大型空间模拟器总体检漏技术

论述了大型空间环境模拟器的总体检漏技术,针对大型模拟器的特点,从设计、加工到安装调试等过程介绍了检漏方法的选择,并着重介绍了氦质谱检漏法可检灵敏度的分析,对大型模拟器的检漏方案进行了全过程的设计.     

红外隐身涂料颜料发射率研究

测试了多种颜料末及其在以酚醛树脂为粘合剂制成涂料的情况下（８￣１４）μｍ波段的平均红外发射率。研究发现，金属颜料的发射率一般较低，着色颜料的发射率一般都比较高，掺锡氧化铟（ＩＴＯ）半导体颜料红外发射率较低。还研究了颜料粉末发射率与将颜料制成涂料后发射率的关系。     

长寿命卫星热控涂层性能退化及其对卫星热特征的影响

分析了卫星热控涂层在轨运行时所面临的复杂的空间辐照环境,在国 内外试验数据的基础上,给出了热控涂层在空间辐照环境作用下的退化模型,得到了退化前 后热控涂层光学性能变化的表达式,预测了几种常用热控涂层在空间环境下的退化结果。并 以一颗地球同步轨道模拟星为例,分析热控涂层性能退化对卫星热特征尤其是对卫星红外辐 射特性的影响。
     

旋转弹制导技术的研究

旋转弹为近程、低空、快速反应的单舰防空导弹,主要拦截、攻击掠海飞行的反舰导弹和高速飞机,旋转弹主要采用红外被动寻的制导,具有操作简单、反射后不管的特点,飞行过程中采用单通道控制模式,用一对舵面和一个舵机来控制导弹飞行。点源红外寻的导引头探测的不是目标实体,而是目标红外辐射的中心,为了使导弹能够精确的击中目标的要害,本文根据旋转弹点源红外寻的导引头的特性,研究了前置偏移比例导引律,并结合某便携导弹进行了仿真,结果表明前置偏移比例导引律能够很好地导引导弹飞向目标,具有较好的精度。     

空间大气成分探测傅立叶变换红外光谱仪

文章阐述了用于空间大气成分探测傅立叶变换红外光谱仪的国外发展状况,主要介绍了几种国外先进的高分辨率空间大气探测用傅立叶变换红外光谱仪的结构、应用范围和技术指标,比较了这几种设备的优缺点和技术特点。     

用大面积源检定核应急机载/车载伽玛能谱仪

人工核素大面积源标准是核工业航测遥感中心等单位经过十余年研究建立的新型计量保障标准,使用该标准,可对监测核应急伽玛辐射环境的机载/车载伽玛能谱仪进行检定.使用大面积源标准检定,可以有效地弥补因机载/车载伽玛能谱仪系统的角响应影响因素复杂而难于模拟计算的缺陷,为监测核应急伽玛辐射环境的机载/车载伽玛能谱仪提供了量值传递的保障.本文介绍了大面积源检定的原理和技术方法.     

A strategic “viewfinder” for SETI research

One of the most important reasons why unsuccessful results have been obtained so far by the SETI Project is due to the fact that no sure targets to aim at have been available up-to the present state of research. All-sky surveys, even if very accurate and complete, might result to be time-consuming. SETI needs at least one effective “viewfinder” in order that a true targeted research is carried out with a possible success. The best foundation to get this can be identified with the search for the evidence of extraterrestrial astro-engineering activity in form of the Dyson spheres predicted by theory. The existence of such stellar objects can be ascertained by finding the evidence of two main signatures in stars of solar spectral type: infrared excess and anomalous light curves due to transiting artificial objects. These are probably the most powerful viewfinders in order to allow SETI techniques for intelligent signal search to be aimed at more appropriate targets. This paper is not intended to be a research paper but rather a review paper whose goal is not to present calculations and/or operational research but rather to be a research proposal for a more focused research in SETI just using Dyson Spheres as crucial markers.     

A neutral gas mass spectrometer to measure the chemical composition of the stratosphere

The Polar Balloon Atmospheric Composition Experiment (P-BACE) is a new generation of neutral gas mass spectrometer based on the time-of-flight principle. P-BACE is the scientific experiment on the Mars Environment Analog Platform (MEAP) flown successfully on a balloon mission in summer 2008. The MEAP mission was flown with a 334,000 m³ helium balloon in the stratosphere on a semicircular trajectory from northern Sweden around the North Pole to Canada using the summer northern hemispheric wind current. The atmospheric conditions at an atmospheric altitude of 35–40 km are remarkably similar to those on the surface of Mars and thus the balloon mission was an ideal testbed for our mass spectrometer P-BACE. Originally this instrument was designed for in situ measurements of the chemical composition of the Martian atmosphere.P-BACE has a unique mass range from 0 to 1000 amu/q with a mass resolution m/Δm (FWHM) > 1000, and the dynamic range is at least six orders of magnitude. During this experiment, the acquisition of one mass spectrum is a sum of 65,535 single spectra, recorded in a time frame of 66 s.The balloon mission lasted 5 days and had successfully demonstrated the functionality of the P-BACE instrument during flight conditions. We had recorded more than 4500 mass spectra. With little modifications, P-BACE can be used on a planetary mission for Mars, but for example also for Venus or Mercury, if placed on a satellite.     

Near infrared studies of the massive X-ray binary 2S 0114+65

We present near-infrared spectroscopy of the massive X-ray binary 2S 0114+650. These observations covering the spectral range 1.08–2.35 μm span the region where Paschen and Brackett series recombination lines of hydrogen are expected to be seen, namely, Paβ , Brγ and Br 10–17 lines. The absence of any of these lines in emission supports earlier inferences that the optical component in 2S 0114+650 is unlikely to be a Be star but rather a B type supergiant. Near-IR photometry gives J = 8.78, H = 8.53 and K = 7.96; these values show marginal variations from earlier reported measurements.     

分光计调节环节的补充及其应用

分光计是各高等院校在大学物理实验课教学中常用的一种仪器装置。分光计的调节对大学生基本实验技能的训练和培养有着十分重要的作用。本人在大学物理实验课全面开放式教学中,通过《分光计的使用》实验项目的教学实践、探索,提出了对分光计调节环节的补充建议,不仅使分光计调节环节的要求更加严谨,而且在实践教学的学生实验成绩评定考核方面,以及在实验指导教师对实验仪器装置精密度的检测方面都具有十分现实的应用意义。