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.     

导弹发射车主机发电时带外供电的方法

对某型导弹发射车主机发电的供电体制进行了简要分析 ,提出了增加外供电体制的措施和方法。外供电方案的实施 ,不仅为部队的平时训练提供了方便 ,而且为提高导弹发射车的可靠性和生存力提供了必要条件 ,增强了整个武器系统的战斗力。     

空间智能桁架自适应模糊振动控制

研究了一种基于自适应模糊控制器的空间智能桁架振动控制方法。在考虑剩余模态影响的条件下建立了空间智能桁架的独立模态空间振动控制方程,并对自适应模糊控制器作改进,证明了控制系统的稳定性。仿真结果表明:该自适应模糊控制器可有效抑制桁架振动,控制效果明显优于传统模糊控制,同时能抑制控制溢出和观测溢出。     

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．     

桁架结构尺寸和形状协同优化方法研究

在满足特定规范和约束条件下,设计出重量最轻的结构具有重要的工程意义。提出一种桁架结构形状、尺寸并行协同优化方法,该方法将桁架结构优化问题拆分为形状优化和尺寸优化两个子问题,通过并行协调实现尺寸设计变量和形状设计变量同时达到最优解;完成了三个典型桁架结构形状优化算例,结果表明：该方法对于桁架结构形状优化可行,且算法简洁,收敛快。     

重型货物空投系统过程仿真及特性分析

建立了货物空投系统仿真计算模型,包括货台在舱内和舱外全过程的运动特性、降落伞拉直和充气过程的轨迹特性计算等,提出了伞群模拟和多吊带系统分析的新方法。结合目前已有的降落伞性能计算模型和物伞系统运动模型,对重型货物空投全过程进行了完整计算,开发了空投过程三维动画仿真软件,通过与试验数据的对比,表明本模型能很好地满足应用的需要。分析了空投速度、伞包安装位置和牵引比等因素对空投过程的影响,指出了实际系统的改进方向。     

激波风洞重模型气动力试验研究

在激波风洞上进行气动力试验时,风洞启动时巨大的冲击载荷使模型-天平受到充分的激励,从而形成惯性干扰力,并与真实气动力混杂在一起,甚至完全覆盖气动力,降低了试验精准度,使得试验模型的质量受到极大的限制。本文介绍了CARDC-dia.2米激波风洞进行大、重模型的压电天平气动力试验研究情况,包括天平设计、天平校准、惯性补偿和风洞试验等几个方面。研究结果表明:气动力试验模型质量可从过去的500g增加到8kg,模型长度可达1m。从而提高了激波风洞测力试验能力,能满足高超声速飞行器试验的需求。     

脉冲爆震火箭发动机引射模态的起爆实验研究

为实现脉冲爆震火箭发动机(PDRE)引射模态下主爆震室的起爆,采用航空煤油和氧气作为推进剂,设计了PDRE引射模态的模型机,采用压电传感器测量主爆震室中爆震波的压力和速度.在主爆震室中成功实现了5 ～8Hz稳定连续的爆震,爆震波的峰值压力能够达到3MPa,爆震波以1600～ 2000m/s左右的速度在主爆震室中传播.实验结果表明:PDRE引射模态下主爆震室的DDT距离,远低于常规高能电喷起爆下的两相PDRE的DDT距离;高频PDRE引射模态下主爆震室的起爆难度加大;加长主爆震室、末端增加收敛段可以提高引射模态的爆震性能.     

某型民用运输机主起落架连接区结构静力试验

飞机静力试验是飞机试验的重要内容之一,是验证飞机结构强度和静力分析正确性的重要手段。为验证某型民用运输机主起落架连接区结构满足静强度要求,以及有限元计算分析的正确性,在静力试验飞机上进行了主起落架连接区结构静力试验。通过全机有限元模型和细节有限元模型分析计算,进行加载、应力\应变、位移试验数据与有限元计算值的分析对比,计算值与试验数据符合较好。     

基于现代教育技术的专业建设

概述了现代教育技术对教学各环节的作用、专业建设中主要要素 ,论述基于现代教育技术的专业建设中应考虑的要素 ,提出专业建设必须立足于现代教育技术的运用。