Model Development and Adaptive Imbalance Vibration Control of Magnetic Suspended System

对星载磁悬浮单框架控制力矩陀螺,建立其转子的平动与转动的动力学方程。所建模型反映了转子的动、静不平衡特性,以及转子运动与框架、星体运动的耦合关系。模型是主动磁悬浮控制与动框架效应分析的基础。对动、静不平衡量未知的转子,设计了自适应对中控制器。在分散PD、比例交叉反馈控制器与高低通滤波器的基础上,通过动、静不平衡量的辨识与补偿控制,使转子绕其惯量主轴旋转,衰减角动量交换执行机构高速转子因不平衡而对基座产生的干扰力,消除星上主要颤振源,达到降低卫星姿态抖动的目的。     

无电极洛伦兹力推力器技术发展研究

近年来,为了适应深空探测、载人航天、航天器在轨服务等空间任务的需求,大推力、高比冲、长寿命、高推力密度的高功率电推进技术吸引了众多学者的持续关注.相比于其他类型的高功率电推进技术,无电极洛伦兹力推力器(ELF)在推力密度、推重比等指标上具有明显优势,且从原理上克服了电极烧蚀对高功率电推力器寿命的制约,具有广阔的应用前景...     

添加微量铜对FeCoNbSiB合金非晶形成能力及磁性的影响

采用工业用硼铁为主要原料制备一种FeCoNbSiBCu大块非晶合金.采用差示扫描量热分析、X射线衍射分析、扫描电镜及能谱分析对合金的非晶形成能力进行研究.结果表明,通过添加微量Cu可以显著提高FeCoNbSiB合金玻璃形成能力,当添加Cu的原子比含量为0.5at%～0.7at%时,合金的非晶形成能力明显提高.采用振动样品磁强计对铸态样品的软磁性能进行研究.结果表明,当Cu的加入量为0.5at%时,非晶合金的软磁性能得到提高.     

脉冲爆震发动机气动阀性能分析

通过数值模拟和试验对两种不同结构的脉冲爆震发动机(PDE)气动阀进行了研究.结果表明, 两种气动阀都能在PDE工作中起到单向阀功能, 双旋流气动阀由于切向旋流作用, 其雾化、掺混作用优于锥形气动阀, 而锥形气动阀阻力损失小.同时, 还数值模拟了锥形气动阀关闭后的流场结构, 得到了进气过程中及气动阀关闭后PDE内的流场分布, 结果显示, 气动阀关闭后, 大涡很快脱落形成一系列小涡, 大大增强了流场内的紊流度.      

Monopolar structure of the Sun in between polar reversals and in Maunder Minimum

After a polar reversal in one hemisphere the Sun has two polar caps of the same sign, leaving it in a kind of monopolar state. It may take months before a polar reversal occurs in the other hemisphere. The situation may have been extreme in the Maunder Minimum where the northern hemisphere most probably did not have polar reversals during several cycles, while the southern hemisphere may have had some. This may affect the interplanetary field and thus the cosmic rays reaching the Earth. Using the relation between the Wolf number and the speed of the global magnetic field regions the yearly mean Wolf number has to exceed 40 in order to have polar reversals, hence per hemisphere we expect that it must exceed 20. This may be used to give a definition of a deep minimum.     

离心式分级机分级理论与分级效能研究

介绍了离心式分级机的工作原理，分析了离心式分级机的流场特性，重点研究了速度特性和压力特性的分布规律，对离心机的分级效能以及改进方案进行了探讨，论述了细粉出口附加二次引风以及二相流入口速度对提高分级效率的的影响。     

Variation of energetic particle precipitation with local magnetic time

The detailed study of the precipitation of magnetospheric particles into the atmosphere is complicated by the rather complex spatial configuration of the precipitation region and its variability with geomagnetic activity. In this paper we will introduce polar oval coordinates and apply them to POES observations of 30 keV to 2.5 MeV electrons and comparable protons to illustrate the dependence of particle precipitation on local time and geomagnetic activity. These coordinates also allow an easy separation of the spatial precipitation patterns of solar and magnetospheric particles. The results indicate that (a) the spatial precipitation pattern of energetic magnetospheric electrons basically follows the pattern of the field parallel Birkeland currents up to MeV energies and (b) at least in the mesosphere the influence of magnetospheric electrons is comparable to the one of solar electrons. Implications for modeling of atmospheric chemistry will be sketched.     

利用ABAQUS软件进行航空机轮刹车热分析

飞机着陆过程中的动能主要被刹车机轮吸收,从而导致机轮温度升高。使用C/C复合材料热库后,这种情况更加明显。过高的温度对机轮及相关件的强度和工作性能将产生严重损害,容易造成刹车起火、爆胎,甚至引起灾难性事故。热分析的目的在于优化设计,为减热防热提供理论指导。传统的热分析手段仅能完成对体容温度的评估,不能定量给出机轮零部件的温度历程,成为机轮设计的薄弱环节。利用ABAQUS软件,可方便地完成刹车机轮的热分析。结果表明,热量施加方式对计算结果影响很小,而薄膜系数选取有很大影响。在所给的条件下,刹车后大约13 s,刹车盘局部达到最高温度约为983℃。计算结果与实测温度曲线变化趋势基本一致。     

Attempt to identify a source mechanism of Mercury’s sodium exosphere by a spectrometer using Fabry–Perot etalon

The Mercury’s Sodium Atmosphere Spectral Imager (MSASI) on BepiColombo (BC) will address a range of fundamental scientific questions pertaining to Mercury’s exosphere. The measurements will provide new information on regolith–exosphere–magnetosphere coupling as well as new understanding of the dynamics governing the exosphere bounded by the planetary surface, the solar wind and interplanetary space. MSASI is a high-dispersion visible spectrometer working in the spectral range around sodium D2 emission (589 nm). A tandem Fabry–Perot etalon is used to achieve a compact design. We presents a design of the spectral analyzer using Fabry–Perot interferometer. We conclude that: (1) The MSASI optical design is practical and can be implemented without new or critical technology developments; (2) The thermally-tuned etalon design is based on concepts, designs and materials that have good space heritage.     

New index of long-term variations of galactic cosmic ray intensity

We find that the soft rigidity spectrum of the Galactic Cosmic Ray (GCR) intensity variations for the maximum epoch and the hard rigidity spectrum for the minimum epoch calculated based on the neutron monitors experimental data (1960–2002) are related with the various dependence of the diffusion coefficient on the GCR particle’s rigidity for different epoch of solar activity. This dependence is stronger in the maximum epoch than in the minimum epoch of solar activity, and is provided by the essential temporal rearrangements of the structure of the Interplanetary Magnetic Field (IMF) turbulence from the maxima to minima epoch of solar activity. We also show that the rigidity spectrum of GCR intensity variations is harder for the effective rigidities ∼(10–15) GV (by neutron monitors data), than for the effective rigidities ∼(25–30) GV (by neutron monitors and muon telescopes data). A general scenario of GCR modulation versus solar activity is settled on the essential temporal rearrangements of the structure of the IMF turbulence. Therefore, the temporal changes of the power law rigidity spectrum exponent can be considered as a vital (new) index to explain the 11-year variations of the GCR intensity. We assume that ∼(70–80)% of the changes of the amplitudes of the 11-year variations of GCR intensity is related with the changes of the IMF turbulence versus solar activity.