Efficient radiative recombination of multinode-type excitons up to room temperature in CuCl thin films

We report the observation of anomalous temperature dependences of degenerate four-wave mixing spectra in CuCl thin films with high crystalline quality. The observed temperature dependence is in good agreement with the phase-decay-constant dependence of calculated induced-polarization spectrum. An excitonic state with large radiative width can be observed at high temperatures as superradiance is faster than the dephasing process. We succeeded in observing the DFWM signal up to room temperature based on the extremely large radiative width peculiar to the thickness region beyond the long-wavelength approximation regime.     

Influence of surface roughness on the reflective properties of snow

In this paper the influence of 3D effect on snow reflection function (SRF) and albedo is studied in the framework of the stochastic radiative transfer theory. In particular, the corresponding equations for the averaged intensity of reflected light are solved for the ensemble of realizations of the stochastic field κ(r), describing the distribution of 3D elements on the flat semi-infinite snow layer (SISL). The reflection from the underlying SISL is modeled using the solution of the 1D radiative transfer equation. The corresponding look-up tables were compiled beforehand and used in the simulation process. In accordance with the previous studies, it was found that the albedo of snow layer is reduced (in particular, in the infrared region), if 3D effects are taken into account. There is no such a reduction, if light absorption in snow is absent. The 3D effects may increase or decrease SRF depending on the sastrugi fraction and illumination/observation conditions.     

Cloud 3D effects on broadband heating rate profiles: I. Model simulation

Solar broadband heating directly drives the atmospheric and ocean circulations, and is largely determined by cloud spatial 3-diminesional (3D) structures. To study the cloud 3D effects on radiation, a 3D broadband Monte-Carlo radiative transfer model, along with an Independent Pixel/Column Approximation (IPA) method, is used to simulate radiation and heating rate of three typical cloud fields generated by cloud resolving models (CRM). A quantitative and statistical estimation of cloud 3D effects has been developed to investigate the impact of cloud 3D structures on both heating rate strength, STD_Bias, and vertical distribution, CorrCoef. The cloud 3D structures affect some clouds more in heating rate strength and others more in vertical distribution. It is crucial to use the combination of CorrCoef and STD_Bias for better quantitative evaluation of the 3D effects. Furthermore, there is no simple way to define a critical resolution (or average radius), within which the IPA heating rate profiles closely represent the true 3D heating rate profiles. The critical radius (or resolution) strongly depends on solar incident angle as well as cloud vertical distribution. Also, the critical radii for clear-sky columns are larger than for cloudy columns, although the corresponding STD_Bias for clear-sky columns are smaller than for cloudy columns. Analysis based on two different statistical average methods illustrates that the cloud 3D effects due to the dimensionality difference between the 3D clouds (circle average) and 2D clouds (line average) significantly impact on the heating rate profiles.     

混浊大气介质调制传递函数的一般特征

基于混浊介质的调制传递函数(MTF)和在各向同性漫射光源照射下平行平面混浊介质出射光强度分布之间的等效原理,利用辐射传输算法DISORT数值计算了几种典型的均匀大气混浊介质的MTF,获得了整个空间频域内MTF的一般特征.结果显示,大气介质的MTF不但依赖于介质的光学厚度(散射和吸收),也依赖于介质的散射相函数.给出了大...     

非弹性散射对水体遥感反射率影响的数值模拟

基于矩阵算法建立了一个可用于模拟水体非弹性散射过程的水体辐射传输数值模型.该模型采用单个均匀介质层中辐射能量随深度增大而呈指数衰减的假设,将非弹性散射作为源矩阵算子引入到矩阵算法当中进行解算.通过Mobley水体辐射传输标准问题7的验证以及与Hydrolight 5.0结果的比较,说明该模型对多次散射和非弹性散射的处理...     

辐射传输的格子Boltzmann模拟

辐射动力学理论是描述辐射传输是重要手段,基于此,本文建立了辐射能和辐射动量守恒方程,并基于Chapman-Enskog多尺度展开方法实现了从辐射传输Boltzmann方程到宏观方程的推导,进而建立了适于一维辐射传输的2分量格子Boltzmann模型。数值结果与精确解吻合较好,表明本文提出的LBM方法具有很好的准确性和稳...     

量纲分析法求解辐射热传导自相似解

通过量纲分析,将辐射流体方程简化为一阶常微分方程组的形式,进而结合数值计算求得热波烧蚀自相似解。流体方程涉及的内能、状态方程表达式采用依赖于温度、密度两个参量的形式,且参数可调,适用性较广。源边界条件可为恒温、恒流、恒压、常密等情况。以恒温源为例,给出了X射线加热Au壁时烧蚀质量与烧蚀压的定标关系,与文献结果及MULTI辐射流体程序计算结果吻合较好。

     

海洋水色水温扫描仪精确大气漫射透射比计算

海洋水色水温扫描仪(COCTS)是中国海洋水色系列卫星上的主遥感器,主要用于探测我国及全球部分海域的海洋水色和水温环境信息.大气漫射透射比计算是COCTS大气校正的必需过程,直接影响COCTS大气校正和水色信息反演的精度.提出了基于加倍法解大气-海洋耦合矢量辐射传输方程的大气漫射透射比精确计算方法,通过与SeaWiFS精确大气漫射透射比查找表计算结果的比较,结果表明计算相对误差小于1.5%,而当观测天顶角小于60°时,计算相对误差小于0.5%,可以用来生成COCTS的精确大气漫射透射比查找表.在此基础上,生成了专门针对COCTS的精确大气漫射透射比查找表.     

间接驱动冷冻双壳层点火靶的设计和分析

双壳层靶中,由于燃料被高Z壳层包裹,其点火方式要求燃料整体点火,不同于单壳层中心热斑点火。结合点火条件和对于其中物理过程的认识,设计了间接驱动的冷冻双壳层点火靶。利用冷冻的氘氚（DT）燃料,可适当提高双壳层靶的燃料装量,获得和NIF装置条件下中心热斑点火靶相当的放能。间接驱动下,X射线烧蚀并驱动外壳层碰撞内壳层,把能量传递给内壳层,进而压缩和点燃冷冻的DT燃料。壳层碰撞过程是能量传递的关键,通过调整内外壳层的质量比,提高了碰撞效率,相应地降低了靶丸点火的能量需求。一维数值模拟分析了该点火靶的内爆过程及定性分析了其中的流体力学不稳定性。同时,也指出了泡沫中形成的辐射冲击波对内壳层的预热效应,即辐射冲击波的致稳效应,能够很好地抑制内壳层外界面处的不稳定性发展,进而会减弱高Z内壳层和燃料的混合。     

辐射输运菱形差分SN方程的扩散综合加速方法

讨论辐射输运菱形差分S_N方程的源迭代加速方法,在一维情形下给出与输运算子离散相容的线性多频灰体加速计算格式.数值算例表明该加速算法是健壮有效的.