空间目标的空基红外测量技术

地基红外测量系统由于受大气衰减和天空背景的影响,对空间目标的探测能力有限。针对此问题,提出了采用空基红外测量系统实现空间目标红外特性测量的设想,通过从决定红外测量系统探测能力的信噪比和调制对比度2个方面出发,推导出了红外测量系统作用距离公式。并利用大气传输软件计算了长波红外在不同高度下的大气透过率、天空背景,理论分析给出了不同高度的空基红外测量系统对不同辐射面积空间目标的探测距离。仿真结果表明,当空基平台高度大于10km时,长波红外不仅可以观测到光照区内的低轨空间目标,而且还可以观测到阴影区内辐射面积不小于40m~2的低轨空间目标。     

民用飞机大气传感器低速验证试验研究

飞机的大气传感器是获得飞机外部大气参数的重要的测量仪器,如果大气传感器自身精度不够,或者由于布置不合理引起的误差,就会引起飞行危险。为了验证气动设计的布局方案,选出传感器位置比较优化的方案,得到机头静压值随迎角变化不变的区域,同时总结出民机大气数据传感器布局设计验证的风洞试验方法。通过低速测压风洞试验和缩比传感器（风标和七孔探针）,测量得到大气传感器不同布局位置的气动特性。结果表明：大气传感器的布局位置对测量结果影响相当重要;试验结果与计算结果符合良好,满足气动设计要求。     

Infrared radiation simulation of exhaust system by coupling FVM with narrow band k-distribution

A three-dimensional infrared radiation code for exhaust system was developed by the finite volume method coupled with narrow band k-distribution in non-gray absorbing-emitting media. The final infrared signature had considered the atmosphere effect, and the simulation values were favorably consistent with testing ones. The results indicate that the relative errors considering the effect of atmosphere compared with that of the contrary condition reduce by 31%, it shows that when simulating the infrared radiation of the target which is received by the infrared detectors, even the calculation band is in atmospheric windows 3~5 μm, the effect of atmospheric transmission on infrared signature of the target should not be neglected.      

Detection Statistics for Laser Radar in Atmospheric Turbulence with Fluctuating Targets

The probability of detection and false-alarm rates are developed for laser radar systems perturbed by background radiation, fluctuating targets, and atmospheric turbulence. In particular, some results on the decibel loss due to atmospheric turbulence are presented.     

大气及地面红外辐射对高空飞机长波低发射率红外隐身效果的影响

计算分析了蒙皮反射的大气及地面红外辐射对高空飞机采用低发射率材料的红外隐身效果的影响.蒙皮温度采用恢复温度,红外辐射采用反向蒙特卡罗法计算.考虑了夏季和冬季两种典型大气和地面条件,亚声速巡航和超声速巡航两种飞行状态.结果表明:蒙皮对背景红外辐射的反射使得低发射率材料对飞机红外辐射强度的抑制效率降低1.5%~6%;考虑反射的背景红外辐射时,探测距离增加20%~70%;背景红外辐射对低速飞机的红外辐射影响较大,且夏季比冬季更明显;当飞行速度较低时,降低飞机上表面发射率,当飞行速度较高时,降低飞机全部表面的发射率,可获得更好的红外隐身效果.      

基于地球红外背景模拟的 水云大气影响初步分析

为支持地球红外背景的模拟研究,以天基观测为前提,计算了2个大气窗口下,4个具有典型大气和地表特征的区域在水云大气下的路径透过率和各成分辐射亮度。通过相对变化比例,讨论了地球背景模拟中水云与地表的图像区分以及地域的影响。结果表明,水云对地球背景辐射传输影响显著:云层下方辐射会被强烈衰减,同时观测路径中的散射辐射大幅增强。在同一选定区域下,积云大气的观测路径亮度相对无云大气下变化最大,在相同水云类型条件下,大气散射和太阳散射亮度在不同区域区别较大,说明在模拟水云地球背景时不能忽略地域的影响。计算和分析结果可为地球背景模拟中的水云红外图像生成提供一定的数据基础和技术支持。     

