雾对光偏振态影响的实验研究     

LIU Rui-fang  刘瑞芳  王振会  肖韶荣  徐娟 《南京气象学院学报》2006,29(6):815-818

测量了不同人土雾浓度下垂直偏振入射光的透射光强。利用实验数据，分析了垂直、平行方向上透射光强的变化趋势。得出平行偏振分量透射光强大致呈指数下降的趋势，垂直偏振分量透射光强先略微上升而后下降。由退偏振度随雾浓度的变化讨论了退偏产生的原因，指出雾浓度较低时，雾滴可近似视为球形。基于光的偏振特性，从理论上分析并计算得到光在雾中传输时透射、散射光强。实验结果对研究光在雾中传输及分析大气中雾对透射光偏振态的影响有一定的参考价值。  相似文献   

Performance of a Reconfigured Atmospheric General Circulation Model at Low Resolution   总被引：3，自引：2，他引：3  

WEN Xinyu  ZHOU Tianjun  WANG Shaowu  WANG Bin  WAN Hui  LI Jian 《大气科学进展》2007,24(4):712-728

Paleoclimate simulations usually require model runs over a very long time.The fast integration version of a state-of-the-art general circulation model (GCM),which shares the same physical and dynamical processes but with reduced horizontal resolution and increased time step,is usually developed.In this study,we configure a fast version of an atmospheric GCM (AGCM),the Grid Atmospheric Model of IAP/LASG (Institute of Atmospheric Physics/State Key Laboratory of Numerical Modeling for Atmospheric Sciences and Geophysical Fluid Dynamics),at low resolution (GAMIL-L,hereafter),and compare the simulation results with the NCEP/NCAR reanalysis and other data to examine its performance.GAMIL-L,which is derived from the original GAMIL,is a finite difference AGCM with 72×40 grids in longitude and latitude and 26 vertical levels.To validate the simulated climatology and variability,two runs were achieved.One was a 60-year control run with fixed climatological monthly sea surface temperature (SST) forcing,and the other was a 50-yr (1950-2000) integration with observational time-varying monthly SST forcing.Comparisons between these two cases and the reanalysis,including intra-seasonal and inter-annual variability are also presented.In addition,the differences between GAMIL-L and the original version of GAMIL are also investigated. The results show that GAMIL-L can capture most of the large-scale dynamical features of the atmosphere, especially in the tropics and mid latitudes,although a few deficiencies exist,such as the underestimated Hadley cell and thereby the weak strength of the Asia summer monsoon.However,the simulated mean states over high latitudes,especially over the polar regions,are not acceptable.Apart from dynamics,the thermodynamic features mainly depend upon the physical parameterization schemes.Since the physical package of GAMIL-L is exactly the same as the original high-resolution version of GAMIL,in which the NCAR Community Atmosphere Model (CAM2) physical package was used,there are only small differences between them in the precipitation and temperature fields.Because our goal is to develop a fast-running AGCM and employ it in the coupled climate system model of IAP/LASG for paleoclimate studies such as ENSO and Australia-Asia monsoon,particular attention has been paid to the model performances in the tropics.More model validations,such as those ran for the Southern Oscillation and South Asia monsoon, indicate that GAMIL-L is reasonably competent and valuable in this regard.  相似文献   

The Atmospheric Oxidation of the HS Radical: Reaction with NO2     

Stella M. Resende 《Journal of Atmospheric Chemistry》2007,56(1):21-32

The atmospheric reaction between HS and NO₂ was theoretically investigated at 298 K and 1 atm of pressure. Our results show that the first reaction step will lead to the formation of HSNO₂ or HSONO, spontaneously and exothermically. HSONO easily decomposes into HSO + NO. On the other hand, HSNO₂ can hardly dissociate in the reactants, and its isomerization to other adducts is much hindered. Production of HNO + SO and SNO + OH was found to be unfavorable. Thus, the main products would be HSO + NO and HSNO₂, and new investigations focusing on the atmospheric fate of HSNO₂ are suggested. A general discussion of the fate of HS under atmospheric conditions is presented. Recent investigations indicate that NO₂, O₂ and N₂O should be the most important oxidants of HS, while the O₃ influence will not be significant.  相似文献   

Planetary waves in coupling the lower and upper atmosphere   总被引：1，自引：1，他引：1  

A.I. Pogoreltsev  A.A. Vlasov  K. Frhlich  Ch. Jacobi 《Journal of Atmospheric and Solar》2007,69(17-18):2083

The purpose of the paper is to answer the question if planetary waves (PW) are capable of propagating into the thermosphere. First the simplest vertical structure equation of the classic tidal theory accounting for a realistic vertical temperature profile is considered. Analysis and simulation show that the well-known normal atmospheric modes (NM), which are trapped in the lower and middle atmosphere, exhibit a wave-like vertical structure with a large vertical wavelength in the thermosphere. Moreover, the reflection of these modes from the vertical temperature gradient in the lower thermosphere causes appearance of the wave-energy upward flux in the middle atmosphere, and in a linearized formulation this flux is constant above the source region. To investigate a possibility of the NM forcing by stratospheric vacillations and to consider the propagation of different PW up to the heights of the upper thermosphere, a set of runs with a mechanistic Middle and Upper Atmosphere Model has been performed. The results of the simulation show that quasi-stationary and longer-period PW are not able to penetrate into the thermosphere. The shorter-period NM and ultra-fast Kelvin wave propagate up to the heights of the lower thermosphere. However, above about 150 km they are strongly suppressed by dissipative processes. The role of the secondary waves (nonmigrating tides) arising from nonlinear interaction between the primary migrating tides and quasi-stationary PW is discussed. We conclude that PW are not capable of propagating directly up to the heights of the ionospheric F2 region. It is suggested that other physical processes (for instance, the electrostatic field perturbations) have to be taken into account to explain the observed PW-like structures in ionospheric parameters.  相似文献   

