共查询到18条相似文献,搜索用时 656 毫秒
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空间目标的可见光散射与红外辐射 总被引:22,自引:6,他引:16
利用Lowtran7大气传输模型计算了0.4~0.8μm可见光波段的太阳辐射、大气自身的热辐射以及天地背景辐射。利用粗糙面光散射理论与双向反射分布函数计算了空中目标表面对太阳辐射、云层对阳光反射的散射。并利用传热学和背景辐射理论,根据能量守恒定律建立了空间目标表面温度的热平衡方程。以气球为例,计算了不同表面涂层材料的气球在不同地理位置、不同高度、不同时间、温度及辐射功率的变化。分析了空间目标红外辐射特性的一般规律和特征。 相似文献
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空间目标可见光散射特性建模方法研究 总被引:8,自引:2,他引:6
针对空间目标的可见光散射特性提出一种建模方法.在分析空间目标所处的背景辐射环境基础上建立了空间目标背景辐射物理模型.对目标表面进行面元划分后,基于辐射理论引入双向反射分布函数模型来描述目标表面面元的光散射特性,将目标各个表面所有面元散射分量叠加建立了目标可见光散射特性的数学模型.建立目标本体坐标系,通过坐标变换确定目标、背景辐射源与探测器的相对位置关系,利用矢量坐标法确定目标对观测系统的“可视表面”.根据给定的目标几何结构尺寸和物性参量仿真获得了目标在轨光学特性.计算结果验证了建模的有效性. 相似文献
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基于高次余弦散射分布的空间卫星可见光特性 总被引:6,自引:4,他引:2
基于几何光学和辐射理论,研究了空间卫星的可见光散射特性.空间卫星的背景辐射主要包括太阳的直接辐射和地球及大气的散射辐射,根据目标的结构特性与背景特性建立了空间卫星的几何模型和光照模型.分析目标表面状况,入射到目标表面的光线近似服从高次余弦散射分布,根据能量守恒定理及表面材料的高次余弦散射分布特性建立了目标散射特性的数学模型.通过矢量坐标变换确定太阳、地球、观测卫星在目标本体坐标系下的相对位置关系.根据给定的几何尺寸和表面物性参量仿真获得了目标在探测器入瞳处的能量分布及星等特征,目标本体与太阳帆板在探测器入瞳处的辐照度最大量级均为10-12 W/m2.仿真结果表明太阳帆板在目标特性分析时不可忽略,为空间目标的可见光探测提供参考数据. 相似文献
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根据目标所处的背景辐射环境,对空间卫星的紫外散射特性进行建模方法研究。依据目标表面材料属性与表面状况对目标表面进行区域分解与网格划分。基于辐射理论引入双向反射分布函数模型来描述目标表面网格单元的光散射特性,将目标各个表面所有网格单元散射分量叠加建立了目标紫外散射特性的数学模型。利用给定的目标几何结构尺寸和物性参数仿真获得了目标在轨动态光学特性。在某一观测角度下太阳帆板在探测光学系统入瞳产生的辐照度值与卫星本体接近,最大量级为10-11W/m2。仿真结果表明太阳帆板在目标特性分析时不可忽略。 相似文献
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基于三维重建理论的目标光谱散射特性研究 总被引:1,自引:0,他引:1
根据三维重建理论,基于目标的多角度视图,重建了目标表面的三维点云。利用德洛奈三角剖分法结合可见性原理,得到了目标的曲面和曲面面元的法线方向。根据粗糙面散射理论和目标表面的双向反射分布函数(BRDF),结合大气传输软件Modtran计算的某时间、地点的背景光谱辐射亮度,数值分析了目标光谱散射亮度分布特性。以覆盖车衣的汽车为例,重建的三维几何模型误差为4.11%,数值计算了目标在三个波段的光谱散射亮度分布。上述方法可以进一步用于卫星和其他空间目标的光谱辐射、散射特性研究。 相似文献
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本文提出了一种结合MODIS数据产品和MODTRAN模型的典型地形条件空间目标红外辐射特性计算方法。考虑了地形条件和大气环境对空间目标的红外辐射特性影响,应用MODIS 3级陆地,海洋,冰雪圈数据产品得到全球温度分布,地形特征分布,将温度及地形条件代入MODTRAN计算得到地表-目标的辐亮度,进而计算目标的外热流以及表达目标的红外辐射特性。之后以全年第189天为例,计算卫星在某一时刻下的各表面的自身辐射、反射辐射、有效辐射。最后计算目标在不同天顶角下辐射强度随方向角的变化趋势。结果表明,空间目标的红外辐射特性与其运行姿态、所在位置的地形条件、表面材料、观测角度均有关系。 相似文献
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Zhensen Wu Daoyong Li Yanqun Zhang 《International Journal of Infrared and Millimeter Waves》2004,25(8):1201-1209
Considering background radiation of different wave band at different typical time by using Modtran soft, the characteristic of light scattering and the visibility condition of spatial object are discussed. Using bi-directional reflectance distribution function, combining geometry modeling with orbit theory, we numerical calculate light scattering radiation of spatial objects and compare it with the background radiation. The best observation time and station can be obtained by analyzing the conditions of visibility. 相似文献
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Mehdi Baneshi Shigenao Maruyama Atsuki Komiya 《Journal of Quantitative Spectroscopy & Radiative Transfer》2009,110(3):192-84
