电磁抛光装置的结构设计及特性研究

介绍了五轴联动磁流变抛光系统中的关键部件———公自转电磁抛光轮的结构设计进行了详细阐述,创造性的将电刷供电方式应用于该新型抛光轮的结构中。设计并开发了直流供电及交流供电两种驱动电源,并开展了抛光去除特性试验研究,对磁流变抛光过程中的主要控制参量直流线圈电压大小对被抛光工件表面材料去除特性的影响进行了研究。     

基于图的DTAD的简易稳健自动生成算法

二维任意域(含任意多个空腔)的Delaunay三角剖分(简记为DTAD)广泛应用于有限元网格生成等方面。本文提出了一种基于图的DTAD的简易稳健自动生成算法。该算法首先构造任意域中所有边界点集的约束最小生成树,然后将同时满足本文所给三个简易约束算法的边逐次引入初始三角形网格表,形成边界点集的三角剖分,再通过稳健局部优化算法和贴体生成核插入算法自动生成DTAD。本文同时分析了退化及数值计算误差对剖分结果的影响,在提高局部优化的稳健性方面对该算法做了进一步完善,使之能更好地满足任意域网格剖分的要求。文末给出具体应用实例以说明本文所提算法的有效性。     

实用型氢激射器频标锁相接收系统

为了使上海天文台两台氢激射器频率标准更好地适应甚长基线干涉(VLBI)实验的要求,我们充分利用国内外新器件,采用新技术方案,研制出一种实用型氢激射器锁相接收系统。该系统具有接收灵敏度高(≤-120dBm)、噪音系数烛(≤1.8dB)、体积小、自动搜索人锁以及可靠性高等特点。本文主要以系统设计为实例,讨论了氢激射器频标锁相接收系统的总体设计原则、锁相环路的设计考虑和环路对系统的噪声抑制的定量估算等问题。最后,介绍了运用该系统后氢激射器频标的短期频率稳定度达到1.88×10-~(13)/S、3.7×~(-14)/10S、9.2/10~(-15)/100S9.5×10~(-15)/1000s,完全满足了甚长基线干涉实验的需要。     

空间磁场环境模拟线圈驱动恒流源设计

针对空间磁场环境模拟线圈磁感应强度0~20 Gs连续可调,磁场稳定度优于1%的要求,采用前级电压源与后级电流源串联的主电路拓扑结构,结合电压双闭环控制和电流闭环负反馈控制的方法,实现了稳定的电流输出,减小了功率金属-氧化物半导体场效应晶体管(MOSFET)的功耗,提高了恒流源的效率.测试结果表明:恒流源输出电流0~10 A连续可调,霍姆赫兹线圈中心磁感应强度能达到20 Gs的设计要求,电流稳定度优于0.1%,磁场稳定度优于1%.      

纳米NdCoO3对小球粘接高燃速推进剂燃烧性能的影响

采用盐助溶液燃烧法制备了平均粒径为10 nm、分散性良好的钙钛矿型纳米NdCoO3。用DSC考察了不同质量分数的纳米NdCoO3对AP和双基粘接剂热分解的影响,研究了纳米NdCoO3对小球粘接高燃速推进剂燃烧的催化作用。结果表明,随纳米NdCoO3催化剂质量分数的增加,催化效率先增大后减小,在质量分数为3%时催化效率最佳,此时AP高温分解峰温大幅降低,双基粘接剂的分解峰温也得到降低,二者的表观分解热增大。同时,对应的小球粘接高燃速推进剂燃速较高,压强指数较低。     

复材加热组件一体成型制备及其热/力学性能研究

针对玻纤/环氧复合材料,采用平板硫化机热压成型制备工艺,将预封装的石墨烯加热元件内嵌于复材夹层中,从而制备得到复材加热组件。实验证明,该制备方法对石墨烯复合材料的阻值及发热影响较小,保证了石墨烯加热元件的防/除冰效率。基于复材加热组件,进行了热/力学性能实验和低温除冰实验。实验结果表明,复材加热组件的温升速率随热流密度的增加而增大,并且铺层位置对复材加热组件的温升具有较大影响。在冷环境除冰实验中,环境温度为-20℃,热流密度为0.3 W/cm²时,相较于传统电加热组件,复材加热组件的除冰时间大幅减小,能耗减少约30%,为进一步制备复材加热机翼奠定了基础。     

