H5飞机调油方法研究

对Ｈ５飞机经过了计算、论证、试飞，在此基础上提出了一种既安全又能充分发挥飞机飞行性能，同时又使动作程序化的调油方法－－规划调油法。用这种调油就可以大大地减少飞行员操纵飞机进的注意力分散，更利于集中精力操纵飞机，以保证飞行的安全。     

滑油量对恒速传动装置的影响

本文介绍了中外航空公司飞机发动机恒速传动装置几个故障典例及造成的危害,分析了填加滑油量不当对发动机恒速传动装置的影响,提出了预防措施。     

Emergence of a Habitable Planet

We address the first several hundred million years of Earth’s history. The Moon-forming impact left Earth enveloped in a hot silicate atmosphere that cooled and condensed over ∼1,000 yrs. As it cooled the Earth degassed its volatiles into the atmosphere. It took another ∼2 Myrs for the magma ocean to freeze at the surface. The cooling rate was determined by atmospheric thermal blanketing. Tidal heating by the new Moon was a major energy source to the magma ocean. After the mantle solidified geothermal heat became climatologically insignificant, which allowed the steam atmosphere to condense, and left behind a ∼100 bar, ∼500 K CO₂ atmosphere. Thereafter cooling was governed by how quickly CO₂ was removed from the atmosphere. If subduction were efficient this could have taken as little as 10 million years. In this case the faint young Sun suggests that a lifeless Earth should have been cold and its oceans white with ice. But if carbonate subduction were inefficient the CO₂ would have mostly stayed in the atmosphere, which would have kept the surface near ∼500 K for many tens of millions of years. Hydrous minerals are harder to subduct than carbonates and there is a good chance that the Hadean mantle was dry. Hadean heat flow was locally high enough to ensure that any ice cover would have been thin (<5 m) in places. Moreover hundreds or thousands of asteroid impacts would have been big enough to melt the ice triggering brief impact summers. We suggest that plate tectonics as it works now was inadequate to handle typical Hadean heat flows of 0.2–0.5 W/m². In its place we hypothesize a convecting mantle capped by a ∼100 km deep basaltic mush that was relatively permeable to heat flow. Recycling and distillation of hydrous basalts produced granitic rocks very early, which is consistent with preserved >4 Ga detrital zircons. If carbonates in oceanic crust subducted as quickly as they formed, Earth could have been habitable as early as 10–20 Myrs after the Moon-forming impact.     

基于因子模糊化BP神经网络的磨损颗粒识别

在引入了一套磨粒形态学描述子来提取磨损颗粒的显微形态特征的基础上 ,采用人工神经网络技术 ,编制了用于磨损颗粒自动识别的 BP网络计算机模拟程序。在网络训练的过程中应用了本文引入的因子模糊化训练方法 ,使训练速度大大加快 ,以异或问题为例 ,速度可提高 5～ 1 0倍。应用此网络对磨粒测试库进行识别实验 ,识别正确率在 90 %以上 ,并且识别速度很快 ,大大优于传统的磨粒识别方法。     

地中式混凝土油罐的数值模拟

对正在开展的战略石油储备,提出用地中预应力混凝土罐进行石油储存.应用结构分析软件ANSYS对巨型混凝土单壁罐和双壁罐进行弹性分析,指出罐壁环向应力几乎全部由温度荷载造成,罐壁温度场和温度应力具有明显时间性,储油初期罐壁温差最大,96?h后罐壁顶部拉应力达到最大;设置中间保温层后,内罐应力减小,外罐应力增大,应对内、外罐连接支墩做特殊设计,以满足罐壁温度变形.     

对流层特大暴雨天气对电离层变化的影响

研究气象活动对电离层变化的影响．利用时序叠加方法，通过对1958-1998年期间发生在武汉的5次特大暴雨天气事件对武汉上空电离层变化的影响进行分析，发现：(1)特大暴雨能够引起低电离层，fbEs和，f0Es参量较明显地减小；(2)特大暴雨对电离层F区寻常波描迹的最低虚高h′F和电离层等效峰高hpF的参量也有一定影响，且随着雨量的增大这种影响作用也会增加；(3)特大暴雨对电离层其他参量影响甚弱或没有影响．本文认为，特大暴雨天气事件对电离层的影响主要来自于动力过程，特别是特大暴雨激发的或相伴的大气重力波、潮汐波和行星波等长周期大尺度过程的作用．     

非线性油膜支承裂纹转子振动特性分析

 以具有无限长轴承和无限短轴承支承的横向裂纹转子为研究对象,分析在非线性油膜力与横向裂纹联合作用时,Jeffcott转子的动力特性,并将其与刚性支承情况进行比较。结果表明轴承油膜力的存在对裂纹转子的振动影响较大,一般将降低转子的振动,这样势必增加转子裂纹故障诊断的难度。所以,在进行裂纹转子的故障诊断时,必须考虑到支承条件的影响,建立合理的动力学模型。     

某重型燃气轮机放气活门及排气管路的改进设计

针对某重型燃气轮机放气系统放气活门在结构设计上存在的问题,经过分析和论证,提出了改进方案,通过计算验证了该方案可以实施。     

冷轧机补偿原理及其控制算法

液压压下控制系统是冷连轧机控制系统中十分重要的组成部分,它主要实现机架辊缝大小的控制,对于轧制板材的板形有着直接的影响.在轧制过程中,由于轧辊偏心(包括工作辊和支撑辊)、油膜厚度的波动、轧机的弹跳等因素.为了解决这些问题,对于液压压下控制系统中存在的偏心补偿、油膜补偿和弹跳补偿进行了深入的理论分析,研究了冷连轧机液压压下控制系统中偏心补偿、油膜补偿、弹跳补偿的数学模型、实现过程,并与国内外相关理论进行了对比,阐述了各自的优缺点.     

论石油企业QHSE管理体系的建立

根据我国石油企业的实际 ,探讨了石油企业建立QHSE管理体系的方法与措施。