共查询到20条相似文献,搜索用时 218 毫秒
1.
2.
基于MDA法计算水雾粒子红外隐身粒径 总被引:1,自引:0,他引:1
水雾隐身技术是一种较为理想且经济适用的目标特征信号控制技术。本文从辐射传输方程出发,考虑水雾粒子的本身辐射和散射,提出以红外表观透射率评价水雾粒子的红外隐身性能。应用Modified Differential Approximation(MDA)法结合MIE理论,计算了水雾粒子红外表观透射率随水雾粒子浓度和粒径的变化关系,得到水雾粒子最佳红外隐身粒径。结果表明:水雾粒子的红外表观透射率随粒子浓度的增加而减小,但当粒子的浓度增加到一定值时,红外表观透射率基本保持不变;水雾粒子的红外表观透射率随粒径的增加先减小后增大,当探测波段为3~5μm时,水雾粒子的最佳红外隐身粒径为6μm;而探测波段为8~12μm时,水雾粒子的最佳红外隐身粒径为12μm。 相似文献
3.
4.
5.
大气中大量存在的复合粒子会对激光传输效率产生很大影响。由于空气中水蒸气含量较高,以C作为凝结核外层包裹以水的核壳结构微粒对光传输具有明显的散射效应。本文应用Mie散射理论对C@H_2O核壳结构微粒的散射特性进行了理论分析和数值计算,首先给出了不同入射波长、核粒子半径以及水膜厚度条件下散射强度分布变化曲线;其次给出了不同入射波长、核粒子半径以及水膜厚度条件下偏振变化情况;最后讨论了光学截面与粒子半径之间的关系。结果表明各参数对前向散射强度影响较大,入射波长越大散射强度越弱,C核半径增大粒子的前向散射增强,水膜厚度增大粒子的前向散射增强,而后向散射无明显影响;入射波长较大时,粒子在多个角度出现线偏振光,入射波长增大、碳核半径变大、水膜厚度增大,偏振度峰值都会增多;随着入射波长的增大,散射截面最大峰值位置向着半径增大的方向移动,并伴随一定的振荡现象,散射和消光截面在碳核半径为0.1μm左右达到最大值。 相似文献
6.
7.
8.
基于组合拟合法的冰晶粒子的光散射计算 总被引:1,自引:0,他引:1
利用组合拟合法计算了冰晶粒子的单次散射特性。给出了消光效率因子、单次散射反照度及非对称因子的拟合公式,利用拟合公式对有效粒子尺度为20μm和120μm的六种冰晶粒子的消光效率因子、单次散射反照度及非对称因子进行了计算。结果表明,粒子的消光效率因子、单次散射反照率和非对称因子随着入射波长的增加有着较大的起伏,后两者随着波长的增加而变化趋势基本一致;对于单次散射反照率来说,在可见光波段,反照率非常接近于1;在短波段,粒子的非对称因子变化较小,并且随着波长的增加,非对称因子会逐渐增大。 相似文献
9.
为了研究尘埃等离子体中带电尘埃的粒子半径、粒子浓度和带电荷数对量子通信性能的影响,首先根据Mie散射理论得到单个带电尘埃粒子的光散射截面;然后通过粒子浓度求出总的消光截面,得出链路衰减的数学模型,提出了带电粒子特性与量子纠缠度的关系;针对退极化信道,当单个尘埃粒子所吸附带电粒子的个数为50时,给出了尘埃粒子半径、粒子浓度与信道容量和量子误码率的定量关系.仿真结果表明,当量子信号的传输距离为10km时,尘埃粒子浓度从1×10~(10) m~(-3)增加到10×10~(10) m~(-3),信道容量从0.6726降低到0.1075;尘埃粒子半径从0.1μm增加到10μm时,量子误码率由1.334×10~(-3)增加到5.309×10~(-3).由此可见,尘埃等离子体中带电尘埃粒子的半径和浓度对量子卫星通信性能有显著的影响.因此,为确保量子通信的可靠性,应根据所探测到的等离子体环境的状况,调整卫星通信系统的各项指标参数. 相似文献
10.