Science objectives of the magnetic field experiment onboard Aditya-L1 spacecraft

The Aditya-L1 is first Indian solar mission scheduled to be placed in a halo orbit around the first Lagrangian point (L1) of Sun-Earth system in the year 2018–19. The approved scientific payloads onboard Aditya-L1 spacecraft includes a Fluxgate Digital Magnetometer (FGM) to measure the local magnetic field which is necessary to supplement the outcome of other scientific experiments onboard. The in-situ vector magnetic field data at L1 is essential for better understanding of the data provided by the particle and plasma analysis experiments, onboard Aditya-L1 mission. Also, the dynamics of Coronal Mass Ejections (CMEs) can be better understood with the help of in-situ magnetic field data at the L1 point region. This data will also serve as crucial input for the short lead-time space weather forecasting models.The proposed FGM is a dual range magnetic sensor on a 6?m long boom mounted on the Sun viewing panel deck and configured to deploy along the negative roll direction of the spacecraft. Two sets of sensors (tri-axial each) are proposed to be mounted, one at the tip of boom (6?m from the spacecraft) and other, midway (3?m from the spacecraft). The main science objective of this experiment is to measure the magnitude and nature of the interplanetary magnetic field (IMF) locally and to study the disturbed magnetic conditions and extreme solar events by detecting the CME from Sun as a transient event. The proposed secondary science objectives are to study the impact of interplanetary structures and shock solar wind interaction on geo-space environment and to detect low frequency plasma waves emanating from the solar corona at L1 point. This will provide a better understanding on how the Sun affects interplanetary space.In this paper, we shall give the main scientific objectives of the magnetic field experiment and brief technical details of the FGM onboard Aditya-1 spacecraft.     

Analysis of a long-duration AR throughout five solar rotations: Magnetic properties and ejective events

Coronal mass ejections (CMEs), which are among the most magnificent solar eruptions, are a major driver of space weather and can thus affect diverse human technologies. Different processes have been proposed to explain the initiation and release of CMEs from solar active regions (ARs), without reaching consensus on which is the predominant scenario, and thus rendering impossible to accurately predict when a CME is going to erupt from a given AR. To investigate AR magnetic properties that favor CMEs production, we employ multi-spacecraft data to analyze a long duration AR (NOAA 11089, 11100, 11106, 11112 and 11121) throughout its complete lifetime, spanning five Carrington rotations from July to November 2010. We use data from the Solar Dynamics Observatory to study the evolution of the AR magnetic properties during the five near-side passages, and a proxy to follow the magnetic flux changes when no magnetograms are available, i.e. during far-side transits. The ejectivity is studied by characterizing the angular widths, speeds and masses of 108 CMEs that we associated to the AR, when examining a 124-day period. Such an ejectivity tracking was possible thanks to the multi-viewpoint images provided by the Solar-Terrestrial Relations Observatory and Solar and Heliospheric Observatory in a quasi-quadrature configuration. We also inspected the X-ray flares registered by the GOES satellite and found 162 to be associated to the AR under study. Given the substantial number of ejections studied, we use a statistical approach instead of a single-event analysis. We found three well defined periods of very high CMEs activity and two periods with no mass ejections that are preceded or accompanied by characteristic changes in the AR magnetic flux, free magnetic energy and/or presence of electric currents. Our large sample of CMEs and long term study of a single AR, provide further evidence relating AR magnetic activity to CME and Flare production.     

双边永磁励磁游标电机运行原理及电磁特性仿真研究

为了进一步提高电机的功率密度和转矩密度,以满足直驱系统低速、大转矩的运行工况,提出一种新型双边永磁励磁游标(DPMEV)电机。该电机定子和转子上均放置有永磁体,利用定、转子齿对气隙磁导的双向调制作用,将两组永磁体产生的永磁磁场调制成少极数、高转速的有效谐波磁场,并根据有效谐波磁场设计电枢绕组,从而使定、转子上两组永磁体同时与电枢绕组耦合。介绍了DPMEV电机的拓扑结构。基于等效磁路法,对该电机的气隙磁通密度进行了分析,表明该电机可利用气隙磁导的双向调制作用,实现电机功率密度和转矩密度的有效提高。在深入分析电机工作原理的基础上,通过有限元法对DPMEV电机进行了计算和分析,验证了该电机具有适用于直驱系统的高功率密度和高转矩密度特性。     

5A90铝锂合金的蠕变时效行为及机理

研究了在不同时效温度和应力水平的影响下,5A90铝锂合金的蠕变时效行为和微观组织及力学性能演变规律和机理。实验采取先加载后加热的方法,即考虑了蠕变时效非等温阶段。结果表明:在恒定外加应力175MPa下,加热至100、130和160℃时的非等温蠕变应变分别为0.026%、0.036%和0.069%;160℃下等温阶段保持18 h后的蠕变应变达到1.207%,远大于130℃下的0.079%和100℃下的0.039%;蠕变应变速率随温度升高而增加;由于蠕变损伤,160℃下出现蠕变第3阶段。研究了130℃下不同应力水平对微观组织和力学性能演变的影响,发现应力为175 MPa时,非等温蠕变变形很明显,但在125和150 MPa下加热至120℃之前不会发生蠕变,并且等温蠕变应变随应力增大而增加;较高的应力可以促进δ′(Al3Li)、S(Al2MgLi)相的析出和长大;在蠕变时效初期,应力越大,位错密度越小,而在蠕变时效的后期则相反;与125和150 MPa相比,合金在175 MPa下蠕变时效初期表现出最低的强度和最好的塑性,而在蠕变时效后期则相反,这归因于位错强化和δ′相强化之间的协同作用。