表贴式永磁电机的两种充磁方式

研究了表贴式永磁电机的两种充磁方式。首先利用已有文献电机参数验证了有限元模型的正确性,对比分析了两种充磁方式下电机磁密和磁钢磁势的分布特点,研究表明内转子结构平行充磁方式具有提供更大的气隙磁通潜力,而外转子结构则相反。接着研究了两种充磁方式,不同气隙下气隙总磁通随极对数和磁钢厚度的变化规律。同时明确了两种充磁方式各自使用场合,给出了最佳磁钢厚度的取值范围。本文工作有助于正确选择表贴式永磁电机的充磁方式和磁钢厚度,以发挥磁钢潜力,改善电机性能。     

rom 15 sel

with primary goat embryonic fibroblast showed no difference from traditional feederlayer-based culture method used in mouse and human. The putative primary EG colonies were multilayer clumps ofcompact cel     

微重力科学与应用研究（上）

空间微重力环境的独特物理现象对航天器各系统均产生无法回避的影响，在型号研制中正确计入微重力效应是航天事业发展中的一个重要研究领域。在现阶段，航天器发动机再启动相关的微重力研究以及载人航天防火安全相关的微重力研究应当引起人们的高度重视。随航天事业的发展，微重力效应问题日益会严重起来（结构动力学、耦合动力学、多相流温控、低重星球场着陆撞击……），进行深入广泛的微重力效应研究对保证航天器飞行任务完成有着不应忽视的作用     

ERG理论在房地产营销中的应用

在房地产营销中，我们根据ERG多层次需求理论，从S．T．P战略出发，将房地产市场进行细分（Segmentation）后，分析目标客户群（Targeting）并实施产品定位（Positioning）。通过进行4P营销组合，即满意的产品（Product）、适当的价格（Price）、有效的分销渠道（Place）和促销手段（Promotion）最终达到顾客满意。     

民航机场建立呼叫中心的作用及实施对策

论文介绍了呼叫中心的技术原理，在分析民诱机场商务活动的现状的基础上，阐述了呼叫中心的特点及其在机场经营业务中的作用，提出了民航机场呼叫中心的模型，最后论述了民航机场实施呼叫中心的对策。     

数学教学中培养创造能力的探索

本文结合多年教学实践，对激发学生的创造意识，培养发散思维，运用创造技法等方面进行了探索。     

计算机帧时间对半实物仿真的影响

半实物仿真试验中,要求计算机帧时间与计算积分步长相一致,但在实际试验中不容易精确地做到。本文分析了这种不一致给半实物仿真试验带来的影响,给出了解决的办法,文章中还给出了一实例来说明。     

Field formation around negatively biased solar arrays in the LEO-plasma

Heavy emission caused by impacting plasma ions results in a fast discharging effect of the initially large surface potentials on the dielectric solar cells. This eventually counteracts the energization process of the plasma ions to the cover glasses and leaves no significant electric fields. Thus, with an existing thermal plasma, electrons are again able to reach dielectric surfaces. Strong localized electric fields of the order of several 10 kV/cm form near the interconnector-cover glass interface.     

The Electron Radiation Belt

Electron radiation belts can change dramatically in a few seconds or slowly over years. Important issues in understanding such changes are: (1) What is the source of electrons in the radiation belts? (2) How important is radial diffusion compared to other radial transport mechanisms? (3) What are the detailed changes in the magnetosphere that produce radial diffusion? (4) Why is the response of the electron radiation belt to changes in the solar wind different from that of substorms and of the ring current? (5) Are processes other than radial transport, such as wave-particle interactions, important in energizing electrons in the radiation belts?     

EUV emission from normal galaxies

Using data from the Wide Field Camera EUV all-sky survey, we have established upper limits to the EUV flux from a sample of 30 bright, nearby, non-active spiral galaxies. These galaxies were chosen to be those most likely to be detected in the EUV on the basis of (i) low interstellar absorption within our own galaxy, (ii) brightness in other wavebands, (iii) high star formation activity, and (iv) proximity. The derived EUV upper limits are restrictive, and establish for the first time that the EUV flux escaping from galaxies does not constitute a major component of their bolometric luminosity, and in particular that it cannot be the sink for the energy injected into the interstellar medium by supernova explosions, as had been suggested following the failure to detect this power in the X-ray band.