Introduction to Meridian Space Weather Monitoring Project

The Meridian Project is a ground- based network program to monitor solar-terrestrial space environment, which consists of a chain of ground-based observatories with multiple instruments including magnetometers, ionosondes, HF and VHF radar, Lidar, IPS monitors, sounding rockets etc. The chain is mainly located in the neighborhood of 120°E meridian, and is thus named the Meridian Project. It has officially been approved by the Chinese government and will be finished by 2009. This talk will give an overview of the Meridian Project and the proposed International Space Weather Meridian Circle Program.     

碳含量对耐蚀软磁合金1J116磁性能的影响

分别从磁化理论和数理统计两个方面分析了影响耐蚀软磁合金1J116磁性能的因素。对某钢厂不同生产时期的生产质量水平通过理论计算进行了评估;研究了化学元素C不同含量对材料磁性能的影响;通过计算得到了提高磁性能的有效C含量范围。     

航空发动机进口整流支板防冰槽裂纹故障分析

为了排除某型发动机进口整流支板裂纹故障,利用故障树的排查方法分析了故障原因,并对试验件进行了断口分析、尺 寸测量、动应力及残余应力测试、防冰槽结构形式及表面状态疲劳对比试验。结果表明：支板防冰槽裂纹产生的主要原因是进气机 匣焊接后残余应力较大,且防冰槽边缘存在应力集中,在试车过程中,防冰槽应力集中处在转子叶片激振的作用下萌生裂纹并扩 展。针对故障原因开展了结构改进设计与试验,提出了修改防冰槽宽度、倾角尺寸及增加重熔层控制等措施,使得该故障得以排除。     

GPS中频信号和IMU信号模拟及验证

为了研究GPS/INS（Inertial Navigation System）组合导航方案和算法,设计了一种GPS中频信号和IMU（Inertial Measurement Unit）信号的软件模拟器.首先建立了载体的运动模型,然后介绍了信号的仿真方法.根据载体的运动产生IMU信号,载体的典型运动包括平飞运动、横滚运动、俯仰运动和偏航运动.建立了典型的干扰模型,包括欺骗式干扰和压制式干扰（窄带干扰、宽带干扰、连续波干扰和锯齿调频连续波干扰等4种）,实现了干扰环境下的场景模拟.GPS/INS组合导航软件接收机对模拟器输出的数据进行解算,结果表明：信号的仿真算法是正确的,模拟器可以为组合导航接收机提供有效的中频信号和IMU信号.     

飞机产品客户化浅析

民用飞机是特殊商品,不同航空公司以及同一航空公司的不同发展阶段,由于其产品经营理念的差别,几乎每架飞机都是与众不同的,因此飞机产品客户化是航空公司和飞机制造商共同关注的话题。空客公司的民用系列飞机获得了世界的认可,其客户选型工作可以提供很好的参考。通过研究分析空客公司的客户选型相关工作,为我国大型客机客户化设计积累必要的技术储备和参考借鉴,并为我国大型客机产品客户化提出了研究方向。     

基于故障观测器的无人机直接自修复控制

提出一种基于故障观测器的无人机直接自修复控制。首先,根据系统本身存在的故障,设计了一个非线性故障观测器对其进行观测。其次,设计了一个快速终端滑模面和直接自修复控制器,将指数函数和符号函数引入到新型滑模面里。同时引入了自适应技术,对不确定的故障估计其上界。最后,通过对无人机进行了相应的仿真数值验证得出所提方法的有效性。     

On two kinds of intermediate orbits for asteroid explorations

In the paper, two kinds of intermediate orbits for asteroid explorations are proposed. One is around the collinear libration points of the Sun-asteroid restricted three-body problem. The other is around the asteroid itself. The first kind of intermediate orbit is applicable to asteroids with known masses, while the second is suitable for asteroids with unknown or negligible masses. Analytical solutions of these two intermediate orbits in the simplified models are introduced first, and then numerical algorithms are used to refine them to obtain the true orbits in the real force model. At last, the problem of station-keeping is addressed. The linear optimal feedback control law is used, and numerical simulations are made to both kinds of intermediate orbits. The results show that both kinds of orbits are feasible. The cost is reasonable and mainly depends on the initial insertion error.     

载人航天器大气环境控制系统性能集成分析

考虑到载人航天器大气环境控制系统设计参数和控制参数众多,文章建立了一种载人航天器大气环境控制系统性能集成仿真分析模型,包括舱体模块、航天员模块、舱压控制模块、温湿度控制模块和二氧化碳净化模块。利用该模型对载人航天器常规工作模式下大气环境控制系统性能进行了计算分析,得到了在不同热负荷水平下载人航天器密封舱空气各个参数随在轨时间的变化趋势,结果表明:氧分压控制、二氧化碳净化和人区温湿度控制之间存在着密切的相互影响关系,不可孤立地进行分析。此外,文章还分析确定了非常规工作模式下热负荷水平允许上限,为载人航天器工作模式的确定提供了依据。研究结果有助于载人航天器大气环境控制系统的设计和流程改进。     

Recent Development and Preliminary Results of Chinese Meridian Project

The Meridian Project is a ground-based network program to monitor solar-terrestrial space environment, which consists of a chain of 15 ground-based observatories located roughly along 120°E longitude and 30°N latitude. The Meridian project started in 2008, and its construction was completed by 2011. The integration and test phase of the Meridian Project conducted in 2011 demonstrated its observation capabilities as expected. The project will be in full operation in 2012. This report gives an overview of the recent development and preliminary results of the Meridian Project since 2010.      

Dynamical evolution of high area-to-mass ratio objects in Molniya orbits

For special demands, some notable orbit types have been developed by human, including the Molniya orbits, which have a relatively high eccentricity up to about 0.7, and a period of 12 h. Considering that space debris with high area-to-mass ratio (A/M) has been discovered, such objects may also exist in Molniya orbits due to spacecraft and upper stages fragmentation events. However, there are not sufficient studies of the complex dynamical phenomena of such orbits. These studies can enrich the knowledge about the long-term evolution of these orbits, be helpful to propose uncatalogued objects observation and identification, and also set the protected region as well as active debris removal. In this paper, the characteristics of 2:1 resonance of Molniya satellite orbits are studied. A large set of numerical simulations, including all the relevant perturbations, is carried out to further investigate the main characteristics, and special attention is payed to the dynamical evolution of objects with high A/M, particularly affected by the direct solar radiation pressure. The long-term dynamical evolution of orbital elements, as well as the dependency of lifetime on the A/M value, is discussed.