沙尘气溶胶粒子群的散射和偏振特性

根据Mie散射理论,以对数正态分布函数描述沙尘气溶胶粒子群的粒径尺度分布,计算了沙尘气溶胶粒子群在0.2～40μm波段间对太阳短波辐射和地球大气长波辐射的单次散射反照率、散射相矩阵函数,揭示了不同相对湿度时,沙尘粒子群对入射辐射的散射和偏振的特征.结果表明,沙尘粒子群的单次散射反照率随着入射波长的增加有较大起伏,不同相对湿度条件下,变化趋势基本一致;在可见光、近红外波段单次散射反照率随湿度增加而变大,湿度95％时非常接近于1;大于10μm的热红外波段单次散射反照率随相对湿度增加而减小,具有较强的吸收辐射能力.散射辐射强度受湿度影响较小,随散射角的增加呈现先减小后增大的趋势,且增大的趋势随着波长的增加而减弱;不同波段上,线偏振和圆偏振随散射角和相对湿度变化存在差异;在前向和后向仅对入射辐射为圆偏振辐射产生圆偏振散射;散射光的偏振特性及其湿度差异主要表现在后向散射区,多以拱形形式体现.拱顶峰值散射角位置存在差异,且峰值散射角随相对湿度的降低向后向漂移.     

大气粒子散射特性及其对空间偏振分布的影响

利用米氏散射理论分析O2,N2,CO2,水滴和气溶胶等粒子的散射与偏振特性,通过随机传输理论仿真不同粒子影响下的偏振分布,并与检测结果进行比对,对粒子散射特性及其对空间偏振特性分布的影响进行了系统的理论研究.计算了不同粒子的散射系数和吸收系数随尺寸和复折射率的变化规律,研究了典型气态分子和非气态粒子偏振度及散射光强随散...     

一种内混合气溶胶粒子模型光散射的等效性

以包含灰尘、黑碳和水三种成分的单分散内混合初次气溶胶为例,利用消光、吸收、散射效率因子和不对称因子,探讨了以等效折射率描述具有不同成分的内混合气溶胶粒子系统的适用性.结果表明,在尺度参数为0.1～25时不同半径比下,消光、吸收和散射效率因子的等效性较好,相对误差分别在3％、3％和4％以内;不对称因子的等效性相对稍差,相对误差在13％以内.当半径比a/b小于1/5,即内混合体中所含灰尘和黑碳较少时,等效折射率实部和虚部值基本可以确定,而不必考虑尺度参数的影响.用除散射相函数之外的其他光学量来等效时,较为容易找到等效的气溶胶粒子.     

单分散长椭球形气溶胶粒子的散射相函数研究

选取冰晶、沙尘和碳黑等典型气溶胶粒子为例, 应用T矩阵方法, 探讨了单分散长椭球形气溶胶粒子的散射相函数随纵横比、尺度参数和折射率的变化规律.折射率虚部为0时, 以纵横比为0.4的冰晶粒子和等表面积的球形冰晶粒子为例, 将两者的相函数比值ρ划分为5个数值区域: 1) 0°附近的前向散射ρ≈1, 2) 从5°左右到30°左右ρ>1, 3) 从30°～35°到80°～110°ρ<1, 4) 从80°～110°到150°～160°ρ1, 5) 160°以后ρ<1. 同等条件下, 由于折射率的变化, 沙尘粒子ρ<1对应的范围扩大至更大角度, 而ρ1和ρ<1对应的角度区域均相应减小, 而碳黑粒子的ρ1和ρ<1对应的角度区域则消失, ρ演变为3个数值区域.上述长椭球形粒子散射相函数的结论为气溶胶粒形检测和分析提供了理论依据.     

利用DDA方法计算大气气溶胶粒子光学特性

大气气溶胶是大气的重要组成部分,其光学特性是研究大气辐射传输特性的重要参量。本文基于DDA方法,对不同形状气溶胶粒子的光学特性进行计算,得到气溶胶粒子的消光因子、吸收因子随波长变化的数值结果。结合Muller散射矩阵,给出了气溶胶粒子散射强度和极化度的角分布,为研究大气辐射传输提供了有效的方法。     

取向比对圆柱状冰晶粒子光散射特性的影响

利用T矩阵方法研究卷云中圆柱状粒子取向比对散射特性的影响,计算了在小尺度范围内圆柱状冰晶粒子的散射特征量如散射相函数、消光效率因子、不对称因子及单次散射反照率,并将计算结果与等表面积、等体积及等效体积与投影面积比三种情况下的球形粒子的相应值进行了对比.结果表明:体积与投影面积比等效最接近真实值;取向比对不同尺度柱状粒子散射特性的影响存在相似性且有必要加以考虑;此外,发现等表面积、不同取向比粒子的散射相函数有一交点.     

