A Structured Mesh Euler and Interactive Boundary Layer Method for Wing/Body Configurations

To compute transonic flows over a complex 3D aircraft configuration, a viscous/inviscid interaction method is developed by coupling an integral boundary-layer solver with an Eluer solver in a ＂semi-inverse＂ manner. For the turbulent boundary-layer, an integral method using Green＇s lag equation is coupled with the outer inviscid flow. A blowing velocity approach is used to simulate the displacement effects of the boundary layer. To predict the aerodynamic drag, it is developed a numerical technique called far-field method that is based on the momentum theorem, in which the total drag is divided into three component drags, i.e. viscous, induced and wave-formed. Consequently, it can provide more physical insight into the drag sources than the often-used surface integral technique. The drag decomposition can be achieved with help of the second law of thermodynamics, which implies that entropy increases and total pressure decreases only across shock wave along a streamline of an inviscid non-isentropic flow. This method has been applied to the DLR-F4 wing/body configuration showing results in good agreement with the wind tunnel data.     

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.     

人体头部受撞击脑损伤界限的研究

脑损伤的研究，是生物力学研究的重要问题之一，其研究涉及到医学、力学的很多方面。本文将承受撞击的颅脑看成一个整体，同时又考虑其结构和力学性质。采用粘弹性的Kelvin体进行计算分析，比较分析三种不同的判据对实际人脑的损伤的判断的影响。     

平板上钝缘舵在超声速绕流中的三维分离特性研究

对于平板上的直立钝缘舵在M_∞=1.79、2.04和2.50的条件下,研究了该平板干扰区中的三维分离特性。着重讨论了钝缘直径、舵面迎角和来流马赫数对主分离线位置和形状的影响。分析了该类三维分离在性态上更强地依赖于无粘流动特性。此外,还对分离区内的二次分离发展过程和形态进行了初步讨论。     

小型弹体转动惯量的测定

阐述了对称式三线摆的结构原理及该摆微角与大角摆动周期的计算方法 ,利用此摆可以测量构件的转动惯量。当 RL <130 、φ0 <6 0°时 ,该装置的测量准确度优于 1%。     

大迎角细长旋成体绕流结构演变过程实验研究

 通过烟流显示和测压实验, 系统地观察和分析了尖拱头细长旋成体绕流结构随迎角的演变过程。实验发现在不同迎角下, 不仅细长旋成体绕流结构形态不同, 而且不同流态结构的演变过程所含迎角范围较小,几乎在几度迎角内就可完成。     

中等高超声速弹体头,尾形状对气动性能影响的实验研究

六种常规弹体在两种细长比下头部和尾部形状时CN,Xcp的影响进行实验研究，实验名义Mach数为4．0，4．5，5．0和6．0，a＝0°～6°（或0°～8°）。获得了一些对高超声速飞行器研制有实用价值的结果。     

高分辨率格式与钝舵绕流数值模拟

 采用Beam-Warming/TVD格式，Roe二阶、三阶以及四阶通量差分分裂格式数值计算雷诺平均Navier-Stokes方程，湍流附加粘性采用Baldwin-Lomax模型计算，针对超声速绕钝圆舵流动进行了数值模拟比较研究，计算给出了流场的详细结构，物面压力分布与实验值符合良好，尤其是Roe三阶格式给出了较好的计算结果，两个超声速回流区以及湍流边界层分离也得到了很好的数值模拟。     

空间飞行体与等离子体在压缩区内的非稳态相互作用研究

研究了空间飞行体在运动过程中，其前端压缩区内飞行体与等离子体的、非稳态相互作用问题，得到了在强天线辐射源高频场作用下的控制方程．通过计算表明，飞行体上的天线可作为调制不稳定性的激发源，在等离子体中激发起很强的电磁孤波．     

惯性解耦的多体系统动力学方程

对一类含自由－自由弹性梁的多体系统动力学方程进行了研究，利用多体系统的结构特性和运动特性对其动力学方程进行了简化，使惯性质量矩阵为对角形，得到了惯性解耦的多体系统动力学方程，在方程的数值求解时，可提高计算速度和精度，为多体系统动力学的实时仿真提供方便。