Radio Heliographic Diagnostics of Solar Activity That Governs Space Weather

In this paper, the possibility and some results of radioheliographic study of space weather solar factors are shortly described.     

A Theoretic Interpretation of Movement of the Cusp Equatorward Boundary

A preliminary model is proposed to describe quantitatively the position and movement of cusp equatorward boundary. This integrated model, consisting of an empirical model of the magnetopause and a compressed dipolar model of Open/Closed field line, connects quantitatively the solar wind conditions, subsolar magnetopause and cusp equatorward boundary. It is shown that the increasing solar wind dynamic pressure and the increasing southward Interplanetary Magnetic Field (IMF) component drive the magnetopause to move inward and the cusp equatorward. This model is adopted to interpret quantitatively the cusp movement of August 14, 2001 observed by Cluster. The results show that the subsolar magnetopause moved earthward from 10.7 He to 9.0 Re during the period of 002300-002800 UT, and correspondingly the cusp equatorward boundary shifted equatorward. The observations of Cluster C1 and C4 show the cusp equatorward boundary that Cluster Cl and C4 were crossing during same interval moved equatorward by 4.6°. The cusp equatorward boundary velocity computed in the theoretical model (10.7km/s) is in good agreement with the observed value (9.4km/s) calculated from the data of CIS of Cluster C4 and C1.     

关于IMF北向分量特强时的太阳风－磁层－电离层耦合

Relationship between the solar wind-magnetosphere energy coupling function and the energy consumption in the magnetospheric system is tested by the samples during period of northward B_z(>10 nT) of IMF. It is shown that the energy function which can well describe the solar wind-magnetosphere coupling when B_z>0 is no more applicable for B_z>10 nT, but the coupling still exists, the effects of which are mainly found at the polar cap. Dst often turns to positive when B_z> 10 nTand the coupling mechanism is different from that when B_z<0. New coupling function has to be introduced to describe the solar wind-magnetosphere coupling for the case of B_z> 10 nT.      

磁场辅助电火花加工平台开发及SiCp/Al加工试验研究

结合微细电火花加工的技术特点,对微细电火花加工控制系统进行模块化设计,完成了磁场辅助电火花加工系统试验平台搭建,基于LabWindows/CVI环境开发了人机交互操作界面,进行了磁场辅助电火花微孔加工试验,验证了该微细电火花加工机床的稳定性。单脉冲试验结果表明,放电持续时间随着磁感应强度的增大而变长,磁感应强度的增大使放电凹坑直径增加、深度减小,材料去除体积增大。微孔加工试验结果表明,适当的外部磁场对电火花加工性能有显著的提升作用。施加0.3 T的外部磁场时,材料去除率得到提高,表面粗糙度有所降低。体积分数越大的SiC_p/Al复合材料去除率提高越明显,体积分数为65%的SiC_p/Al复合材料在施加外部磁场后,材料去除率提升高达96.85%。     

基于矢量磁强计的磁场梯度张量仪误差校正方法

卫星在轨运行时,本体会产生一定的磁干扰,一般通过伸杆将传感器远离卫星本体安装,或者通过多个磁场传感器测量磁场梯度的方法来消除卫星本体的磁干扰.使用磁场梯度张量仪测量磁场梯度时,张量仪本身的构型会给测量带来误差.通过对5种主要的张量仪构型进行误差仿真,对比5种构型的张量测量误差,发现十字形构型张量仪的测量误差最小.除了构型带来的误差,张量仪的主要测量误差还包括组成张量仪的三轴磁强计本身的误差和非对准误差.本文使用椭球拟合算法对磁强计本身的误差进行校正,校正后磁强计测量总场的均方根误差为0.864nT.针对张量仪的非对准误差,提出了正交系间非对准误差的校正方法.仿真结果表明,校正后的非对准角度误差≤3.2×10-5 rad,能够很好地降低张量仪的非对准误差.      

表贴式永磁同步电机永磁体偏心气隙磁场解析

采用分区域的方法对表贴式永磁同步电机磁极偏心的气隙磁场进行推导解析。将求解区域分为永磁体区域、气隙区域、定子槽区域和基于分离变量法利用各区域的边界条件得出相关系数,并在计及永磁体偏心的情况下求解电机气隙磁场。解析模型能够计算电机空载和负载气隙磁场的分布。将解析模型计算结果与有限元分析结果进行对比,发现所建立的解析模型具有较高的准确度。     

任意形状平面载流线圈在远点处的磁场计算

在电磁场中,经常计算圆环、矩形、三角形等规则平面载流线圈特殊点（如中心轴线上）的磁场分布规律,而复杂一些的问题,例如规则平面载流线圈的远点和任意点的磁场分布规律由于数学处理繁杂一般不加以计算.实践中通过对规则平面载流线圈中心轴线上任意一点和与该线圈共面的对称线上的任意一点的磁场分布规律的整理分析,用二者合成的方法,经推广得出一般性规律,可以解决任意形状的平面载流线圈在远点处这一类的磁场计算问题.     

一种求解任意形状导体目标内谐振时表面电流的有效方法

用矩量法求解闭合导体目标的电场积分方程或磁场积分方程将得到不正确的表面电流。提出了一种确定正确表面电流的有效方法，即正确的表面电流由非谐振模电流和归一化的谐振模电流与一未知复因子的乘积组成，通过令闭合导体内给定点的总电场为零可得该未知复因子。计算了一无限长理想导体圆柱谐振时的表面电流，所得结果与解析解一致，进而证明了本方法的有效性和准确性。     

均匀磁场中铁磁流体润滑的轴颈轴承

当均匀外加磁场强度从0增加到 0.12 MA/m时, 在高剪切速率下铁磁流体润滑膜的承载能力提高25%,而在低剪切速率下, 承载能力可提高 35%。所以, 从实用的观点来看, 铁磁流体润滑是为了利用外磁场来调节轴承的承载性能, 而不是为了获得高承载力。为了避免轴承承载能力受到限制, 需要将铁磁流体密封与润滑膜分离开来。分析表明均匀磁场和剪切速率对姿态角的影响甚为微小。