高超声速进气道附面层分离无源被动控制

为了控制超燃冲压发动机进气道唇口反射激波诱导的附面层分离,根据其流动特征,提出了附面层泄除-吹除互相驱动的自适应、无源、被动控制方案。并采用空间HLLE格式、LU-SGS隐式推进、多块结构网格的有限体积法数值模拟程序对该流动现象进行了数值模拟。数值结果表明,施加自适应无源被动控制后,分离区长度减小为无控制时的45%,控制区域的总压恢复系数和流场均匀性提高。从而证实了自适应、无源、被动控制抑制高超声速进气道附面层分离的可行性。     

日冕边界条件与太阳风共转相互作用

本文根据第二十太阳周太阳风数据的统计分析结果,用太阳风二维理想流体模型探讨近太阳区的不同边界条件太阳风与共转相互作用对1AU处太阳风各参数影响,得到共转相互作用不能引起太阳风速度和马赫数的反相扰动,推断在太阳风加速区温度扰动对太阳风的影响最大,而在太阳风传播区速度扰动对太阳风的影响最大.     

叶尖泄漏流/尾迹掺混对串列转子非设计点性能影响

在串列转子设计中,为研究前后排叶片周向位置的变化所引起的泄漏流/尾迹之间掺混的变化对串列转子近失速点性能的影响,首先建立了泄漏流/尾迹掺混分析模型.模型分析结果指出流动掺混可以有效减小通道下游堵塞.在模型分析的基础上,进一步在高负荷串列转子中进行了不同周向位置的对比研究,对模型进行了验证;研究发现在近失速工况,对比无掺混情况,后排叶尖泄漏流/前排尾迹掺混使叶尖堵塞减少了近20%,从而使得高负荷串列转子的失速裕度相对提高了11.7%.      

叶轮机械三维粘性动静叶干涉的数值模拟

本文发展了 1套模拟叶轮机械三维粘性动静叶干涉的数值方法。在成熟的空间离散方法基础上 ,提出了 1种高效的双时间步隐式时间推进方法 ,并构造了一种保证守恒的动静叶交界面处的数值通量计算方法。本文对某三维亚音速涡轮的动静叶干涉进行了数值模拟 ,结果与实验符合较好。     

SETI implications of gravitational assist via chaotic trajectories of binary objects

Extrapolating from the technique of gravitational assist via chaotic trajectories of binary objects, this paper considers how such techniques might be used in other systems. We examine which types of systems are the best candidates for harvesting gravitational energy for payload ejection. We also consider what signatures might be present in either the asteroid orbits or radiation of the central body if extraterrestrial intelligences were to use such techniques about these candidate systems.The simulation studies show that current technology cannot approach the sensitivity needed to detect either of these signals. Instead, we provide these results as guidance to studies in coming decades on patterns that may indicate the use of an asteroid ejection system.     

集成火星进入弹道的开伞过程动力学特性研究

针对火星探测任务设计阶段的需求,提出集成再入弹道、开伞过程仿真一体化设计方法。首先,利用质点动力学模型,计算质点弹道,进行探测器进入过程的飞行轨迹仿真,获得开伞初始状态。其次,基于任意拉格朗日-欧拉（ALE）方法,建立开伞过程的流固耦合（FSI）动力学模型,进行典型工况开伞过程数值模拟,分析开伞动压和马赫数对降落伞充气过程的影响。数值模拟开伞过程伞衣几何外形变化和降落伞的流固耦合动力学行为,得到开伞过载变化曲线、伞衣阻力面积变化等典型特征参数。计算结果表明,降落伞开伞动力学的数值仿真方法为火星再入、减速和着陆（EDL）过程的概念设计提供了一定的参考依据。     

基于非定常面元/黏性涡粒子法的低雷诺数滑流气动干扰

针对太阳能无人机螺旋桨滑流与机翼的气动干扰,考虑了低雷诺数流动下气体黏性和压缩性影响,并根据黎曼边界条件和涡量等效原则建立了能够快速计算分析螺旋桨-机翼气动干扰的非定常面元/黏性涡粒子的混合方法。首先使用有试验数据的风洞模型以及数值模拟技术对混合方法进行验证,在此基础上研究了不同安装位置与工况下螺旋桨与机翼的气动干扰。结果表明:螺旋桨对轴向气流的加速以及滑流诱导的上洗和下洗效应使机翼气动力呈现出增升增阻的现象,机翼升阻比有所下降。较大的弦向间距以及较高的垂直安装位置在减缓机翼升阻比下降的同时也使得螺旋桨拉力有所减小。对于多个螺旋桨的气动干扰,不同的桨叶旋转方向导致机翼气动力不同的变化规律,当旋转方向与机翼翼尖涡反向时,螺旋桨滑流能够抑制翼尖涡的强度,提高机翼气动效率。     

MHD modeling of the outer heliosphere: Achievements and challenges

An overview is presented of magnetic-field-related effects in the solar wind (SW) interaction with the local interstellar medium (LISM) and the different theoretical approaches used in their investigation. We discuss the possibility that the interstellar magnetic field (ISMF) introduces north–south and east–west asymmetries of the heliosphere, which might explain observational data obtained by the Voyager 1 and Voyager 2 spacecraft. The SW–LISM interaction parameters that are responsible for the deflection of the interstellar neutral hydrogen flow from the direction of propagation of neutral helium in the inner heliosheath are outlined. The possibility of a strong ISMF, which increases the heliospheric asymmetry and the H–He flow deflection, is discussed. The effect of the combination of a slow-fast solar wind during solar minimum over the Sun’s 11-year activity cycle is illustrated. The consequences of a tilt between the Sun’s magnetic and rotational axes are analyzed. Band-like areas of an increased magnetic field distribution in the outer heliosheath are sought in order to discover regions of possible 2–3 kHz radio emission.