具有载荷扰动抑制的卫星姿态控制方法及验证

针对载荷转动对星体产生的呈周期变化的干扰,开展了干扰抑制方法研究。利用干扰的周期特性,基于李亚普诺夫原理设计了参数未知的周期干扰力矩的辨识算法,实现了卫星姿态的自适应控制。最后进行了物理仿真试验,利用真实的星载计算机和控制部件,在气浮台上进行了试验验证,结果表明,算法有效地抑制了载荷转动的干扰,卫星的姿态稳定度提高了50%,且算法简单,易于星上软件实现。     

永磁同步电机积分反步自适应控制

针对外界干扰导致永磁同步电机(PMSM)固有参数发生变化的问题,将新型的智能控制理论引入到PMSM控制系统中,提出了一种新颖的带有积分环节的反步自适应法的控制方法。该控制器能够利用交轴电流动态抑制或消除参数的变化对系统的影响,基于Lyapunov稳定性原理设计被控系统的控制律和自适应律,并引入积分环节,增强被控系统的稳定性,缩短速度响应的时间。仿真试验证明,该控制器能够有效地抑制电机固有参数的变化对被控系统的影响,保证了系统的强鲁棒性和动静态性能。     

An analytical model of prominence dynamics

Solar prominences are magnetic structures incarcerating cool and dense gas in an otherwise hot solar corona. Prominences can be categorized as quiescent and active. Their origin and the presence of cool gas ($～{10}^4$?K) within the hot ($～{10}^6\text{K}$) solar corona remains poorly understood. The structure and dynamics of solar prominences was investigated in a large number of observational and theoretical (both analytical and numerical) studies. In this paper, an analytic model of quiescent solar prominence is developed and used to demonstrate that the prominence velocity increases exponentially, which means that some gas falls downward towards the solar surface, and that Alfvén waves are naturally present in the solar prominences. These theoretical predictions are consistent with the current observational data of solar quiescent prominences.     

东方红三号卫星的机械太阳阵和通信天线

介绍了中德合作研制、生产东方红三号机械太阳阵和通信天线的有关技术和项目的进展情况。机械太阳阵的设计是在经过自行验证的技术基础上进行的,有了这些经验,加上计算机设计优化,能够满足苛刻的质量和刚度要求。通信天线的主要特点是收发共用和全极化复用。它是通过两套7喇叭馈源阵照射极化敏感反射器实现的。天线电性能和结构性能均满足技术要求。     

The Expansion of Coronal Plumes in the Fast Solar Wind

Coronal plumes are believed to be essentially magnetic features: they are rooted in magnetic flux concentrations at the photosphere and are observed to extend nearly radially above coronal holes out to at least 15 solar radii, probably tracing the open field lines. The formation of plumes itself seems to be due to the presence of reconnecting magnetic field lines and this is probably the cause of the observed extremely low values of the Ne/Mg abundance ratio. In the inner corona, where the magnetic force is dominant, steady MHD models of coronal plumes deal essentially with quasi-potential magnetic fields but further out, where the gas pressure starts to be important, total pressure balance across the boundary of these dense structures must be considered. In this paper, the expansion of plumes into the fast polar wind is studied by using a thin flux tube model with two interacting components, plume and interplume. Preliminary results are compared with both remote sensing and solar wind in situ observations and the possible connection between coronal plumes with pressure-balance structures (PBS) and microstreams is discussed. This revised version was published online in June 2006 with corrections to the Cover Date.     

UMAC伺服同步控制技术在轨迹制孔上的实现

根据轨迹制孔设备的结构特点和工艺需求,设计研制了一套基于UMAC多轴运动控制器的轨迹制孔控制系统.阐述了UMAC多轴运动控制器的硬件调试系统搭建、软件的应用和设计方法,同时重点介绍了虚轴同步技术在轨迹制孔控制系统中的应用,通过运动控制并给出了测试记录和制孔试验,验证了基于UMAC的伺服同步控制技术在多轴运动控制器在轨迹制孔设备中的实际应用效果的有效性.     

波箔型径向气体箔片轴承-转子系统升降速动态特性试验

为了研究以波箔型径向气体箔片轴承为支承的轴承-转子系统动力学特性,专门设计了波箔型径向气体箔片轴承试验台,质量为0.458kg的转子在该试验台上实现了超过80000r/min的运转速度.径向轴承为波箔型径向气体箔片轴承,止推轴承为多叶箔片轴承.试验结果表明:波箔型径向气体箔片轴承能够实现转子高速运行,在转子起飞后具有良好的运行稳定性,其轴承支承处振动位移幅值一直维持在20μm之内.由于驱动涡轮受到不平衡气流力的作用,转轴升速时的起飞转速要高于降速时的起飞转速.      

CHANGES OF THE THERMOSPHERE DENSITY IN THE SUNSHINE AND SHADE AREA OBSERVED BY "SZ-2" ATMOSPHERIC DENSITY DETECTOR

In this paper, thermosphere density data of "SZ-2" Atmospheric Density Detec tor From February to April 2001 are used to study the changes of the thermo sphere density in the sunshine and shaded area during solar and geomagnetic activity. The results show that in the sunshine area, the peak value of atmo spheric density changes as F10.7 varies; during geomagnetic activity, the peak value of atmospheric density in the shaded area increases as Ap increases, and start off with higher latitude, therefore move to lower latitude.     

SPACE CHEMISTRY RESEARCHES IN CHINA DURING 2000-2001

Over the past two years, significant progress in space chemistry has been made in China. The research fields include meteorites, pre-solar materials, science researches of the moon, effects of the space debris on space environment, and heterogeneity of the Earth. Chinese Lunar Exploration Project Some studies are also dedicated to one important space mission "Chinese Lunar Exploration Project". In this paper, the main achievements are outlined, and some concepts and hypotheses are briefly revised.     

两冕流间CME事件数值模拟的改进

通过偶极子场和六极子场适当叠加，改进猜解磁场，使猜解磁场在太阳南北极符号相反，然后采用理想磁流体力学方程组(MHD)，由猜解磁场与太阳风流动相互作用计算出稳态自洽解，得到定性上与观测比较接近的具有两个冕流的背景结构．在两个冕流间采用具有同心圆磁场位形的触发模型触发CME事件，研究CME的日冕传播特征．模拟结果表明，CME被约束在两冕流间传播，CME闭磁场位形和磁云横截面磁场位形相似，可以解释1AU处观测磁云的部分特征；在CME附近，存在压力和Lorentz力起主要作用的区域，这可以为分析1AU处CME事件的观测数据提供帮助．