精密定位与测量技术在真空低温环境下的应用

分析了圆感应同步器和磁栅的特性,提出了在真空低温的特殊环境下进行精密测量的方法。     

双极型磁选态单束铯束管内铯原子运动轨迹的算法改进

针对简化算法得到的铯原子运动轨迹精度不高的结果,通过分析磁选态单束铯束管内双极型选态磁铁的磁场分布,提出了不简化磁场梯度和有效磁矩,用布利厄施-施多厄方法求解铯原子运动方程的算法。用此算法得到的铯原子运动轨迹与通常采用的简化算法得到的轨迹相比,最大差异约为10 mm。此计算结果影响管内机械组件的安装对中位置,可用于束光学模拟计算,提高短期稳定度指标。     

线圈压床伺服控制技术应用

WPN系列数控线圈压床是集机、电、液、计算机控制为一体的大型变压器线圈生产的设备。其控制系统采用了先进的多轴运动控制卡作为主控制系统,辅助以液压伺服系统、数据采集与处理系统、安全防护系统的全新结构、性能先进的伺服数控线圈压床。     

基于超导的重力梯度敏感线圈电磁特性分析

为了利用超导块体的完全抗磁性与敏感线圈的电感变化测量重力梯度,需要对敏感线圈的电磁特性进行分析.利用盘状超导敏感线圈产生磁场,首先分析单匝线圈在场点产生的磁感应强度,再通过叠加得到场点的总磁感应强度.选取设计参数对线圈外小间距范围内的磁感应强度进行计算可知,径向分量沿线圈径向保持稳定值,而轴向分量变化较大.质量块对总磁...     

基于磁力研磨法对微型槽的精密研磨研究

微型喷嘴旋流槽棱边去毛刺及槽底面光整用传统加工方法难以实现,利用磁力研磨法能够很好实现旋流槽棱边去毛刺及槽底面的光整加工.文中分析了磁力研磨法对棱边去毛刺及槽底面光整的加工机理,并进行了有限元理论分析和试验验证,利用3D超景深电子显微镜观察并记录喷嘴旋流槽加工前后照片,验证结果表明,永磁研磨机可以很好地实现对微型喷嘴旋流槽棱边去毛刺及槽底面光整研磨.     

P70霍尔推力器新型缓冲腔磁路对预电离及放电的影响

为有效利用从P70霍尔推力器放电通道进入缓冲腔的快电子能量,考虑两个磁场特征以提高缓冲腔预电离率。一是提高磁感应强度,二是缓冲腔内从气体分配器到放电通道方向的负梯度。采用FEMM有限元磁场计算软件,在不改变推力器电离和加速通道内优化磁场特征的前提下,设计的新型缓冲腔磁路满足上述磁场特征。放电实验结果表明,在新型缓冲腔磁路下放电电流低频振荡幅值更小。新型磁路有助于延长推力器寿命,有助于电离和加速通道内电离与加速区的分离。     

Model Development and Adaptive Imbalance Vibration Control of Magnetic Suspended System

对星载磁悬浮单框架控制力矩陀螺,建立其转子的平动与转动的动力学方程。所建模型反映了转子的动、静不平衡特性,以及转子运动与框架、星体运动的耦合关系。模型是主动磁悬浮控制与动框架效应分析的基础。对动、静不平衡量未知的转子,设计了自适应对中控制器。在分散PD、比例交叉反馈控制器与高低通滤波器的基础上,通过动、静不平衡量的辨识与补偿控制,使转子绕其惯量主轴旋转,衰减角动量交换执行机构高速转子因不平衡而对基座产生的干扰力,消除星上主要颤振源,达到降低卫星姿态抖动的目的。     

Evolution of coronal mass ejection/shock system in interplanetary space

The evolution of coronal mass ejection/shock system is investigated by numerically solving the usual set of two-dimensional single-fluid polytropic magnetohydrodynamic equations from 1 R_s to 1 AU in the meridian plane. The simulation result reveals that the coronal mass ejection/shock system formed near the sun evolves into the magnetic cloud/shock system near the earth’s orbit through the following three phases: the initial formation, the dominant latitudinal expansion and the similar expansion.     

Relativistic solar protons in the ground level event of 23 February 1956: New study

In this study we applied again to the outstanding solar particle event of 23 February 1956, the largest one in the entire history of observations of solar cosmic rays. Due to significant improvement of the analysis/modeling techniques and new understanding of physical processes in the solar atmosphere and interplanetary space, a possibility arises to interpret the old data in the light of modern concept of multiple particle acceleration at/near the Sun. In our new analysis the data of available then neutron monitors and muon telescopes are used. The technique of the analysis includes: (a) calculation of asymptotic cones of ground-based detectors; (b) modeling of cosmic ray detector responses at variable parameters of the flux of solar relativistic protons; (c) determination of primary solar proton parameters outside magnetosphere by comparison of computed responses with observations. Certain evidence was obtained that the flux of relativistic solar protons consisted of two distinct components: prompt and delayed ones. The prompt component with exponential energy spectrum caused a giant impulse-like increase at a number of European cosmic ray stations. The delayed component had a power-law spectrum and was a cause of gradual increase at cosmic ray stations in the North American region. A numerical simulation of the proton acceleration in the vicinity of the magnetic reconnection region brings to the proton spectrum with exponential dependence on energy. This agrees with observational data for the prompt component. It is also shown that the huge increase in ∼5000% on neutron monitors was due to the prompt component only with the exponential proton spectrum. The power-law spectrum of comparable intensity gave considerably smaller effect.     

磁尾等离子体片对流对亚暴的影响

采用2(1/2)维全粒子电磁模拟方法研究了等离子体片中稳态对流及局地爆发高速流对磁层亚暴触发过程的影响.研究发现,地向瞬时局地高速流可触发磁场重联,导致储存于磁尾磁场能量的快速释放.但是,等离子体片稳态对流可抑制磁尾磁场重联过程.此项研究结果表明,局地爆发高速流能够触发磁层亚暴;而行星际磁场(IMF)持续南向时的稳态磁层对流期间,不易发生亚暴.