发动机进排气系统对飞机气动特性影响的数值研究

为了分析发动机与飞机系统耦合过程中产生的气动力特性,准确获取实际使用条件下的飞机升阻特性,以带动力的某半模飞机模型为研究对象,开展了三维流场数值仿真计算,利用风洞试验数据对计算方法进行了验证,总结了溢流阻力及排气干扰阻力的变化规律,结果表明:发动机状态变化对飞机升阻特性影响明显,在选定的发动机工作参考状态下,溢流阻力在飞机系统升力与阻力方向的分量随捕获面积比的增大分别增大、减小,排气系统实际工作状态偏离选定的参考状态越远,干扰阻力在飞机系统升力和阻力方向分量的绝对值越大。     

空间非合作目标多指包络抓捕路径设计

针对现有空间非合作目标抓捕中存在无固定抓捕点以及待抓捕目标存在动态性等问题,提出了一种"主-从"式多指包络抓捕路径设计算法。首先,为了降低多指包络构型设计中的自由度,将多指机构分为一根主手指和其余从手指两类。然后,为了实现对具有动态性的空间非合作目标的抓捕,采用误差跟踪控制方法使主手指的基关节与包络点之间的运动保持同步。接着,引入单向距离的概念衡量主手指构型和包络边相似度,并利用快速搜索随机树算法寻找使得单向距离最小的主手指关节角取值。进一步,根据多指机构的结构模型,确定其余从手指的构型。最后,根据包络条件选择能够约束住空间非合作目标运动的有效包络构型。通过对可以简化为扁平型的空间非合作目标和一般性三维空间非合作目标这两类目标的包络抓捕仿真可以得出,所设计的算法可适用于一般性空间非合作目标的包络抓捕,同时计算复杂度也大大降低。     

基于阻抗控制的空间机械臂目标捕获技术研究

针对7自由度空间机械臂在目标捕获过程中的应用,根据机械臂末端执行器与目标适配器导向插入过程中存在接触碰撞的特点,提出一种阻抗控制方法,将机械臂末端测量的反作用力和力矩转化为位置增量,从而提高机械臂的主动柔性。并建立MATLAB/ADAMS联合仿真模型进行仿真验证,利用ADAMS的碰撞模型模拟接触捕获时的力学过程。仿真结果表明,本文提出的阻抗控制方法可以减小机械臂末端作用力和关节的驱动力矩,补偿了机械臂位置控制的误差,从而保证了机械臂对目标的捕获精度。     

捕捉激波的群速度控制方法

回顾及综述了群速度控制方法基本原理、发展过程及最新进展。群速度控制方法是通过控制色散误差以捕捉间断的一种数值方法。该方法通过在间断两侧采用不同色散类型的格式,将数值波的传播压制在间断附近,避免数值振荡向周围扩散,从而达到抑制数值振荡的效果。该方法主体上采用数值色散抑制振荡,实际使用中仅需补充较低水平的数值耗散就可将振荡压制在可接受的范围内。因而群速度控制格式的总体耗散水平较低,易于实现小尺度波的高分辨率捕捉,是复杂流动高分辨率数值模拟的有效方法。     

Properties of transit trajectory in the restricted three and four-body problem

In the restricted three-body problem if the Jacobi constant is just below the value corresponding to Lagrangian point only a little neck exists around the equilibrium point and capture trajectories are indicated as low-energy. Capture properties depend on the dynamics around these critical points and qualitative results can be obtained using linearized systems. In this paper, to study transit trajectory properties in the restricted three and four-body problem, the Earth–Moon–Sun–Satellite system is considered as example and studied using different models. In the circular restricted three-body problem (Earth–Moon–Satellite), transit, non transit and asymptotic trajectories, are easily identified by using the principal reference frame. Dynamics around Lagrangian point are then studied introducing the Moon eccentricity into the elliptical restricted three-body model. A preferential region for transit orbit is individuated and studied as a function of eigenvalue properties. To introduce the Sun effect, the bi-circular four-body model is considered and dynamics around Lagrangian points studied as a function of angular distance between Earth–Sun and Earth–Moon line. Finally, results obtained in the elliptical three-body model and bi-circular four-body model, are compared with numerical simulations using real Sun–Moon–Earth ephemeris.     