气溶胶凝聚粒子散射特性的数值计算

利用Cluster-cluster aggregation (CCA)模型,模拟了由相同数目球形原始微粒凝聚而成的四种随机取向气溶胶凝聚粒子.根据物质的电结构,将气溶胶凝聚粒子离散为一系列偶极子,结合离散偶极子近似方法,在获得每一个偶极子的电偶极矩之后,数值计算了气溶胶凝聚粒子散射强度的角分布,并分析了散射强度随入射光入射角度和气溶胶凝聚粒子尺寸参数变化的规律.结果显示:当散射角较小时,气溶胶凝聚粒子取向和入射光的入射角度对散射强度影响不大,当散射角增大时,散射强度则明显依赖于气溶胶凝聚粒子取向和入射光的入射角度;对于不同尺寸参数的气溶胶凝聚粒子,在同一角度入射情况下,随尺寸参数的增加,气溶胶凝聚粒子的散射主要集中于前向散射.     

气溶胶凝聚粒子散射特性的数值计算

利用Cluster-cluster aggregation (CCA)模型,模拟了由相同数目球形原始微粒凝聚而成的四种随机取向气溶胶凝聚粒子．根据物质的电结构,将气溶胶凝聚粒子离散为一系列偶极子,结合离散偶极子近似方法,在获得每一个偶极子的电偶极矩之后,数值计算了气溶胶凝聚粒子散射强度的角分布,并分析了散射强度随入射光入射角度和气溶胶凝聚粒子尺寸参数变化的规律．结果显示：当散射角较小时,气溶胶凝聚粒子取向和入射光的入射角度对散射强度影响不大,当散射角增大时,散射强度则明显依赖于气溶胶凝聚粒子取向和入射光的入射角度;对于不同尺寸参数的气溶胶凝聚粒子,在同一角度入射情况下,随尺寸参数的增加,气溶胶凝聚粒子的散射主要集中于前向散射．     

Au粒子在不同基质中Mie散射特性的研究

根据Mie散射理论,给出了金属粒子的散射、消光和吸收截面以及散射场强度的计算公式,并数值计算了在λ=r=1μm时,金属Au粒子在五种不同的基质中的散射截面和散射光强,结果表明基质折射率越大散射特性越强。     

湿度影响下的气溶胶粒子的偏振特性

气溶胶散射特性对大气辐射和气候研究具有重要意义。为研究气溶胶在不同相对湿度下的散射特性,根据Mie散射理论建立了湿度偏振模型,在0.55μm的可见光下,分析比较了3种气溶胶的单粒子和粒子群在不同相对湿度下的偏振特性。结果表明,相对湿度变化对气溶胶偏振度有规律性的影响,尤其在120°~150°的后向散射角区域,3种粒子偏振度都随相对湿度的增大而增大,说明了部分后向散射角上散射光偏振度能有效反映气溶胶粒子随相对湿度变化的信息。     

Pure elastic resonance scattering of an obliquely incident plane acoustic wave by a submerged infinite cylinder

I.IntroductionTheResonanceScattcringThcory(RST)asanimportantmethodtoana1yzeacousticscat-teringofsubmergede1asticbodieswascxtcnsivelyuscdforcy1indrica1andspherica1geometries,inc1udingsolidstructuresandho11owoncs.RSTismain1yappliedtostudytheresonancescat-teringspcctra(oracousticspcctra)ofanc1astictargctcxcitedby'theinciderttacousticwavesoastOidentifythetargct.Tocxtracttheresonancescattcringspcctra,anappropriatebackgroundsuchasrigidbackgroundorsoftonemust-besubtractcd.Expcrimenta1ly,theReson…     

Visualization of the sound scattering by a cylinder

The schlieren method is applied to visualizing the sound scattering ofa cylinder immersed in the liquids.Images of the echoes,caused by normal andoblique incidence from a cylinder,are obtained for two kinds of liquids:(1)theliquid is composed of a transparent liquid;and(2)the liquid is composed of twonon-mixable transparent liquids.It is found experimentally that the echo canbe caused by the discontinaites in the shadow zone.This fact is utilized to dem-onstrate the locus of the helical surface wave creeping along the surface of thecylinder.For such cases the three-dimensional image can be described by thismethod and has not to use the system with special appliances and complexalgorithm.     

