A simple yet more accurate model to calculate solar radiative flux in the inhomogeneous atmosphere

A simple yet more accurate semiempirical model is developed to calculate solar radiative flux in the optically inhomogeneous atmosphere. In the model a parameterized expression of spherical reflectance and transmitance of the atmosphere is confirmed, and the weighted single scatter albedo and weighted asymmetric factor are introduced to fit four empirical correction factors responsible for radiative fluxes in the inhomogeneous atmosphere. For both clean and turbid models, there are 120060 sets of radiative flux simulations for accuracy checks of the model, which cover 0-50 cloud optical depths, 0-0.8 surface reflectance, Junge and Log-normal aerosol size distributions, and 0-0.05 imaginary parts of aerosol refractive indexes. In case of the homogeneous atmosphere, standard errors of the 120060 upward fluxes from the present model are 1.08% and 1.04% for clean and turbid aerosol models, respectively; and those of the downward fluxes are 4.12% and 3.31%. In case of the inhomogeneous atmosphere, standard errors of the upw ard fluxes from the present model are 3.01% and 3.48% for clean and turbid aerosol models.respectively; and those of the downward fluxes are 4.54% and 4.89%, showing a much better accuracy than the results calculated by using an assumption of the homogeneous atmosphere.     

Deep array electromagnetic sounding on the Baltic Shield: External excitation model and implications for upper mantle conductivity studies

The BEAR array of simultaneous electromagnetic (EM) observations probes the deep crustal and upper mantle conductivity structure of the Baltic Shield searching for the lithosphere–asthenosphere boundary beneath. The adequate interpretation of the results of this unique high latitude natural field EM sounding requires proper understanding of the actual external excitation conditions because conventionally used plane wave model assumptions may be substantially violated in the vicinity of inhomogeneous polar sources. The paper presents an overview of the morphology and statistics of source distortions in the BEAR EM field transfer functions (TF) and the ways of their suppression. The stability of the final TF estimates obtained with the exclusion of intensive non-stationary auroral effects is further justified. The external excitation model effective for the whole BEAR observation period is inferred from the array distribution of the inter-station geomagnetic transfer functions. The model is supported by the results of polar ionosphere–magnetosphere current system studies, based on the simultaneous ground and satellite geomagnetic observations, and sets bounds for the “plane wave” approach in the BEAR data interpretation to avoid unfounded inferences on the upper mantle electrical properties. The signatures of the lithosphere–asthenospere boundary under Fennoscandia derived from the BEAR data are summarized and its resolution within the traditional plane wave interpretational paradigm is analysed assuming the presented external source pattern and estimated TF uncertainties caused by the source inhomogeneity.     

"05.6"东北暴雨中尺度对流系统研究Ⅰ:常规资料和卫星资料分析

应用常规气象资料与卫星资料相结合的办法,研究了2005年6月10日午后在黑龙江省中东部发生的暴雨中尺度对流系统(MCSs)的大尺度环流背景、大气层结演变特征、下垫面条件以及中尺度对流系统。结果表明:此次暴雨(简称“05.6”东北暴雨)是发生在高空槽东移加深过程中的一次对流天气过程。中尺度对流系统处于前倾疏散的高空槽槽前,高空辐散,低空辐合,为MCS发生提供了有利的大尺度动力条件。暴雨发生前对流层低层有西南—东北走向的湿舌,为暴雨提供了有利的水汽条件。高空干冷平流与低空的暖湿平流形成的差动平流,造成此处大气的层结不稳定度增强。此外,从地面接收到的太阳辐射能量分布情况来看,下垫面不均匀加热引起的热力环流是这次暴雨过程中尺度对流系统发生发展的一个重要的触发机制。研究地面中尺度切变线演变与此次暴雨对流系统发生发展的关系发现,切变线上对流强弱分布是不均匀的,其中在弧形切变线曲率最大处的对流最强,与沙兰河上游暴雨有关的对流云团就出现在这个地区。以上事实表明,地面中尺度切变线可能是此次暴雨发生发展的另一个关键因素,而造成切变线上对流发展不均匀的原因可能和切变线走向与环境风场的配置有较大关系。     

电场垂直入射面的非均匀电磁波在导电媒质界面的类全反射横向偏移

利用电磁波在导电媒质界面反射系数的附加相角，导出了电场垂直于入射面的非均匀电磁波在导电介质界面的类全反射横向偏移，并对横向偏移进行了相关计算，绘出了横向偏移随入射角的变化曲线. 结果表明：入射角在相移常数临界角、衰减常数临界角和90°处，横向偏移曲线存在三个间断点. 当入射角等于这三个角时，横向偏移为无穷大，即电磁波将沿界面传播；当入射角在这三个角附近时，横向偏移变得非常大.     

地质雷达在三峡工程施工阶段应用研究

长江三峡工程施工阶段面临众多复杂的工程地质问题和施工技术难题。寻找一种快捷、高分辨无损探测手段查明施工中出现的隐蔽的地质缺陷或质量问题,无疑对施工进度和施工质量起到保证作用,采用地质雷达手段,探明了开挖过程中花岗岩体不均匀风化分布范围：圈定出较大断层及风化夹层的延伸范围和产状;并进行了专用高速公路质量检查等,文章结合三个实例介绍应用情况。经现场验证,探测结果与实际情况吻合,应用效果显著。     

波向对变风向响应理论模式的检验

基于文圣常等提出的风浪成长标准曲线和普遍采用的无因次方法,将理论导出的波向对变风向响应模式表达成在资料处理中常采用的无因次形式,分别用Holthuijsen等的观测结果和Gao等用WAM模式数值计算的结果进行检验和比较.结果表明,所提出的理论结果较其他计算结果更与实测值相吻合.     

