等离子体隐身技术探讨

阐述了等离子体隐身的概念和原理,进而分析了等离子体隐身的关键技术和发展状况。     

基于等离子体激励的圆柱绕流控制实验研究

为验证低雷诺数条件下,采用大气压等离子体流动控制技术进行圆柱绕流控制的有效性,设计了圆柱绕流实验系统,并开展了圆柱绕流实验研究.实验研究表明,在雷诺数为1.35×104和1.90×104的条件下,等离子体激励器产生的流动扰动,能够有效控制圆柱体绕流的流动分离,并显著改善分离流场,增涡、减涡效果明显.实验结果表明,大气压等离子体流动控制技术是钝体绕流流动特性控制的一种有效手段.     

微等离子体转化二氧化碳发射光谱诊断

火星大气层的主要成分为二氧化碳,如果能够利用低温等离子体方法高效分解二氧化碳,使其转化为氧气和一氧化碳加以利用,可以大幅降低航天员生命保障相关载荷长途运输的成本,进一步提高生命保障能力.低温等离子体放电过程中会产生大量活性组分,可以在数百度温度下实现二氧化碳的高效解离,是具有很大潜力的二氧化碳解离与转化方式.设计了一种...     

直流电弧等离子体炬数值模拟与诊断

直流电弧等离子体炬内部物理过程复杂且具动态性,较难对其进行准确描述与深入研究,且其工作温度较高,其状态参数难以使用常规方式测量。针对直流电弧等离子体炬,建立流动、传热和电磁相互耦合的数值模型,基于Fluent软件对直流电弧等离子体炬进行三维数值模拟和特性分析,设计并搭建了一套热焓探针实验系统,完成对直流电弧等离子体炬射流参数的测量分析。结果表明:建立的数值模型模拟结果与实验测量结果吻合较好,误差在10%以内;炬内温度与速度最大值与工作气流量呈正相关,均出现在靠近阴极区域,且沿轴线逐渐降低;等离子体炬内高温区与高电流密度区重合。     

铝合金冷挤压工艺的优化

本文介绍了6A02、6063铝合金冷挤压试验过程。通过专门装置测试铝合金冷挤压中不同凹模表面粗糙度、挤压速度、润滑剂、坯料状态的下的挤压力,利用正交试验L9(34)得出最优工艺参数。结果表明冷挤压过程中模具表面并非越光越有利于成形,坯料也要针对不同的挤压材料应选用不同的热处理方法。本实验为铝合金冷挤压提供了可行的实验方法和生产依据。     

夏热冬冷地区居住建筑节能设计分析

推动建筑向节能、绿色、智能化方向发展,是国际建筑界实践可持续发展理念的大趋势,也是中国经济社会发展面临的重要任务。我国居住建筑节能,从八十年代初起步,从全国总体情况看,节能标准在北方地区推行较早,近一两年来,我省尤其是南昌市的节能标准执行力度正在不断加大。本文通过对冬冷夏热地区一栋宿舍建筑实例进行节能设计分析,得出冬冷夏热地区"宿舍"建筑节能设计外维护结构的一般设计标准。     

Four-peak longitudinal distribution of the equatorial plasma bubbles observed in the topside ionosphere: Possible troposphere tide influence

In this paper we consider an idea of the troposphere tide influence on the character of the longitudinal variations in the distribution of the equatorial plasma bubbles (EPBs) observed in the topside ionosphere. For this purpose, the obtained EPB longitudinal patterns were compared with the thermosphere and ionosphere characteristics having the prominent “wave-like” longitudinal structures with wave number 4, which are uniquely associated with the influence of the troposphere DE3 tides. The characteristics of the equatorial mass density anomaly (EMA), equatorial ionization anomaly (EIA), zonal wind and pre-reversal E?×?B drift enhancement (PRE) were used for comparison. The equinox seasons during high solar activity were under consideration. It was obtained that the longitudinal patterns of the EMA and zonal wind show the surprising similarity with the EPB distributions (R???0.8, R???0.72). On the other hand, the resemblance with the ionosphere characteristics (EIA, PRE) is rather faint (R???0.37, R???0.12). It was shown that the thermosphere zonal winds are the most possible transfer mediator of the troposphere DE3 tide influence. The most successful moment for the transfer of the troposphere DE3 tide energy takes place in the beginning of the EPB production, namely, during the seed perturbation development.     

Local stability analysis of interface region of astrophysical viscous shear flows with a gradual velocity gradient

In this paper, we extend the stability analysis of cold sharp shear flows to warm astrophysical cases with, inevitable, gradual velocity gradient in the interface region in the presence of viscosity effect. Using linear perturbation theory as well as the local approximation method, the instability growth rate of the excited electromagnetic modes has been investigated for the relativistic and non-relativistic cases of solar wind interacting with interstellar plasma medium. Results show that astrophysical shear systems with a small velocity gradient in the transition region are more stable rather than larger ones. Moreover, dependent on the viscosity coefficient value, the viscosity effects could have a positive role on the instability growth rate of the system in some range of initial bulk velocity, while it plays a destructive role in other velocity ranges.     

A Three-Dimensional Simulation of Collisional-Interchange-Instability in the Equatorial-Low-Latitude Ionosphere

We present a three-dimensional simulation of collisional-interchange-instability in the equatorial-low-latitude F region of ionosphere. The instability is responsible for the generation of large plasma density depletion or bubble. General 3D potential and continuity equations are derived to simulate the phenomena. To understand the linear aspect of the instability, the general 3D linear growth rate is derived using 3D potential equation. The linear growth characteristics are compared with earlier field-aligned-integrated growth analyses. The numerical simulation of bubble in the 3D spherical polar geometry is finally presented. Distinct evolution characteristics of bubble in 3D and 2D simulation are further discussed.     

非平衡电弧加热射流光谱学诊断方法：第一部分 氩射流

从一般意义上给出了非平衡电弧加热射流光谱学诊断方法和结果。表明非平衡亚声速电弧加热射流中心是ＬＴＥ的，沿径向形成一非平衡囊兜，囊兜的最深位置约在１／２射流半径处。