Evolution of coronal mass ejections in the early stage

This work reports the investigation of two coronal mass ejections (CME) observed in white light, H, EUV and X-ray by various instruments both in space and on ground on February 18, 2003 and January 19, 2005, respectively. The white light coronal images show that the first CME began with the rarefaction of a region above the solar limb and was followed by the formation of its leading edge at the boundary of the rarefying region at altitude of 0.46 R from the solar surface. The rarefaction coincided the slow rising phase of the filament eruption, and the CME leading edge was observed to form as the filament eruption started to accelerate apparently. In the early stage of the second CME, a bright loop was first observed above the solar limb with height of 0.37 R in EUV images. We found that the more gradual CMEs initial process, the larger the timing difference between CMEs and their associated flares. The lower part of the filament brightened in H images as the filament rose to a certain height. These brightenings imply that the filament may be heated by magnetic reconnection below the filament in the early stage of the eruption. We suggest that the possible mechanism which led to the formation of the CME leading edge and cavity is magnetic reconnection which occurred under the filament when it reached a certain height.     

Force-free magnetic field in a cylindrical flux rope without a constant alpha

It is generally assumed that magnetic fields inside interplanetary magnetic clouds and flux ropes in the solar photosphere are force-free. In order to model such fields, the solution of rot B = B is commonly used where  = const. But comparisons of this solutions with observations show significant difference. To treat this problem,we examine the solutions with .     

Solar Elemental Composition Based on Studies of Solar Energetic Particles

Solar abundances can be derived from the composition of the solar wind and solar energetic particles (SEPs) as well as obtained through spectroscopic means. Past comparisons have suggested that all three samples agree well, when rigidity-related fractionation effects on the SEPs were accounted for. It has been known that such effects vary from one event to the next and should be addressed on an event-by-event basis. This paper examines event variability more closely, particularly in terms of energy-dependent SEP abundances. This is now possible using detailed SEP measurements spanning several decades in energy from the Ultra Low Energy Isotope Spectrometer (ULEIS) and the Solar Isotope Spectrometer (SIS) on the ACE spacecraft. We present examples of the variability of the elemental composition with energy and suggest they can be understood in terms of diffusion from the acceleration region near the interplanetary shock. By means of a spectral scaling procedure, we obtain energy-independent abundance ratios for 14 large SEP events and compare them to reported solar wind and coronal abundances as well as to previous surveys of SEP events.     

乙烯基硅橡胶生胶中低分子的脱除

由于硅橡胶是用催化平衡的方法制备，生胶中含有约3％的挥发性的低分子量环体，会对硅橡胶的热真空失重（TML）、可凝挥发物性能（CVCM）有极大影响。为使所制得的硅橡胶符合空间级材料要求，分别采用溶剂抽提法和热真空处理法来脱除乙烯基硅橡胶中的小分子，通过比较处理前后硅橡胶的分子量及其分布、TML、CVCM，对比了两种方法脱除小分子的效果；并制备得到了符合空间级标准的硅橡胶。     

军用飞机大修过程质量控制方法研究

结合飞机大修的常规流程,分析了各阶段产生的故障信息,从全面质量管理理念出发选取监控点,研究了故障数据分析方法,并利用C控制图实现了在不同维修工序后对大修飞机质量特性波动的定量认识、评估、处理和监控,保证了军用飞机大修后的安全性和可靠性。     

Direct thrust test and asymmetric performance of porous ionic liquid electrospray thruster

In order to meet the demand of CubeSats for low power and high-performance micro-propulsion system, a porous ionic liquid electrospray thruster prototype is developed in this study. 10 × 10 conical emitter arrays are fabricated on an area of 3.24 cm² by computer numerical control machining technology. The propellant is 1-ethyl-3-methylimidazolium tetrafluoroborate. The overall dimension of the assembled prototype is 3 cm × 3 cm × 1 cm, with a total weight of about 15 g (with propellant). The performance of this prototype is tested under vacuum. The results show that it can work in the voltage range of ±2.0 kV to ±3.0 kV, and the maximum emission current and input power are about 355 μA and 1.12 W. Time of Flight (TOF) mass spectrometry results show that cationic monomers and dimers dominate the beam in positive mode, while a higher proportion of higher-order solvated ion clusters in negative mode. The maximum specific impulse is 2992 s in positive mode and 849 s in negative mode. The thrust is measured in two methods: one is calculated by TOF results and the other is directly measured by high-precision torsional thrust stand. The thrust (T) obtained by these two methods conforms to a certain scaling law with respect to the emission current (I_em) and the applied voltage (V_app), following the scale of T ∼ I_emV_app^0.5, and the thrust range is from 2.1 μN to 42.6 μN. Many thruster performance parameters are significantly different in positive and negative modes. We speculate that due to the higher solvation energy of the anion, more solvated ion clusters are formed rather than pure ions under the same electric field. It may help to improve thruster performance if porous materials with smaller pore sizes are used as reservoirs. Although there are still many problems, most of the performance parameters of ILET-3 are good, which can theoretically meet the requirements of CubeSats for micro-propulsion system.     

导弹质量特性测量装置设计

设计了一种导弹质量、质心、转动惯量一体化测量设备，可在同一台设备设计上完成导弹质量、轴向和径向质心、俯仰偏航方向的转动惯量测量。该装置主要由测试平台、活动支架、沿导弹纵轴滑动的精确定位机构、三个测力传感器和一个倒扭摆机构组成。了该装置质量特性测量方法，定量分析了测量误差，并总结了此类装置设计的几个关键问题。     

虚拟仪器技术在发动机质心测量中的应用

研究了虚拟仪器技术在发动机质心测量中的应用，建立了电测系统的误差模型，对电测系统的误差进行校正，最终测试结果表明整个测量系统的测量精度得到了提高。     

克服旋转导弹螺旋运动的方法研究

本文结合旋转导弹自身的特点，提出了一种通过主动控制弹体内部活动质量块的运动来克服旋转弹螺旋运动的方法，这将有助于提高旋转导弹的合中精度。文中针对大气层外飞行的旋转导弹进行仿真研究，计算结果证实了该方法的有效性和可行性。     

多分支管道若干流动现象和特性的探讨

在稳定的多分支管道流动中，对于相同的主管道流量，各分支管道中可以有不同的稳定流动状况与之对应．分支管道中的稳定流动状态，不仅取决于主管道中的流量，而且取决于主管道和分支管道中的流量调整变化过程．实验表明：对于具有相同尺寸，相同几何形状的多个分支管道而言，分支管道距主管道入口端的位置顺序越靠前，则通过该分支管道的流量越小．虽然实验中的多分支管道流动是属于非常复杂的湍流，但实验表明主管道的流量与各分支管道的流量之间存在一简单的线性关系．实验还表明，主管道入口的壁面静压与备分支管道出口的壁面静压之间存在抛物线关系．