Cosmic Rays,Clouds, and Climate

A correlation between a global average of low cloud cover and the flux of cosmic rays incident in the atmosphere has been observed during the last solar cycle. The ionising potential of Earth bound cosmic rays are modulated by the state of the heliosphere, while clouds play an important role in the Earth's radiation budget through trapping outgoing radiation and reflecting incoming radiation. If a physical link between these two features can be established, it would provide a mechanism linking solar activity and Earth's climate. Recent satellite observations have further revealed a correlation between cosmic ray flux and low cloud top temperature. The temperature of a cloud depends on the radiation properties determined by its droplet distribution. Low clouds are warm (>273K) and therefore consist of liquid water droplets. At typical atmospheric supersaturations (1%) a liquid cloud drop will only form in the presence of an aerosol, which acts as a condensation site. The droplet distribution of a cloud will then depend on the number of aerosols activated as cloud condensation nuclei (CCN) and the level of super saturation. Based on observational evidence it is argued that a mechanism to explain the cosmic ray-cloud link might be found through the role of atmospheric ionisation in aerosol production and/or growth. Observations of local aerosol increases in low cloud due to ship exhaust indicate that a small perturbation in atmospheric aerosol can have a major impact on low cloud radiative properties. Thus, a moderate influence on atmospheric aerosol distributions from cosmic ray ionisation would have a strong influence on the Earth's radiation budget. Historical evidence over the past 1000 years indicates that changes in climate have occurred in accord with variability in cosmic ray intensities. Such changes are in agreement with the sign of cloud radiative forcing associated with cosmic ray variability as estimated from satellite observations.     

煤油燃气温度的测量方法研究

在全面分析煤油燃气辐射特性的基础上，结合煤油燃气的具体特点，提出了适合于测量煤油燃气温度的辐射测量方法[4]，并且建立了辐射测温系统，通过对煤油燃气温度的实际测量，验证了辐射测温法测量燃气温度的可行性。     

红外测温中环境辐射影响的分析

对物体进行辐射测温时,若被测物体温度接近环境温度,则环境因素对测量结果影响较大.为了提高测量精度,依据普朗克定律通过数值计算得出红外测温中环境温度影响比率在不同物体温度、环境温度和辐射波长的值以及它们之间的关系,并在此基础上分析了若使环境辐射的影响可忽略则被测物体所满足的最低温度.最后讨论了环境辐射对比色测温的影响.     

Ultraviolet spectrometer experiment for the Voyager mission

The Voyager Ultraviolet Spectrometer (UVS) is an objective grating spectrometer covering the wavelength range of 500–1700 Å with 10 Å resolution. Its primary goal is the determination of the composition and structure of the atmospheres of Jupiter, Saturn, Uranus and several of their satellites. The capability for two very different observational modes have been combined in a single instrument. Observations in the airglow mode measure radiation from the atmosphere due to resonant scattering of the solar flux or energetic particle bombardment, and the occultation mode provides measurements of the atmospheric extinction of solar or stellar radiation as the spacecraft enters the shadow zone behind the target. In addition to the primary goal of the solar system atmospheric measurements, the UVS is expected to make valuable contributions to stellar astronomy at wavelengths below 1000 Å.     

A concept of a spacecraft with small initial mass placed in the near-earth orbit by a laser rocket engine

A method and results of calculating the laser radiation power values necessary to place an artificial earth satellite in orbit are presented; the values depend on the initial vehicle mass, velocity of the working fluid efflux from the laser rocket engine nozzle, velocity of vehicle motion, optimal values of thrust-to-weight ratio taking into account irreversible energy losses in the rocket engine jet. The possibility of creating a spacecraft with small initial mass is substantiated. A layout scheme of the propulsive system is proposed that makes it possible to divide total laser radiation power and to use atmospheric air as a working fluid.     

模型表面温度对光电特性影响的实验研究

对在JF-10氢氧爆轰驱动高焓激波风洞中开展烧蚀材料模型表面温度对光电特性影响的实验方法进行了探索。风洞实验状态的驻室总压约为20MPa,驻室总温约为6000K,自由流速度约为4km／s。实验以锑化铟多单元红外成像系统与电离列阵测试装置为测量手段,用以烧蚀材料为头部的球头钝锥体模型,实验测量激波层中红外辐射的横向剖面分布和壁面附近电离密度的剖面分布,并在烧蚀材料加热和不加热两种情况下进行了对比实验。实验结果表明：烧蚀材料的加热加强了模型头部激波层中的红外辐射,同时也增大了模型表面的电子密度。     

Cosmic Ray Induced Ion Production in the Atmosphere

An overview is presented of basic results and recent developments in the field of cosmic ray induced ionisation in the atmosphere, including a general introduction to the mechanism of cosmic ray induced ion production. We summarize the results of direct and indirect measurements of the atmospheric ionisation with special emphasis to long-term variations. Models describing the ion production in the atmosphere are also overviewed together with detailed results of the full Monte-Carlo simulation of a cosmic ray induced atmospheric cascade. Finally, conclusions are drawn on the present state and further perspectives of measuring and modeling cosmic ray induced ionisation in the terrestrial atmosphere.     