复合金属粒子散射强度分布的计算与分析

根据Mie散射理论,对金银复合粒子的散射强度和偏振度进行了数值计算与理论分析,得到了散射强度、偏振度与散射角、入射波长及核壳大小之间的关系。结果表明,入射波长越大,前向散射越强,易出现线偏振光;而核壳半径越大,背向散射越弱,易出现退偏振现象。该结论对金银复合材料光学特性方面的开发和应用提供理论参考。     

Scattering matrices for horizontally oriented ice crystals

Scattering matrices for horizontally oriented ice crystals are calculated with a code based on the geometric optics. The main physical regularities inherent to the scattering matrices are discussed. Degree of polarization of the scattered light is shown to be a qualitative criterion of number of photon trajectories that contribute effectively to the scattered light. The inverse scattering problem of retrieving aspect ratios of the horizontally oriented hexagonal ice plates from polarization of the scattered light in the bistatic sounding scheme has been proposed and discussed.     

随机粗糙柱面的激光散射特性研究

扩展面光源如太阳光与激光光源有明显的差异,因此它们照射到随机粗糙柱面后的散射特性也不同。利用随机面元模型,详细分析了刚性随机粗糙柱形表面的激光散射特点,建立了实用化的随机粗糙柱面激光散射理论模型,并给出了正入射时几种情况下的激光散射图像。结果表明,不管哪种情况,正入射时柱面的激光后向散射都很强,而偏离后向的激光散射分布与表面的粗糙度及照射光斑与柱面直径的关系等有关。     

随机粗糙柱面的激光散射特性研究

 扩展面光源如太阳光与激光光源有明显的差异,因此它们照射到随机粗糙柱面后的散射特性也不同。利用随机面元模型,详细分析了刚性随机粗糙柱形表面的激光散射特点,建立了实用化的随机粗糙柱面激光散射理论模型,并给出了正入射时几种情况下的激光散射图像。结果表明,不管哪种情况,正入射时柱面的激光后向散射都很强,而偏离后向的激光散射分布与表面的粗糙度及照射光斑与柱面直径的关系等有关。     

Vibrational spectra of high- and low-density amorphous ice,ice Ic,and ice Ih by neutron scattering

Abstract

The vibrational spectra of high- and low-density amorphous ice made ice Ic and Ice Ih have been obtained at 15 K using inelastic incoherent neutron scattering     

Gustav Mie and the scattering and absorption of light by particles: Historic developments and basics

Gustav Mie was a professor of physics with a strong background in mathematics. After moving to the University of Greifswald in North-Eastern Germany he became acquainted with colloids, and one of his PhD students investigated the scattering and attenuation of light by gold colloids experimentally. Mie used his previously acquired knowledge of the Maxwell equations and solutions of very similar problems in the literature to concisely treat the theoretical problem of scattering and absorption of light by a small absorbing sphere. He also presented many numerical examples which completely explained all the effects that had been observed until then. Since all calculations were done by hand, Mie had to limit his theoretical results to three terms in infinite expansions, thus he only could treat particles smaller than 200 nm at visible wavelengths. Mie's paper had remained hardly noticed for the next 50 years, most likely because of the lack of computers. It experienced a revival later and up to now it has been referenced more than 4000 times, owing to the widespread use of Mie's approach in sciences such as astronomy, meteorology, fluid dynamics and many others.Gustav Mie did not consider his work on scattering of light by small particles as very important, since he just tried to explain the effects which his students had observed. He concentrated on hot topics in theoretic physics, e.g., the theory of matter. He wrote several textbooks, e.g., on relativity, gravitation theory, and electromagnetism, and all of them had run into several editions.     

Light scattering by “soft” parallelepipeds of arbitrary size

A generalisation of the earlier proposed method of light scattering analysis based on the expansion into a spatial spectrum with the aid of the sampling Kotel'nikov-Shannon functions is done. This method has been applied so far only to the case of small particles in the frame of Rayleigh-Gans approximation. Being generalised, the method could be applied to the analysis of scattering from optically “soft” particles of arbitrary dimension and shape in the approach equivalent to that of WKB. The case of scattering from a parallelepiped is analysed by this method. The indicatrices and the integral cross-sections are obtained and their features discussed.     

New studies on scattering properties of different kinds of soot and carbon-black

New polarization and brightness curves as a function of scattering angle are studied at λ=632.8 and 543.5 nm using PROGRA2 instruments (Propriétés Optiques des Grains Astronomiques et Atmosphériques) for four different kinds of soot and for two samples of carbon-black levitating in the cloud. The soot samples are also studied on the deposited surface. Two of the soot samples are issued from incomplete combustion of Toluene liquid solvent under two different combustion conditions. Two others are issued from a solid polymer. Polymethyl Methacrylate or PMMA under two different combustion conditions. These new studies are done using new more sensitive cameras than previous ones, allowing darker agglomerates to be detected.