SiCP/Al复合材料棱镜组件研磨工艺方法研究

通过对SiCp/Al复合材料棱镜组件研磨工艺试验及其结果分析,总结、优化了研磨工艺参数、研磨砂种类、粒度、研磨时间、研磨工艺过程等参数,研磨出的棱镜组件符合其精度要求,为棱镜组件在平台上的安装精度提供了基础.     

Acceleration at the termination shock: Anisotropies and spectra

Low-energy termination shock particle populations observed by the Voyagers upstream of the shock exhibited strong field-aligned beaming with anisotropies of the order of unity. The Parker transport equation is valid only for nearly isotropic phase space distributions and is inapplicable to these highly beamed populations. The usual approach is to revert to the more general focused transport equation retaining pitch-angle information. We developed a complimentary technique employing a three-moment expansion of the Skilling equation using Legendre polynomials. We investigate the effects of adiabatic focusing and reflection on the diffusive acceleration process at oblique shock waves. It is shown that low-energy particle intensities are discontinuous and sharply peaked at the shock, consistent with the observations. Particle spectra are not only harder than the power laws predicted from diffusive transport theory, but also exhibit spectral gaps near the low-energy acceleration threshold due to more efficient acceleration by scattering and mirroring. Our model also predicts upstream anisotropies as high as 100% for highly oblique shocks whereas downstream distributions are nearly isotropic.     

Solar Energetic Particle Composition, Energy Spectra, and Space Weather

Recent progress in measuring the composition and energy spectra of solar energetic particles (SEPs) accelerated by CME-driven shocks is reviewed, including a comparison of the observed charge-to-mass dependence of breaks in SEP spectra with model predictions. Also discussed is a comparison of SEP and CME kinetic energies in seventeen large SEP events, and estimates of the SEP radiation dose that astronauts would be subject to once they venture outside the protective cover of Earth’s magnetosphere.     

Cosmic Rays at High Heliolatitudes

The Ulysses spacecraft has been the first to orbit the Sun over its poles and to explore the heliosphere at these high heliolatitudes. It has now completed two fast latitude scans, one at solar minimum and one at solar maximum. Since its launch in October 1990, this mission has led to several surprising discoveries concerning energetic particles, cosmic rays, Jovian electrons, the solar wind, the heliospheric magnetic field and the global features of the heliosphere. This review addresses mainly the propagation and modulation of cosmic rays and other charged particles, from both an observational and theoretical point of view, with emphasis on what has been learned from exploring the inner heliosphere to high heliolatitudes. This is done for solar minimum and maximum conditions. The review is concluded with a summary of the main scientific discoveries and insights gained so far from the Ulysses mission.     

On the Differences in Composition between Solar Energetic Particles and Solar Wind

Although the average composition of solar energetic particles (SEPs) and the bulk solar wind are similar in a number of ways, there are key differences which imply that solar wind is not the principal seed population for SEPs accelerated by coronal mass ejection (CME) driven shocks. This paper reviews these composition differences and considers the composition of other possible seed populations, including coronal material, impulsive flare material, and interplanetary CME material.     

减速器内部金属屑运动仿真分析

为掌握因轴承磨损产生的金属屑在直升机中间减速器内部流场中的运动状态，针对其固-液-气三相流特征建立了金属 屑颗粒受力平衡方程和多相流模型-离散相模型（VOF-DPM）耦合的CFD仿真模型。基于离散相运动方程编程计算及采用CFD仿 真分析方法获得了减速器内部颗粒的运动轨迹、运动速度，并据此对比验证了VOF-DPM耦合模型的正确性；利用CFD仿真分析 了颗粒在流体中运动时各种附加力对颗粒运动轨迹的影响，探究连续相空气、滑油与离散相颗粒三者之间的相互作用机理。结果 表明：连续相和离散相耦合作用对颗粒运动的影响较小，轨迹误差约5%、速度误差约3%，可忽略不计；虚质量力、压力梯度力和 Magnus升力对颗粒运动轨迹影响较大，Saffman升力对颗粒运动轨迹影响较小，而热泳力与布朗力不适用于直升机中间减速器固- 液-气三相流情形。     

C/ SiC 材料在国外空间光学系统上的应用

C/SiC复合材料具有高的比强度、低的热变形敏感度以及在高低温环境下的适应性,这使其成为目前最具前途的空间光学系统应用材料.本文总结了国外一些国家C/SiC的制备方法及其在空间技术上的具体应用.     

Erosion degradation characteristics of a linear electro-hydrostatic actuator under a high-frequency turbulent flow field

The paper proposes a performance degradation analysis model based on dynamic erosion wear for a novel Linear Electro-Hydrostatic Actuator (LEHA). Rather than the traditional statistical methods based on degradation data, the method proposed in this paper firstly analyzes the dominant progressive failure mode of the LEHA based on the working principle and working conditions of the LEHA. The Computational Fluid Dynamics (CFD) method, combining the turbulent theory and the micro erosion principle, is used to establish an erosion model of the rectification mechanism. The erosion rates for different port openings, under a time-varying flow field, are obtained. The piecewise linearization method is applied to update the concentration of contaminated particles within the LEHA, in order to gain insight into the erosion degradation process at various stages of degradation. The main contribution of the proposed model is the application of the dynamic concentration of contamination particles in erosion analysis of Electro-Hydraulic Servo Valves (EHSVs), throttle valves, spool valves, and needle valves. The effects of system parameters and working conditions on component wear are analyzed by simulations. The results of the proposed model match the expected degradation process.     

带有SiC涂层的C/C复合材料的氧化行为

采用包埋法在C/C复合材料表面制备了SiC高温防氧化涂层。利用SEM和XRD等方法对涂层的微观形貌和晶相组成进行了观察与分析,并对带涂层试样在室温~1 500℃范围内的氧化行为进行了研究。结果表明,涂层主要由β-SiC和少量的游离Si组成,涂层表面有裂纹存在,涂层与C/C复合材料基体结合良好,呈现犬牙状结合。在室温~1 500℃之间,带SiC涂层C/C复合材料的氧化行为可分为4个阶段,涂层在高温区具有较好的防氧化性能。     

SiB4 微粉在化学气相渗透SiC 过程中的变化

采用SEM、EDS、XRD分析了SiB4微粉化学气相渗透(CVI)SiC后的组成和结构,并用热力学计算研究了SiB4微粉在CVI SiC过程中变化的原因。结果表明:在CVI SiC过程中SiB4微粉不发生分解,但在近表层处氧化生成SiO2和B2O3。用SiB4浆料浸渍结合CVI工艺对C/SiC基体进行自愈合改性时,难以形成均匀致密的基体。