球面密封结构密封性能初步测试

球面密封结构是卫星推进系统中重要的密封结构。为了对它的密封性能进行研究,专门设计了一个试验平台,选择了相应的检漏设备、充气设备和安装设备。经过试验,发现了密封表面加工质量对密封性能的影响。经过分析,研究了球面结构的泄漏机理,提出了保证密封性能的措施。     

Integral inversion of GRAIL inter-satellite gravitational accelerations for regional recovery of the lunar gravitational field

We present an integral-based approach for high-resolution regional recovery of the gravitational field in this article. We derive rigorous remove-compute-restore integral estimators relating the line-of-sight gravitational acceleration to an arbitrary order radial derivative of the gravitational potential. The integral estimators are composed of three terms, i.e., the truncated integration, the low-frequency line-of-sight gravitational acceleration, and the high-frequency truncation error (effect of the distant zones). We test the accuracy of the integral transformations and of the integral estimators in a closed-loop simulation over the Montes Jura region on the nearside of the Moon. In this way, we determine optimal sizes of integration radii and grid discretisation. In addition, we investigate the performance of the regional integral inversion with synthetic and realistic GRAIL observations. We demonstrate that the regional inversion results of the disturbing gravitational potential and its first order radial derivative in the Montes Jura mountain range are less contaminated by high-frequency noise than the global spherical harmonic models.     

Multi-beam sounding ionograms in the polar cap region: Absorption induced by proton precipitations

The simulation of the multi-beam ionograms in the polar cap region, assessing absorption effect is performed. It is reasonable to distinguish among four different mechanisms responsible for absorption: regular absorption due to solar UV illumination, absorption associated with energetic particles precipitation, absorption connected with X-rays flare and additional absorption in Auroral oval area. In this paper the absorption attributed to proton precipitations is envisaged. The computational model of the high-latitude ionosphere with irregularities oriented to application for the high frequency wave propagation problem was elaborated (Zaalov et al., 2005). A number of the quasi-vertical ionograms in the polar cap region were simulated on the basis of this model. A well-known algorithm (Sauer and Wilkinson, 2008) is applied for the absorption effects calculation. The simulated high-latitude ionograms with the absorption effect and the measured ionograms exhibit quite a good resemblance. This paper illustrates the importance of the understanding and taking into account the absorption effect in the presence of the various structural features in the polar ionosphere (in particular, patches of enhanced electron density) in interpreting ionosonde data.     

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.     

基于电子束蒸发沉积的曲面纳米薄膜均匀性研究

半球谐振子金属化是半球谐振陀螺研制过程中的重要环节，针对半球表面薄膜制备均匀性难以实现的问题，提出了一种将薄膜沉积实验和光学模拟相结合的方法。本文采用电子束蒸发技术在半球上沉积Au薄膜，利用台阶仪测量球面上不同位点的薄膜厚度，将平面上的膜厚等效为半球曲面上的膜厚，研究球面薄膜的均匀性，得出了在半球内外表面上薄膜的膜厚分布；同时对薄膜沉积均匀性进行光学模拟，将半球探测器上辐照度等效为实验中沉积所得到的薄膜厚度，计算得出的半球探测器上辐照度分布与实验测量结果一致性较好，可为半球谐振子纳米薄膜的均匀性制备提供理论基础。     

High-resolution, coupled thermosphere–ionosphere models for space weather applications

Current first-principles global models of the coupled thermosphere–ionosphere (T–I) system use grids that are too coarse to simulate the mesoscale and small-scale structures that occur in this complex system. These small-scale and mesoscale structures have a great effect on global-scale neutral and plasma distributions and have important consequences for daily space weather. In this paper, we present a new first-principles, high-resolution, T–I nested grid (TING) polar cap model that incorporates multiple nesting levels and two-way interaction. The TING model simulation of the electron densities and temperatures demonstrates the importance of high spatial resolution. It is found that both the mid-latitude electron density trough and its associated dawn electron temperature peak are more pronounced and structured in the nested grid than in the coarse grid. Using the TING model to simulate ionospheric F₂ region electron density variations with geomagnetic activity and universal time (UT) is also discussed.     

基于飞行测量的弹性轴承试验载荷谱修正和寿命评估方法

球柔性旋翼系统在我国自主设计的直升机上获得了广泛的应用，弹性轴承在其中承担着重要角色，它提供了旋翼旋转过程中桨叶的挥舞、摆振和扭转运动，传递了旋转产生的离心力、挥舞方向的升力和摆振方向扭矩产生的切向力。文章讨论了不同设计阶段弹性轴承载荷谱的获得，基于飞行载荷测量的弹性轴承载荷谱修正，不同载荷谱对弹性轴承损伤影响的等效分析方法和弹性轴承寿命评估。     

基于球堆叠的月壤蓄热器传热特性数值研究

月壤蓄热是月球原位资源利用的一种重要方式，也是解决未来月球基地能源需求的最具潜力的途径之一。针对月壤蓄热过程，建立了基于球形堆叠的月壤蓄热器多孔介质蓄热模型。蓄热器的壳体采用登月舱下降级的燃料罐，流体传热介质采用氦气。通过数值模拟的方法研究了不同流动压降下月壤蓄热球堆叠方式、球直径对蓄热器传热过程的影响规律和机理，并分析了蓄热动态过程。研究结果表明，月壤蓄热球在简单立方体均匀堆叠（SC）和面中心立方体均匀堆叠(FCC)两种方式下，SC堆叠方式的综合蓄热指数比FCC模式可提高302%；同时还发现月壤蓄热球的直径存在最优值，可使得蓄热器在单位泵功下获得最大的蓄热量，并且该最佳值随着流体进出口压差增加而减小。该研究可为未来月壤蓄热器的设计和优化提供理论指导。     

特殊复合球铰3-RPS并联机构及其连续刚度模型

采用矢量微分法研究了在大载荷作用下,兼顾支链和铰链刚度以及雅克比矩阵变化等影响因素的3-RPS并联机构完整连续刚度模型.基于螺旋理论分析了3-RPS并联机构支链及铰链构件所受作用力与机构外载荷之间的力平衡关系.采用矢量微分法分析了3-RPS并联机构动平台位姿变化与支链及铰链构件变形之间的关系.采用矢量微分法对机构的力学平衡方程进行微分,建立了完整的连续刚度模型,最后进行了数值模拟分析,结果表明并联机构刚度受载荷和位姿变化影响,简化刚度模型与完整刚度模型在工作空间边界处差值较大.     

空间大型星载抛物面天线研究进展

抛物面天线作为星载天线的重要组成部分,在深空探测、移动通信、国防事业、气象监测等方面均具有广泛应用,近年来随着上述学科的快速发展,抛物面天线的研究也越来越受到人们的重视。针对空间大型星载抛物面天线的发展与需求,首先系统地概括了国外星载抛物球面天线的发展现状,综述了刚性、网状以及充气式星载抛物球面天线,对各类星载抛物球面天线的结构、性能进行了较为详细的描述和分析,对国内在该领域的部分研究成果进行了简述。然后梳理了星载抛物柱面天线的发展,对国内外具有代表性的抛物柱面天线进行了介绍,对抛物球面天线和抛物柱面天线进行了参数对比与分析。接下来对近年来针对星载抛物面天线的相关技术进行了介绍。最后对星载抛物面天线的发展趋势做了简要分析与预测。