轮控小行星探测器建模及跳跃移动仿真

小行星探测器在弱引力环境下无法采用传统的轮式机构进行移动。为解决该问题,采用反作用飞轮对探测器跳跃移动进行控制,并分析了该方案的可行性。根据Hertz碰撞定律及简化的Karnopp切向摩擦力模型,建立了探测器与地面的接触力模型。分析了轮控小行星探测器的起跳过程,给出了探测器静止起跳所需要的最小飞轮力矩关系。考虑到反作用飞轮存在惯性、粘滞、摩擦等情况,建立了轮控探测器的姿态动力学模型,并对探测器在均匀重力场下的连续跳跃过程进行了控制策略设计及仿真。结果表明:基于飞轮控制的小行星探测器跳跃移动在微重力环境下是可行的,且可以通过施加合适的控制力矩维持探测器跳跃的方向及跳跃过程的稳定性。     

激光功率与底面状态对选区激光熔化球化的影响

为研究激光功率与底面状态对选区激光熔化熔池流动的影响，基于离散单元法建立了选区激光熔化铺粉模型，采用粒径分布与实验相符的马氏体时效钢粉末分别铺展到平坦底面和增材底面上，将计算获得的粉末分布导入到基于有限体积法建立的选区激光熔化熔池计算流体力学模型中，研究激光功率和基板底面粗糙度对熔池流动和熔道表面形貌的影响。采用激光单道扫描实验验证铺粉模型和选区激光熔化模型。结果表明：随着激光功率的降低，单位长度的球化数量增加；由于增材底面使熔池润湿性变差，同时又对熔池流动行为产生扰动，使得增材粗糙底面上熔道的球化数量增加。选区激光熔化铺粉模拟及激光单道扫描模拟结果与实验结果吻合较好。本研究可为选区激光熔化工艺中工艺参数的选择提供理论指导。     

Dynamics of a spacecraft and normalization around Lagrangian points in the Neptune–Triton system

The problem of a spacecraft orbiting the Neptune–Triton system is presented. The new ingredients in this restricted three body problem are the Neptune oblateness and the high inclined and retrograde motion of Triton. First we present some interesting simulations showing the role played by the oblateness on a Neptune’s satellite, disturbed by Triton. We also give an extensive numerical exploration in the case when the spacecraft orbits Triton, considering Sun, Neptune and its planetary oblateness as disturbers. In the plane a × I (a = semi-major axis, I = inclination), we give a plot of the stable regions where the massless body can survive for thousand of years. Retrograde and direct orbits were considered and as usual, the region of stability is much more significant for the case of direct orbit of the spacecraft (Triton’s orbit is retrograde). Next we explore the dynamics in a vicinity of the Lagrangian points. The Birkhoff normalization is constructed around L₂, followed by its reduction to the center manifold. In this reduced dynamics, a convenient Poincaré section shows the interplay of the Lyapunov and halo periodic orbits, Lissajous and quasi-halo tori as well as the stable and unstable manifolds of the planar Lyapunov orbit. To show the effect of the oblateness, the planar Lyapunov family emanating from the Lagrangian points and three-dimensional halo orbits are obtained by the numerical continuation method.     

Numerical prediction and wind tunnel experiment for a pitching unmanned combat air vehicle

The low-speed flowfield for a generic unmanned combat air vehicle (UCAV) is investigated both experimentally and numerically. A wind tunnel experiment was conducted with the Boeing 1301 UCAV at a variety of angles of attack up to 70 degrees, both statically and with various frequencies of pitch oscillation (0.5, 1.0, and 2.0 Hz). In addition, pitching was performed about three longitudinal locations on the configuration (the nose, 35% MAC, and the tail). Solutions to the unsteady, laminar, compressible Navier–Stokes equations were obtained on an unstructured mesh to match results from the static and dynamic experiments. The computational results are compared with experimental results for both static and pitching cases. Details about the flowfield, including vortex formation and interaction, are shown and discussed, including the non-linear aerodynamic characteristics of the vehicle.     

基于图剖分的多块结构网格负载平衡方法

负载平衡是影响并行计算性能的重要因素。针对多块结构网格,给出了一种改进的多层次图剖分负载平衡方法。该方法设计了新的网格剖分算法,采用改进的子块分裂方法与图剖分算法的循环调用实现结构对接网格剖分,并通过建立不同物体重叠网格间的连接关系,实现了结构重叠网格的负载平衡。采用2个典型算例对方法进行了对比验证,数值结果表明,子块分裂方法对剖分结果具有重要影响,采用循环调用算法及改进的子块分裂方法能有效地实现计算负载均衡及通信量优化,同时显著减少了网格块数及因虚网格导致的内存需求,有利于提高并行效率。该负载平衡方法与网格拓扑无关,适用于多块结构对接网格及重叠网格,且整体型剖分方式对于多块结构重叠网格具有更好的剖分效果。     

