双流制窄轨电力机车用异步牵引电机设计

将牵引电机应用于双流制窄轨电力机车时,由于窄轨机车轨距小,所以牵引电机安装空间异常狭小,比一般牵引电机在安装空间、电机结构、电磁负荷等方面的要求更加苛刻。针对窄轨双流制电力机车的运用特点和特殊要求进行了分析,提出了牵引电机的设计要求和关键技术难点,并对关键技术难点给出了相应的分析和解决措施。对该牵引电机的制造过程及电机试验测试情况进行了论述。试验结果表明,该牵引电机达到了设计预期,完全能满足设计要求。     

热处理对FeCo-2V-0.5Cr软磁合金力学与磁学性能的影响

针对FeCo-2V-0.5Cr软磁合金,研究了真空热处理时间对其微观组织结构、力学与磁学性能的影响规律,发现在800℃下热处理时间为2h左右时,合金的抗拉强度和延伸率达到最佳,同时仍保持良好的软磁性能,抗拉强度、延伸率以及矫顽力分别为867.8MPa、10.4%以及2.0Oe。进一步对该合金进行附加磁场下的真空热处理,重点研究了合金的交流损耗与矫顽力随附加磁场方式包括磁场撤除温度与磁场下保温时间的变化规律,发现适当的磁场热处理对合金相关力学性能影响不大,但由于合金中产生了单轴各向异性而使合金矫顽力进一步降至1.6Oe。     

石英加速度计零件毛刺控制

针对现阶段石英加速度计零件的毛刺问题,分析了现有处理方法的缺陷.从被动去除和主动控制两条途径入手,以轭铁零件为例,在加工中引用了少无毛刺加工技术,并引进了新的去毛刺方法.强度检测结果表明,这两种方法的运用显著改善了毛刺控制的效果,值得推广和运用.     

泵浦激光频率波动对核磁共振陀螺仪 零偏稳定性的影响研究

本文研究了泵浦激光频率波动对核磁共振陀螺仪零偏稳定性的影响.通过分析核磁共振陀螺仪理论模型和自旋光泵浦极化129Xe的过程,阐述泵浦激光频率波动对陀螺仪零偏稳定性的影响机理.结果表明,泵浦光频率波动会导致核磁共振陀螺仪零偏稳定性下降约3个数量级.泵浦光频率波动是制约核磁共振陀螺仪性能提升的重要因素.     

The effects of the solar magnetic polarity and the solar wind velocity on Bz-component of the interplanetary magnetic field

We have studied the effect of both solar magnetic polarity and the solar wind velocity on the Bz-component of the interplanetary magnetic field, IMFBz, for the minimum activity of the solar cycles 21, 22, 23 and 24. We made a statistical study of IMFBz in the first section which is considered as an extension of Lyatsky et al. (2003). They made a statistical study of IMFBz for two periods of minimum solar activity 22 and 23 related to 1985–1987 and 1995–1997 when the solar magnetic field had opposite polarity. Our results seem to be consistent with the results obtained by Lyatsky et al. (2003). We found that there is a dependence of IMFBz on the IMFBx and the solar magnetic polarity for the minimum periods of the selected four solar cycles. In addition, we found that there is a dependence of IMFBz on the solar wind velocity.     

多功能水冷壁排管爬壁机器人的研制

介绍了一种新研制开发的永磁吸附式双履带结构爬壁机器人，主要应用于火力发电站的大型排管锅炉中的水冷壁排管壁面的清扫和检测，并能够在检测到壁面厚度小于预置的极限值处发出报警信号、打标记，具有较高的推广应用价值。文中阐述了该机器人的结构、磁路的优化设计、自动测厚、打标系统和控制系统的研制。目前，该机器人已经经过多次现场试验。各项指标均已达到设计要求。     

Solar flare forecasting model supported with artificial neural network techniques

Nowadays operational models for solar activity forecasting are still based on the statistical relationship between solar activity and solar magnetic field evolution. In order to set up this relationship, many parameters have been proposed to be the measures. Conventional measures are based on the sunspot group classification which provides limited information from sunspots. For this reason, new measures based on solar magnetic field observations are proposed and a solar flare forecasting model supported with an artificial neural network is introduced. This model is equivalent to a person with a long period of solar flare forecasting experience.     

磁转速表指针摆动的故障分析

就磁转速表活动系统的动态特性以及在附加交变力矩的作用下，指针摆动随转速变化的规律，从理论上进行了分析，并结合实际探讨了指针摆动的故障原因。     

The evolution of mirror type magnetic fluctuations in the magnetosheath based on multipoint observations

Two orbits were selected in January–February 2006 when the separation between the Cluster spacecraft was large and mirror type magnetic field fluctuations were observed by all spacecraft in different regions of the terrestrial magnetosheath. Minimum variance analysis was applied to find the mirror type fluctuations, and the amplitude of the fluctuations was determined individually. Mirror mode structures are moving along the streamlines frozen in the plasma. A model was developed for the calculation of plasma flowtime from the bow shock to the observation point. The growth rate of the field strength perturbations was estimated by comparing the amplitudes of fluctuations observed simultaneously at distant locations (∼10,000 km) based on the assumption that δB ∼ exp(γt). The obtained growth rate values were about an order of magnitude smaller than those provided by linear models and they decreased in the inner regions of the magnetosheath, indicating some saturation in the growth of the waves when proceeding towards the magnetopause. The results of these two case studies suggest that mirror type fluctuations originate from the compression region downstream of the quasi-perpendicular bow shock, and the growth of the fluctuations cannot be described by linear approximations.     

人工辅助心脏用永磁轴承盘式无刷电机设计与研究

介绍了一种应用于人工辅助心脏的永磁轴承无位置传感器盘式无刷直流电动机的结构与电磁场仿真计算方法及结果,并对其温度场进行仿真计算。该电机体积重量小,无机械轴承,避免了对血液的破坏,且运行安全可靠。