Pigmented coatings with high reflectivity against solar irradiation can be used to control unwanted thermal heating that occurs as materials absorb sunlight such as heat in buildings that increases cooling loads. However, these surfaces produce glare that is unpleasant to the eye, and the coatings themselves can damage the appearance of the coated object. We introduce a new optimization method that embraces both thermal and aesthetic requirements. Our proposed coatings maximize the reflectivity of the near infrared (NIR) region to reduce thermal heating, while for aesthetic appeal they also minimize the visible (VIS) reflected energy received by human eyes, especially at wavelengths where eye sensitivity is high. The optimization parameter is defined as the ratio of the total reflected energy in the NIR region to that in the VIS region weighted by human eye sensitivity. Titanium dioxide is used as the pigment, and databases of its radiative properties are constructed using the Mie theory. To compute reflectivity, nongray radiative heat transfer in an anisotropic scattering monosized pigmented layer, with independent scattering, including direct and diffuse solar irradiations, is analyzed using radiation element method by ray emission model (REM2). Colors are calculated and optimization parameter is evaluated by using spectral reflectivity. Finally, the optimum values of particle size, volume fraction of pigment, and coating thickness are obtained. 相似文献
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V. Grünhut R. A. Depine 《The European Physical Journal D - Atomic, Molecular, Optical and Plasma Physics》2011,62(2):227-236
To study the scattering properties of metamaterials, we generalize two scattering methods
developed for conventional (non-magnetic) isotropic materials to the case of materials
with arbitrary values (positive or negative) of magnetic permeability and electric
permittivity. The generalized methods are used to study the changes produced in the
reflectivity of a metamaterial surface with localized roughness when the relative
refractive index changes sign. Our results show that, unlike the case of a plane surface
whose reflectivity is unaffected by the change of sign of the relative refractive index,
in rough surfaces the change of sign is manifested in the reflectivity, even for very low
roughness, particularly in observation directions away from the specular direction. 相似文献
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Alexander M. Zarubin 《Optics Communications》1993,100(5-6):491-507
Coherence properties of primary partially coherent radiations (light, X-rays and particles) elastically scattered from a 3D object consisting of a collection of electrons and nuclei are analyzed in the Fresnel diffraction region and in the far field. The behaviour of the cross-spectral density of the scattered radiation transverse and along to the local direction of propagation is shown to be described by respectively the 3D Fourier and Fresnel transform of the generalized radiance function of a scattering secondary source associated with the object. A relativistic correct expression is derived for the mutual coherence function of radiation which takes account of the dispersive propagation of particle beams in vacuum. An effect of the spatial coherence of radiation on the temporal one is found; in the Fresnel diffraction region, in distinction to the field, both the longitudinal spatial coherence and the spectral width of radiation affect the longitudinal coherence. A solution of the 3D inverse scattering problem for partially coherent radiation is presented. It is shown that squared modulus of the scattering potential and its 2D projections can be reconstructed from measurements of the modulus and phase of the degree of transverse spatial coherence of the scattered radiation. The results provide a theoretical basis for new methods of image formation and structure analysis in X-ray, electron, ion, and neutron optics. 相似文献
