银膜的原子氧剥蚀效应及其防护的试验研究

 空间太阳电池板作为空间飞行器电源系统的重要组成部分,它的正常工作对飞行器的运行起着非常重要的作用,而作为互连片的银材料,可能会与空间环境中的原子氧发生反应,生成不导电的氧化物,从而影响空间太阳电池板的有效寿命。本文在原子氧效应地面模拟试验设备中,对银以及镀有不同防护层的银膜进行了原子氧效应地面模拟试验研究,对试验前后试样的外观、质量进行了比较,获得了银在设备中的反应特点,同时对不同防护镀层的有效性进行了验证,为银互连片在空间太阳电池板上的应用及其防护提供了设计依据。     

多胞金属管受径向冲击时的吸能特性

针对某武器装备发射环节对能量吸收提出的要求,并结合当前薄壁金属管件的研究背景以及能量吸收的性能指标,分析了多细胞管件在受径向冲击时的吸能特性。结合实际工况,制定了传统多胞管和夹层多胞管两方面共5种方案,并运用ANSYS/LS-DYNA程序,对其进行逐一建模仿真。最后的结论分析显示,在工艺允许的情况下,夹层多胞管的4板Ⅰ向方案在能量吸收特性方面表现更加优越。     

Characterization of Solar Coronal Holes and Plumes Using Spectroscopic Diagnostic Techniques Applied to SOHO/CDS Observations

Results from a series of SOHO/Coronal Diagnostic Spectrometer (CDS) observations of coronal holes and plumes are presented, including analysis of a low-latitude plume observed in August 1996. Spectroscopic diagnostic techniques using the CHIANTI atomic database are applied to derive the plasma parameters: electron density, temperature, and element abundances. The results are compared with quiet sun values. Coronal electron densities in the holes are found to be about 2 × 10⁸ cm^-3, a factor of two to three lower than in the quiet sun. The plasma thermal distribution exhibits differences between coronal holes, the quiet sun and plumes. For example, the peak of the emission in coronal holes is at a lower temperature (T ⋍ 8 × 10⁵ K) than in the quiet sun (T ⋍ 1 × 10⁶ K), while plumes are cooler (T ⋍ 7.6 × 10⁵ K) and show a different distribution, closer to an isothermal state. This revised version was published online in June 2006 with corrections to the Cover Date.     

O5+ in High Speed Solar Wind Streams: SWICS/Ulysses Results

Recent observations with UVCS on SOHO of high outflow velocities of O⁵⁺ at low coronal heights have spurred much discussion about the dynamics of solar wind acceleration. On the other hand, O⁶⁺ is the most abundant oxygen charge state in the solar wind, but is not observed by UVCS or by SUMER because this helium-like ion has no emission lines falling in the wave lengths observable by these instruments. Therefore, there is considerable interest in observing O⁵⁺ in situ in order to understand the relative importance of O⁵⁺ with respect to the much more abundant O⁶⁺. High speed streams are the prime candidates for the search for O⁵⁺ because all elements exhibit lower freezing-in temperatures in high speed streams than in the slow solar wind. The Ulysses spacecraft was exposed to long time periods of high speed streams during its passage over the polar regions of the Sun. The Solar Wind Ion Composition Spectrometer (SWICS) on Ulysses is capable of resolving this rare oxygen charge state. We present the first measurement of O⁵⁺ in the solar wind and compare these data with those of the more abundant oxygen species O⁶⁺ and O⁷⁺. We find that our observations of the oxygen charge states can be fitted with a single coronal electron temperature in the range of 1.0 to 1.2 MK assuming collisional ionization/recombination equilibrium with an ambient Maxwellian electron gas. This revised version was published online in June 2006 with corrections to the Cover Date.     

低速轴流压气机旋转失速演化机制研究

为深入探讨轴流压气机旋转失速机理,利用全环非定常数值模拟在出口边界添加节流阀模型模拟压气机节流过程,通过试验测量与数值模拟结果对比分析,澄清了低速轴流压气机失速先兆及失速团的产生和演化过程。研究结果表明：压气机在转子叶片安装角存在几何偏差的情况下,spike型失速先兆是由2阶模态的整阶扰动演化而来,并最终直接形成2个大尺寸全叶高的失速团;与轴对称转子模型相比,考虑存在几何偏差的转子模型的数值模拟结果更为接近试验测量结果。     

折叠状航天器太阳电池阵在轨热分析(Ⅱ)--计算结果和分析

采用 SIP算法 ,对高 H =2 0 0 km的在轨航天器折叠状太阳电池阵的三维不稳定温度分布做了数值分析。计算时仔细考虑了不同时刻电池阵不同的热输入。计算网格 N =N1 × N2 × N3=14× 2 2× 2 2 =6776,初始温度T0 =2 78K。获得了抛罩 -展开Δ t=3 2 5 4 s间隔内 4块折叠状太阳电池阵三维不稳定温度场响应特点。比较了考虑和不考虑地球入射辐射对电池阵温度分布的影响。本文分析对航天器发射进而对折叠状太阳电池阵展开时刻的认定有重要参考价值     

Parameter optimization for torsion spring of deployable solar array system with multiple clearance joints considering rigid–flexible coupling dynamics

In this paper, four novel evaluation indices and corresponding hierarchical optimization strategies are proposed for a deployable solar array system considering panel flexibility and joint clearance. The deployable solar array model consists of a rigid main-body, two panels and four key mechanisms, containing torsion spring mechanism, closed cable loop mechanism, latch mechanism and attitude adjustment mechanism. Rigid and flexible components are established by Nodal Coordinate Formulation and A...     

含多间隙柔性可展帆板动力学建模及仿真

为研究柔性和多级铰链间隙对帆板展开过程动力学特性的影响,以月球车两级往复可展太阳帆板为研究对象,采用修正Coulomb模型表述摩擦力,通过接触碰撞力描述间隙,运用有限元法进行帆板柔性化,进而建立多间隙-柔性耦合的动力学模型。采用变步长伦哥库塔法进行数值求解,模拟帆板展开过程,分析了多间隙和柔性对帆板质心加速度、铰链间隙碰撞力等参数的影响。结果表明,在保证展开机构刚度要求的前提下,帆板柔性可补偿因铰间隙引起的加速度波动,减弱间隙处碰撞的剧烈程度,减小碰撞力幅值,进而改善帆板展开机构的动态特性。研究结果可用于指导月球车两级往复可展太阳帆板等同类型的可展机构动态优化设计。     

多学科设计优化在空间站太阳翼构型设计中的应用

论述了空间站太阳翼构型的优化问题及应当考虑的设计参数、设计约束、优化目标以及组装建造阶段,分析了优化问题涉及的学科和参数耦合关系;以一个虚拟的空间站服务舱为例,探讨了其太阳翼构型优化建模,给出了3个单目标优化模型,包括设计变量、约束条件和目标函数,比较并说明了优化结果,表明优化合理有效。