Formation flying for magnetic sails around artificial equilibrium points

This paper investigates the problem of magnetic sail-based spacecraft formation control around the artificial equilibrium points (AEPs), which can eliminate the requirement of the propellant. The thrusts are achieved by utilizing the interaction between the solar wind and the artificial magnetosphere generated by superconducting current coil onboard. The circular restricted three-body problem (CRTBP) of magnetic sail is discussed including the allowed regions and linear stability of AEPs, the locations of collinear AEPs and the possibility of existence of periodic orbits around the collinear AEPs. Next, the dynamical models of magnetic sail formation around the collinear AEPs are established. A novel fast fixed-time nonsingular terminal sliding mode controller (FFNTSM) based on fixed-time disturbance observer (FTDO) is developed to account for external disturbances. Several numerical simulations are conducted to substantiate that spacecraft formation can be precisely controlled by the proposed propellantless propulsion method in the presence of external disturbances.     

光纤环非互易相位误差尾纤补偿方法研究CSCD

针对光纤环的热致非互易误差的补偿方法进行研究,并通过仿真分析与实验验证,证明了某种光纤环尾纤长度与光纤环热致非互易误差之间的关系。根据等效介质理论和Mohr理论,建立了光纤环热致非互易相位误差仿真分析模型,并利用该模型计算了不同温度环境条件下,某类型光纤环顺逆时针方向光纤长度发生变化时,陀螺仪输出的全温零位漂移的变化量。仿真及实验结果表明,在1℃/min温变速率条件下,总长约800m的光纤环圈顺逆时针方向光纤长度相差约0.5m时,光纤环全温零位漂移量缩小了0.4(°)/h。研究结果得出了针对此类型的光纤环,当光纤环尾纤每减少0.5m,其热致非互易相位误差减小0.4(°)/h的规律。该项研究成果为后续优化光纤环的全温精度奠定了基础。     

基于三维原子磁强计的核磁共振陀螺仪实验优化

核磁共振陀螺仪内嵌三维原子磁强计是实现核磁共振陀螺仪小型化的一种有效途径,故介绍了一种基于三维原子磁强计的核磁共振陀螺仪.对影响三维原子磁强计性能的重要参数进行了优化,得到了较优的x轴、yy轴和z轴磁强计信号标度因子,进而实现了更灵敏的三维原子磁强计.在三维磁场闭环锁定6000 s后,测得核磁共振陀螺仪的角度随机游走和零偏稳定性分别为0.038(°)/h1/2和0.94(°)/h.     

磁场作用下的TIG电弧行为分析

在磁流体动力学理论的基础上,针对外加纵向磁场作用下的钨极氩弧焊(TIG)电弧在旋转圆柱坐标系中建立了不同电流密度的数学模型.通过Fluent用户自定义函数进行编程开发,对其流场和电磁场进行耦合求解,得到了外加纵向磁场作用下的TIG电弧热场和流场的分布规律.结果 表明,纵向磁场作用下的TIG电孤温度场呈现空心钟罩形态,并...