基于Maxwell 3D的不同磁路双定子单转子电磁制动器制动力矩研究

对于双定子单转子电磁制动器,研究了两种磁路结构方案。借助Maxwell软件三维求解器,采用有限元法对两种磁路结构的电磁制动器进行仿真分析,验证了其可行性。比较了两种磁路下电磁制动器的转子电涡流、制动力矩,不同励磁电流下制动力矩响应情况,不同转子材料下制动力矩响应情况以及不同气隙长度下制动力矩响应情况。结果表明双定子单转子电磁制动器第一种磁路结构制动特性优于第二种。     

一种无需轴对准的磁罗盘正交度测试方法

给出了一种可自动化的测试双轴磁传感器正交角度的方法：正交磁场法,该方法操作简便,无需被测传感器的精密装夹;整个测量过程中没有装配操作,完全消除了由于装配的不一致性带来的误差。与常用的磁矢量投影法相比较,本方法可较快地测得双轴磁传感器的正交度,且达到较高的精度。     

拍合式电磁阀动态响应仿真分析与试验验证

根据电磁阀空载试验结果和电磁阀数学模型,对影响电磁阀响应时间的因素进行了分析.利用有限元方法和磁路分析法分别建立了拍合式电磁阀的仿真模型,用两种模型计算出不同弹簧刚度、弹簧预变形、衔铁质量、放电回路电阻、线圈匝数、非工作气隙下电磁阀的响应特性,以及这些参数对响应时间的影响程度.两种仿真计算结果和试验进行了对比,结果基本一致,根据结果分析了两种仿真方法的优缺点.总结出电磁阀在设计、生产时应重视的技术环节,对以后电磁阀设计工作具有指导意义.     

一种磁悬浮开关磁阻电机用轴向径向磁轴承

为了克服现有永磁偏置轴向径向磁轴承的缺陷,研究了一种新型结构的磁悬浮开关磁阻电机用永磁偏置轴向径向磁轴承.分析其结构及工作原理,利用等效磁路法进行分析,得出了轴向悬浮力及径向悬浮力的数学模型,并对数学模型进行了线性化处理,得出了其轴向、径向位移刚度和电流刚度.给出了磁极面积、控制线圈安匝数、定转子结构等主要参数的设计方法,给出了样机参数,用有限元对样机进行了三维仿真分析.理论研究和仿真分析表明:该永磁偏置轴向径向磁轴承结构紧凑,轴向控制磁通和径向控制磁通彼此解耦,控制更加容易,适用于高速、低功耗等场合.      

天线指向机构位置伺服的H_∞-PID控制研究

针对大型卫星天线指向机构高精度高可靠性的要求,研制了一种永磁同步电机驱动的新型天线指向机构.在建立双质量体驱动模型的基础上,以ITAE(时间乘以误差绝对值积分)为优化指标,在H_∞混合灵敏度约束下PID参数的稳定域内,采用遗传算法对PID控制器的参数进行了优化.最后采用优化的PID控制器对指向机构进行了控制仿真和实验验证,结果表明系统具有响应快速而平稳、抗负载扰动和模型误差能力强的特点.     

Model development and adaptive imbalance vibration control of magnetic suspended system

A system model is developed to describe the translational and rotational motion of an active-magnetic-bearing-suspended rigid rotor of a single-gimbal control moment gyro (SCMG) onboard a rigid satellite. This model closely reflects the motion characteristics of the rotor by considering the dynamic and static imbalance as well as the coupling between the gimbal's and the rotor's motion on a satellite platform. Adaptive autocentering control is strictly constructed for the preceding rotor with unknown dynamic imbalance. The rotor achieves its rotation about the principal axis of inertia by identifying the little rotational angles from the geometric axis to the principal axis and then using the results to tune a stabilizing controller, which is composed of a decentralized PD controller with cross-axis proportional gains and high-pass and low-pass filters. The main disturbance in the wheel spinning can thereby be completely removed and the vibration acting on the satellite can be attenuated.     

磁力传动联轴器在数字气体活塞压力计上的应用

介绍了磁力传动联轴器的结构、工作原理以及在数字气体活塞压力计上的应用.磁力传动联轴器解决了数字气体活塞压力计绝压工作模式的传动密封问题,为数字气体活塞压力计的成功研制提供了密封保证.     

实现柔性机翼后缘形状变化的综合优化(英文)

Adaptive wings have long used smooth morphing technique of compliant leading and trailing edge to improve their aerodynamic characteristics. This paper introduces a systematic approach to design compliant structures to carry out required shape changes under distributed pressure loads. In order to minimize the deviation of the deformed shape from the target shape, this method uses MATLAB and ANSYS to optimize the distributed compliant mechanisms by way of the ground approach and genetic algorithm （GA） to remove the elements possessive of very low stresses. In the optimization process, many factors should be considered such as airloads, input displacements, and geometric nonlinearities. Direct search method is used to locally optimize the dimension and input displacement after the GA optimization. The resultant structure could make its shape change from 0 to 9.3 degrees. The experimental data of the model confirms the feasibility of this approach.     

Observational study of magnetic chirality of solar active regions

We present the evolution of magnetic field and relationship with the magnetic (current) helicity in solar active regions from a series of photospheric vector magnetograms obtained at Huairou Solar Observing Station near Beijing, and also longitudinal magnetograms by MDI of SOHO, white light and 171 Å images by TRACE and soft X-ray images by Yohkoh.The conclusions in the analysis of the formation process of complex and delta magnetic configuration in some super active regions are the following: (1) The magnetic shear and gradient provide the non-potentiality of the magnetic field of active regions reflecting the existence of electric current. (2) Some of large-scale delta active regions could be due to the emergence of highly sheared non-potential magnetic flux bundles from the subatmosphere with amount of magnetic helicity, in addition to the emergence of twisted magnetic ropes. (3) We also present some results on the study of the magnetic (current) helicity in solar active regions.     

Power-law spectra of energetic electrons in solar flares from the maximum entropy and dimensional considerations

The maximum entropy formalism and dimensional analysis are used to derive a power-law spectrum of accelerated electrons in impulsive solar flares, where the particles can contain a significant fraction of the total flare energy. Entropy considerations are used to derive a power-law spectrum for a particle distribution characterised by its order of magnitude of energy. The derivation extends an earlier one-dimensional argument to the case of an isotropic three-dimensional particle distribution. Dimensional arguments employ the idea that the spectrum should reflect a balance between the processes of energy input into the corona and energy dissipation in solar flares. The governing parameters are suggested on theoretical grounds and shown to be consistent with solar flare observations. The flare electron flux, differential in the non-relativistic electron kinetic energy E, is predicted to scale as $E^{-3}$. This scaling is in agreement with RHESSI measurements of the hard X-ray flux that is generated by deka-keV electrons, accelerated in intense solar flares.