径向磁力轴承系统的时间响应特性分析

本文介绍了径向磁力轴承控制系统的二次型性能指标加仅矩阵的选择,径向磁力轴承的跟踪特性和抗干扰特性分析,并给出了仿真曲线。     

基于变速积分的高速电机磁悬浮控制系统设计

针对磁悬浮高速电机的磁轴承-转子系统,设计了基于MCU+FPGA的数字控制系统。为实现转子系统的高转速下稳定控制,在建立了磁轴承-转子闭环控制系统模型的基础上,针对常规PID控制系统的超调振荡问题和PD控制系统的转子位移静差问题,利用变速积分的思想设计了改进的PID控制器。实验表明,在消除了系统静差的同时明显减小了系统的超调量和调节时间,说明设计的控制系统具有很好的动态特性和稳态精度。     

The damping of small-amplitude oscillations in quiescent prominences

The presence of small-amplitude oscillations in prominences is well-known from long time ago. These oscillations, whose exciters are still unknown, seem to be of local nature and are interpreted in terms of magnetohydrodynamic (MHD) waves. During last years, observational evidence about the damping of these oscillations has grown and several mechanisms able to damp these oscillations have been the subject of intense theoretical modelling. Among them, the most efficient seem to be radiative cooling and ion-neutral collisions. Radiative cooling is able to damp slow MHD waves efficiently, while ion-neutral collisions, in partially ionised plasmas like those of solar prominences, can also damp fast MHD waves. In this paper, we plan to summarize our current knowledge about the time and spatial damping of small-amplitude oscillations in prominences.     

Tilts and polarity separation in the sunspot groups and active regions at the ascending and descending phases of the cycle 23

The Solar Feature Catalogues for sunspots and active regions measured with SOHO/MDI instrument and Ca II K3 spectroheliograph of the Paris-Meudon Observatory are analyzed with the automated classification technique for sunspot groups and active region polarities. We report the first classification results for daily variations of tilt angles (normal and trigonometric ones) in sunspot groups (SG) and active (AR) regions in the cycle 23. The average normal tilts are presented for every year at the ascending and descending phases of the cycle 23 which are similar to those deduced by other authors for the cycles 19–22. The normal tilts of both the sunspot groups and active regions are shown to increase in the ascending phase and a decrease in the descending phase. Similar to SG and AR areas, the trigonometric tilts are shown to have the noticeable North–South asymmetry with the Southern hemisphere dominant in the selected ascending and descending periods. The normal tilt variations with latitude follow Joy’s law revealing a periodicity along the meridian of about 10° and reaching the maximum of 14° at the latitude of about 32° corresponding to the top of the ‘royal zone’ where the sunspots appear. The variations of polarity separation with a latitude are in an anti-phase with those of the tilts reaching a maximum at the latitude of 35° and showing a small positive separation for the groups/active regions in a vicinity of the average tilts ±40°. The ratio R of the polarity separation to the trigonometric tilt fits the linear function of a latitude φ as R = −0.0213φ − 0.1245 confirming positive separation for the polarities of active regions with the average tilts, or the dominance of activity in the Southern hemisphere activity, for the selected period of observations.     

The method for predicting solar proton events

Dynamic processes in the interplanetary space have been investigated using time variations in time parameters of the cosmic-ray rigidity spectrum. Change of heliosphere electromagnetic characteristics has been found out to precede sporadic phenomena on the Sun. In particular, it is shown that sporadic phenomena are followed by generation of local polarization electric fields, decrease of the magnetic-field strength in small-scale heliospheric structures, and increase of the potential difference between the pole and the plane of the ecliptic. These features allow prediction of solar proton events in advance (from several hours to several tens of hours) with a high degree of confirmation.     

Element and Isotopic Fractionation in Closed Magnetic Structures

Recent papers have suggested that the slow solar wind is a super-position of material which is released by reconnection from large coronal loops. This reconnection process is driven by large-scale motions of solar magnetic flux driven by the non-radial expansion of the solar wind from the differentially rotating photosphere into more rigidly rotating coronal holes. The elemental composition of the slow solar wind material is observed to be fractionated and more variable than the fast solar wind from coronal holes. Recently, it has also been reported that fractionation also occurs in 3He/4He. This may be interpreted in the frame-work of an existing model for fractionation on large coronal loops in which wave-particle interactions preferentially heat ions thereby modifying their scale-heights. This revised version was published online in June 2006 with corrections to the Cover Date.     

再入飞行器表面磁流体发电装置数值模拟

提出了钝锥型再入飞行器上的表面磁流体发电装置方案,采用低磁雷诺数近似下的磁流体力学模型对其进行了流动与静电场耦合的数值模拟,由此建立了表面磁流体发电装置中的物理图像.数值模拟结果表明,在典型再入条件(飞行高度46 km,速度7 km/s)下,所提出表面磁流体发电装置方案能够实现兆瓦级(电功率1.28MW)能量输出,电能提取导致再入飞行器阻力增大13.7%,对飞行器壁面总热流值的影响并不显著,但发电区域及其下游壁面的热流密度分布发生明显变化,该区域内热流密度峰值发生于电极的前、后缘.     

空间电子设备辐射屏蔽方法的研究与软件实现

研究了空间电子设备辐射屏蔽分析的方法,利用计算机辅助设计(CAD)技术和软件开发工具,将复杂繁琐的计算过程编写成流程化的程序;利用三维CAD技术的二次开发功能,从Candence软件生成的记录文件中提取出信息,在计算机图形环境中高效自动地生成电路板模型;借助计算机交互技术,实现剂量点坐标的自动提取和保存;利用办公软件个性化设置功能,设计出提取背景信息的接口,实现了最终报告文档的自动生成.开发出的软件最终成功地实现了在不同结构和布局的空间电子设备中,在不同方向和位置上累积的空间带电粒子剂量值的计算,为电子设备结构的抗辐射设计提供了参考和依据.     

永磁振动台磁路计算与仿真

根据磁场理论,介绍永磁振动台磁路工作原理以及磁隙计算方法,以北京强度环境研究所振动试验系统（AS—VA0．6）为例,校核磁隙的磁场强度,运用静磁场有限元仿真方法,通过对比可以看出理论值、仿真值与实测值是一致的,通过有限元方法,并对其进行简单优化与分菥。     

控制器参数对电磁轴承系统超谐共振区特性的影响

本文对PID控制的单自由度电磁轴承-转子系统由于力-电流／位移的非线性特性所引起的非线性振动进行了分析研究，并对控制器参数改变时，系统在三次超谐共振区的特性进行了分析。