应用γ-Reθ湍流模型和PSE方法研究高超声速流动

采用考虑转捩的γ-Reθ湍流模型研究了高超声速复杂流动,结合PSE(parabolic stability equa-tion)稳定性分析方法和e-N方法,通过给出边界层最不稳定点的参数,用以控制γ-Reθ的转捩经验关联式,减少对经验参数的依赖.计算了锥体高超声速流场,得到的壁面换热量和边界层转捩位置与实验吻合较好.计算了平板激波/边界层干扰和高超声速拐角压缩流场,得到了准确的波系结构、压力分布和分离区的大小.结果表明,该方法与传统湍流模型相比具有较大的优越性.     

低雷诺数条件下跨声速转子轴向倾斜缝处理机匣扩稳研究

采用非定常数值方法对低雷诺数条件下50%,75%和100%三种不同轴向叠合量的轴向倾斜缝处理机匣结构对NASA Rotor 37跨声速压气机转子的扩稳效果进行了研究.结果表明,引入处理机匣后,附面层径向涡得到了很好的抑制,由附面层径向涡所引发的叶顶阻塞区大为减小,虽然又引发了由叶顶间隙涡对叶顶所造成的阻塞,但引入处理机匣后对压气机稳定性仍有较大的改善,能有效提高压气机转子的失速裕度.      

超声速非平行边界层的非线性稳定性研究(英文)

用非线性抛物化稳定性方程(NPSE),研究超声速非平行边界层的扰动波的非线性演化过程。发展了高精度的数值方法,对NPSE进行有效求解和稳定推进。计算得到了各谐波的振幅增长曲线和不同的扰动剖面函数,特别是展示了谐波之间的非线性作用的物理特征,包括流向涡、展向涡和Λ结构的形成和演化等,以进行转捩过程的机理研究和分析。NPSE的计算结果显示了这个新方法是研究超声速边界层非线性稳定性的有效方法。     

星点图像的目标提取算法研究

对于星点灰度重心法等亚像素提取算法来说,需要提取星点区域内的每一个像素。基于扫描的边界搜索法只能获取目标的边界像素,文中对其进行了扩展,通过判断边界像素中最大最小行列数来确定目标区域的具体范围,从而提取目标区域内的每一个像素。针对大视场星点图像目标范围小、相互间距离远的特点,为减小计算量,提出了基于视框搜索的目标提取算法。通过实验证明,基于视框的算法在计算量上比基于边界搜索的算法减少3/4。     

小攻角高超声速钝锥边界层失稳特性

利用高阶紧致格式,采用直接数值模拟(DNS)和线性稳定性(LST)分析方法,对高超声速边界层的失稳机制和转捩特点进行了研究.通过对马赫数为6的2?攻角高超声速钝锥边界层的稳定性分析发现:小攻角高超声速钝锥边界层存在多枝不稳定模态;周向速度使钝锥的稳定性特征与不考虑周向速度时有本质的差别;转捩线在接近背风面处出现拐折现象是由失稳模态发生转换引起的.      

氧-乙炔焊焊接区热效应的探索

探讨了物体的热惰性和绝热效应对焊接的影响,讨论了采用银铜焊料进行氧－乙炔焊时应该运用的火焰和火焰的高温区域．分析了自由氧和自由碳在焊接中的影响．     

简单转子系统油膜稳定界限的计算分析

对简单转子支承系统的油膜稳定区进行了计算研究.通过建立包含支承阻尼和转子外阻尼在内的弹性支承滑动轴承系统模型,计算了该转子系统的油膜稳定界限,并对稳定界限进行分析,讨论了提高转子系统稳定性的措施.分析结果表明:减小转子系统的刚度,是提高系统油膜稳定性的有效办法.     

大气辐射传输对红外探潜的影响分析

针对红外探潜的特点,在建立了红外探潜系统作用距离方程的基础上,利用大气辐射传输软件仿真分析了水蒸汽、二氧化碳、海洋气溶胶等因素对红外探潜的影响。结果表明,这些因素对红外探潜效能具有较大影响。     

Resonance transitions associated to weak capture in the restricted three-body problem

An interesting dynamics is studied in the restricted three-body problem where a particle abruptly transitions between resonance states, called a resonance hop. It occurs in a region about the secondary mass point which supports weak capture. This region, called a weak stability boundary, was recently proven to give rise to chaotic dynamics. Although it was numerically known that the resonance hop was associated with this boundary, this process was not well understood. In addition, the dynamical structure of the weak stability boundary has not been well understood. In this paper, we give a way to reveal the global structure of the weak stability boundary associated to resonance motions. This structure is shown to be surprisingly rich in resonant periodic motions interconnected by invariant manifolds. In this case, nearly all the motions are approximately resonant in nature where resonance hops can occur. The correlation dimension of orbits undergoing resonant motions, associated to the weak stability boundary, is also examined. The dynamics analyzed in the present paper is related to that studied by J. Marsden et al. under the perspective of Lyapunov orbits and the associated invariant manifolds. Applications are discussed.     

Free librations of the two-layer Moon and the possibilities of their detection

Based on the forthcoming second stage of the Japanese Lunar mission ILOM (2013), when an optical telescope will be set on the surface near one of the Lunar poles, the possibility to detect free Lunar modes (Chandler-like wobble and free-core nutation) is considered. The difference between the Lunar Eulerian and Chandler-like wobble is explained. The terms “arbitrary libration” and “free libration” are discussed. The geometrical and physical interpretations of the free polar motion over the Lunar surface are considered from the viewpoints of Lunar surface-based observations and the Lunar Navigation Almanac. The dependencies of the free libration period on the core’s radius, density, and ellipticity are modelled and discussed.