空间2-RSSS机构的误差分析

对低速运动带间隙空间2-RSSS机构的误差展开研究,首先建立了带间隙的空间2-RSSS机构的误差模型,并基于二力杆假设把约束副间隙误差转化成为杆长误差,在保持精度的条件下简化了误差模型.其次推导了敏度矩阵的参数化表示,并建立了该机构的误差仿真模型,求解了敏度矩阵的参量,该敏度矩阵解法结合了符号推导的规律性明显和数值计算结果精确的优势.最后基于数值仿真验证了近似敏度矩阵求解的有效性,并对该机构的误差进行了分析,给出了在确定加工精度条件下约束副间隙影响指向误差的关键参数以及这些关键参数的优化设计准则.      

空间光学系统真空热试验污染控制经验综述

真空热试验过程中光学系统可能受到严重污染,因此需制定严格的污染控制措施。文章对NASA、ESA、JAXA 等航天机构的卫星光学系统真空热试验中典型、有代表性的污染控制经验进行了综述,并对我国光学系统真空热试验污染控制提出了若干建议。     

火箭基组合循环发动机性能迭代算法研究

火箭基组合循环(简称RBCC)发动机性能分析模型的研究对于RBCC发动机结构的优化设计具有重要意义。本文结合RBCC发动机的结构特点和工作原理建立了RBCC发动机性能分析模型,并对RBCC发动机性能计算方法进行了研究。结合RBCC发动机引射模态和亚燃冲压模态的工作特点,通过迭代计算使进气道、混合段、燃烧室之间的参数耦合,实现了对RBCC发动机引射模态与亚燃冲压模态性能的快速分析。文章通过算例验证了算法的可行性,并通过与文献结果的对比验证了计算结果的可信度。     

基于STL文件和有限元法的在轨航天器关键部件热计算

针对STL(stereo lithography)文件在传递复杂几何实体模型信息方面具有精度高的特点,提出了一种基于STL文件计算复杂结构角系数和外热流的方法.根据单元和节点的拓扑关系识别六面体网格边界单元并进行辐射换热计算.详细阐述了基于STL文件和有限元法进行复杂结构的角系数和外热流的计算方法.研究了导热-辐射耦合计算的有限元方法.最后利用有限元法计算航天器关键部件在轨的三维瞬态温度场.      

新型弹射装置弹射动力源虚拟仿真计算

通过对某新型弹射装置的工作原理分析,建立其物理模型并进行简化;以空气动力学、工程流体力学和动力学系统建模为理论基础,建立弹射机构的物理和数学仿真模型,并利用计算分析软件求得弹射机构的动态参数的变化规律,对弹射过程的动态参数进行研究,为设计新的弹射机构提供理论依据。     

Experimental and theoretical investigation of encounter of a group of particles with protecting elements of spacecraft

We present the results of comprehensive experimental and theoretical investigations of encounter with a barrier of a group of bodies thrown with a high-velocity. Throwing of a group of particles (from two to twelve bodies) was realized on a ballistic route using powder and light-gas units of different calibers in the range of velocities 500–3500 m/s. The process of particle throwing was controlled by acting aerodynamic forces. In experiments on collisions with barriers of a finite thickness (which imitates the protective shield of spacecraft) the number of particles in a homogeneous stream was varied from 2 to 7 at changing the flux density (distances between particles). Experimental data are obtained on variations of the area and mass of back-surface splinters. Numerical calculations simulated a knock of 2 to 4 particles against a barrier in the cases of normal impact and at an angle. The calculations were performed in three-dimensional formulation and applying criteria of complete destruction of material. The appearance of additional destruction centers in the barrier due to mutual influence of particles is revealed. Simple criteria are obtained for estimating the degree of interference of particles and the character of barrier destruction.     

A specific case of stability of cylindrical precession of a satellite

In a central Newtonian gravitational field, the motion of a dynamically symmetrical satellite along an elliptical orbit of arbitrary eccentricity is considered. The particular motion of the satellite is known when its axis of symmetry is perpendicular to the orbit plane, and the satellite rotates about this axis with a constant angular velocity (cylindrical precession). A nonlinear analysis of stability of this motion has been performed under the assumption that the geometry of the satellite mass corresponds to a thin plate. At small values of orbit eccentricity e the analysis is analytical, while numerical analysis is used for arbitrary values of e.     

About one problem of trajectory optimization

The optimization problem for trajectories of spacecraft flight from the Earth to an asteroid is considered in this paper. The flight is realized in the central Newtonian gravitational field of the Sun with a possibility of gravitational maneuvers near planets. Perturbation maneuvers are taken into account using the method of point area of action with a limitation on the flyby altitude. The spacecraft is controlled by changing the value and direction of the engine thrust. The problem is solved taking into account constraints on the launch time, flight duration, and minimum distance to the Sun.     

Orbital stability of planar oscillations of a satellite in a circular orbit

We consider the attitude motion of a satellite with a circular orbit in a central Newtonian gravitational field. The satellite is a solid body whose mass geometry is that of a plate. A nonlinear analysis is made of orbital stability of planar oscillations of the satellite at which its middle or major axis of inertia is perpendicular to the orbit plane. At small amplitudes of oscillations the analysis of stability was made analytically, while for arbitrary amplitudes the numerical analysis was performed.     

Optimization of low-thrust transfers in the three body problem

We consider transfers with low thrust in an arbitrary field of forces. The modified method of transporting trajectory [1–4] is used for optimization of the transfers. The complexity of finding the transporting trajectory of a preset type can be the main obstacle to application of this method. This challenge is solved for the three-body problem in the Hill motion model. Numerical analysis of the method is performed using an example of the transfers to halo-orbits around the solar-terrestrial libration points.