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Determination of the size of a radiation source by the method of calculation of diffraction patterns
I. N. Tilikin T. A. Shelkovenko S. A. Pikuz D. A. Hammer 《Optics and Spectroscopy》2013,115(1):128-136
In traditional X-ray radiography, which has been used for various purposes since the discovery of X-ray radiation, the shadow image of an object under study is constructed based on the difference in the absorption of the X-ray radiation by different parts of the object. The main method that ensures a high spatial resolution is the method of point projection X-ray radiography, i.e., radiography from a point and bright radiation source. For projection radiography, the small size of the source is the most important characteristic of the source, which mainly determines the spatial resolution of the method. In this work, as a point source of soft X-ray radiation for radiography with a high spatial and temporal resolution, radiation from a hot spot of X-pinches is used. The size of the radiation source in different setups and configurations can be different. For four different high-current generators, we have calculated the sizes of sources of soft X-ray radiation from X-ray patterns of corresponding objects using Fresnel-Kirchhoff integrals. Our calculations show that the size of the source is in the range 0.7–2.8 μm. The method of the determination of the size of a radiation source from calculations of Fresnel-Kirchhoff integrals makes it possible to determine the size with an accuracy that exceeds the diffraction limit, which frequently restricts the resolution of standard methods. 相似文献
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The time-dependent radiation transfer in a semi-infinite stochastic medium of binary Markovian mixture with Rayleigh scattering is presented. A formalism, developed to treat radiation transfer in statistical mixtures, is used to obtain the ensemble-averaged solution. The average reflectivity, radiant energy and net flux are computed for specular-reflecting boundary. For the sake of comparison, we use two different weight functions in our calculations. 相似文献
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基于激光尾场加速的全光汤姆孙散射能够提供高质量X射线束并大大减小装置的尺寸.与分光式相比,自反射式的构架可以降低实验的时空同步难度,但是由于激光尾场电子加速和汤姆孙散射过程耦合, X射线优化难度大,目前缺乏参数优化的相关报道.本文用数值模拟修正解析理论的方法,定量分析了激光尾场电子加速和汤姆孙散射过程中激光和电子束的焦斑、脉宽、能量等参数变化情况,并给出了激光在等离子体镜上的反射率,从而实现了用解析公式计算而非数值模拟跟踪参数变化,在保证精度的同时节约了计算时间.另外,利用修正后的公式优化了给定激光条件下的自反射式全光汤姆孙散射X射线,通过改变等离子体密度和等离子体镜位置这两个参数给出了最优X射线亮度和光子产额,该方法为将来结合人工智能优化控制全光汤姆孙散射光源提供了理论基础. 相似文献
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The possibility is theoretically examined, of the observation of “structure-induce” surface plasmon polariton modes on semi-finite free electron metals and semiconductors, using the Otto ATR configuration. This is achieved by introducing spatial dispersion into a model double step-function surface density profile. For both metals and semiconductors it is shown that well-defined minima in the reflectivity plots are associated with structure-induced modes. Furthermore, these modes occur quite strongly below the critical angle, which suggests that they are best developed in their radiative form. 相似文献