难加工合金材料复杂曲面磁性磨料光整加工技术

磁性磨料光整加工技术是一种非常重要的光整加工技术,与低频振动和超声振动相结合,可实现高精度、高质量和高效率的光整加工。介绍了磁性磨料光整加工、振动辅助磁性磨料光整加工及超声辅助磁性磨料光整加工技术的原理和特点及相关的国内外研究现状。根据难加工合金材料复杂曲面的特点,提出实现复杂曲面磁性磨料光整加工,需要就以下问题开展进一步研究和探索:通过提高加工间隙的磁通量密度及磁能与其他能量复合来提高光整加工效率;建立复杂曲面磁性磨粒光整加工过程控制函数;探讨在磁极工具的空间几何约束作用下复杂曲面磁性磨料光整加工工艺的规划方法等。     

空间光学敏感器/探测器荷电粒子屏蔽技术综述

空间光学敏感器/探测器是航天器的重要组成部分或重要类型,然而大量存在的空间荷电粒子会造成探测器件本底噪声及性能损伤,对空间探测任务产生不良影响。目前对空间荷电粒子的影响缺乏定量评估手段,广泛采用的质量屏蔽、磁偏转和反符合技术在空间荷电粒子屏蔽方面均存在局限性。在对上述方法进行综述的基础上,提出了基于电磁复合场的空间光学敏感器/探测器荷电粒子屏蔽装置的设计思路。     

电磁阻尼器性能参数试验研究

电磁阻尼器性能与多种因素有关,在电磁阻尼器基本性能试验研究基础上,制作了一个电磁阻尼器模型,进行了涡流板厚度参数影响的试验研究:做了3种厚度涡流板在不同频率、不同位移情况下的试验,得到了涡流板厚度对阻尼器性能影响的定性结论。     

利用生物信息学数据及工具合成表达链霉亲和素基因

目的:人工合成表达链霉亲和素基因,制备链霉亲和素磁珠复合物用于核酸分离.方法:利用NCBI、BCM等提供的生物信息及软件工具,将链霉亲和素蛋白的基因进行密码子优化,并分割成互为重叠的小片段寡聚核苷酸链,采用化学和酶促合成相结合的方法合成编码链霉亲和素蛋白基因.将纯化的链霉亲和素通过偶联剂与带羧基的磁粒共价结合,用于快速...     

MEMS磁场传感器的设计及测试

以U型梁为主要结构设计了一种新型的洛伦兹力驱动的磁场传感器,检测在磁场中作切割磁力线运动的金属线上的感生电压,实现磁场测量.首先介绍了传感器的工作原理,并用振动理论对传感器的受力及响应进行了分析,接着用有限元软件建立结构模型并对其振动模态和频率进行了仿真.该MEMS磁场传感器采用标准的CMOS工艺加上后处理来实现.最后...     

超声乳化法制备纳米Fe3O4磁性颗粒及壳聚糖表面改性

采用超声乳化法制备纳米Fe3O4磁性颗粒,以壳聚糖作为表面活性剂,制备具有生物亲和性的水基Fe3O4磁流体.研究了Fe2+/Fe3+摩尔比、超声时间和表面活性剂用量对磁流体性能的影响.结果表明:当Fe2+/Fe3+摩尔比为1:1·5,滴加氨水时反应温度为70℃时,可制备理想纳米Fe3O4磁性颗粒;超声时间为7·5min左右,质量分数1%的壳聚糖溶液体积占FeO溶液总体积的50%时,有利于壳聚糖分子的包覆,使磁流体具有较高的比饱和磁化强度及稳定性.     

Nd~(3+)的稳定能与晶场参数及磁交换作用的关系

基于单离子模型,通过对Nd3+磁晶各向异性哈密顿数值的求解,研究了温度趋于0 K时,Nd3+离子稳定能与晶场参数及磁交换作用的关系.结果表明,对于强磁物质(如NdCo5,Nd2Co17,Nd2Fe14B等),Nd3+贡献的稳定能与晶场参数B20近似成正比,而对磁交换作用的变化不敏感.     

基于巨磁阻抗效应表征材料磁结构的模型

研究了一种可用于磁结构表征的基于巨磁阻抗效应分析材料磁结构的模型.在建立巨磁阻抗效应与简化磁结构对应关系模型的基础上,结合磁化矢量正交分解手段,通过调节巨磁阻抗效应与简化磁结构对应关系模型特征参量的方法,获得了各种形状的巨磁阻抗曲线,根据拟合得到的解叠子谱特征,可获知材料内部磁结构的组成和特征.研究结果对于磁性材料内部磁结构的新型表征方法及其内部结构的控制具有重要的意义.     

Enhanced anti-sunward flow near local noon during a period of horizontal IMF and high solar wind velocity <Emphasis Type="Italic">V</Emphasis><Subscript><Emphasis Type="Italic">Y</Emphasis></Subscript>

It is believed that a southward interplanetary magnetic field (IMF) is mainly responsible for the energy input from solar wind into the magnetosphere. This paper presents an unusual case of strong anti-sunward plasma flow (up to 2 km/s) in the polar cap ionosphere and large cross-polar cap potential (CPCP) during a period of horizontal IMF (|B _Z | < 2 nT) observed by both ACE (at the L1 point) and Geotail (on the dusk flank of the magnetosheath). The CPCP is even higher than that under preceding B _Z ≈ −23 nT. Furthermore, GOES8 observed that the magnetosheath field turns northward as the anti-sunward plasma flow and CPCP start to increase, which implies that the magnetosheath field interacting with the Earth’s magnetopause has significantly rotated and differs from the IMF observed by ACE and Geotail. In accordance with previous theoretical work, we suggest that the magnetic field line draping produces a southward magnetosheath field and enhances anti-sunward plasma flow and the CPCP.     

The effects of the guide field on the structures of electron density depletions in collisionless magnetic reconnection

Two-dimensional particle-in-cell simulations are performed to investigate the formation of electron density depletions in collisionless magnetic reconnection.In anti-parallel reconnection,the quadrupole structures of the out-of-plane magnetic field are formed,and four symmetric electron density depletion layers can be found along the separatrices due to the effects of magetic mirror.With the increase of the initial guide field,the symmetry of both the out-of-plane magnetic field and electron density depletion layers is distorted.When the initial guide field is sufficiently large,the electron density depletion layers along the lower left and upper right separatrices disappear.The parallel electric field in guide field reconnection is found to play an important role in forming such structures of the electron density depletion layers.The structures of the out-of-plane magnetic field By and electron depletion layers in anti-parallel and guide field reconnection are found to be related to electron flow or in-plane currents in the separatrix regions.In anti-parallel reconnection,electrons flow towards the X line along the separatrices,and are directed away from the X line along the magnetic field lines just inside the separatrices.In guide field reconnection,electrons can only flow towards the X line along the upper left and lower right separatrices due to the existence of the parallel electric field in these regions.