基于多阶段决策的侦察卫星任务规划研究

为解决侦察卫星任务规划中合理分配任务和避免信息传输冲突的问题,建立了基于多阶段决策的侦察卫星任务规划模型,包括任务分配模型和传输调度模型,并根据运筹学的基本原理,给出了求解模型的基本方法,从求解结果来看,该模型具有一定的理论与应用价值。     

Traverses for the ISECG-GER design reference mission for humans on the lunar surface

This study explores the Design Reference Mission (DRM) architecture developed by Hufenbach et al. (2015) as a prelude to the release of the 2018 Global Exploration Roadmap (GER) developed by the International Space Exploration Coordination Group (ISECG). The focus of this study is the exploration of the south polar region of the Moon, a region that has not been visited by any human missions, yet exhibits a multitude of scientifically important locations – the investigation of which will address long standing questions in lunar research. This DRM architecture involves five landing sites (Malapert massif, South Pole/Shackleton crater, Schrödinger basin, Antoniadi crater, and the South Pole-Aitken basin center), to be visited in sequential years by crew, beginning in 2028. Two Lunar Electric Rovers (LER) are proposed to be tele-robotically operated between sites to rendez-vous with crew at the time of the next landing. With engineering parameters in mind we explore the feasibility of tele-robotic operation of these LERs between lunar landing sites, and identify potential high interest sampling locations en-route. Additionally, in-depth sample collection and return traverses are identified for each individual landing site across key geologic terrains that also detail crew Extra-Vehicular Activity (EVA). Exploration at and between landing sites is designed to address a suite of National Research Council (2007) scientific concepts.     

圆轨道航天器在轨加注任务空间燃料站部署问题

在轨服务技术因在航天器故障修复、寿命延长及军事方面有重大辅助作用而越来越受到各航天大国的重视,作为在轨服务技术重要组成部分的在轨燃料补给技术也越来越受到关注。文章针对圆轨道航天器在轨燃料加注任务,将空间燃料站技术与多目标在轨加注技术相结合,对基于燃料站的在轨加注模式进行了研究,提出了一种基于聚类分析的在轨加注任务调度及优化算法。通过对双脉冲轨道转移问题的求解与分析,获得了轨道转移速度增量和轨道参数之间的关系,在此基础上分析了圆轨道航天器在轨加注任务调度问题,并根据调度模型的变量和约束关系,建立了圆轨道航天器在轨加注任务多目标规划模型,并采用免疫遗传算法对加注任务调度空间燃料站选址问题进行了研究。以30颗目标航天器的在轨加注任务为例进行了数值仿真,并由燃料消耗的计算结果验证了算法的有效性。     

“嫦娥4号”月球背面着陆区月壳及深部结构特征

深部月壳和月幔物质结构是月球科学探测的关键问题之一。“嫦娥4号”初步将月球背面南极—艾肯（South Pole-Aitken,SPA）盆地内的冯·卡门（Von Kármán）撞击坑作为着陆点,具有重要的科学研究价值。结合月球重力、地形、布格重力、月壳厚度等地球物理数据,综合对冯·卡门撞击坑的月壳及其深部结构特征进行了分析。结果显示：冯·卡门撞击坑重复撞击到南部的冯·卡门M撞击坑上,后者的中央峰具有明显的布格正重力异常和线性的布格重力梯度特征,显示出高密度的幔部物质向上涌起;冯·卡门撞击坑极有可能穿透了该区域的整个月壳,并挖掘出了深部月幔的物质;该区域南部月壳厚度较薄小于5 km,北部平均月壳厚度在15～20 km,月壳平均密度为2 630 kg·m^-3,比背面高地月壳密度高,且平均孔隙度为9%,低于月球的平均孔隙度12%。     

“嫦娥4号”中继星任务分析与系统设计

作为"嫦娥4号"任务的重要组成部分,中继星将为着陆器和巡视器提供中继通信支持。不同于其它月球探测器,中继星首次选择了绕地月L2平动点运行的晕(Halo)轨道以保证对月球背面的着陆器和巡视器提供连续的中继通信服务,面临诸多技术挑战。在对中继星任务特点进行分析的基础上,梳理了研制中的技术难题,包括使命轨道的选择、使命轨道的到达和长期维持、中继通信体制选择等,并提出了解决方案。中继星的总体设计方案概述也在文中给出。     

