自动配平系统驱动电路故障分析与改进

针对某型飞机配平系统故障，对其原因、危害性进行了详细分析．并采取了措施对系统进行设计改进，解决了系统设计缺陷。     

Spectroscopy peculiarities of thermal plasma of electric arc discharge between electrodes with Zn admixtures

Plasma of the free burning electric arc between Ag–SnO₂–ZnO composite electrodes as well as brass electrodes were investigated. The plasma temperature distributions were obtained by Boltzmann plot method involving Cu I, Ag I or Zn I spectral line emissions. The electron density distributions were obtained from the width and from absolute intensity of spectral lines. The laser absorption spectroscopy was used for measurement of copper atom concentration in plasma. Plasma equilibrium composition was calculated using two independent groups of experimental values (temperature and copper atom concentration, temperature and electron density). It was found that plasma of the free burning electric arc between brass electrodes is in local thermodynamical equilibrium. The experimental verification of the spectroscopic data of Zn I spectral lines was carried out.     

SF6分解气的近红外在线检测技术研究

为满足SF6绝缘电气设备故障监测与预警的实际需求,分析了国内分解气检测研究现状.对比近红外与中红外吸收光谱检测技术,提出近红外吸收光谱技术在线检测的技术方案.计算分析待测气体特征谱线的吸收系数、吸收光程和电路信噪比对精度的影响,完成系统参数设计.提出SF6分解气在线检测系统方案,实现对H2S、HF和CO这3种气体测量.数据分析表明,系统检测精度优于5×10-7,表明该系统满足电力行业在线测量的需求.     

俯仰三角翼的流态及结构

本文对俯仰三角翼的流动特性进行了实验研究，给出了俯三角翼的截面流态特点，对三角翼俯仰 运动的流动机理进行了分析。     

UVCS/SOHO Observations of Spectral Line Profiles in Polar Coronal Holes

Ultraviolet emission line profiles have been measured on 15-29 September 1997 for H I 1216 Å, O VI 1032, 1037 Å and Mg X 625 Å in a polar coronal hole, at heliographic heights ? (in solar radii) between 1.34 and 2.0. Observations of H I 1216 Å and the O VI doublet from January 1997 for ? = 1.5 to 3.0 are provided for comparison. Mg X 625 Å is observed to have a narrow component at ? = 1.34 which accounts for only a small fraction of the observed spectral radiance, and a broad component that exists at all observed heights. The widths of O VI broad components are only slightly larger than those for H I at ? = 1.34, but are significantly larger at ? = 1.5 and much larger for ? > 1.75. In contrast, the Mg X values are less than those of H I up to 1.75 and then increase rapidly up to at least ? = 2.0, but never reach the values of O VI.     

Spectroscopic Constraints on Models of Ion-cyclotron Resonance Heating in the Polar Solar Corona

Using empirical velocity distributions derived from UVCS and SUMER ultraviolet spectroscopy, we construct theoretical models of anisotropic ion temperatures in the polar solar corona. The primary energy deposition mechanism we investigate is the dissipation of high frequency (10-10000 Hz) ion-cyclotron resonant Alfvén waves which can heat and accelerate ions differently depending on their charge and mass. We find that it is possible to explain the observed high perpendicular temperatures and strong anisotropies with relatively small amplitudes for the resonant waves. There is suggestive evidence for steepening of the Alfvén wave spectrum between the coronal base and the largest heights observed spectroscopically. Because the ion-cyclotron wave dissipation is rapid, even for minor ions like O⁵⁺, the observed extended heating seems to demand a constantly replenished population of waves over several solar radii. This indicates that the waves are generated gradually throughout the wind rather than propagated up from the base of the corona. This revised version was published online in June 2006 with corrections to the Cover Date.     

导弹大迎角下非线性诱导滚转力矩数值研究简

 采用计算流体力学（CFD）数值模拟方法,研究战术导弹大迎角状态下涡破裂导致滚转力矩随迎角非线性增长引起舵面控制能力不足的现象。首先通过标准模型的数值分析,验证了所采用的CFD方法具有三角翼前缘涡破裂现象的捕捉能力;然后采用雷诺平均Navier-Stokes方程对某“++”字正常布局导弹构型（含弹翼、弹身、尾舵和整流罩等）进行了数值模拟,结果显示亚声速状态下滚转力矩在迎角大于20°时出现非线性增长,导致全动尾舵的滚转控制能力不足。通过分解各部件对滚转力矩的贡献,并分析流场结构,探明了该现象发生的流动机理,其主要原因是：随着迎角的增长,弹体迎风面的尾舵前缘涡首先发生破裂,导致其平衡诱导滚转力矩的作用被削弱。     

激光诱导碳等离子体在强激光冲击合成金刚石微晶中的作用

通过对Ｒａｍａｎ光谱及激光诱发碳等离子体的进一步分析研究，讨论了强激光冲击合成金刚石微晶过程中碳等离子体的作用机制。碳等离子体可视为高活性、高动能碳粒子集团，其对石墨相的作用同时包括能量传输和质量传输两个过程，因此碳等离子体在促进石墨相结构畸变、结构重组乃至相变方面起到了重要的作用；从能量阈值角度分析了碳等离子体与石墨相之间的四种磁撞类型，并据此对Ｒａｍａｎ谱线随激光功率密度的变化规律提出了较为合     

一些大涡内部的轴向流(英文)

用氢气泡法显示了两种大涡，即平板起动涡和细干扰线在圆盘前诱发的大涡的内部流动结构。它们的轴向流，涡核的孤立波，以及向破裂的演变。     

GaInP2外延膜中施主—受主对复合发光带的能量关量

通过变温与变激发强度的近红外光致发光研究了用ＭＯＣＶＤ方法、生长在ＧａＡｓ衬底上的Ｇａ０．５Ｉｎ０．５Ｐ（ＧａＩｎＰ２）外延薄膜的１．１７ｅＶ发射带的发光特性。１．１７ｅＶ发光带性质与０．９９ｅＶ及０．８５ｅＶ发光带的性质有着明显的差别。１．１７ｅＶ发光带的机理可用施主－受主对的复合发光来解释，其中施主－受主对系白处在Ｇａ格位上的Ｓｉ（ＳｉＧａ）及其最邻近的Ｇａ空位（ＶＧａ）所组成，记作ＳｉＧａ－ＶＧａ。考虑到ＧａＩｎＰ２中存在着很强的电子－格子耦合作用及其Ⅲ族子格子为部分有序，所以在施主－受主对复合发光中应计及Ｆｒａｎｃｋ－Ｃｏｎｄｏｎ位移△ＦＣ及该对在等效的部分有序势场中的相互作用能Ｅｓ（ＤＡＰ）。Ｘ—射线衍射实验表明，部分有序结构相当于成分调制，因而可用Ｋｒｏｎｉｇ－Ｐｅｎｎｅｙ模型来计算Ｅｓ（ＤＡＰ）值。这样，我们就导出了施主－受主对复合发光的新的能量表示式。