storms TEC values above the altitude of 715 km are 2–3 times higher than during undisturbed conditions. These effects of dayside ionospheric uplift occur owing to the “super-fountain effect” and last few hours while the enhanced interplanetary electric field impinged on the magnetopause.