用于飞机概念设计的设计要求输入和初步定参数环境

为了在飞机概念设计过程中给新型号的设计要求组织和基本参数估算提供便捷且可扩展的工具而开发了设计要求与初步定参数环境(EDRIPS)。在这一环境中，设计可以通过友好的用户界面交互地输入飞机的性能要求、构造任务剖面和选取有效载荷，然后以此为基础从约束分析所得的可行域中选取设计点，进而利用一种改进的估算飞机起飞重量的方法进行任务分析以得到飞机的基本设计参数。介绍了各模块的实现措施和所采用的方法。最后通过对一个设计实例的分析验证了EDRIPS应用于飞机概念设计的有效性和可靠性。     

A novel compilation method of comprehensive mission spectrum of aero-engine maneuvering load based on use-related mission segment

Comprehensive Mission Spectrum (CMS) of an aero-engine can reflect the usage characteristics of the engine. It can provide load input for engine life prediction and accelerated mission test. In this paper, a novel compilation method of CMS of aero-engine maneuvering load based on mission segment is proposed. Firstly, the use-related Typical Mission Segment (TMS) of maneuvering load is divided and identified according to spectral characteristics. Secondly, the mathematical model of different kinds of TMS are established based on stochastic process theory. Finally, the CMS of maneuvering load is compiled based on TMS. The proposed method can accurately quantify the compilation of CMS. The compiled CMS shows good agreement with the original load spectrum. According to damage consistency inspection, the compiled CMS is consistent with the damage caused by the original load spectrum in terms of low cycle fatigue.     

Reducing mission operations costs through spacecraft autonomy: the near earth asteroid rendezvous (near) experience

With a maximum time of 12 days out of ground contact and a round-trip light time as high as 56 minutes, The Near Earth Asteroid Rendezvous (NEAR) spacecraft requires a moderate degree of onboard autonomy to react to faults and safe the spacecraft. Beyond the basic safing requirements, additional functions are carried out onboard. For example, on-board calculation of the Sun, Earth, asteroid, and spacecraft positions allow the spacecraft to autonomously orient itself for science and downlink operations. On-board autonomous momentum management during cruise relieves Mission Operations from planning, scheduling, and carrying out many manual momentum dumps. During development, additional operations, such as center-of-mass management during propulsive maneuvers and optical navigation were also considered for onboard autonomy on the NEAR spacecraft, but were not selected. The allocation of functions to onboard software or to ground operations involved tradeoffs such as development time for onboard software versus ground software, resource management, life cycle costs, and spacecraft safety.After two years of cruise operations, considerable experience with the NEAR autonomy system has accrued. The utility of some autonomous capabilities is greater than expected, others less so. Software uploads increased spacecraft autonomy in some cases, and the impact on Mission Operations can be assessed. Allocation of functions between spacecraft autonomy and ground operation during development of future missions can be improved by applying the lessons learned from the NEAR experience.     

航空动力装置任务可靠度模糊预计与分配的综合

根据Vague集的直觉性，定义一种判定Vague值真值的函数，进而给出一种确定Fuzzy隶属度的方法。将此方法应用于模糊综合评判理论，得到一种在设计初期根据专家意见，预计航空动力装置任务可靠度的模糊决策方法。根据预计值和比例组合分配法的思想，先按任务可靠度模型的等效串联模型进行任务可靠度指标的分配，然后再对等效串联模型中冗余部分的指标进行分配。     

A Novel Magnetic Configuration for Space Radiation Active Shielding

Space radiation has been identified as the main health hazard to crews involved in manned Mars missions. Active shielding is more effective than passive shielding to the very energetic particles from cosmic rays. Particle motion in a magnetic field is studied based on the single-particle theory and Monte Carlo method. By comparing the shielding efficiency of different magnetic field configurations, a novel active magnetic shielding configuration with lower mass cost and power consumption is proposed for manned Mars missions. The new magnetic configuration can shield 92.8% of protons and 84.4% of alpha particles with E < 4 GeV·n-1, when considering the passive shielding contribution of 10.0 g·cm-2 Al Shielding, the required magnetic stiffness can be reduced from 27 Tm to 16 Tm. The detailed analysis of mass cost and power consumption shows that active shielding will be a promising means to protect crews from space radiation exposure in manned Mars missions.