推力室中压力剧烈振荡区域的燃烧特性分析

在不施加任何扰动的情况下,对液氧/煤油双组元液体火箭发动机模型燃烧室进行三维非稳态数值模拟,获得了其中的压力自激振荡现象。基于定义的能够辨识定容和定压燃烧特征的第三邓克尔数分析了压力剧烈振荡区域的燃烧特性。结果表明,在压力剧烈振荡区域内,第三邓克尔数取值很大,即发生了准定容燃烧或介于定容和定压之间的燃烧过程。可见尽管液体火箭发动机燃烧室整体表现为定压燃烧特性,但在头部附近区域出现了局部具有非定压特性的燃烧过程,其产生的压力膨胀波来不及迅速传播而使当地的压力迅速升高,形成了定容弹效应,从而导致了燃烧不稳定性的发生。该压力峰的传播及其与室壁相互作用在燃烧室中产生声学不稳定性,与研究燃烧不稳定性的定容弹试验机理相同。     

Seasonal variations in vertical distribution of meteor decay time as observed from meteor radars at 8.5°N and 80°N

The decay times of meteor radar echoes have been used for decades to investigate characteristics of the mesosphere and lower thermosphere (MLT) region. As the meteor echo decay time depends on background atmospheric parameters, in the present communication, we examine the seasonal variation of the vertical distributions of underdense meteor echo decay times with respect to echo strength. Observations from two similar radars located at two distinct geographical locations, Thumba (8.5°N, 77°E) and Eureka (80°N, 85.8°W) were used for the present study. Here, the radar received signal power is categorized into strong and weak echoes and vertical profiles of their decay times are constructed. It has been noticed that the monthly mean decay time vertical profile turning altitude (i.e., inflection point) varies in the range of 80–87?km of altitude depending on latitude. The turning altitude is observed at relatively lower heights in the winter than in summer at both the latitudes. The present analysis shows that the meteor decay time below the mean turning altitude follows a decreasing trend with decreasing altitude, which is quite distinct to the behaviour of ambipolar diffusion. It is also observed that there is a difference in mean decay time of strong and weak echoes below 90?km of altitude, which is very prominently seen at lower altitudes. This difference shows a seasonal pattern at high latitude, but does not show any seasonal variation at low latitude. The present results are discussed in light of current understanding of the meteor decay time.     

II型裂纹扩展与绝热剪切带传播的数值对比

通过数值计算的方法,对比绝热剪切带内裂纹扩展和预制II型疲劳裂纹扩展的动态性能参数。分析热塑失稳现象中裂纹的传播与绝热剪切带传播的关系。采用ABAQUS/CAE进行二维模型建立,预制疲劳裂纹和绝热剪切带,分析计算了材料在2种情况的应力应变时间曲线、II型动态应力强度时间历程以及裂纹扩展速度。计算结果表明,预制绝热剪切带与预制疲劳裂纹对于材料的破坏方式影响一致,即裂纹跟随绝热剪切带传播最终导致材料失效。     

About the equilibrium and stability of the magnetopause

This paper offers a model of the magnetopause based on the theory of the contact discontinuity; the boundary layer between the two states of space plasma. The structure of the magnetopause is explored for the effects of polarization, and the profiles of the polarizing electrostatic field are obtained.     

About the equilibrium and stability of non-electroneutral current sheaths

In this paper, we prove the necessity of using the Cauchy problem, i.e., initial value problem, for solving the equilibrium (steady state) current sheet. In this connection, it appears that equilibrium current sheaths exhibit structural instability.     

某型液体火箭发动机燃烧不稳定性鉴定实验研究

采用脉冲枪装置,在液体火箭发动机燃烧室中产生燃烧波,对发动机燃烧过程进行人为激励;通过实验参数测量系统,测量激励前后燃烧室的脉动压力和机械振动频率等参数,分析燃烧室脉动压力的振荡衰减率,进行发动机燃烧不稳定性鉴定实验研究.结果表明:该型液体火箭发动机燃烧过程对脉冲扰动是稳定的.     

边界形状影响等离子体射流扩展特性的实验研究

为了探索燃烧室边界形状在控制燃烧稳定性方面的特性,设计了圆柱型和圆柱渐扩型充液室,运用高速录像系统研究了等离子体射流在充液室中的扩展过程。结果表明：等离子体射流在液体工质中扩展时,等离子体一液体两相流体速度差较大,TaylorHelmh01tz不稳定效应强烈,圆柱型充液室中,Taylor空腔界面自由,界面增长随机脉动性较大;渐扩型充液室能够使两相流边界受到约束,使Taylor空腔沿着充液室边界逐级扩展,从而减弱了Taylor-Helmholtz不稳定效应,有效抑制了界面增长的随机脉动性。放电电压、喷嘴直径和渐扩结构因子△D／L对Taylor空腔扩展过程均有不同程度的影响,通过对这些参数的优化匹配,可以在一定程度上实现对射流扩展过程的控制。     

The structure of Kelvin–Helmholtz vortices with super-sonic flow

We have done two-dimensional simulations of the Kelvin–Helmholtz instability (KHI) with super-sonic flow using the CIP method. The linear analyses of a simple uniform density case show that the KHI cannot grow vigorously when the velocity jump is more than twice the sound speed (when the flow speed relative to the vortex is super-sonic). In this study, by situating a high density contrast across the shear layer, we set the flow in only one of the sides to be super-sonic and then show that the KHI does grow and rolls up a vortex. The formation of a shock is essential for the KHI vigorous growth and the structure of the vortex is strongly influenced by the shock geometry. The results should have substantial implications to velocity shear layer dynamics involving large density jump, such as planetary magnetospheric boundary layers.     

有声腔燃烧室的声学特性实验

为了掌握声腔对燃烧室声学特性的影响规律,采用冷态实验方法,研究了带有轴向直圆孔声腔的模拟燃烧室的声学特性,其中声腔长度、开口面积比（声腔横截面积除以燃烧室横截面积）和个数均可调节.研究结果表明:燃烧室固有频率随声腔长度的增加而逐渐减小;声腔存在最佳深度,能够抑制一阶切向振型,该最佳深度不受声腔开口面积比影响,略小于1/4一阶切向波长;对抑制一阶切向振型而言,声腔存在最佳开口面积比,在本研究中约为0.17;声腔的分布对燃烧室的声学特性影响较大,相同开口面积比下,声腔个数越多,声波衰减越快.