质子辐照聚酰亚胺薄膜的力学性能退化机理

利用自制的Φ800 mm空间综合辐照试验设备和X射线光电子能谱等分析手段对质子辐照聚酰亚胺薄膜的力学性能退化及机理进行了研究。研究发现:薄膜的断裂伸长率和拉伸强度随质子辐照注量的增加而呈指数减小,弹性模量基本不变;质子辐照后聚酰亚胺薄膜仍具有较好的热稳定性,但其在紫外可见光波段透射率降低,透射光谱发生红移;分子键的断裂和交联是质子辐照聚酰亚胺薄膜力学性能降低的主要原因。     

空间机械臂运动控制的地面仿真验证技术

空间机械臂是在轨进行舱外巡检、航天员辅助出舱的关键活动机构,其在轨操作的运动过程需要在地面进行预先规划生成运动控制指令,再通过数字仿真与推演对运动控制指令进行验证,以确保机械臂操作全程的安全性和高效性.针对上述问题,本文主要从运动空间限制、运动速度限制和关节力矩限制等方面设计了地面仿真验证框架,提出了基于运动学与动力学...     

CCSDS空间网络互联协议发展及启示

空间互联网将是由各种区域网构成的复杂异构网络,为了使其能够逐步实现自动化运行,网络效益得到最大程度的发挥,须做好网络互联的顶层规划与设计,并开发具体的标准技术.根据近年CCSDS (Consultative Committee for Space Data Systems,空间数据系统咨询委员会)发布的建议书,以及相关工作组的项目规划情况,介绍了SSI(Solar System Internetwork,太阳系互联网)体系结构、IPoC(IP over CCSDS space links,在CCSDS空间链路之上承载IP),以及DTN(Delay Tolerant Networking,容延迟网络)等标准项目.从CCSDS空间网络互联技术的发展历程不难得出结论:我国未来空间网络互联应注重区域网之间互联的顶层设计;区域网内部各子网之间的互联技术应选择以航天任务需求牵引为主;DTN将在区域网之间互联以及区域网从简单到复杂发展中都发挥重要作用.     

TBCC飞行器发动机尺寸选型及爬升策略设计

针对临近空间高速飞行器爬升航迹问题，提出了一种涡轮冲压组合发动机尺寸选型的依据和一种固体火箭助推器辅助加速的爬升策略。以本文设计的一型临近空间高速飞行器为原型，基于hp自适应Radau伪谱法开展爬升航迹优化研究，将最优控制问题转化为非线性规划问题，以爬升消耗燃料质量最小为目标，利用序列二次规划算法求解最优航迹。在此基础上，分析了涡轮冲压组合发动机尺寸选型和采用固体火箭助推器加速爬升策略对爬升航迹和巡航航程的影响。结果表明，选取合理的发动机尺寸和助推器辅助爬升策略，均可有效减少飞行器爬升消耗燃料质量，提升巡航航程。     

集中式平台自由销售代码共享研究与应用

在对目前世界范围内,航空公司之间普遍采用的代码共享合作方式进行分析的基础上,结合中国民航的实际情况,提出了同时使用中国民航传统集中式订座系统平台,系统内两家航空公司之间自由销售模式的代码共享系统解决方案,并对该设计方案的高灵活性、低成本消耗等特点进行了具体的分析。     

一种利用自然能飞行的临近空间浮空器研究

为实现临近空间浮空器的持久区域驻留和机动飞行,文章所研究的一种利用自然能飞行的临近空间浮空器利用自然界的热能和风能,通过简易可行的技术手段实现飞行高度和轨迹的控制,有望解决临近空间浮空器面临的能源问题和热问题。文章介绍了该新型浮空器的系统组成和主要特点,分析了该新型浮空器在设计最大运行高度处的浮重平衡,进行了系统设计参数的分析。该新型浮空器由超热空气和氦气提供浮力,计算结果表明氦气囊所占比例越大,所需的浮空器半径越小,且随着设计最大运行高度的升高及超热值的减小,所需的浮空器半径增大。     

LARES successfully launched in orbit: Satellite and mission description

On February 13th 2012, the LARES satellite of the Italian Space Agency (ASI) was launched into orbit with the qualification flight of the new VEGA launcher of the European Space Agency (ESA). The payload was released very accurately in the nominal orbit. The name LARES means LAser RElativity Satellite and summarises the objective of the mission and some characteristics of the satellite. It is, in fact, a mission designed to test Einstein's General Relativity Theory (specifically ‘frame-dragging' and Lense-Thirring effect). The satellite is passive and covered with optical retroreflectors that send back laser pulses to the emitting ground station. This allows accurate positioning of the satellite, which is important for measuring the very small deviations from Galilei–Newton's laws. In 2008, ASI selected the prime industrial contractor for the LARES system with a heavy involvement of the universities in all phases of the programme, from the design to the construction and testing of the satellite and separation system. The data exploitation phase started immediately after the launch under a new contract between ASI and those universities. Tracking of the satellite is provided by the International Laser Ranging Service. Due to its particular design, LARES is the orbiting object with the highest known mean density in the solar system. In this paper, it is shown that this peculiarity makes it the best proof particle ever manufactured. Design aspects, mission objectives and preliminary data analysis will be also presented.     

火箭整流罩声振环境缩比特性研究

针对火箭整流罩全尺寸声振环境试验过程中难度大、成本高的问题，通过量纲分析的方法建立了缩比模型的相似准则，研究并获得了缩比模型与原模型之间内部声场、壁面振动加速度的关系，并使用声学有限元方法(FEM)进行了仿真计算。仿真结果表明，缩比模型与原模型场点处声压级相吻合，壁面振动加速度成一定的比例关系，符合缩比准则结果。该方法为火箭整流罩的声振环境预示和试验提供了理论依据。     

UVCS/SOHO Observations of H I Lyman Alpha Line Profiles in Coronal Holes at Heliocentric Heights Above 3.0 R⊙

The Ultraviolet Coronagraph Spectrometer (UVCS) on the Solar and Heliospheric Observatory (SOHO) has been used to measure spectral line profiles for H I Lyα in the south polar coronal hole at projected heliocentric heights from 3.5 to 6.0 R_⊙ during 1998 January 5–11. Observations from 1.5 to 2.5 R_⊙ were made for comparison. The H I Lyα profile is the only one observable with UVCS above 3.5 R_⊙ in coronal holes. Within this region the outflowing coronal plasma becomes nearly collisionless and the ionization balance is believed to become frozen. In this paper, the 1/e half widths of the coronal velocity distributions are provided for the observed heights. The velocity distributions include all motions contributing to the velocities along the line of sight (LOS). The observations have been corrected for instrumental effects and interplanetary H I Lyα. The half widths were found to increase with projected heliographic height from 1.5 to 2.5 R_⊙ and decrease with height from 3.5 to 5 R_⊙. This revised version was published online in June 2006 with corrections to the Cover Date.     

航天器空间环境干扰力矩分析与仿真研究

针对航天器在轨运行时所受到的空间环境干扰力矩进行建模分析,并通过实时解算和矢量叠加的方式进行仿真研究,尤其对太阳光压力矩与大气阻力力矩的建模与仿真提出了新的方法,该方法通过建立光照面与迎风面的判断准则,准确地对太阳光压力矩与大气阻力力矩进行了估计。对各种空间环境干扰力矩的精确建模与仿真为航天器精确姿态控制设计及系统姿态控制方案和控制执行机构的选取提供了依据,文中提出的方法简单易用,工程实现性强,为未来的工程应用提供了一定的理论依据。