太阳宁静区色球磁场观测

利用中国科学院北京天文台怀柔太阳磁场望远镜,对日面中心宁静区光球和色球磁场进行了长时间的积分观测。通过对光球、色球以及色球不同层次的长时间积分的观测发现,网络磁元从光球到色球扩展不大,并且部分内网络磁元升到了色球。这些结果对描述太阳磁场的两大模型提出了挑战。      

磁悬浮动量轮全滑模变结构控制

通过事先给定系统期望运动轨迹,设计出仿射非线性系统变结构控制的切换函数,该切换函数满足系统的初始状态在滑模面内的要求,因而在变结构控制的作用下,可以保证系统从初始时刻就一直运动在滑模面上,是一种全滑模变结构控制,具有比传统变结构控制更好的鲁棒性。研究还表明,约束在滑模面内的期望运动方程就是系统的滑模运动方程,系统的运动能够较好的跟踪设定的期望轨迹。将全滑模变结构控制应用于四轴型磁悬浮动量轮的控制,获得了良好的控制效果。     

可用于航天助推发射的高温超导磁悬浮技术

为了满足低成本、高安全可靠的可重复使用航天运载器发展需要,磁悬浮助推发射技术以其高地面起飞速度,提供了一种可能的技术途径。设计和研究了一种永磁导轨与高温超导体作用形成的磁悬浮系统。通过建立磁悬浮单元准静态力测试系统,分析了块状高温超导体在永磁导轨上方不同位置作用的悬浮特性。然后建立高温超导磁悬浮缩比研究试验平台,其包括4个磁悬浮单元和7米双永磁导轨。通过测试和分析试验平台在不同场冷高度和载荷条件下的悬浮特性,得出低场冷高度有利于提高磁悬浮发射装置的横向稳定性。     

基于简化FXLMS算法的磁悬浮控制力矩陀螺动框架效应精确补偿方法实验研究

磁悬浮控制力矩陀螺（MSCMG）是一种用于航天器姿态控制的高精度长寿命惯性执行机 构,动框架效应补偿是MSCMG实现高精度性能的关键技术之一。然而现有的FXLMS补偿算法由 于模型复杂、计算量大而难以实际应用。通过分析MSCMG磁轴承对象特性,提出一种简化FXL MS算法,将对象滤波器简化为常数对角阵,大幅度减少了算法计算量。对简化算法进行了仿 真,并在MSCMG样机上面进行了动框架效应补偿实验。实验结果表明：简化后的自适应控制 系统,收敛性好,跟踪速度快,具有理想的精度和较强的鲁棒性。
     

2001年9月15日Cluster卫星对电流片的观测研究

2001年9月15日0430-0515 UT期间,Cluster卫星多次穿越磁尾电流片.由FGM、CIS等仪器获得了电流片磁场,粒子速度等数据变化情况,并得到了磁尾高速流的两次明显反转.本文采用GSM坐标系.利用求磁场空间梯度张量的方法获得了越尾电流,其电流密度的峰值为28nA/m2.并对电流片在垂直方向上的摆动和在晨昏方向的波动现象进行了分析.数据显示此时电流片为薄电流片并有一个变薄的趋势,其厚度大约为0.2-0.3 Re.磁场重联时地向流与尾向流均超过了1000 km/s,并测得了电流片的法线方向和运动速度,从而得到了磁尾电流片的结构和运动情况.      

行星际扰动与不同级别磁暴强度关系的研究

利用1997-2004年间ACE卫星太阳风观测的时均值数据和相应的Dst指数,针对Dstmin≤-50 nT的磁暴,分析了行星际参数(Bz,Ey,v,Pk,|B|,ε'=vxB2zsin4(θ/2))与Dst指数的相关关系.验证了Ey,Bz与Dst指数的良好相关性;按磁暴强度的不同,发现磁暴强度越大,行星际参数与磁暴强度(Dstmin)的相关性就越好.对于中等磁暴(-100 nT＜Dstmin≤-50 nT),行星际参数与磁暴强度的相关系数不高.如果把磁暴分为两个档次,即-150 nT＜Dstmin≤-50 nT的磁暴和Dstmin≤-150 nT的磁暴,计算结果表明,ε'与Dst指数的相关性是最好的.在诸多行星际参数中,就单一因素来说,Ey对磁暴强度影响最大,Bz对磁暴强度影响次之.      

