柔性航天器动力学建模的伪坐标形式Lagrange方程

航天器动力学建模过程中，常采用伪坐标形式Lagrange方程。文章针对多柔体航天器的情况，利用Hamilton原理，导出了柔性航天器动力学建模的伪坐标形式Lagrange方程，并由此建立了由中心体和柔性附件组成的全柔性航天器的动力学方程。     

卫星太阳电池阵的刚-柔耦合动力学

研究了卫星太阳电池阵在多点撞击过程中的刚-柔耦合动力学问题．基于Jourdain速度变分原理和单向递推组集方法，建立了柔性多体系统的动力学模型．用Hertz撞击法则建立了撞击力和撞击处的局部变形关系，分别用刚体模型和柔性体模型仿真计算了太阳电池阵的撞击力、撞击时间，揭示了变形运动和大范围运动的相互耦合作用．     

1997-2003年太阳质子事件源区的卡林顿经度分布

分析了1997-2003年期间的59个太阳质子事件,太阳质子事件源区的卡林顿经度带.分析结果表明,质子事件源区主要集中在10°-45°,135°-155°,180°-215°,230°-260°,265°-310°,345°-360°,还有4个质子耀斑分散在72°,74°,93°和107°上.其中最强的活动卡林顿经度带的经度范围是265°-310°,次之为卡林顿经度带135°-155°,最弱的是卡林顿经度带180°-215°最强的活动经度是卡林顿经度272°.1997-2003年期间峰值通量大于100 pfu,质子耀斑南半球发生次数为18,北半球发生次数为10;同一活动经度上的质子事件具有重现的规律,重复出现的时间间隔短的为27天,长的超过4年.     

PE—3284中型计算机内存扩充

介绍了ＰＥ—３２８４中型计算机内存扩充的方法，包括硬件电路设计，操作系统和应用软件的改进．     

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.     

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.     

一种盲多波束形成GNSS天线阵抗干扰算法

天线阵抗干扰是现代卫星导航接收机抗干扰的重要手段。传统的天线阵波束形成类算法能够在抑制干扰的同时提升抗干扰后输出信噪比,但是在信号捕获阶段,由于缺少先验信息的支持,该类算法无法在信号方向形成增益。因此,提出了一种盲多波束形成的天线阵抗干扰算法,通过形成多个波束覆盖天线阵上半球面,可在无先验信息的条件下对卫星信号形成增益,从而提升信号捕获阶段信噪比,使得接收机在干扰环境中具备更强的信号捕获能力。仿真结果表明:与传统的天线阵抗干扰算法相比,提出的算法能够在有效抑制干扰的同时显著提升接收机信号捕获成功率。     

Radio Diagnostics of the Solar Flare Reconnection

First, high-frequency (HF) slowly drifting pulsating structures are interpreted as radio emissions of electron beams accelerated in the magnetic reconnection volume and injected into magnetic islands (plasmoids). Then, the time evolution of plasma parameters (density, magnetic field, etc.) in a 2-D MHD model of solar flare reconnection is computed numerically. Assuming plasma radio emission from locations where the “double-resonance’’ instability generates upper-hybrid (UH) waves due to unstable distribution function of suprathermal electrons, the radio spectra and spatial source structures in the reconnection region are modeled. By comparison of the modeled and observed spectra a remarkable similarity has been found between the computed narrow-band emission and the observed lace bursts. Finally, a new diagnostics of the reconnection process is proposed.     

波导缝隙在模拟阵列环境中的有源导纳值计算方法

通过分析、综合关于波导缝隙天线阵的两种常用的综合设计方法（实验测量设计和理论计算设计法）的优缺点，提出了用理论分析计算的方法求解模拟阵列环境中波导缝隙的有源导纳和谐振长度值的设想和具体实现方法。这样既省去了实验测量设计法中测试部件的加工和测量过程，又充分地发挥了理论计算设计法适合于对小型波导缝隙阵进行分析与设计的特点，将会大大地减少波导缝隙天线阵综合设计的工作量。     

激波加速的密度分层流体交界面的演化

采用了自适应的非结构网格和基于有限体积法的二阶Godunov格式，数值模拟了在不同强度的激波作用下两种不同密度流体交界面的演化过程，详细给出了交界面上由于斜压效应产生的涡列的演化过程。