航空发动机滑油系统断油时主推力球轴承的瞬态热分析

对在航空发动机滑油系统断油时的主推力球轴承瞬态热进行了分析。在分析基础上,应用弹流润滑理论给出了主推力球轴承产生损伤的条件,确定了中断供油时主推力球轴承的允许极限温升,或允许中断供油时主推力球轴承安全工作的极限时间,从而给出了主推力球轴承中断供油30S的安全余度。计算及其结果可为发动机整机试车及润滑系统设计提供参考。     

论科学技术是第一生产力与教育的关系

本文以马克思主义政活经济学原理为基础,以“科学技术是生产力”为基本出发点,论证了“科学技术是第一生产力”这一论断的正确性。同时,笔者从马克思教育思想出发,对教育与劳动力再生产以及教育与科学技术再生产之间的关系进行了详尽的论述,并论证了科学技术对教育的反作用。     

SOHO contribution to the understanding of mass supply and flows in the solar corona

We expect a variety of dynamic phenomena in the quiescent non-flaring corona. Plasma flows, such as siphon flows or convective flows of chromospheric material evaporating into the corona, are expected whenever a pressure differences is established either between the footpoints or between the coronal and chromospheric segments of a coronal loop. Such flows can induce phenomena of spatial and temporal brightness variability of the corona. In particular, evaporation induces a net mass input into the corona and consequently coronal density enhancements. Flows are also expected in the regions where energy is released during magnetic reconnection. From the observational point of view the dynamics of the solar atmosphere has been investigated in great detail mostly in the lower transition region with the HRTS, and during flares with theSolar Maximum Mission andYohkoh. The high spectral, temporal and spatial resolution of theSOHO ultraviolet spectrometers should enable us in the near future to fill the gap providing a continuous coverage from the chromosphere to the corona, in the 10⁴–10⁶ K domain, and therefore to best study the dynamics throughout the solar atmosphere.     

随机载荷作用下构件疲劳可靠性分析方法

 本文建立了用于随机载荷作用下构件疲劳可靠性分析的二维应力强度干涉模型。当影响疲劳强度的诸因素为随机变量时,给出了在二维应力强度干涉模型中考虑这些因素的方法,并用蒙特卡罗(MonteCarlo)方法求解了该模型。最后将上述模型应用于工程实际。     

一个非线性拟协调退化壳有限元

 根据非线性协调有限元列式方法,构造了几何非线性拟协调9结点四边形退化壳有限元。首先给出9结点四边形退化壳单元的几何描述和位移模式;接着讨论了非线性协调有限元列式方法;假设应力和应变;然后用所构造的壳单元,进行了方板、圆拱、球壳和圆柱壳的数值分析,并同精确解以及其他单元的解答进行了比较。结果表明本文壳单元是准确的和有效的。     

The Cold-Dense Plasma Sheet: A Geotail Perspective

GEOTAIL observations of the low-latitude boundary layer (LLBL) in the tail-flanks show that they are the region where the cold-dense plasma appears with stagnant flow signatures accompanied by bi-directional thermal electrons (< 300 eV). It is concluded from these facts that the tail-LLBL is the site of capturing the cold-dense plasma of the magnetosheath origin on to the closed field lines of the magnetosphere. There are also cases that strongly suggest that the cold-dense plasma entry from the flanks can be significant to fill a substantial part of the magnetotail. In such cases, the cold-dense plasma is not spatially restricted to a layer attached to the magnetopause (that is, the LLBL), but continues to well inside the magnetotail, constituting the cold-dense plasma sheet. Inspired by the fact that these remarkable cases are found for northward interplanetary magnetic field (IMF), a statistical study on the status of the near-Earth plasma sheet is made. The results show that the plasma sheet becomes significantly colder and denser when the northward IMF continues than during southward IMF periods, and that the cold-dense status appears most prominently near the dawn and dusk flanks. These are consistent with the idea that, during northward IMF periods, the supply of cold-dense ions to the near-Earth tail from the flanks dominates over the hot-tenuous ions transported from the distant tail.     

根据损伤理论计算树脂材料的断裂性能

基于损伤理论,计及裂尖前方空穴和微裂纹等缺陷的影响,利用材料在性能实验中变形过程的损伤变化与含裂纹材料在裂纹扩展过程中的损伤变化的相似性,得到用材料的性能曲线计算材料断裂韧性的方法,并将计算结果与实验结果相比较,结论较为吻合。所提出的用材料的性能曲线直接计算其断裂韧性的方法有可能推广于其他高分子材料。     

立足民航,培养跨世纪高层次人才：——民航学院研究生教育初探

从社会需求、民航需求、民航学院自身的需求出发,分层次论述了培养跨世纪人才的重要意义。通过分析民航科技发展的特点,指出了民航跨世纪高层次人才应具备的素质。最后,根据学院的实际情况,着重从学科建设、课程设置、导师队伍建设、管理等方面提出了培养民航跨世纪高层次人才的几点思考。     

飞船返回舱俯仰振荡的动态稳定性研究

本文研究了以平衡攻角为中心作单自由度俯仰振荡的飞船返回舱 ,其动态稳定形态随来流M∞ 的变化。设θ(t)是由平衡攻角起算的俯仰振荡角 ,Cm 是作用在飞船返回舱上的气动俯仰力矩系数 ,Cμ(θ, θ)· θ是机械阻尼力矩 (自由飞行时为零 ,实验时要计入其影响 ) ,文中给出飞船返回舱在平衡攻角处的俯仰振荡动态稳定性判据 ,并证明λ =λ(M∞) = Cm θ0+Cμ(0 ,0 ) 1 - Cm ¨θ0 是决定动稳定形态的重要参数。如果随M∞ 的变化 ,λ(M∞)由λ<0经过λ =0变化到λ>0 ,则飞船返回舱将由稳定的点吸引子形态 (即稳定在平衡攻角状态 )演化为周期吸引子形态 (即作周期振荡 )。对应于λ(M∞) =0的马赫数就是飞船返回舱的俯仰运动出现Hopf分叉的临界马赫数Mcr 。本文首先分析了飞船返回舱所受动态气动俯仰力矩的依赖状态变量 ,然后应用非线性动力学理论对飞船返回舱的俯仰运动进行了定性理论分析 ;最后耦合求解俯仰振荡方程和非定常Navier Stokes方程 ,数值模拟了飞船返回舱俯仰振荡随来流马赫数变化的Hopf分叉过程 ,验证了分析结论     

单旋翼式直升机气动布局的几个问题

通过对某型号直升机气动布局设计，介绍了在直升机总体设计中选择直升机气动外形，平尾和尾桨的参数及益的一些基本方法。文中还介绍了对应的风洞试验结果，并将其与理论计算结果进行对比。实例应用证明，该方法是十分有效的。