磁悬浮柔性转子系统变学习速率单神经元PID控制

磁悬浮轴承柔性转子系统的转速范围较大,固定的控制参数很难同时保证系统所需的低频和高频特性。本文在一般单神经元PID控制的基础上,将转速信号引入磁悬浮轴承数字控制器,在不同转速段选择不同的学习速率以调节控制参数得到合适的磁悬浮轴承的刚度和阻尼。试验结果表明,变学习速率单神经元自适应PID控制能够明显减小转子在各阶临界转速时的振幅,有助于磁悬浮轴承柔性转子系统的安全稳定运行。     

压力对Fe_（16）N_2结构和磁性的影响

用基于密度泛函理论的第一性原理方法,系统地研究了压力对Fe16N2体系结构和磁性的影响。结果表明仅仅离N位最远的Fe Ⅲ拥有一个约为2.84μB的大磁矩,而FeⅠ和Fe Ⅱ原子没有大磁矩产生。此外,还发现从0到47 GPa,总磁矩和单胞体积随着压力的增加单调减小,然而,在48 GPa的压力作用下,伴随着单胞体积的剧减,体系总磁矩消失。     

磁探仪应召搜潜建模与仿真

依据经典的磁探仪应召搜潜方法,以某型反潜巡逻机为背景,建立了反潜巡逻机利用磁探仪执行平行航线、扩展矩形和螺旋形搜潜模型.对3种方法的搜潜概率进行分析,仿真了相同潜艇运动模型条件下,潜艇初始位置散布、初始距离、潜艇经济航速和海洋环境磁噪声对搜潜概率的影响.实验结果表明:相同条件下,螺旋形搜潜效能最高;潜艇只进行航速机动时...     

冷原子导引囚禁磁场的计算及分析

为了研究冷原子在磁导引中的运动规律,设计优化导体结构、电流和偏置磁场,本文根据毕奥-萨伐尔定律计算理想化导体的常规数值解,并由Matlab和VC混合编程设计出导线磁场计算工具;根据麦克斯韦方程组选择Ansoft MaxweU计算宽导线、复杂结构导体、通交变电流等情况的有限元数值解.取宽度为100μm,高度为10μm的宽...     

光学材料带电粒子辐照效应等效模拟试验方法研究

文章研究了空间带电粒子对光学材料辐照效应的等效模拟试验方法.在辐照试验研究基础上,针对光学材料分析了空间带电粒子辐照试验中辐照源选择、能谱效应,综合与顺次辐照效应和加速试验等几个关键问题,并根据空间带电粒子对光学材料的损伤特点,提出了模拟材料内部吸收荆量分布的等效试验方法.     

等通道转角挤压工艺制备超细化合金的研究与进展

等通道转角挤压技术（简称ECAP）是制备超细晶粒金属块材的最新研究领域之一。本文阐述了ECAP的研究目的与意义。说明了ECAP的原理，探讨了ECAP的国内外研究现状及进展，指出了ECAP急待解决的五大问题，具有较好的实用价值。     

Synthesis of Iron-containing Carbon Microparticles from Deoiled Asphalt and Ferrocene

The deoiled asphalt as the carbon source and the ferrocene as the metal source and the catalyst precursor were chosen to synthe-size iron-containing carbon microparticles through co-carbonization at the temperature of about 450 ℃ for 3 h. The resulting products were treated at 2 000 ℃ for 2 h. All samples were examined by high resolution transmission electron microscopy (HRTEM) and X-ray diffraction (XRD). The results show that the iron particles in the heat-treated material are completely coated by carbon. In addition to the fully filled carbon microparticles as well as hollow carbon ones, also form carbon fibers with hollow centers. The formation mechanism of the as-prepared products was discussed briefly.     

烧蚀材料的多光谱真温测量法

应用棱镜分光式多波长光电高温计对氧乙炔焰烧蚀材料的真实温度进行了测量。精心地选择波段及处理方法使烧蚀材料剥离、水蒸汽及烟雾影响减至最小，采用一点标定技术解决了高温区标定问题。     

对叔丁基苯甲酸稀土杂化发光材料的研究

本文合成了几种稀土金属离子（Eu^3＋，Tb^3＋，Dy^3＋）与对叔丁基苯甲酸的二元有机配合物，且将其不同浓度的光活性组分引入TEOS（正硅酸乙酯）基质中利用溶胶-凝胶法水解缩聚得到粉末状固体材料。同时采用了紫外吸收，荧光激发与发射光谱，扫描电镜等手段对样品进行了表征，表明该材料具较高的发光性能，得到了理想的稀土离子特征荧光且发射强度随配合物浓度增加而递增，没有出现明显的浓度淬灭现象。     

New Insights on Geomagnetic Storms from Model Simulations Using Multi-Spacecraft Data

The forecast of the terrestrial ring current as a major contributor to the stormtime Dst index and a predictor of geomagnetic storms is of central interest to ‘space weather’ programs. We thus discuss the dynamical coupling of the solar wind to the Earth's magnetosphere during several geomagnetic storms using our ring current-atmosphere interactions model and coordinated space-borne data sets. Our model calculates the temporal and spatial evolution of H⁺, O⁺, and He⁺ ion distribution functions considering time-dependent inflow from the magnetotail, adiabatic drifts, and outflow from the dayside magnetopause. Losses due to charge exchange, Coulomb collisions, and scattering by EMIC waves are included as well. As initial and boundary conditions we use complementary data sets from spacecraft located at key regions in the inner magnetosphere, Polar and the geosynchronous LANL satellites. We present recent model simulations of the stormtime ring current energization due to the enhanced large-scale convection electric field, which show the transition from an asymmetric to a symmetric ring current during the storm and challenge the standard theories of (a) substorm-driven, and (b) symmetric ring current. Near minimum Dst there is a factor of ∼ 10 variation in the intensity of the dominant ring current ion specie with magnetic local time, its energy density reaching maximum in the premidnight to postmidnight region. We find that the O⁺ content of the ring current increases after interplanetary shocks and reaches largest values near Dst minimum; ∼ 60% of the total ring current energy was carried by O⁺ during the main phase of the 15 July 2000 storm. The effects of magnetospheric convection and losses due to collisions and wave-particle interactions on the global ring current energy balance are calculated during different storm phases and intercompared. This revised version was published online in August 2006 with corrections to the Cover Date.