辐射发射与辐射法测温—如何接近表面真实温度

从辐射测法中辐射率变化对温度的影响，讨论了多色辐射测量法的发展与应用实践，比较了不同处理方法的优缺点。     

Numerical simulation of the infrared radiative signatures of liquid and solid rocket plumes

In this paper, a finite volume method was developed to compute the infrared radiative signatures of both liquid and solid rocket plumes, and to investigate the radiative signatures on two wavebands, 2–6 and 8–12 μm bands, respectively. This method is based on the radiative transport equation for local thermodynamic equilibrium, which accounts for radiative heat transfer in inhomogeneous emitting, absorbing, and non-isotropic scattering media. The radiative properties of combustion gases are computed by using the Elsasser narrow band model, and that of particles are computed by using the Mie scattering theory. A numerical method is applied to solve the following three problems. The first one is the computation of the radiative heat transfer in an absorbing, emitting and isotropic scattering homogeneous cylindrical medium in which the radiative flux is presented. The other two are the computations of the infrared radiation of plumes from the liquid and solid rockets in which both the source and apparent radiant intensities are presented as results. The atmospheric absorption effect on the radiation of plumes is also considered by calculating the atmospheric transmittance using MODTRAN. Some of these results, compared with those available in the literature, have shown satisfactory agreement in most cases.     

固液混合火箭发动机喷焰红外辐射特性分析

为了研究固液混合火箭发动机喷焰在不同飞行状态的红外辐射特性,建立了固液两相状态下喷焰的红外辐射计算模型,获得了喷焰在2~12μm波段的红外辐射.将喷焰的温度、压力、摩尔组分等作为输入条件,米氏散射(Mie)模型计算颗粒相的散射,采用有限体积法(FVM)离散辐射传递方程,利用中分辨率大气辐射传输(MODTRAN)模型计算不同观测距离的大气透过率,编程计算得到不同飞行高度,不同观测方向下喷焰的红外辐射.结果表明喷焰红外辐射亮度与温度分布类似,在2.7~3.0μm和4.2~4.5μm波段范围内的辐射较强,高温粒子在近红外比远红外对总辐射的贡献大,太空与地面观测不同飞行高度的发动机喷焰辐射率因大气衰减的不同而有所差异,可为目标跟踪与发动机设计提供参考.      

Theory of formation of the ionosphere

Current knowledge about the solar radiation and absorption and ionization cross sections of atmospheric gases is reviewed. Next the main observed features of ionospheric layers are summarized. Using CIRA 1965 model atmospheres the heights of the peak of the ionization rate are calculated for a number of solar emission lines and it is made clear which of these lines are responsible for the formation of E and F1 layers. The mechanism of electron removal in the F and upper E regions as well as in the lower regions is considered, and the mechanism of formation and some behaviours of each ionospheric layer is discussed. In particular, the equatorial F2 layer is briefly considered. Discrepancies are pointed out between the values of the recombination coefficient and the rate constant for ion-atom interchange reaction obtained from ionospheric observations and from laboratory experiments. Inconsistency of the values of the intensity of solar radiation measured by rocket techniques and inferred from ionospheric considerations is also noted. Some evidence is presented suggesting that corpuscular radiation may be responsible for part of the ionization in the ionosphere even in temperate latitudes.     

能见度测量技术现状及发展趋势综述

介绍了大气能见度测量的基本原理及主要方法;讨论了国内外能见度测量技术及仪器的研究现状;总结了测量能见度的几种主要方法的优缺点;分析了能见度测量技术研究中有待攻克的问题;探讨了能见度测量技术的发展趋势。     

金属壁面红外辐射能的测试技术研究

本文介绍了金属壁面红外辐射能的测试方法、测试原理和测试设备, 并对铁板和不锈钢板的红外辐射特性进行了初步的实验研究, 研究加热温度对材料辐射率的影响。试验结果表明该测试方法是可行的, 测试设备是可靠的。      

飞行状态对太阳能飞机中组件性能的影响

基于光伏组件产生功率模型，研究了太阳能飞机中飞行速度、高度、时间及区域等状态参数影响组件性能的规律。以单晶硅组件及Xihe太阳能飞机为研究对象，当飞机飞行速度增加时，组件产生的功率随之增加但趋于饱和。原因在于速度的增加能有效降低组件的表面温度，但提升是有限的。飞机所需的功率随飞行速度呈现指数增加，且组件产生的功率与飞机所需的功率有能量平衡点。组件产生的功率随飞行高度的增加而增加，但有饱和的趋势。原因在于，当飞行高度上升，大气温度随之下降，组件表面温度下降；同时海拔越高，大气密度和大气通透率越大，太阳辐射增加，从而组件产生的功率增加了；饱和的原因在于组件本身性能的限制。一天之中，组件产生的功率基本以太阳时12点为中心左右近似对称，中午最强；一年中组件性能在夏季最强，冬季最弱。原因在于组件性能主要由所受太阳辐射决定。随着纬度的增加，组件产生的功率减小。原因在于，纬度越高，太阳高度角越小，组件所能接受到的太阳辐射也就越小；纬度越低，组件总产生功率越高且平稳。纬度低的地区更适合太阳能飞机的飞行。该文为太阳能飞机的能量分配、长时间驻空提供一定的帮助。