在已知大气气溶胶折射率和气溶胶谱分布的基础上, 对近红外波段的气溶胶衰减特性进行了研究。利用Mie散射理论计算并讨论了气溶胶的消光、散射、吸收效率因子随尺度参数的变化和消光系数随半径和波长的变化, 并且在MATLAB中对各种变化情况进行了仿真。结果表明, 三种气溶胶粒子的消光和散射能力依次为沙尘性粒子, 水溶性粒子, 烟煤。消光系数在粒子半径和入射波长相近时达到最大, 并且粒子半径对消光、散射、吸收系数的影响比入射波长更明显。这些结论可以为红外辐射在大气中的衰减计算和分析提供依据。 相似文献
11.
海雾的遥感光学辐射特性 总被引:4,自引:2,他引:2
为实现海雾的卫星自动监测,利用大量AVHRR3/NOAA17卫星观测数据,比较不同目标物(海雾区、不同云系及晴空下垫面)在可见光、近红外波段的反射辐射特性差异,统计分析了海雾的遥感光学辐射特性.结果表明,海雾区三通道反射率满足RCh1RCh3a>RCb2,甚至出现RCh3a>RCh1>RCh2不同于其它目标物(RCh1>RCh2>RCh3a.运用Streamer辐射传输模式模拟了海雾、不同云系在卫星高度处的三通道反射率特性,从理论上进一步验证了海雾所具有的光学辐射特性,同时指出,Ch3a的反射率对粒子粒径的响应明显,即粒子粒径越小,Ch3a的反射率越高.通过米氏散射理论对这一现象进行原因分析. 相似文献
12.
基于中纬度卷云冰晶双峰、热带卷云冰晶三峰分布模型,利用Mie散射理论计算了1~13脚范围内中纬度及热带卷云的消光系数、散射系数、吸收系数。计算结果表明,由不同形状冰晶构成的热带卷云的相应光学参数比中纬度卷云的光学参数大些,但11支子弹玫瑰形状的相应参数要小一些;两种卷云在2.8~3.1μm,9.8~13μm范围内都存在两个基本相同的透射通带;在计算中纬度卷云的光学参数时,可以只考虑中空六棱柱与实心六棱柱中的一种,但计算热带卷云的光学参数时,实心六棱柱与空心六棱柱需要同时考虑。 相似文献
13.
This paper reports that heat insulating property of infrared reflective coatings is obtained through the use of pigments which diffuse near-infrared thermal radiation.Suitable structure and size distribution of pigments would attain maximum diffuse infrared radiation and reduce the pigment volume concentration required.The optimum structure and size range of pigments for reflective infrared coatings are studied by using Kubelka-Munk theory,Mie model and independent scattering approximation.Taking titania particle as the pigment embedded in an inorganic coating,the computational results show that core-shell particles present excellent scattering ability,more so than solid and hollow spherical particles.The optimum radius range of core-shell particles is around 0.3 ~ 1.6 μm.Furthermore,the influence of shell thickness on optical parameters of the coating is also obvious and the optimal thickness of shell is 100-300 nm. 相似文献
14.
O. R. Musaev E. Sutter J. M. Wrobel M. B. Kruger 《Applied Physics A: Materials Science & Processing》2013,110(2):329-333
The eutectic alloy of BiInSn was ablated in water by UV pulsed radiation. Electron microscopy of the ablated material shows spherical particles that fall into three size regimes: those with diameters of ~0.5 μm, crystalline and amorphous particles with dimensions of ~30 nm, and amorphous particles that are approximately 1 nm across. The 30-nm amorphous particles are homogeneous, while there are two types of 30-nm crystalline particles, those that separate into three phases and those that are homogeneous. The existence of different characteristic sizes is explained by two mechanisms: phase explosion and Rayleigh instability of the ejected melt. 相似文献
15.