Propagation and interaction of interplanetary transient disturbances. Numerical simulations

We study the heliocentric evolution of ICME-like disturbances and their associated transient forward shocks (TFSs) propagating in the interplanetary (IP) medium comparing the solutions of a hydrodynamic (HD) and magnetohydrodynamic (MHD) models using the ZEUS-3D code [Stone, J.M., Norman, M.L., 1992. Zeus-2d: a radiation magnetohydrodynamics code for astrophysical flows in two space dimensions. i – the hydrodynamic algorithms and tests. Astrophysical Journal Supplement Series 80, 753–790]. The simulations show that when a fast ICME and its associated IP shock propagate in the inner heliosphere they have an initial phase of about quasi-constant propagation speed (small deceleration) followed, after a critical distance (deflection point), by an exponential deceleration. By combining white light coronograph and interplanetary scintillation (IPS) measurements of ICMEs propagating within 1 AU [Manoharan, P.K., 2005. Evolution of coronal mass ejections in the inner heliosphere: a study using white-light and scintillation images. Solar Physics 235 (1–2), 345–368], such a critical distance and deceleration has already been inferred observationally. In addition, we also address the interaction between two ICME-like disturbances: a fast ICME 2 overtaking a previously launched slower ICME 1. After interaction, the leading ICME 1 accelerates and the tracking ICME 2 decelerates and both ICMEs tend to arrive at 1 AU having similar speeds. The 2-D HD and MHD models show similar qualitative results for the evolution and interaction of these disturbances in the IP medium.     

航天飞机系统两体分离问题的探讨

本文简要地叙述了美国研究轨道器与外挂贮油箱,轨道器与载机分离问题的概况。对垂直起飞两级入轨的并联两机的分离问题,提出了研究模型并作了具体分析,着重提出了实现两机安全分离需要解决的技术难点。 二级航天飞机的两机分离问题,是未来航天高技术领域的关键技术之一,本文阐述了解决两体并联分离问题我国现有的技术水平,并提出了解决该问题的技术方案。     

Development process of muzzle flows including a gun-launched missile

Numerical investigations on the launch process of a gun-launched missile from the muzzle of a cannon to the free-flight stage have been performed in this paper. The dynamic overlapped grids approach are applied to dealing with the problems of a moving gun-launched missile. The high-resolution upwind scheme(AUSMPW+) and the detailed reaction kinetics model are adopted to solve the chemical non-equilibrium Euler equations for dynamic grids. The development process and flow field structure of muzzle flows including a gun-launched missile are discussed in detail.This present numerical study confirms that complicated transient phenomena exist in the shortly launching stages when the gun-launched missile moves from the muzzle of a cannon to the freeflight stage. The propellant gas flows, the initial environmental ambient air flows and the moving missile mutually couple and interact. A complete structure of flow field is formed at the launching stages, including the blast wave, base shock, reflected shock, incident shock, shear layer, primary vortex ring and triple point.     

导引头量测故障下的增量式三维制导律设计

考虑导引头量测故障下拦截机动目标的末制导问题,以提高制导系统的鲁棒性、降低制导增益、减小系统残差、避免视线角速率剧烈振荡/发散为目的,基于增量式控制方法设计了一种具有鲁棒增强特性的三维末制导律。首先,将末制导问题转化为零化视线角速率的控制问题。其次,通过弹目相对距离及视线角速率定义辅助变量,给出传统的滑模制导律作为设计参考。然后,基于增量式非线性动态逆滑模控制方法,充分挖掘视线角加速度估计信息及上一采样时刻的制导指令,得到增量式三维鲁棒制导律。最后,在目标机动及导引头量测故障下,分析并比较了两种制导律所产生的系统残差。理论分析及多工况仿真结果表明,增量式制导律不仅对目标机动及大范围失效的导引头量测故障具有强鲁棒性,而且所需制导增益也较小,同时避免了末端视线角速率严重发散的问题     

舰载飞机着舰拦阻动力学研究综述简

 拦阻着舰过程通常被认为是舰载飞机事故率最高的阶段,因此,自从有了航空母舰和舰载飞机,拦阻着舰动力学就一直是国内外相关研究人员的研究热点。本文从拦阻钩、拦阻装置和起落架3个关键部件着手,比较详细地论述了舰载飞机着舰拦阻涉及到的关键动力学问题及其研究现状,重点对拦阻钩弹跳动力学及其载荷分析、拦阻索动力学及其载荷分析、下沉速度、非对称拦阻对起落架载荷的影响、拦阻系统动力学等方面进行了综述。最后,对着舰拦阻动力学研究的发展趋势进行了展望。