小卫星临近作业轨道和姿态联合控制

建立了小卫星相对轨道和姿态的误差动力学模型,根据作业任务和姿态指向要求确定了小卫星相对轨道和姿态的期望运动;采用相对轨道和姿态联合控制策略,并考虑小卫星作业过程中质量和转动惯量的不确定性,设计了自适应全状态反馈控制律;数值仿真结果表明该控制律具有较强的自适应性。     

Aerosols and clouds in the upper troposphere–lower stratosphere region detected by GOMOS and ACE: Intercomparison and analysis of the years 2004 and 2005

Satellite-based limb occultation measurements are well suited for the detection and mapping of polar stratospheric clouds (PSCs) and cirrus clouds. PSCs are of fundamental importance for the formation of the Antarctic ozone hole that occurs every year since the early 1980s in Southern Hemisphere spring. Despite progress in the observation, modeling and understanding of PSCs in recent years, there are still important questions which remain to be resolved, e.g. PSC microphysics, composition, formation mechanisms and long-term changes in occurrence. In addition, it has recently become clear that cirrus clouds significantly affect the global energy balance and climate, due to their influence on atmospheric thermal structure.     

Lower-mesospheric inversion layers over brazilian equatorial region using TIMED/SABER temperature profiles

Lower-mesospheric inversion layers (MILs) were studied using the temperature profiles observed by TIMED/SABER over Cariri (7.5°S, 36.5°W), Brazil, in 2005. A total 175 MILs were identified with the maximum occurrence in April and October and the minimum in January and July. The lower MIL is located in a height region from 70 to 90 km, with the peak at around 83 ± 4 km with the temperature of 205 ± 5 K, and the thickness of 4–10 km. The results show large amplitudes of MILs during equinoxes and minimum in solstices, with a clear semiannual variation. A general feature of lower MIL in monthly mean profile was observed twice a year, one from February to May, and the other from August to October with a downward shift of the top level. These results suggest that formation and long persistence of MIL is an important factor to investigate propagation of atmospheric gravity waves in the mesosphere-lower thermosphere (MLT) region.     

一种模拟整星热环境的小型单机热平衡试验

文章通过对一个典型的单机热分析和热试验的研究,提出了一种小型单机热平衡试验方法,模拟单机在整星环境下的热平衡试验,以避免只为验证其热设计而再次补做整星热平衡试验。为准确模拟单机在星内的辐射和导热过程,通过灰体间辐射热网络法和仪器安装板处单元体热平衡法,给出了等效辐射特征点和等效导热特征点的确定方法;并结合试验结果,对模型修正的合理性、局限性进行了分析,提出了在实际应用过程中应注意的问题。     

Advances in the Researches in Middle and Upper Atmosphere in 2006—2008

This paper summarizes the research results obtained by Chinese scientists and/or through international collaborations in 2006—2008.Specifically,this paper focus on the research fields in the middle and upper atmosphere,including developments in facilities and instruments,and the advancements in scientific issues.     

整星隔振技术的原理分析

用刚度—质量—阻尼模型分析在地面振动试验条件下带隔振器的卫星振动传递函数,得 到隔振前后振动传递函数与卫星模态阻尼、卫星频率下降率和隔振器损耗因子的关系。据此 关系,从抑制共振响应峰值和隔离中高频振动两方面提出了整星隔振器刚度和阻尼设计的若 干准则。     

基于时空结构的卫星智能诊断模型研究

针对卫星这类复杂系统的故障诊断,提出了基于时空结构的智能故障诊断系统模型(iFDS),从系统结构,结构模型,推理机制、流程模型等方面进行论述,通过对各种故障诊断方法进行融合,实现了卫星系统网络化、个性化、远程并行诊断的智能故障诊断.在故障推理机制研究中,将故障分为系统故障、多发故障和单元故障3类,分别对每一类故障提出相应的智能故障推理方法.     

国外卫星星座自主运行技术发展综述

综述国外卫星星座自主运行技术的研究和发展情况,重点介绍了导航星座、移动通信星座和区域覆盖星座的自主导航和自主轨道控制技术的发展现状,并对实现星座自主控制的关键技术进行了分析。这为我国发展星座自主控制技术提供参考。     

利用6S进行月光条件下遥感器信号模拟研究

以太阳为光源的卫星遥感器,可以采用6S或MODTRAN等辐射传输计算软件对其入瞳处的辐亮度进行计算。而在微光或月光条件下,遥感器是对观测目标反射的月亮辐射进行遥感观测,因此在进行辐射传输计算时需要代入月球的辐照度数据。可以利用已公布的月球表面反射率和已知的大气层外太阳辐照度来计算月球辐照度,并对6S辐射传输计算进行适当的修改进行计算。通过对月球辐照度计算原理进行了详细的描述并计算得到了波长在0.250μm~1.500μm范围内的月球表面辐照度,并给出了一个宽波段遥感器的微光动态范围。     

AOS虚拟信道链路控制器和VCDU合路器的设计实现

在深入研究高级在轨系统(AOS)标准和对星载数据系统进行分析的基础上,设计实现了AOS虚拟信道链路控制器和虚拟信道数据单元(VCDU)合路器。该设计采用现场可编程门阵列(FPGA)实现高级在轨系统虚拟信道链路控制(VCLC)子层的位流业务和虚拟信道存取(VCA)子层的VCA业务,完成了位流协议数据单元(B_PDU)的构造,VCDU的组装、调度、填充和定界等功能,实现了对整星数据流的统一管理。在卫星的星载数据系统设计中,将有效载荷数据和航天器平台数据合一,形成统一数据流,可以节约频率资源,支持宽带数据传输、实现整星数据流的统一管理,使整个系统更灵活、更开放、更有效,提高卫星的自主管理能力。