K418合金的组织对低周疲劳性能的影响

研究了Ｋ４１８合金不同宏观组织（晶粒度）对低周疲劳性能的影响，同时研究了不同热处理状态下合金组织中的γ’相及其对合金的低周疲劳性能的影响。     

含Nd稀土相对高温钛合金低周疲劳裂纹萌生与扩展行为的影响

实验研究了含稀土Ｎｄ高温钛合金中稀土相颗粒与室温及６００℃低周疲劳裂纹萌生与扩展行为的关系。结果表明，疲劳裂纹在距颗粒一定距离的基体中产生，而不在预先开裂或脱粘的颗粒处萌生。裂纹扩展时绕过颗粒并使裂纹扩展路径曲折化。     

复杂目标红外辐射特性大数据知识表示及建模方法

为了提升复杂目标红外辐射特性建模效率及置信度问题，提出一种目标红外辐射特性的大数据知识表示及建模方法。首先利用机理分析法、主成分分析法确定目标红外辐射特性大数据维度;然后基于主成分分析的结果，进行目标红外辐射特性大数据知识表示，建立目标红外辐射特性仿真模型;最后进行模型的仿真应用，在应用过程中进一步完善目标红外辐射特性数据或知识表示。本文提供的大数据驱动的目标红外辐射特征建模方法，能够推广应用于复杂电磁环境的仿真。     

The European Large Area ISO Survey

The European Large Area ISO Survey (ELAIS) was the largest Open Time survey on the Infrared Space Observatory (ISO). It was designed to explore obscured galaxies and hence quantify the recent star-formation history of the Universe. The final reanalysis of the data has been completed and a band-merged catalogue with associations across many wavelengths compiled and released the data to the global astronomical community (http://astro.imperial.ac.uk/Elais/). This paper summarises some of the key results. 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.     

城郊低密度住宅建筑探讨

本文以作者的实践经验为基础，对低密度住宅的规划及设计要点进行探讨。     

轴对称矢量喷管的气膜冷却及红外辐射耦合计算分析

为考察喷管壁面气膜冷却以及红外辐射特性对高性能航空发动机壁温分布的影响,对燃气红外波带的光谱特性采用窄波段模型计算,对壁面-燃气辐射采用封闭腔模型计算,对喷管收敛段的气膜冷却采用绝热温比计算。对于包含喷管壁面、隔热屏、套筒的多层结构传热建立壁温-热流耦合的热平衡方程,用Newt on-Raphson求解得到喷管及内外结构的壁温。对NASA TN D-1988中试验台架发动机喷管扩张段的气膜冷却及壁温进行验证计算,并详细计算了收敛段采用多排缝槽气膜冷却的轴对称矢量喷管。结果表明:气膜冷却有效降低了喷管收敛段的壁温,使得喷管扩张段成为受热严峻的部位;扩张段偏转改变了扩张段壁面温度和红外辐射的圆周分布,沿偏转方向的壁温和红外辐射都明显低于偏转反方向的,2个方向上的平均壁温相差约4.8%,喷管在后半球的辐射沿偏转方向增强。数值模拟结果与试验测量值吻合良好,可用于发动机喷管壁温分布精确计算。     

The James Webb Space Telescope

The James Webb Space Telescope (JWST) is a large (6.6 m), cold (<50 K), infrared (IR)-optimized space observatory that will be launched early in the next decade into orbit around the second Earth–Sun Lagrange point. The observatory will have four instruments: a near-IR camera, a near-IR multiobject spectrograph, and a tunable filter imager will cover the wavelength range, 0.6 < ; < 5.0 μ m, while the mid-IR instrument will do both imaging and spectroscopy from 5.0 < ; < 29 μ m.The JWST science goals are divided into four themes. The key objective of The End of the Dark Ages: First Light and Reionization theme is to identify the first luminous sources to form and to determine the ionization history of the early universe. The key objective of The Assembly of Galaxies theme is to determine how galaxies and the dark matter, gas, stars, metals, morphological structures, and active nuclei within them evolved from the epoch of reionization to the present day. The key objective of The Birth of Stars and Protoplanetary Systems theme is to unravel the birth and early evolution of stars, from infall on to dust-enshrouded protostars to the genesis of planetary systems. The key objective of the Planetary Systems and the Origins of Life theme is to determine the physical and chemical properties of planetary systems including our own, and investigate the potential for the origins of life in those systems. Within these themes and objectives, we have derived representative astronomical observations.To enable these observations, JWST consists of a telescope, an instrument package, a spacecraft, and a sunshield. The telescope consists of 18 beryllium segments, some of which are deployed. The segments will be brought into optical alignment on-orbit through a process of periodic wavefront sensing and control. The instrument package contains the four science instruments and a fine guidance sensor. The spacecraft provides pointing, orbit maintenance, and communications. The sunshield provides passive thermal control. The JWST operations plan is based on that used for previous space observatories, and the majority of JWST observing time will be allocated to the international astronomical community through annual peer-reviewed proposal opportunities.     

红外目标旋转模拟器校准方法的研究设想

文章简要介绍了红外目标旋转模拟器的结构组成、工作原理,给出了红外目标旋转模拟器的目标温度、平均角速度、角速度波动的校准方法,该校准方法能为光电设备的量值溯源提供解决方案.     

热敏电阻元件低温校准方法研究

介绍了热敏电阻元件低温校准系统的校准原理及校准关键技术,以MF5602型和MF5604型负温度系数热敏电阻元件为例,对校准系统和关键技术、校准方程以及数据拟合方法进行了研究,提出了火箭发动机用热敏电阻元件在低温环境下的校准方法.     

The Silicate Material in Comets

Silicates in comets appear to be a mix of high-temperature crystalline enstatite and forsterite plus glassy or amorphous grains that formed at lower temperatures. The mineral identifications from the 10 and 20 μm cometary spectra are consistent with the composition of anhydrous chondritic aggregate IDPs. The origin of the cometary silicates remains puzzling. While the evidence from the IDPs points to a pre-solar origin of both crystalline and glassy components, the signatures of crystalline silicates appear in the spectra of young stellar objects only at a late evolutionary stage, when comets are the likely source of the dust. This revised version was published online in June 2006 with corrections to the Cover Date.