沙质海岸强浪作用下沿岸输沙问题研究   总被引：1，自引：0，他引：1  

王玉海 《海洋工程》2008,26(4)

在沙质海岸上修建导流堤、丁坝等会引起局部海域水沙动力条件的改变和海床冲淤调整,因此准确预测沿岸输沙率是海岸工程建设前进行优化设计的基础条件之一.首先构建了刻画高强度推移质输沙过程中固-液混合体运动的理论模型,通过寻求模型的特解并推导成1D沿岸输沙率公式.该公式适宜计算强浪作用下的推移质输沙率,已得到了大型波浪水槽、往复流水道和海滩现场实测输沙率资料的良好验证.通过与物理模型试验实测输沙量结果的比较,进一步表明该公式能够较好地预测沙质海岸在寒潮大风浪(或台风浪)作用下的高强度输沙量(骤淤量).  相似文献   

全球纬向平均的海气耦合一维模式分析     

唐佑民 《成都信息工程学院学报》1991,(1)

本文从能量平衡角度,考虑海气相互作用和纬向间的差异,设计了一个纬向平均的海气耦合一维模式,进行了模式平衡态求解、敏感性试验以及随机分析。并对模式部分计算结果进行了与实测资料的比较,验证了模式的合理性和可信性。  相似文献   

NUMERICAL MODELING OF CUMULUS CLOUD CHEMISTRY—PART Ⅰ.MODEL DEVELOPMENT     

赵春生  秦瑜 《Acta Meteorologica Sinica》1996,(3)

A one-dimensional cumulus cloud chemistry model(1CCCM)is developed to simulate cloudphysical processes and chemical processes during the evolution of a convective cloud.The cloudphysical submodel includes a detailed microphysical parameterized scheme of 20 processes.Thechemistry submodel is composed of three parts:gas phase chemistry,aqueous phase chemistry andscavenging of soluble gases.The gas phase reaction mechanism contains 85 reactions among 45species including 13 organics.The aqueous phase reaction mechanism contains 54 reactions among40 species and 12 ion equilibria.Mass of 19 gases is transported between the gas phase and theaqueous phase.With this model,studies may be made to analyze the interactions among processesduring lifetime of a cumulus cloud.  相似文献   

舟山本岛北部灌门水道及邻近海域潮波特性初步研究   总被引：1，自引：0，他引：1  

任剑波  羊天柱 《海洋工程》2008,26(1):77-83

依据2004年在舟山灌门水道及邻近海域获取的同步潮位和潮流资料,对该海域的潮波特性进行了统计和分析,并对分析过程中发现的主要半日分潮经过灌门水道时振幅有较大幅度减小的现象进行了初步研究,认为截面积急剧变化的水道,潮波势能向动能的转换是产生主要半日分潮振幅减小的一个重要因素。这一结论或许有助于解释M2分潮波通过舟山群岛海域振幅明显减小的现象。  相似文献   

Use of the Geometric Elements in Numerical Simulations     

Stéfan Renner  Bruno Sicardy 《Celestial Mechanics and Dynamical Astronomy》2006,94(2):237-248

We derive the transformations to convert the state vector in cartesian coordinates into geometric orbital elements (and conversely the geometric elements into the state vector) for a test particle moving around an oblate planet. These transformations arise from the epicyclic theory and are accurate to second order in eccentricity and inclination. This paper is written to be directly used for computational purposes, such as the numerical study of ring dynamics.  相似文献   

Lyman α radiative transfer in a multiphase medium     

Matthew Hansen  S. Peng Oh 《Monthly notices of the Royal Astronomical Society》2006,367(3):979-1002

Hydrogen Lyman α (Lyα) is our primary emission-line window into high-redshift galaxies. Despite an extensive literature, Lyα radiative transfer in the most realistic case of a dusty, multiphase medium has received surprisingly little detailed theoretical attention. We investigate Lyα resonant scattering through an ensemble of dusty, moving, optically thick gas clumps. We treat each clump as a scattering particle and use Monte Carlo simulations of surface scattering to quantify continuum and Lyα surface scattering angles, absorption probabilities, and frequency redistribution, as a function of the gas dust content. This atomistic approach speeds up the simulations by many orders of magnitude, making possible calculations which are otherwise intractable. Our fitting formulae can be readily adapted for fast radiative transfer in numerical simulations. With these surface scattering results, we develop an analytic framework for estimating escape fractions and line widths as a function of gas geometry, motion, and dust content. Our simple analytic model shows good agreement with full Monte Carlo simulations. We show that the key geometric parameter is the average number of surface scatters for escape in the absence of absorption,     , and we provide fitting formulae for several geometries of astrophysical interest. We consider the following two interesting applications. (i) Equivalent widths ( EWs ). Lyα can preferentially escape from a dusty multiphase interstellar medium if most of the dust lies in cold neutral clouds, which Lyα photons cannot penetrate. This might explain the anomalously high EWs sometimes seen in high-redshift/submillimetre sources. (ii) Multiphase galactic outflows . We show the characteristic profile is asymmetric with a broad red tail, and relate the profile features to the outflow speed and gas geometry. Many future applications are envisaged.  相似文献   

X-ray pre-ionization powered by accretion on the first black holes – II. Cosmological simulations and observational signatures     

Massimo Ricotti  Jeremiah P. Ostriker  Nickolay Y. Gnedin 《Monthly notices of the Royal Astronomical Society》2005,357(1):207-219

  相似文献   

Galaxy clustering and dark energy     

Dipak Munshi  Cristiano Porciani  Yun Wang 《Monthly notices of the Royal Astronomical Society》2004,349(1):281-290

  相似文献   

Error analysis of quadratic power spectrum estimates for cosmic microwave background polarization: sampling covariance     

Anthony Challinor  Gayoung Chon 《Monthly notices of the Royal Astronomical Society》2005,360(2):509-532

  相似文献   

Toy stars in one dimension     

J. J. Monaghan  D. J. Price 《Monthly notices of the Royal Astronomical Society》2004,350(4):1449-1456

  相似文献