飞机动力学和操纵性临界现象

叙述了飞行试验实践中飞机动力学和操纵性方面最典型的临界现象,分析了这些临界现象产生的原因,简述了飞行试验确定这些临界现象某些特性的方法,并提出了改善和预防这些临界现象的方法和描施。     

关于表面裂纹理论的研究与进展(上)

本文简要地介绍了近几十年国内外表面断裂力学理论的发展状况及所取得的一些成果．重点介绍了应力强度因子求法和裂纹扩展速率的描述，同时对应用于圆柱体上的表面裂纹应力强度因子求法及裂纹扩展速率的描述等方面成果进行了评述。     

圆锥杯形件超塑胀形的力学分析

 研究了圆锥杯形件的变形模式,将其成形过程分为三个阶段。根据超塑性力学的基本方程和有关假设,对每一阶段的成形过程进行了分析,得出了各阶段的最佳加载曲线方程,不同加载方式下成形时间的计算方法以及最小厚度等几何参数的计算公式。最后,进行了简短的讨论。     

一种基于星间方向观测的初轨计算方法

基于天基网空间监测的技术背景,用一已知轨道的天基观测平台对不明空间目标的方向观测,在定轨精度要求并不太高的要求下,研究了单颗卫星的天基平台定初轨的问题,并提出了一套基于此观测模型的中低轨空间目标的初轨计算方法。通过模拟生成测角资料对方法进行检验,计算结果显示方法在目前提出的定轨精度下是稳健可行的。     

界面位错的瞬态运动和界面裂纹的自相似扩展

本文首先利用Ｆｏｕｒｉｅｒ和Ｌａｐｌａｃｅ变换并结合Ｃａｇｎｉａｒｄ－ｄｅＨｏｏｐ反演方法求解了单个界面螺位错的瞬态运动问题，然后以单个位错由静止匀速运动的解作为基本解建立奇异积分方程求解了运动集中载荷作用下界面裂纹的反平面非对称自相似扩展，进一步由此解获得ｘｎ型载荷作用下界面裂纹自相似扩展的动应力强度因子     

飞机机翼表面水滴撞击特性计算

根据飞机防冰系统的研制需要，以机翼为对象，对水滴撞击特性的数值计算进行研究，建立了计算模型，研究了计算方法，用相应的计算程序，在广泛的飞行，气象及多种翼型条件下，对水滴撞击特性作了计算，计算结果与国外权威机构公布的数据相比吻合性好，给出了部分计算结果，并对水滴撞击特性计算的应用作了简要分析。     

曲梁弹性波的传播

用特征线法求出了脉冲载荷作用下的控制曲梁运动的Ｍｏｒｌｅｙ方程的数值解，并用Ｐｌａｓｓ的直梁结果验证了曲率趋于零的极限情形，应用性地研究了曲梁中部受冲击载荷作用的弹性波传播问题，计算结果表明：该数值计算方法简便易行、效率高、有良好的收敛性和稳定性。     

二维机翼非定常运动的涡流场显示--沉浮运动

介绍了在水洞中进行的二维机翼沉浮运动的流动显示实验.实验结果揭示了机翼正弦运动时尾迹涡街的特性以及与Strouhal数的关系;发现了在不同参数下存在三种前缘涡的形式;结合数值计算结果说明了二维机翼沉浮运动中产生非定常推力的机理.     

Linear stability of ring systems around oblate central masses

In this paper, we consider the stability of a ring of bodies of equal mass uniformly distributed around a large oblate central mass. The purpose of this and previous papers is to shed light on the stability of Saturn’s rings. Previous papers have been limited by the assumptions that (1) all ring bodies are at the same distance from the central body, (2) the central body acts like a point mass (i.e., is a perfect sphere), and (3) the ring bodies all have the same mass and are evenly spaced around the ring. The third limitation is probably the least important; as long as there are a large number of masses and the mass distribution is approximately uniform then the system should behave as a system of equally-spaced, equal-mass bodies. The first main purpose of this paper is to remove the second limitation. But, the paper also aims to address limitation (1). Recent computer simulations of single-ring systems have shown that the threshold for stability, as determined by a linear stability analysis, matches precisely the stability threshold predicted by simulation. In other words, a linear stability analysis while presumably just a mathematical abstraction actually tells us something quite real. Furthermore, simulations of multi-ring systems suggest that instability comes from azimuthal perturbations; small azimuthal changes are more destabilizing that small radial perturbations. Hence, in this paper, we also consider the situation where the central body consists not just of an oblate central mass but also incorporates a flat ring representing in aggregate all ring bodies at radii other than the one under consideration. The central oblate body together with a flat ring is modeled simply by introducing two oblateness terms to the gravitational potential associated with the central mass. The subsequent analysis is almost identical to the case of a single oblateness term. For Saturn, the oblateness of the central mass is six orders of magnitude more significant than the rings at other radii as a destabilizing influence.     

Deployment of a lander on the binary asteroid (175706) 1996 FG3, potential target of the european MarcoPolo-R sample return mission

The idea of deploying a lander on the secondary body of the binary primitive asteroid (175706) 1996 FG3 is investigated. 1996 FG3 is the backup target of the European sample return space mission MarcoPolo-R under assessment study at the European Space Agency in the framework of the M3 Medium-Class mission competition. The launch will take place in 2022–2024, depending on its selection at the end of 2013. A lander is indicated as an optional payload, depending on mass availability on the spacecraft. Obviously, the possible complexity of a lander deployment is also an important parameter to take into account. Here we demonstrate that, considering worst case scenarios and low requirements on the spacecraft GNC and deployment mechanism, the operations are easy to implement and safe for the main spacecraft. The concept of operations is to deploy a light lander from the L₂ Lagrange point of the binary system, on a ballistic trajectory that will impact the secondary asteroid. The fundamental principles of this strategy are briefly presented and a detailed model of 1996 FG3 is considered, to which the strategy is applied. We show that the deployment is successful in 99.94% of cases.