曲锥前体/三维内转进气道一体化设计与分析

对圆锥流场在不同攻角条件下的气动特征进行分析,以流线追踪技术为基础,发展了一种曲锥前体/三维内转进气道一体化设计方法,获得了三个几何参数对一体化方案外形和性能的影响规律。研究发现,三维内转进气道侧壁外扩角对进气道流量捕获系数影响明显,而捕获形状圆心角对进气道的影响主要表现在几何特征上。此外,进气道流量捕获系数随外压缩段总长度的增大而减小。基于对捕获形状的研究,设计了一种曲锥前体/三维内转进气道,并通过数值模拟对该方案进行研究。结果表明:在设计点来流马赫数为6.0时,该方案进气道流量捕获系数能够达到0.93,且具有0.61的总压恢复系数;在非设计点来流马赫数为5.0时,流量捕获系数能够保持在0.86,总压恢复系数为0.77。      

一种仿生附着装置柔顺关节的优化设计

为提高仿生附着装置在捕获空间非合作目标物时对目标运动参数的适应性,设计了一种3自由度串联柔顺关节,可通过关节嵌入系统后的协调运动来辅助装置被动适应运动目标物姿态,并在运动过程中基于弹簧、阻尼缓冲器组成的关节柔顺机构及其能量耗散原理来降低目标物动能。为验证、优化关节性能,通过ADAMS虚拟样机软件建立了基于柔顺关节的仿生附着装置捕获过程运动学与动力学模型,分析了柔顺关节3组弹簧刚度系数、黏滞阻尼系数对非合作目标物捕获状态的影响,并利用ADAMS-iSIGHT联合仿真平台,通过多岛遗传算法对上述弹簧、阻尼器的重要参数进行了优化,极大提高了柔顺关节的能量耗散效果,同时保证了可捕获目标物运动参数达到规定要求。      

Contingency and recovery options for the European Student Moon Orbiter

This paper presents an overview of the analysis performed on the lunar orbit and some of the possible contingencies for the European Student Moon Orbiter (ESMO). Originally scheduled for launch in 2014 –2015 as a piggyback payload, it was the only ESA planned mission to the Moon. By way of a weak stability boundary transfer, ESMO is inserted into an orbit around the Moon. Propellant use is at a premium, so the operational orbit is selected to be highly eccentric. In addition, an optimization is presented to achieve an orbit that is stable for 6 months without requiring orbit maintenance. A parameter study is undertaken to study the sensitivity of the lunar orbit insertion. A database of transfer solutions across 2014 and 2015 is used to study the relation between the robustness of weak capture and the planetary geometry at lunar arrival. A number of example recovery scenarios, where the orbit insertion maneuver partially or completely fails, are also considered.     

Study of the 28 October 2003 and 20 January 2005 solar flares by means of 2.223 MeV gamma-emission line

By the data on intensity-time profiles of the neutron capture line of 2.223 MeV we have studied some characteristics of two solar flares, 28 October 2003 and 20 January 2005 (INTEGRAL and CORONAS-F observations, respectively). The SINP code was applied making allowance for the main processes of neutron interactions and deceleration in the solar plasma, character of neutron source, losses of neutrons and density model of the solar atmosphere. Comparison of the computed time profiles of 2.223 MeV line with observed ones for the flare of 28 October 2003 confirms the results obtained earlier for three other flares. Namely, the effect of density enhancement (EDE) in the sub-flare region, as well as the variations (hardening) of accelerated particle spectrum in the course of the event have been confirmed. The usual modeling procedure by the SINP code, however, seems to be inapplicable to the event of 20 January 2005. Possible causes of density enhancements during some flares and peculiarities of the 20 January 2005 flare are discussed.     

三维湍流高速进气道内外流场的高效高分辨率解

本文提出一种高效、高分辨率求解三维复杂流场的隐式算法，并成功地用于求解高速进气道内外流场的三维、可压缩、雷诺平均Ｎａｖｉｅｒ－Ｓｔｏｋｅｓ方程组，获得了三个工况五种流场的三维数值解；与有关实验数据比较，结果令人满意。这种算法由Ｊａｍｅｓｏｎ－Ｔｕｒｋｅｌ的ＬＵ分解法和张涵信ＮＮＤ格式的数值通量耦合而成，湍流采用ＢａｌｄｗｉｎＬｏｍａｘ模型。大量数值计算表明，该算法能捕捉到复杂的激波系，有较好的激波