The Cool Interstellar Medium

Infrared spectroscopy and photometry with ISO covering most of the emission range of the interstellar medium has led to important progress in the understanding of the physics and chemistry of the gas, the nature and evolution of the dust grains and also the coupling between the gas and the grains. We review here the ISO results on the cool and low-excitation regions of the interstellar medium, where T _gas≲ 500 K, n _H∼ 100–10⁵ cm⁻³ and the electron density is a few 10⁻⁴. JEL codes: D24, L60, 047 Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA.     

内反射红外光谱在污染物成分测试中的应用

介绍了内反射光谱的原理及其在放气沉积污染物成分测试中的应用。     

Use of Optical Characteristics to Identify Orbiting Material

Knowledge of the observable properties of orbital debris is necessary to validate debris models for both the low Earth orbit (LEO) and the geosynchronous Earth orbit (GEO). Current methods determine the size and mass of orbital debris based on knowledge or assumption of the material type of the piece. Improvement in the knowledge of material is the goal of the research described herein. The process of using spectral absorption features to determine the material type is explored. A review of the optical measurements of orbital debris as well as current research in the area is discussed. Reflectances of common spacecraft materials are compared. The need for, and advances made possible by obtaining real data are explored. The prospects of the venture are investigated.     

钢与胶粘剂粘接界面的XPS分析

结合氩离子枪刻蚀技术，用X射线电子能谱(XPS)对钢与胶粘剂粘接的界面进行研究，分析了粘接过程中元素的化学环境变化，并对粘接机理进行了探讨。结果表明，胶粘剂中酚醛树脂在界面区域与钢之间存在化学结合，而氯化橡胶与钢之间以范德华力粘接。     

Tomography system for measurement of gas properties in combustion flow field

This paper describes a self-designed fiber-coupled tomography system and its application in combustion diagnostics. The tomographic technique, which combines tunable diode laser spectroscopy and algebraic reconstruction technique, enables the simultaneous reconstruction of temperature and gas concentration with both spatial and temporal resolutions. The system measures a maximum diameter of 35 cm in a circular area with a minimum spatial resolution of 1 mm×1 mm and temporal response of up to 1 kHz. Simulations validate the effects of the beam arrangement and discrete grid on reconstruction accuracy, and give the optimal beam arrangements. Experiments are made to demonstrate the tomography method, and systems are constructed in laboratory and on engineering test benches.     

高超声速流的电子束诊断法(英文)

本文描述用电子束辉光法测量高超声速流中平均密度、速度以及密度变化特征的物理原理和过程。对此法用于平板上激波层稳定性问题的适用范围和限制条件作了分析。内容通过风洞实验结果加以说明。     

航空装备综合诊断的现状与发展设想

综合诊断是伴随着装备的发展和对装备保障能力的要求不断提高而产生和发展的,为此将国外航空装备综合诊断技术的发展历程以及各综合诊断系统的具体组成进行了对比,阐述了当前我国航空装备故障诊断的情况,分析了综合诊断的支撑技术和发展趋势,提出在我国航空装备的维修保障中实施综合诊断的必要性,并对我国建立面向多机型、多专业、以网络为中...     

角分辨紫外光电子谱仪校正因子的测量和计算

测量并分析计算了角分辨紫外光电子谱仪的电子能量分析器的聚焦特性 ,分析计算了紫外光斜入射时光电信号的校正因子。结果表明 :偏离分析器聚焦中心 β角的光电子被分析器接收的几率为高斯函数exp( - β2 /β0 2 ) ,且 β0 =3.5° ;斜入射光电信号的校正因子是光入射角α的函数且大于cosα     

UVCS/SOHO Observations of H I Lyman Alpha Line Profiles in Coronal Holes at Heliocentric Heights Above 3.0 R⊙

The Ultraviolet Coronagraph Spectrometer (UVCS) on the Solar and Heliospheric Observatory (SOHO) has been used to measure spectral line profiles for H I Lyα in the south polar coronal hole at projected heliocentric heights from 3.5 to 6.0 R_⊙ during 1998 January 5–11. Observations from 1.5 to 2.5 R_⊙ were made for comparison. The H I Lyα profile is the only one observable with UVCS above 3.5 R_⊙ in coronal holes. Within this region the outflowing coronal plasma becomes nearly collisionless and the ionization balance is believed to become frozen. In this paper, the 1/e half widths of the coronal velocity distributions are provided for the observed heights. The velocity distributions include all motions contributing to the velocities along the line of sight (LOS). The observations have been corrected for instrumental effects and interplanetary H I Lyα. The half widths were found to increase with projected heliographic height from 1.5 to 2.5 R_⊙ and decrease with height from 3.5 to 5 R_⊙. This revised version was published online in June 2006 with corrections to the Cover Date.     

显微拉曼光谱在物品鉴别上的应用

根据拉曼散射的基本原理 ,利用拉曼光谱仪 ,可以对物质进行简单而科学的分析。显微拉曼分析技术的发展为鉴别某些物品的真伪提供了一种新的手段。文章介绍了一些茶饮料和水晶饰品的显微拉曼鉴别实例。