On the effects of dynamical turbulence on the perpendicular diffusion of low-energy cosmic ray electrons

Diffusion perpendicular to the heliospheric magnetic field plays an integral role in the transport of charged particles in the heliosphere. In this study the perpendicular diffusion coefficient of low-energy cosmic ray electrons is calculated, using an equation derived from the random ballistic decorrelation interpretation of nonlinear guiding centre theory. An observationally motivated 2D turbulence power spectrum is assumed and the effects of various turbulence inputs on the resulting perpendicular diffusion coefficient are investigated. The perpendicular diffusion coefficients are first determined at 1 AU, for both magnetostatic and dynamical turbulence conditions. These solutions are also evaluated for radial distances of 0.1 AU to 10 AU to further investigate the values of the perpendicular diffusion coefficients in the very inner heliosphere. The results of this study show that the dissipation range of the turbulence power spectrum provides a negligible contribution towards the perpendicular diffusion coefficient, and that solutions derived using only the energy containing range serve as good approximations for solutions derived assuming the full 2D turbulence power spectrum. Finally, it is shown that the effects of dynamical turbulence, as considered in the present study, do not affect the perpendicular diffusion coefficients derived from the scattering theory considered here.     

IVIDIL experiment onboard the ISS

The experiment IVIDIL (Influence of Vibrations on Diffusion in Liquids) is scheduled to be performed in forthcoming fall 2009 onboard the ISS, inside the SODI instrument mounted in the Glovebox on the ESA Columbus module. It is planned to carry out 39 experimental runs with each of them lasting 18 h. The objective of the experiment is threefold.     

Relation between different theories for cosmic ray cross field diffusion

In the past few year several theories have been presented for describing cosmic ray scattering across the mean magnetic field. It is the purpose of the present article to discuss the relation between these different theories in order to improve our understanding of cosmic ray perpendicular scattering and to explore the parameter regimes for which these different theories are valid.     

三元乙丙橡胶粘接工艺研究

通过粘接面处理、粘接压力、胶层厚度、胶层涂刷方式等方面对三元乙丙橡胶粘接性能进行了研究。结果表明,铝合金应喷砂后阳极化、三元乙丙橡胶生胶用乙酸乙脂擦拭、熟胶进行表面打磨;采用三次刷涂,胶层厚度控制在0.1～0.15mm;硫化压力5～10MPa是较好的粘接工艺方法。     

Random walk of magnetic field lines: Subdiffusive,diffusive, and superdiffusive regimes

One- and two-dimensional models of magnetic field fluctuations and turbulence are widely used in space-, astrophysical, and laboratory contexts. In the present article we use a generalized form of the turbulence wave spectrum to calculate field line diffusion coefficients analytically and numerically. General conditions are derived for which field line wandering behaves subdiffusively, diffusively, and superdiffusively.     

连接参数对Ti53311S 高温钛合金TLP 连接接头性能的影响

采用Cu作为中间层实现了Ti53311S合金的TLP连接,通过SEM、EDS方法分析了接头界面的微观组织,研究了接头界面微观组织及力学性能随TLP连接温度及保温时间的变化规律。结果表明:TLP连接接头的典型界面结构为Ti53311S/β-Ti/Ti、Cu(Sn)金属间化合物/β-Ti/Ti53311S。随着TLP连接温度的升高或保温时间的增加,焊缝宽度逐渐增加,Cu元素向母材侧的扩散程度更加充分,化合物相分解消失,接头室温抗拉强度先大幅升高后趋于稳定,连接工艺为980℃/20 min时,接头抗拉强度达到最大值899 MPa。     

薄层碳纤维斜纹布层压板二次胶接试验研究

将复合材料薄板二次胶接技术应用在小型无人机机翼主承力结构上，对于降低机翼盒段的制造成本具有重要的工程应用价值。采用碳纤维斜纹布制2 mm 薄板进行单搭接结构拉剪试验，分析3 种不同型号的胶粘剂对该薄板的适配性以及胶层厚度和层压板铺层角度对二次胶接强度的影响，并通过ABAQUS 软件进行模拟验证。结果表明：使用SY-23B 环氧结构胶，胶层厚度为0.2 mm、铺层方式为［（0/90）］8 -［（0/90）］8 的结构件，胶接性能最优，结构剪切强度可以达到18.2 MPa，满足小型无人机受力盒段的胶接强度要求，二次胶接成形的机翼受力盒段具有轻质化、低成本的优点。     

固体发动机试车燃气的扩散及对环境的影响

对地处复杂山区的固体火箭发动机试车站的燃气组成及燃气在大气中的扩散和对环境的影响,采用理论预测、数学模式和监测相结合的方法进行了系统研究,配合进行了同步的气象特征研究.评估了不同大气稳定度下污染浓度的分布,提出了有效的防污染措施.     

高性能铝基复合材料的颗粒分布及界面结合

采用常规粉末冶金和高能球磨粉末冶金法制备了B4Cp/Al复合材料，研究了B4C颗粒分布与界面结合特点、形成机制以及对材料性能的影响。结果表明，17％（体积分数）B4Cp/6061Al复合材料的屈服和抗拉强度分别为415MPa和470MPa，比常规粉末冶金复合材料分别提高了69％和70％。微观分析表明，高能球磨粉末冶金复合材料中B4C颗粒均匀分布、颗粒与基体之间存在近百纳米厚度的界面层，界面层由呈带状且有序分布的微细铝晶粒和弥散分布的纳米颗粒组成。高能球磨过程中，铝粉末在钢球表面形成冷焊层，B4C不断被挤入而均匀化是实现颗粒均匀分布的主要机制；球磨过程中铝粉末表面氧化层破碎暴露出新鲜铝表面且与镶嵌与铝粉末中的B4C颗粒形成界面结合是获得良好界面结合复合材料的重要条件     

中间层厚度对陶瓷扩散焊接头应力分布影响的数值分析

采用有限元计算方法，对平面应变、平面应力两种应力状态下含中间层的陶瓷接头界面上应力分布规律进行数值分析。得到了接头界面上正应力和剪应力沿板定的分布曲线。结果表明，中间层材料厚度小时，两种应力状态下的正应力和剪应力在接头界面上滑板定的分布基本均匀。中间层材料厚度增大，平面应变状态下试件中部的正应力增大并出现峰值；平面应力状态下在试件自由瑞边缘正应力增大并出现峰值。两种应力状态下界面上的剪应力由板中央到板边缘逐渐增大，界面上边缘处最大剪应力的值也随中间层厚度的增加而增大。因此，在保证接头接合良好的前提下，应采用小厚度的中间层。