聚苯乙烯粉末选择性激光烧结成型机理的研究

分析了聚苯乙烯粉末材料选择性激光烧结成型机理,并通过填充改性方法提高其成型性能.结果表明,添加无机填料可提高聚苯乙烯粉末材料烧结性能,而且,多种填料同时添加,效果更明显.     

高校隐性激励与师资队伍稳定问题研究

文章探讨了高校激励形式的分类以及隐性激励在师资队伍稳定方面的重要性，指出了高校建立完善的隐性激励机制的途径。     

先进的变载吸能器

传统的定载吸能器以50百分位男性乘员满足95％生存率为条件设计，它不能为全体乘员提供保护，变载吸能器能够根据乘员重量而调节动作载荷，为全体乘员提供最合理的保护，同时可以大大降低吸能器的冲击行程。     

A Comparative Study of the Influence of the Active Young Sun on the Early Atmospheres of Earth, Venus, and Mars

Because the solar radiation and particle environment plays a major role in all atmospheric processes such as ionization, dissociation, heating of the upper atmospheres, and thermal and non-thermal atmospheric loss processes, the long-time evolution of planetary atmospheres and their water inventories can only be understood within the context of the evolving Sun. We compare the effect of solar induced X-ray and EUV (XUV) heating on the upper atmospheres of Earth, Venus and Mars since the time when the Sun arrived at the Zero-Age-Main-Sequence (ZAMS) about 4.6 Gyr ago. We apply a diffusive-gravitational equilibrium and thermal balance model for studying heating of the early thermospheres by photodissociation and ionization processes, due to exothermic chemical reactions and cooling by IR-radiating molecules like CO₂, NO, OH, etc. Our model simulations result in extended thermospheres for early Earth, Venus and Mars. The exospheric temperatures obtained for all the three planets during this time period lead to diffusion-limited hydrodynamic escape of atomic hydrogen and high Jeans’ escape rates for heavier species like H₂, He, C, N, O, etc. The duration of this blow-off phase for atomic hydrogen depends essentially on the mixing ratios of CO₂, N₂ and H₂O in the atmospheres and could last from ∼100 to several hundred million years. Furthermore, we study the efficiency of various non-thermal atmospheric loss processes on Venus and Mars and investigate the possible protecting effect of the early martian magnetosphere against solar wind induced ion pick up erosion. We find that the early martian magnetic field could decrease the ion-related non-thermal escape rates by a great amount. It is possible that non-magnetized early Mars could have lost its whole atmosphere due to the combined effect of its extended upper atmosphere and a dense solar wind plasma flow of the young Sun during about 200 Myr after the Sun arrived at the ZAMS. Depending on the solar wind parameters, our model simulations for early Venus show that ion pick up by strong solar wind from a non-magnetized planet could erode up to an equivalent amount of ∼250 bar of O⁺ ions during the first several hundred million years. This accumulated loss corresponds to an equivalent mass of ∼1 terrestrial ocean (TO (1 TO ∼1.39×10²⁴ g or expressed as partial pressure, about 265 bar, which corresponds to ∼2900 m average depth)). Finally, we discuss and compare our findings with the results of preceding studies.     

舱门机构运动的计算机模拟

1.构造及其原始数据 滑轨舱门收放机构由中、侧滑轨、三角支架、外伸臂、链条条、链轮、液压马达及减速装置等组成(图1)。一根中滑轨布置在43框前飞机对称平面内与飞机外形的下零纵线相贴合,两根侧滑轨分别布置在43框后机身的两侧,舱门的前端由一个接头铰支在三角支架上,三角支架的前支点与链条相连,舱门的后部和两个外伸臂固接,     

整体叶轮数控展成电解加工的计算机辅助编程

分析了整体叶轮数控展成电解加工的数据处理及编程参数计算方法,用C++语言实现计算机辅助数控编程。     

A NEW EXPRESSION OF FATIGUE SIZE FACTOR

ＡＮＥＷＥＸＰＲＥＳＳＩＯＮＯＦＦＡＴＩＧＵＥＳＩＺＥＦＡＣＴＯＲ￥ＹａｏＷｅｉｘｉｎｇ（ＤｅｐａｒｔｍｅｎｔｏｆＡｉｒｃｒａｆｔＥｎｇｉｎｅｅｒｉｎｇ，ＮＵＡＡ２９ＹｕｄａｏＳｔｒｅｅｔ，Ｎａｎｊｉｎｇ２１００１６，Ｐ．Ｒ．Ｃｈｉｎａ）Ａｂｓｔｒａ...     

关于工业机器人运动学反问题的两种解法

本文发展了求解工业机器人运动学反问题的两种新方法:几何法和迭代法,分别适用于可解和不可解工业机器人的工作空间综合。     

构建现代企业制度下的激励机制

国有企业改革的关键是要构建现代企业制度,而激励机制的陈旧落后将严重制约现代企业活力的发挥。本文结合我国过去计划经济体制下国有企业存在的激励问题,探讨了新时期构建现代企业制度下的激励机制的思路。     

系统群进化环境的模型设计

由于系统群复杂性的增加和有关实践的非成熟性，开发了一个系统化的方法来进行进化活动显得十分必要。本提出了一个系统群进化的综合环境的设计模型，介绍了该环境的设计思想，操作的流程，主要的模块以及如何运用系统构架知识来支持系统的进化，最后给出了该环境设计的高层结构。