电磁轴承电磁铁单边工作控制方式的实现

由于电磁力与位移及励磁电流的强非线性,使电磁轴承AMB(Active Magnetic Bearing)系统精确建模比较困难,较高的偏置电流增加了系统的功耗,系统的高刚度与大范围稳定又是一对矛盾体.为此,在建模型时,以电磁力为控制量,将电磁力计算公式、电磁铁及功率放大器集成为电磁力构件,避开了电磁力非线性的影响;在基础电流为0.2 A时,采用电磁轴承单边的工作方式,实现了系统的高刚度;以模糊控制方法解决了系统高刚度与大范围稳定的矛盾.仿真与试验表明:以电磁力构件的方式构造电磁轴承模型有较好的精度,采用单边的工作方式降低了系统的功率损耗,采用模糊控制方法实现了系统大范围稳定小范围内高刚度.      

大型铁磁性物体近场磁异常场数值仿真

磁异常探测是一种在地球物理领域有着广泛应用的探测方法,磁异常场的空间分布规律信息是磁异常探测的主要理论依据。对矩形铁磁性物体空间磁场模型进行了推导,利用ANSYS Maxwell分析了大型铁磁性物体近场的磁异常场空间分布规律。针对不同地磁场方向条件,得到了近场空间磁感应强度总量分布及矢量分布规律,揭示了在不同条件下磁感应强度模量场和矢量场都具有普遍的对称性和规律性。通过对仿真模型进行缩比试验,测量了类似条件下模型近场的磁感应强度模量场和矢量场信息,验证了仿真得到的磁异常场空间分布规律的一致性和正确性。      

Assessment of depth to magnetic sources using high resolution aeromagnetic data of some parts of the Lower Benue Trough and adjoining areas,Southeast Nigeria

High resolution airborne magnetic data acquired between 2005 and 2010 were used to determine depth to shallow and deep magnetic sources in some parts of Southeastern Nigeria. Various depth estimation methods such as standard Euler deconvolution (SED), source parameter imaging (SPI), spectral depth analysis (SDA) and two dimensional (2-D) forward modeling were applied. Results obtained from SED, SPI and models of profiles 1 and 2 indicate that the Abakaliki Anticlinorium (AA) and Ikom-Mamfe Rift (IMR) regions are dominated by short wavelength magnetic anomalies caused by extensive tectonic events. The SED map showed depth to shallow and deep magnetic sources ranging from ~ 16.6 to ~ 338.3 m and ~ 394.3 to ~ 5748.1 m respectively. Likewise, depth estimates from the SPI map varies from ~ 147.1 to ~ 554.2 m (shallow magnetic sources) and ~ 644.2 to ~ 6141.6 m (deep magnetic sources). The result obtained from SDA revealed depths to deep magnetic basement in the range of ~ 769 to ~ 6666 m with an average of ~ 3449 m. Also, it showed that depth to shallow magnetic sources vary between ~ 119 and ~ 434 m with mean of ~ 269 m. The 2-D forward modelling showed maximum depth values of ~ 4700, ~4600 and ~ 6500 m in the models of profiles 1, 2 and 3 within the Anambra Basin (AB), Afikpo Syncline (AS) and Calabar Flank (CF) respectively. Generally, from all the various methods applied the results indicate that AB, AS and CF are dominated by long wavelength anomalies. The 2-D models indicated that the basement framework is undulant. Also, depth estimates involving the various methods used in this study correlate strongly with each other in the AB, AS and CF geological regions.     

Magnetic storm cessation during sustained northward IMF

Times of sustained strong northward IMF can interrupt the magnetic storm development and lead to lower levels of geomagnetic activity for many hours. During 1997–2000 we have found two events of this kind observed on November 8, 1998 and October 13, 2000. In both cases, the storms started as usual after arrival of ejecta with a southward IMF component from the Sun to the Earth, but ceased after several hours due to the onset of sustained northward IMF leading to the faster recovery process. After the passage of this so-called positive domain, the storm development started again. The heliospheric magnetic field intensity remained enhanced and nearly constant. The solar origins of the geomagnetic storm interruptions have been investigated. Tentatively they may be related to strong nonlinear Alfvйn type solitary waves excited by non-stationary coronal current variations with a characteristic time-scale of about a day.     

利用近地点磁场探测数据确定卫星自旋轴参数

阐述了利用近地点磁场探测数据确定卫星自旋轴参数的理论方法和实施步骤,并说明了这种研究对卫星运行和科学探测的重要性.特别强调了需要注意的基本条件,即卫星必须自旋稳定且近地点不很高(1000 km以下).这种方法关键的步骤是,根据卫星轨道数据定出模型磁场数值,比较近地点星载磁强计探测数据和近地点地磁模型数值确定卫星自旋轴的指向.通过对TC-1和TC-2卫星姿态的具体计算,对确定精度和应用效果进行了分析和比较.结果表明,在实际的卫星应用过程中此方法和措施非常有效,在科学分析和将来的卫星运行工程中具有重要的应用意义.     

基于嫦娥一号高能粒子数据的地球磁层屏蔽效应研究

月球绕地球运行轨道约有1/4位于地球磁层内,因此,地球磁层是否会为月球轨道附近高能粒子提供足够的磁场屏蔽对于探索月球活动具有重要影响.嫦娥一号是中国首颗绕月人造卫星,其绕月飞行的工作轨道距离月球表面200 km.通过对嫦娥一号高能粒子探测器(HPD)的探测数据进行分析,比较了当月球位于地球磁层内外6个不同能道(能量范围4～400 MeV)时质子通量的变化,发现当月球位于地球磁层内时,这些能道的质子通量并没有发生显著减少,结果表明地球磁层不能为月球轨道附近高能粒子提供显著的磁屏蔽.     

微型核磁共振陀螺仪的关键技术及发展趋势

微型核磁共振陀螺仪能够兼顾高精度、小体积和低功耗等特点,已成为原子陀螺仪的重要研究方向之一。本文在阐述核磁共振陀螺仪工作原理的基础上详细分析了闭环方案、开环方案和低温超导方案几种技术途径的特点,讨论了微型原子气室、微型磁场线圈、无磁加热等关键技术对核磁共振陀螺仪性能的影响,展望了核磁共振陀螺仪的应用前景和发展趋势。     

用假想磁荷模型计算三维静磁场的解耦问题

本文提出了用假想磁荷模型计算三维静磁场的解耦概念和实施方法,较好地解决了假想磁荷模型中的磁位跃变边界问题。通过实例计算,证明了该概念和方法的正确性。     

磁悬挂天平的电磁铁与控制器设计——磁悬挂天平技术研究之二

本文介绍30mm×30mm 五分力磁悬挂天平的电磁铁结构,讨论电磁铁设计中的几个问题,采用各通道局部补偿的控制方法实现了小气动力作用下飞行器模型的不同姿态悬挂。     

三浮陀螺仪有源磁悬浮加力系统研究

三浮陀螺仪输出轴采用有源磁悬浮,系统工作在分时控制模式下,控制变量为总周期和周期内加力占空比.加力电源类型的选取以及加力电压幅值的确定对电磁力的大小、磁悬浮的功耗有很大影响,进而影响陀螺温度场分布和陀螺精度.在研究了磁悬浮元件电磁特性之后,给出了确定加力电源的基于磁路分析的Flux电磁仿真法.分析给出直流、正弦和方波这三种电源的加力幅值范围为1.7V～ 2V,并结合试验确定1.8V的方波电压加力为最佳方案.实验表明采用该方法分析加力电压是有效的,同时节省了大量实验探索的时间.