《中国物理 B》2021,30(6):64206-064206
When a laser is transmitted in fog, and the water droplets will scatter and absorb the laser, which affects the intensity of the laser transmission and the accuracy of radar detection. Therefore, it is of great significance to study the laser transmission in the fog. At present, the main method of calculating the scattering and attenuation characteristics of fog is based on the radiation transmission theory, which is realized by a large number of numerical calculations or physical simulation methods, which takes time and cannot meet the requirements for obtaining the fast and accurate results. Therefore, in this paper established are a new laser forward attenuation model and backward attenuation model in low visibility fog. It is found that in low visibility environments, the results calculated by the Monte Carlo method are more accurate than those from most of the existing forward attenuation models. For the cases of 0.86-μm, 1.06-μm, 1.315-μm, 10.6-μm typical lasers incident on different fogs with different visibilities, a backscatter model is established, the error between the fitting result and the calculation result is analyzed, the backward attenuation fitting parameters of the new model are tested, and a more accurate fitting result is obtained. 相似文献
16.
17.
Iteration method for the inversion of simulated multiwavelength lidar signals to determine aerosol size distribution 下载免费PDF全文
A new method is proposed to derive the size distribution of aerosol from the simulated multiwavelength lidar extinction coefficients. The basis for this iteration is to consider the extinction efficiency factor of particles as a set of weighting function covering the entire radius region of a distribution. The weighting functions are calculated exactly from Mie theory. This method extends the inversion region by subtracting some extinction coefficient. The radius range of simulated size distribution is 0.1-10.0μm, the inversion radius range is 0.1-2.0μm, but the inverted size distributions are in good agreement with the simulated one. 相似文献
18.
19.
太赫兹波空间传输特性研究对于太赫兹波在空间中的应用具有重要意义.为研究太赫兹波在沙尘暴天气中的传输特性,本文根据沙尘粒子尺度的对数正态分布,应用Mie散射理论和Monte Carlo方法,分析了国内不同地域的六种干沙模态沙尘暴对1—10 THz频段太赫兹波的衰减特性,给出了消光参量和衰减率与频率的关系.结果表明,随着频率的增大,1—10 THz频段太赫兹波的衰减率呈先增加后减小的趋势,沙尘暴的模态不同,太赫兹波衰减较强的频段范围有所不同.为了分析沙粒含水量对太赫兹波传输衰减的影响,计算了不同尺寸的沙尘粒子3个效率因子与含水量的关系,发现粒子尺寸不同,含水量对消光的影响也不同;应用Monte Carlo方法计算了两种湿沙模态的沙尘暴对1—10 THz频段太赫兹波的衰减,给出了衰减率与含水量及频率的关系.结果表明,随沙粒含水量增大,沙尘暴对太赫兹波衰减较强的频段向低频方向移动,含水量小于5%时,太赫兹波衰减率随含水量增大显著增强,湿度较大的沙尘暴天气对太赫兹波的传输衰减影响更大. 相似文献
20.
Riekel C Burghammer M Davies RJ Di Cola E König C Lemke HT Putaux JL Schöder S 《Journal of synchrotron radiation》2010,17(6):743-750
X-ray radiation damage propagation is explored for hydrated starch granules in order to reduce the step resolution in raster-microdiffraction experiments to the nanometre range. Radiation damage was induced by synchrotron radiation microbeams of 5, 1 and 0.3?μm size with ~0.1?nm wavelength in B-type potato, Canna edulis and Phajus grandifolius starch granules. A total loss of crystallinity of granules immersed in water was found at a dose of ~1.3?photons?nm(-3). The temperature dependence of radiation damage suggests that primary radiation damage prevails up to about 120?K while secondary radiation damage becomes effective at higher temperatures. Primary radiation damage remains confined to the beam track at 100?K. Propagation of radiation damage beyond the beam track at room temperature is assumed to be due to reactive species generated principally by water radiolysis induced by photoelectrons. By careful dose selection during data collection, raster scans with 500?nm step-resolution could be performed for granules immersed in water. 相似文献