聚焦脉冲激光大气传输热晕效应的数值分析

利用激光大气传输四维程序对序列脉冲激光大气传输热晕效应进行了数值计算和分析。对于均匀大气路径上聚焦传输序列脉冲激光进行数值仿真计算得到,风场渡越时间内的脉冲数Np在2~6之间有利于传输;然后对实际大气模式下序列脉冲激光进行了数值计算,得到的平均脉冲数-NP可以在一定条件下对序列脉冲激光进行定量表征的结论。     

爆震管内爆燃到爆震转捩过程的实验研究

基于常温常压轴向进气条件下气动阀式两相爆震发动机模型开展爆燃到爆震转捩过程的研究，利用离子探针和高频压力传感器测量了管内火焰传播速度和燃烧压力波。研究结果表明，管内爆震波形成的初始位置在正常火焰面下游的一定位置处，如假设爆震管内波和火焰面是一维的，则在爆震波产生的最初一段时间内，爆震管内将出现三道火焰面：往出口方向传播的正常火焰面和爆震波火焰面及往进口方向传播的回传爆震波火焰面。     

考虑燃料雾化的气液两相连续旋转爆轰数值模拟

为研究气液两相连续旋转爆轰发动机燃烧室内爆轰波的传播特性,以汽油为燃料,富氧空气为氧化剂,建立了欧拉-拉格朗日模型进行二维数值仿真,其中气相方程采用时空守恒元与求解元方法求解,液相方程采用标准四阶龙格库塔法求解。在两相旋转爆轰模型还考虑了液滴雾化破碎过程。计算结果表明：起爆后形成的初始爆轰波经过初始燃料填充区域后逐渐衰减,随后入口附近新生成的压力波经过一系列发展形成了自持稳定传播的旋转爆轰波;旋转爆轰波的传播模态受燃料与氧化剂的喷注压力和氧化剂填充比影响,在不同工况下旋转爆轰波呈现出4种传播模态,即稳定单波模态、稳定双波模态、不稳定双波模态和不稳定单波模态;在双波模态工况下,燃烧室内初始只形成1个爆轰波,后由入口附近局部爆炸产生的压力波发展为新的爆轰波,转化为双波模态后爆轰波的强度略有下降,但燃烧室整体推力更加平稳。     

大气准两年振荡对赤道行星波上传的影响

本文讨论了热带大气行星波在QBO风场中向上传播的规律,并运用数值模拟的方法,得到了开尔文波和混合罗斯贝重力波在QBO不同相位下交替上传的结果。试图用QBO对行星波的调制解释QBO在日地相关性中的作用.      

Modelling and observing Jovian electron propagation times in the inner heliosphere

The propagation of Jovian electrons in interplanetary space was modelled by solving the relevant transport equation numerically through the use of stochastic differential equations. This approach allows us to calculate, for the first time, the propagation time of Jovian electrons from the Jovian magnetosphere to Earth. Using observed quiet-time increases of electron intensities at Earth, we also derive values for this quantity. Comparing the modelled and observed propagation times we can gauge the magnitude of the transport parameters sufficiently to place a limit on the 6 MeV Jovian electron flux reaching Earth. We also investigate how the modelled propagation time, and corresponding Jovian electron flux, varies with the well-known ∼13 month periodicity in the magnetic connectivity of Earth and Jupiter. The results show that the Jovian electron intensity varies by a factor of ∼10 during this cycle of magnetic connectivity.     

水凝物对THz波辐射的衰减研究

文章基于水凝物粒子尺寸与THz波长的大小关系,分别利用Rayleigh近似、Mie理论以及几何光学方法计算了降雨和云雾引起THz波辐射的散射衰减。比较了不同强度的降雨和不同能见度、含水量的云雾对THz波的散射衰减。结果表明,随着频率的增大,THz波段雨衰减先增大后减小;在整个THz波段,含水量较小或能见度较低的云雾的衰减随频率的增大而单调增加,含水量较大或能见度较大的云雾的衰减随频率先增大后减小;在THz波段云雾衰减随能见度的减小和含水量的增加而增大,温度对THz波段的云雾衰减影响不大,在整个THz波段并不存在明显的规律。在THz波频率高端云雾影响较降雨要严重的多。     

速度脉动下分层旋流火焰动态传播结构提取

为了深刻理解分层旋流火焰的动态结构,开展了分层旋流火焰动态的模态分析和参数化研究.实验在BASIS(北京航空航天大学发展的具有台阶隔离段的独立分层旋流燃烧器)上开展,以甲烷为燃料预混燃烧,使用高速摄像捕捉了速度脉动下的CH*化学发光信号动态图像.利用传统的本征正交分解(POD)和重定向POD分析了火焰动态特性,并利用重...     

Propagation of interplanetary shocks into the Earth’s magnetosphere

This paper is devoted to the study of propagation of disturbances caused by interplanetary shocks (IPS) through the Earth’s magnetosphere. Using simultaneous observations of various fast forward shocks by different satellites in the solar wind, magnetosheath and magnetosphere from 1995 till 2002, we traced the interplanetary shocks into the Earth’s magnetosphere, we calculated the velocity of their propagation into the Earth’s magnetosphere and analyzed fronts of the disturbances. From the onset of disturbances at different satellites in the magnetosphere we obtained speed values ranging from 500 to 1300 km/s in the direction along the IP shock normal, that is in a general agreement with results of previous numerical MHD simulations. The paper discusses in detail a sequence of two events on November 9th, 2002. For the two cases we estimated the propagation speed of the IP shock caused disturbance between the dayside and nightside magnetosphere to be 590 km/s and 714–741 km/s, respectively. We partially attributed this increase to higher Alfven speed in the outer magnetosphere due to the compression of the magnetosphere as a consequence of the first event, and partially to the faster and stronger driving interplanetary shock. High-time resolution GOES magnetic field data revealed a complex structure of the compressional wave fronts at the dayside geosynchronous orbit during these events, with initial very steep parts (10 s). We discuss a few possible mechanisms of such steep front formation in the paper.     

一种适用于地球空间传感器网络的TCP Vegas模型

针对地球空间传感器网络中由正反向链路带宽不对称引起的正向链路吞吐量下降问题,提出一种基于时延且能够维持反向链路确认频率的拥塞控制模型。该模型基于反向链路中确认分组的排队时延,在反向链路发生拥塞时,降低确认分组的发送频率,以缓解反向链路的拥塞程度;而在反向链路没有发生拥塞时,加快确认分组的发送频率,以提高正向链路中数据分组的吞吐量。同时,该模型将确认分组的延迟发送时间追加到最小往返时延中,提高了最小往返时延的准确程度,从而提升模型的正向链路拥塞控制效果。仿真试验结果表明,该模型可以有效地解决由于反向链路拥塞所造成的正向链路吞吐量低的问题。     

陕西秦汉时期道路交通发展与文化传播

秦汉 (西汉 )时期的陕西咸阳、长安地区是中国政治、经济、交通和文化的中心 ,这里地处中原腹地 ,从秦修驰 (直 )道到汉通西域 ,道路交通无不是以陕西为中心向四周辐射的 ,成为西北西南边陲的连接地带和东西交通的枢纽。这种得天独厚、地造天成的道路交通条件 ,无不影响着文化的融合、统一和传播。