基于解耦和动态补偿的卫星控制系统设计

针对带大型挠性单翼太阳帆板和偏置动量的三轴稳定卫星,研究如何消除星内外干扰对姿态控制精度影响的卫星控制系统的设计问题。首先对星内外干扰进行了数值分析,进而阐明了在经典控制方案中干扰力矩对姿态控制精度的影响,指出经典控制在克服干扰力矩对姿态控制精度影响方面存在的不足之处。然后根据卫星的动力学特点,提出并论证了在设定角动量交换系统标称值条件下基于解耦和动态补偿的卫星控制系统的设计方案。最后深入分析了在该方案下太阳帆板挠性模态的稳定性。     

多径效应与低仰角跟踪

介绍多径效应产生的机理及对低仰角跟踪的影响。提出低仰角跟踪条件下 ,克服多径效应影响和改善天线跟踪平稳性的几种措施     

砷化镓太阳电池技术的进展与前景

介绍了砷化镓(GaAs)太阳电池的特点，并比较了液相外延(LPE)和金属有机物化学气相沉积(MOCVD)两种外延生长技术。叙述了国外单结、双结与三结GaAs太阳电池的结构、性能、研制及生产情况，分析了GaAs太阳电池的发展方向。最后根据国内GaAs太阳电池的研制进展和空间试用情况，提出了发展我国GaAs太阳电池的设想和建议。     

小推力推进系统起动过程的分析

本文对小推力推进系统各部件建立了数学模型，并对此系统进行了数值计算。计算结果表明，在燃烧时滞较大时，该系统响应较慢，发动机参数的超调量较大，达到稳态所需的时间较长；轨控发动机与姿控发动机共用同一个供应系统时，姿控发动机受燃烧时滞的影响更大。减小燃烧时滞有利于提高发动机在起动过程的响应能力和稳定性。在起动阶段，高室压推进系统比低室压推进系统响应快，高室压轨控发动机的参数能较快地稳定下来，但其超调量较大；高室压姿控发动机虽然响应快，但其超调量大，达到稳态所需的时间长于低室压姿控发动机。本文所得结论为提高小推力推进系统在起动过程的响应能力提供了参考。     

复合材料层板受低速冲击后的剩余刚度与剩余强度研究

本文对玻璃／环氧复合材料层进行了低速冲击实验，研究了这种复合材料在低速冲击后的剩余刚度与剩余强度问题，提出了一个剩余刚度概率分布模型，建立了剩余刚度与剩余强度之间的关系     

航天器总线管理系统的SOC设计与研究

高速、高可靠、低功耗的智能型串行系统总线是航天器进一步发展必须解决的一个关键问题。以1553B总线控制器为例,采用SOC设计方法,研究了航天器系统总线的设计和实现。首先按照1553B总线标准设计了总线管理SOC的系统结构,然后重点解决了SOC设计中的IP开发应用、可靠性设计、容错机制及低功耗实现等关键技术。采用这些SOC设计方法的1553B总线协议处理器取得了一次流片成功,为今后更高速率的航天器总线管理系统的SOC研究提供了一种思路和方法上的借鉴。     

空间太阳能发电和微波与电离层相互作用

本文第一部分研究了空间太阳能热发电，基于所提的评价动力系统的准则，比较了三种热力学系统，并给出了一些参数变化对闭式回热Ｂｒａｙｔｏｎ循环系统的影响，本文第二部分对微波速对电离层中电子的加速和受热进行了数值研究，得出了一些结果。     

Implications of a weak termination shock

Recent observations from the Voyager spacecraft have suggested that the spectrum of the anomalous cosmic ray component is relatively steep at the termination shock, which is believed to be responsible for accelerating these particles. This conclusion argues that the termination shock must be weak, which in turn requires that the upstream Mach number in the solar wind must be quite low, 2.4. It is pointed out that such conditions are unlikely to prevail at all locations along the shock front. However, it is possible for such conditions to exist at the interface between high speed streams at high heliographic latitudes and the region at low latitudes where high and low speed streams have interacted and come into equilibrium. This discussion suggests a preferred location for the injection of the anomalous component into the shock acceleration process.     

Energy flux in the Earth's magnetosphere: Storm – substorm relationship

Three ways of the energy transfer in the Earth's magnetosphere are studied. The solar wind MHD generator is an unique energy source for all magnetospheric processes. Field-aligned currents directly transport the energy and momentum of the solar wind plasma to the Earth's ionosphere. The magnetospheric lobe and plasma sheet convection generated by the solar wind is another magnetospheric energy source. Plasma sheet particles and cold ionospheric polar wind ions are accelerated by convection electric field. After energetic particle precipitation into the upper atmosphere the solar wind energy is transferred into the ionosphere and atmosphere. This way of the energy transfer can include the tail lobe magnetic field energy storage connected with the increase of the tail current during the southward IMF. After that the magnetospheric substorm occurs. The model calculations of the magnetospheric energy give possibility to determine the ground state of the magnetosphere, and to calculate relative contributions of the tail current, ring current and field-aligned currents to the magnetospheric energy. The magnetospheric substorms and storms manifest that the permanent solar wind energy transfer ways are not enough for the covering of the solar wind energy input into the magnetosphere. Nonlinear explosive processes are necessary for the energy transmission into the ionosphere and atmosphere. For understanding a relation between substorm and storm it is necessary to take into account that they are the concurrent energy transferring ways. This revised version was published online in August 2006 with corrections to the Cover Date.     

SOHO: The Solar and Heliospheric Observatory

The Solar and Heliospheric Observatory (SOHO), together with the Cluster mission, constitutes ESA's Solar Terrestrial Science Programme (STSP), the first Cornerstone of the Agency's long-term programme Space Science — Horizon 2000. STSP, which is being developed in a strong collaborative effort with NASA, will allow comprehensive studies to be made of the both the Sun's interior and its outer atmosphere, the acceleration and propagation of the solar wind and its interaction with the Earth. This paper gives a brief overview of one part of STSP, the SOHO mission.