采用进气管涡流控制阀的四气门汽油机缸内涡流运动的研究

研制了一种叶片式进气管涡流控制阀,采用涡流动量计式稳流实验台和Ricardo评价方法,分析了四气门汽油机可变涡流进气管对进气流通特性和缸内涡流特性的影响,并且建立了相对应的三维数值模型,得到进气管与缸内流场更为详尽的数据信息。结果表明,该结构可以对缸内涡流运动强度和进气流量系数进行调节,进气终了涡流比调节范围为0~1.59,平均流量系数调节范围为0.25~0.41;涡流强度增大,流量系数随之减小,适应发动机不同工况对于流量系数和涡流运动的要求。     

冗余铺丝机械手自运动流形分析及优化

针对传统位姿分离式铺丝机械手灵活性不足的特点,为了提高航空复合材料铺丝过程的灵活性和避障碍能力,提出一种位姿耦合式冗余铺丝机械手自运动流形的新算法。由于冗余铺丝机械手各关节之间的强耦合性增加了逆解的求解难度,该算法将冗余铺丝机械手的关节逆解分解为已知的Paden-Kahan旋量子问题以及由位置关节组成的特殊旋量子问题,并针对特殊旋量子问题进行求解得到冗余铺丝机械手全部逆解,这样相对于位姿分离式解法有效提高了冗余铺丝机械手逆解的求解效率以及求解直观性。由于冗余铺丝机械手的逆解呈现出流形的结构,所以根据冗余铺丝机械手自运动流形的多维特性,将冗余铺丝机械手的自运动流形分别映射到位置关节空间和姿态关节空间得到其三维仿真曲线。由于冗余铺丝机械手逆解流形中的优化流形在实际控制中更具应用价值,所以在铺丝机械手末端执行器沿芯模轨迹运动速度平稳的前提下为了使机械手各关节速度变化最小,提出以冗余铺丝机械手关节速度组成的约束泛函为目标得到相应的运动学优化流形,并为后续的最优控制奠定了基础。最后以某型号飞机S形进气道为例验证了所提方法的可行性。     

Lagrangian coherent structures in various map representations for application to multi-body gravitational regimes

The Finite-Time Lyapunov Exponent (FTLE) has been demonstrated as an effective metric for revealing distinct, bounded regions within a flow. The dynamical differential equations derived in multi-body gravitational environments model a flow that governs the motion of a spacecraft. Specific features emerge in an FTLE map, denoted Lagrangian Coherent Structures (LCS), that define the extent of regions that bound qualitatively different types of behavior. Consequently, LCS supply effective barriers to transport in a generic system, similar to the notion of invariant manifolds in autonomous systems. Unlike traditional invariant manifolds associated with solutions in an autonomous system, LCS evolve with the flow in time-dependent systems while continuing to bound distinct regions of behavior. Moreover, in general, FTLE values supply information describing the relative sensitivity in the neighborhood of a trajectory. Here, different models and variable representations are used to generate maps of FTLE, and the resulting structures are applied to design and analysis within an astrodynamical context. Application of FTLE and LCS to transfers from LEO to the L₁ region in the Earth–Moon system are presented and discussed. In an additional example, an FTLE analysis is offered of a few stationkeeping maneuvers from the Earth–Moon mission ARTEMIS (Acceleration, Reconnection, Turbulence and Electrodynamics of the Moon's Interaction with the Sun).     

细长体截面流态拓扑结构演化及其稳定性分析

应用动力系统的稳定性理论,分析了细长体在不同迎角下截面绕流拓扑结构的演化和稳定性.指出旋成体背涡的发展,导致截面流场拓扑结构变化,而由稳定对称旋涡流态变成不稳定对称旋涡流态,进而再在小扰动下变成稳定非对称旋涡流态是导致旋成体非对称背涡出现的基本历程.      

Zero,minimum and maximum relative radial acceleration for planar formation flight dynamics near triangular libration points in the Earth–Moon system

Assume a constellation of satellites is flying near a given nominal trajectory around _L4$L_4$ or _L5$L_5$ in the Earth–Moon system in such a way that there is some freedom in the selection of the geometry of the constellation. We are interested in avoiding large variations of the mutual distances between spacecraft. In this case, the existence of regions of zero and minimum relative radial acceleration with respect to the nominal trajectory will prevent from the expansion or contraction of the constellation. In the other case, the existence of regions of maximum relative radial acceleration with respect to the nominal trajectory will produce a larger expansion and contraction of the constellation. The goal of this paper is to study these regions in the scenario of the Circular Restricted Three Body Problem by means of a linearization of the equations of motion relative to the periodic orbits around _L4$L_4$ or _L5$L_5$. This study corresponds to a preliminar planar formation flight dynamics about triangular libration points in the Earth–Moon system. Additionally, the cost estimate to maintain the constellation in the regions of zero and minimum relative radial acceleration or keeping a rigid configuration is computed with the use of the residual acceleration concept. At the end, the results are compared with the dynamical behavior of the deviation of the constellation from a periodic orbit.