Generation and propagation of the ULF planetary-scale electromagnetic wavy structures in the ionosphere

In the present article, the results of theoretical investigation of the dynamics of generation and propagation of planetary (with wavelength 10³ km and more) ultra-low frequency (ULF) electromagnetic wave structures in the dissipative ionosphere are given. The physical mechanism of generation of the planetary electromagnetic waves is proposed. It is established, that the global factor, acting permanently in the ionosphere—inhomogeneity (latitude variation) of the geomagnetic field and angular velocity of the earth's rotation—generates the fast and slow planetary ULF electromagnetic waves. The waves propagate along the parallels to the east as well as to the west. In E-region the fast waves have phase velocities (2-20) km s⁻¹and frequencies (10⁻¹-10⁻⁴) s⁻¹; the slow waves propagate with local winds velocities and have frequencies (10⁻⁴-10⁻⁶) s⁻¹. In F-region the fast ULF electromagnetic waves propagate with phase velocities tens-hundreds km s⁻¹ and their frequencies are in the range of (10-10⁻³) s⁻¹. The slow mode is produced by the dynamoelectric field, it represents a generalization of the ordinary Rossby-type waves in the rotating ionosphere and is caused by the Hall effect in the E-layer. The fast disturbances are the new modes, which are associated with oscillations of the ionospheric electrons frozen in the geomagnetic field and are connected with the large-scale internal vortical electric field generation in the ionosphere. The large-scale waves are weakly damped. The features and the parameters of the theoretically investigated electromagnetic wave structures agree with those of large-scale ULF midlatitude long-period oscillations (MLO) and magnetoionospheric wave perturbations (MIWP), observed experimentally in the ionosphere. It is established, that because of relevance of Coriolis and electromagnetic forces, generation of slow planetary electromagnetic waves at the fixed latitude in the ionosphere can give rise to the reverse of local wind structures and to the direction change of general ionospheric circulation. It is considered one more class of the waves, called as the slow magnetohydrodinamic (MHD) waves, on which inhomogeneity of the Coriolis and Ampere forces do not influence. These waves appear as an admixture of the slow Alfven- and whistler-type perturbations. The waves generate the geomagnetic field from several tens to several hundreds nT and more. Nonlinear interaction of the considered waves with the local ionospheric zonal shear winds is studied. It is established, that planetary ULF electromagnetic waves, at their interaction with the local shear winds, can self-localize in the form of nonlinear solitary vortices, moving along the latitude circles westward as well as eastward with velocity, different from phase velocity of corresponding linear waves. The vortices are weakly damped and long lived. They cause the geomagnetic pulsations stronger than the linear waves by one order. The vortex structures transfer the trapped particles of medium and also energy and heat. That is why such nonlinear vortex structures can be the structural elements of strong macroturbulence of the ionosphere.     

辽宁省地下水硝酸盐污染成因分析及其防治对策探讨

硝酸盐的含量直接影响地下水的环境质量，对人及动植物均有不同程度危害。通过辽宁省地下水硝酸盐监测资料及大量试验资料分析，对硝酸盐污染因素及其成因类型进行了系统研究，进而提出综合防治措施。     

Reflection and transmission of attenuated waves at the boundary between two dissimilar poroelastic solids saturated with two immiscible viscous fluids

The phenomenon of reflection and transmission of plane harmonic waves at the plane interface between two dissimilar poroelastic solids saturated with two immiscible viscous fluids is investigated. Both porous media are considered dissipative due to the presence of viscosity in pore‐fluids. Four attenuated (three dilatational and one shear) waves propagate in such a dissipative porous medium. A finite non‐dimensional parameter is used to define the effective connections between the surface‐pores of two media at their common interface. Another finite parameter represents the gas‐share in the saturation of pores. An attenuated wave in a dissipative medium is described through the specification of directions of propagation and maximum attenuation. A general representation of an attenuated wave is defined through its inhomogeneous propagation, i.e., different directions for propagation and attenuation. Incidence of an inhomogeneous wave is considered at the interface between two dissipative porous solids. This results in four reflected and four transmitted inhomogeneous waves. Expressions are derived for the partition of incident energy among the reflected and transmitted waves. Numerical examples are studied to determine the effects of saturating pore fluid, frequency, surface‐pore connections and wave inhomogeneity on the strengths of reflected and transmitted waves. Interaction energy due to the interference of different (inhomogeneous) waves is calculated in both the dissipative porous media to verify the conservation of incident energy.     

基于耦合标势与矢势的有限体积法模拟非均匀各向异性地层中多分量感应测井三维响应

为快速有效地研究、考察各向异性地层条件下多分量感应测井的响应特征,本文利用电场标势与矢势的有限体积法研制出三维频率域电磁场响应的数值模拟算法,克服由低频发射或高阻地层产生的低感应数问题,有效提高了三维电磁数值模拟算法的应用范围和计算效率.首先利用电场的标势与矢势将Maxwell方程转化为满足库仑规范条件的耦合势Helmholtz方程,以Yee氏交错非均匀网格中不同位置上的节点为中心建立四种控制体积单元,通过对控制体积单元中电磁场与电导率的积分平均实现耦合势方程和磁偶极子旋度的离散,并得到一个对角占优的大型稀疏复线性代数方程组,然后,通过不完全LU分解预处理和稳定双共轭梯度法快速求解离散方程.数值结果证明了该算法的有效性,并进一步考查了仪器偏心、倾斜井、垂直裂缝等复杂条件下多分量感应的响应特征.