化学液相热梯度致密C/C技术探索

简要分析了化学液相热梯度致密C／C的沉积过程及机理，该工艺用一种液态碳源作基体前驱体，采用梯度加热法，可实现快速致密。结果表明，与传统化学气相致密法相比，该技术能在很短时间（2.5h）内能迅速提高基质材料的密度。     

复合材料壳体固体发动机药柱工作内压三维结构分析

对复合材料壳体的固体发动机药柱在工作内压作用下的变形和三维应力、应变进行了计算。复合材料壳体简化为正交各向异性结构，确定其弹性材料常数和材料的主轴方向，壳体变形计算和多次水压测试结果基本一致，在此基础上进行了药柱的三维应力、应变分析，为药柱完整性分析提供了参考。     

Three-dimensional global simulation of multiple ICMEs’ interaction and propagation from the Sun to the heliosphere following the 25–28 October 2003 solar events

This study performs simulations of interplanetary coronal mass ejection (ICME) propagation in a realistic three-dimensional (3D) solar wind structure from the Sun to the Earth by using the newly developed hybrid code, HAFv.2+3DMHD. This model combines two simulation codes, Hakamada–Akasofu–Fry code version 2 (HAFv.2) and a fully 3D, time-dependent MHD simulation code. The solar wind structure is simulated out to 0.08 AU (18 Rs) from source surface maps using the HAFv.2 code. The outputs at 0.08 AU are then used to provide inputs for the lower boundary, at that location, of the 3D MHD code to calculate solar wind and its evolution to 1 AU and beyond. A dynamic disturbance, mimicking a particular flare’s energy output, is delivered to this non-uniform structure to model the evolution and interplanetary propagation of ICMEs (including their shocks). We then show the interaction between two ICMEs and the dynamic process during the overtaking of one shock by the other. The results show that both CMEs and heliosphere current sheet/plasma sheet were deformed by interacting with each other.     

建国以来职业教育价值观演变研究

职业教育价值观是职业教育的基本问题,是职业教育发展规律的反映。新中国成立以来,我国的职业教育大力发展,职业教育价值观经历了政治价值,经济价值、人本价值的发展过程。     

环簇式塞式喷管中立体激波的拓扑结构

采用仅显示环簇式塞式喷管单元间干涉激波区域网格点作为可视化方法对数值模拟结果进行后处理,得到了直观的三维干涉激波图像,并归纳得到三种干涉激波的拓扑结构和一种脊状能量泄漏区.结合文献中的实验数据分析了三种拓扑结构所造成的干涉损失,为设计提供参考.      

复合材料z-pinning技术的应用与发展

简单介绍了z-pin的种类和复合材料z-pin的拉挤工艺.重点综述了利用热压罐和UAZ~R 两种z-pinning技术及z-pinning在复合材料层板、结构件连接及泡沫夹层复合材料中的应用,同时,提出了当前发展z-pinning技术的对策和建议.     

舱外航天服热试验方法研究

舱外航天服采用主被动相结合的热控方式控制内部的温度,但其外形复杂,影响外热流的因素很多,因此舱外航天服热试验存在着与传统航天器热试验完全不同的特点。文章根据舱外航天服热设计的特点,对舱外航天服的地面热试验方法进行了比较分析和研究,论证了采用等效外热流模拟方法,通过进行舱外航天服系统漏热和散热能力的测试来验证热设计方法的合理性及热试验方法的可行性。     

气-粒两相流对燃气舵工作性能的影响

为了研究气-粒两相流对固体火箭发动机燃气舵的影响,基于固体火箭发动机燃气舵的工作特点,在求解二维Navier-Stokes(N-S)方程的基础上,分别对有无颗粒相的流场进行了数值模拟,并且考虑了颗粒直径为1,10μm和30μm,颗粒质量分数为15%,20%和30%,舵偏角为0°,5°,10°及15°的各种组合工况.结果表明,在相同外界条件下,有颗粒相时舵表面的压力要大于无颗粒相时的表面压力,而且这种差别在迎风面和舵片前半部分表现得比较明显;在气动性能方面,有颗粒相时升力和阻力都要比无颗粒相时大,这种差别随颗粒直径的增大而减小,在一定颗粒质量分数范围内,随颗粒质量分数的增加而增大.      

Towards a unified theory of discrete auroras

Recent theoretical developments in auroral research are reviewed. In spite of the great complexity involved, a unified theory begins to emerge. The framework of this unified theory is provided by the imperfect magnetosphere-ionosphere coupling due to enhanced magnetospheric convection. The auroral potential structures in the imperfect coupling state result from the loss cone constriction on enhanced upward field-aligned currents following enhanced magnetospheric convections. Field-aligned potential drops for the inverted V precipitations are supported by a combination of the double layer process, the pitch-angle anisotropy process, the wave-particle interaction (anomalous resistivity) process, the electrostatic shock and the thermoelectric process in descending order of importance. Quasineutrality along inverted V field lines is maintained primarily by the trapped and back-scattered electrons produced respectively by wave-particle interactions in the magnetosphere and electron-neutral collisions in the ionosphere. Additional electron energization due to the ion cyclotron turbulence may lead to striations along the inverted V field lines to produce thin auroral arcs imbedded in the inverted V precipitation. The formation of discrete auroras can now be understood as a manifestation of the imperfect magnetosphere-ionosphere coupling due to enhanced magnetosphere-ionosphere interaction.     

椭圆型条件矩封闭模型在湍流扩散火焰中的应用

使用考虑分子扩散与湍流扩散的椭圆型CMC模型对钝体绕流扩散火焰进行了数值模拟计算,计算的工况包括CH₄/H₂、CO/H₂和CH₃OH等燃料在空气中的燃烧。在数值计算中使用了k-ε双方程湍流模型和SIMPLE算法,并将计算结果与实验数据进行了对比,讨论了计算结果与实验数据之间偏差产生的原因,还分析了条件平均变量的空间变化。结果表明,条件平均温度、OH、CO和NO等组分的质量分数的计算结果与实验数据有着很好的一致性,说明椭圆型CMC模型是一种能有效地预测湍流非预混火焰中组分浓度和温度的计算方法。