测地线缠绕90°弯管的运动方程

用纤维缠绕90°弯管主要有两种方法:计算机控制缠绕或摆动缠绕弯管机控制缠绕。本文分别讨论在上述方法中测地线缠绕时丝嘴运动规律。 在用计算机缠绕90°弯管时,由于芯模回转,丝嘴既可在三维空间也可在二维空间运动。文中分別给出了在这两种情况下测地线缠绕时丝嘴运动方程。 本文还讨论了实现整螺旋缠绕的条件和最优参数的选取。在缠绕受内压的弯管时,推荐取弯管曲率半径与弯管半径比值近似为4。为实现测地线缠绕90°弯管提供了依据。     

固体发动机试车废气烟团抬升及扩散研究

对固体发动机试车排放废气烟团的抬升和扩散，采用计算与环境监测相结合的方式进行了系统研究，给出了烟团抬升计算公式。     

柔性多体卫星自抗扰控制系统的研究

设计了一种新型的姿态控制器一姿态自抗扰控制器。采用简化了的刚体动力学模型，即把柔性太阳帆板与柔性天线等的振动都看作外干扰，对象的不确定性、未建模动态与外干扰的总量都由自抗扰控制器估计出，再用该估计总量实现动态反馈补偿。该姿态控制器，只需控制输入转换矩阵的估计值，无需精确的卫星动力学模型。改变星体转动惯量或设置干扰力矩情况下的数学仿真表明，所设计的自抗扰控制器具有较小的稳态误差、较快的动态响应及对干扰有较强的抑制能力。     

中低高度卫星轨道调整策略的研究

提出了对中低高度卫星进行轨道调整的简化动力学模型。算例表明：可以通过选择发动机点火点的位置，满足卫星在可测控弧段进行轨道调整的要求。     

一种用于分析旋转对称天线的扩展矩量法

为提高旋转对称天线的计算精度,在等效矩量法(MOM)的基础上,对旋转对称天线表面电流作离散处理,根据伽列金法给出了天线表面的电场积分方程(EFIE),用朱兰成公式求得天线远场。对某旋转对称天线不同频率处的方向图计算结果表明,与等效MOM相比,该法的精度更高。     

摆式陀螺罗盘的运动特性及其分析

从陀螺力学的经典理论出发,建立了摆式陀螺罗盘的力学模型,推导出了具有重力约束的二自由度陀螺的运动方程,以此为基础,分析了摆式陀螺罗盘在阻尼及干扰条件下的运动,给出了干扰对摆式陀螺罗盘的影响的函数表达。     

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。     

Evolution of an electron beam pulse influenced by coulomb collision effects in the solar corona

Electrons accelerated in the corona during solar activity give rise to radio emission events that can be observed over a wide range of frequencies. Among different finer-scale structures in the dynamic spectra observed in the radio range, fast transients with extents of some milliseconds known as solar radio spikes are observed accompaning the background continuum emission. Fundamental to the generation of radio spikes is a propagating electron beam and following its evolution allows us to understand the physical processes occurring in the solar corona. With the use of a numerical Fokker–Planck code we follow a previous numerical study to simulate the propagation of an electron beam pulse injected in a small region at the top of a magnetic field and outwards the solar corona under typical flare conditions. It was found that in large ambient densities of ${10}^{10}$ cm⁻³ at the injection point, Coulomb collision effects have an important effect on the propagation of the electrons, causing that the injected electrons thermalize faster in a time of $0.1$ and $0.4$ s for an electron distribution with a low-energy cut off of 16 and 7 keV respectively and a spectral index of 3. For a tenous ambient medium of density ${10}^9$ cm⁻³ thermalization occurs only for an electron distribution with smaller low-energy cut off (7 keV) with a duration of $\approx$1.5 s, while for a larger low-energy cut off (16 keV) the loss of accelerated electrons is very slow, regardles of the spectral index ($3,7$). The electron loss time by Coulomb collisions, which depends on the low boundary ambient density, might be an important parameter that influences the generation of radio spikes due to the formation of instabilities in the corona.     

Riccati方程的二次代数曲线解

Ｒｉｃｃａｔｉ方程一般没有初等解，但当它有初等解时，解很可能是代数曲线解。给出了Ｒｉｃｃａｔｉ方程存在二次代数曲线解的充要条件，及其有效的求解方法。