南京地区大气边界层晴空回波研究   总被引：10，自引：1，他引：10  

魏鸣  秦学  王啸华  蒋维楣 《南京气象学院学报》2007,30(6):736-744

以2005年6月23日南京多普勒雷达探测的晴空回波演变为例,分析了回波反射率与径向速度从夜间至上午的演变规律,利用实际的气象观测资料,对比了折射指数、地面温度、露点温度、水汽压和气压与回波强度的相关性,进一步探讨了边界层晴空回波与湍流混合特性之间的关系.研究表明:夜间大气的温、压、湿梯度使湍流出现,但湍流未充分混合使梯度维持,并导致折射指数的梯度增加,出现晴空回波;白天升温后湍流的增强使近地层大气充分混合,温、压、湿梯度减弱导致折射指数梯度减小,回波减弱消失.  相似文献   

An immersed boundary method for compressible multiphase flows: application to the dynamics of pyroclastic density currents     

Mattia de’ Michieli Vitturi  Tomaso Esposti Ongaro  Augusto Neri  Maria Vittoria Salvetti  François Beux 《Computational Geosciences》2007,11(3):183-198

  相似文献   

Product study of the reaction of OH radicals with isoprene in the atmosphere simulation chamber SAPHIR     

M. Karl  H.-P. Dorn  F. Holland  R. Koppmann  D. Poppe  L. Rupp  A. Schaub  A. Wahner 《Journal of Atmospheric Chemistry》2006,55(2):167-187

Atmospheric oxidation of isoprene and its oxidation products methacrolein (MACR) and methyl vinyl ketone (MVK) have an important impact on the photochemical activity in the boundary layer, in particular in forested areas. The oxidation of isoprene by OH radicals was investigated in chamber experiments conducted under tropospheric conditions in the atmosphere simulation chamber SAPHIR at the Research Center Jülich. The aim was to determine the product yield of MVK and MACR in the OH-induced isoprene oxidation and the rate constant of their reaction with OH under real atmospheric conditions. The recently published updated degradation scheme for isoprene from Geiger et al. (2003) was used to determine rate constants and product yields. The fractional yields in the isoprene peroxy radical reaction with NO were found to be 0.41±0.03 for MVK and 0.27±0.03 for MACR. The rate coefficient for MACR with OH was found to be in very good agreement with the recommended value of IUPAC Atkinson (Atkinson et al., 2005). while the rate coefficient for MVK with OH was 27% lower.  相似文献   

北京市砂石坑对环境的影响     

任凯珍 《城市地质》2007,2(1):39-41

本文主要从砂石坑对北京地区大气质量、地下水和土地三方面,阐述了砂石坑对环境的影响,并提出了治理建议。  相似文献   

Fairweather atmospheric electricity at Antarctica during local summer as observed from Indian station,Maitri     

C. Panneerselvam  C. Selvaraj  K. Jeeva  K. U. Nair  C. P. Anilkumar  S. Gurubaran 《Journal of Earth System Science》2007,116(3):179-186

Surface measurements of the atmospheric electrical parameters like Maxwell current, electric field and conductivity studied at the Indian station, Maitri (70.75° S, 11.75° E, 117 m above mean sea level), Antarctica, during austral summer have been analyzed for the years 2001 to 2004. A total of 69 days were selected which satisfied the ‘fairweather’ conditions, i.e., days with absence of high winds, drifting or falling snow, clouds, and fog effects. The diurnal variation curve of electric field and vertical current averaged for 69 fairweather days is a single periodic with a minimum at 03:00 UT and a maximum near 19:00 UT, which is very similar to the Carnegie curve. The correlation coefficient between these measured parameters has a high value (more than 0.9) for all the days. During fairweather days the measured current and field variations are similar and hence it is clear that the conductivity is more or less stable. During magnetically disturbed days, the dawn-dusk potential drop has clear influences on the diurnal variation and it modifies the conductivity. Apart from the day-to-day variation in low latitude thunderstorm activity, there are diurnal, seasonal, inter-annual variations in the electric potential and the currents, as well as solar influences on the measured parameters. This study will help us to examine the impact of solar and geophysical phenomena like solar flares, geomagnetic storms and substorms on the global electric circuit.  相似文献   

Theorem of turbulent intensity and macroscopic mechanism of the turbulence development     

Hu YinQiao  Chen JinBei  Zuo HongChao 《中国科学D辑(英文版)》2007,50(5):789-800

Turbulence is one of the most common nature phenomena in everyday experience, but that is not adequately understood yet. This article reviews the history and present state of development of the turbulence theory and indicates the necessity to probe into the turbulent features and mechanism with the different methods at different levels. Therefore this article proves a theorem of turbulent transpor- tation and a theorem of turbulent intensity by using the theory of the nonequilibrium thermodynamics, and that the Reynolds turbulence and the Rayleigh-Bénard turbulence are united in the theorems of the turbulent intensity and the turbulent transportation. The macroscopic cause of the development of fluid turbulence is a result from shearing effect of the velocity together with the temperature, which is also the macroscopic cause of the stretch and fold of trajectory in the phase space of turbulent field. And it is proved by the observed data of atmosphere that the phenomenological coefficient of turbulent in- tensity is not only a function of the velocity shear but also a function of temperature shear, viz the sta- bility of temperature stratification, in the atmosphere. Accordingly, authenticity of the theorem, which is proved by the theory of nonequilibrium thermodynamics, of turbulent intensity is testified by the facts of observational experiment.  相似文献