A 3rd Order WENO GLM-MHD Scheme for Magnetic Reconnection

A new numerical scheme of 3rd order Weighted Essentially Non-Oscillatory (WENO)type for 2.5D mixed GLM-MHD in Cartesian coordinates is proposed. The MHD equations are modified by combining the arguments as by Dellar and Dedner et al to couple the divergence constraint with the evolution equations using a Generalized Lagrange Multiplier (GLM). Moreover, the magnetohydrodynamic part of the GLM-MHD system is still in conservation form. Meanwhile, this method is very easy to add to an existing code since the underlying MHD solver does not have to be modified. To show the validation and capacity of its application to MHD problem modelling,interaction between a magnetosonic shock and a denser cloud and magnetic reconnection problems are used to verify this new MHD code. The numerical tests for 2D Orszag and Tang's MHD vortex,interaction between a magnetosonic shock and a denser cloud and magnetic reconnection problems show that the third order WENO MHD solvers are robust and yield reliable results by the new mixed GLM or the mixed EGLM correction here even if it can not be shown that how the divergence errors are transported as well as damped as done for one dimensional ideal MHD by Dedner et al.      

Multi-scale reconnections in a complex CME

A series of three flares of GOES class M, M and C, and a CME were observed on 20 January 2004 occurring in close succession in NOAA 10540. Types II, III, and N radio bursts were associated. We use the combined observations from TRACE, EIT, Hα images from Kwasan Observatory, MDI magnetograms, GOES, and radio observations from Culgoora and Wind/ WAVES to understand the complex development of this event. We reach three main conclusions. First, we link the first two impulsive flares to tether-cutting reconnections and the launch of the CME. This complex observation shows that impulsive quadrupolar flares can be eruptive. Second, we relate the last of the flares, an LDE, to the relaxation phase following forced reconnections between the erupting flux rope and neighbouring magnetic field lines, when reconnection reverses and restores some of the pre-eruption magnetic connectivities. Finally, we show that reconnection with the magnetic structure of a previous CME launched about 8 h earlier injects electrons into open field lines having a local dip and apex (located at about six solar radii height). This is observed as an N-burst at decametre radio wavelengths. The dipped shape of these field lines is due to large-scale magnetic reconnection between expanding magnetic loops and open field lines of a neighbouring streamer. This particular situation explains why this is the first N-burst ever observed at long radio wavelengths.     

First evidence of anisotropy of GPS phase slips caused by the mid-latitude field-aligned ionospheric irregularities

The mid-latitude field-aligned irregularity (FAI) along the magnetic field line is a common phenomenon in the ionosphere. However, few data reveal the field-aligned ionospheric irregularities. They are insufficient to identify FAIs effects so far, particularly effect on global positioning system (GPS) signals. In this paper, the mid-latitude FAIs by line-of-sight angular scanning relative to the local magnetic field vector are investigated using the denser GPS network observations in Japan. It has been the first found that total GPS L2 phase slips over Japan, during the recovery phase of the 12 Feb 2000 geomagnetic storm were caused by GPS signal scattering on FAIs both for the lines-of-sight aligned to the magnetic field line (the field of aligned scattering, FALS) and across the magnetic field line (the field of across scattering, FACS). The FALS results are also in a good agreement with the data of the magnetic field orientation control of GPS occultation observations of equatorial scintillation during thorough low earth orbit (LEO) satellites measurements, e.g. Challenging Minisatellite Payload (CHAMP) and Satellite de Aplicaciones Cientificas-C (SAC-C). The role of large-angle scattering almost along the normal to the magnetic field line in GPS scintillation is determined by attenuation of the irregularity anisotropy factor as compared with the other factors.     

高速无刷直流电机在磁悬浮惯性执行机构中的应用研究进展

为了满足新一代卫星平台高精度、高稳定度的需求,研制了一种磁悬浮惯性执行机构用功耗低、精度高、体积小、重量轻的高速无刷直流电机,提出了多约束条件下电机定子结构和转子磁体结构的设计优化原则及方法,并就高精度的锁相速度控制以及铁耗和转矩脉动的抑制方法进行了研究.对比分析了国内外高速永磁无刷直流电机在磁悬浮惯性执行机构中的应用研究现状,指明了所提出的设计原则和控制方法对提高磁悬浮惯性执行机构整体性能的有效性.