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质量守恒律在国家气候中心气候谱模式中的应用 总被引：4，自引：2，他引：2
概述了在国家气侯中心气侯谱模式中,引入参考大气和大气质量守恒律,消除了原模式由于模式大气质量不守恒引起的气候漂移计算误差,改进了气候模拟,提高了预报精度. 相似文献
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本模式是原北半球七层原始方程谱模式的发展，它包含了较完整的物理过程。模式的方程组求解方案能有效地克服在散度方程中以及在σ坐标系中在大地形附近计算气压梯度力项时所存在的大量之间小差的问题，模式的非线性项的谱计算方法有其优越性。本文给出了利用本模式以及用实际观测资料的客观分析场为初始场作30天长期数值天气预报试验结果。从多个个例的结果可以看出，模式的预报效果令人满意，在整个30天内，模式的预报误差都比对应的持续性误差小，而且在低纬地区也具有上述特点。这表明，本文提出的全球七层大气环流谱模式具有30天长期数值预报能力。 相似文献
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大气模式对比计划是一项国际性的尝试计划，用来确定真实条件下大气模式的系统性气候误差，要求做１９７９－１９８８年十年的气候模拟（以观测的月平均海表温度和海水分布作为边界条件）。大气模式对比计划由数值试验工作组织织，为世界气候研究计划贡献，在模式性能的主要检验和对比中，大气模式对比计划须包括国际大气模拟团体的参加，除了月平均输出变量之外，每个参与大气模式对比计划的模式将产生逐日的历史善，劳伦期．利弗莫 相似文献
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如何在长时间积分的过程中保证模式大气的质量守恒是数值模式动力框架面临的基本问题之一,对于半拉格朗日动力框架来说, 在理论上要满足质量守恒面临着诸多的困难,质量订正方案不失为一种简单可行的选择。中国气象局数值预报中心的GRAPES_GFS (Global-Regional Assimilation and PrEdiction System, Global Forecast System) 在长时间积分过程中质量损失问题较为明显,该研究工作借鉴C-CAM (Climate-Community Atmosphere Model) 中对地面气压进行订正控制模式质量守恒的思路,在GRAPES_GFS中开发了一种对每个网格内的质量按照不同权重系数进行调整、控制模式大气总质量守恒的算法。经过一系列的试验,验证了该方法在GRAPES_GFS中的可行性,在保证模式质量守恒的情况下可有效减小高度场的预报偏差,缓解模式预报结果中天气系统偏弱的问题,在实际业务预报中有一定应用价值。 相似文献
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模式误差对变分同化过程影响的数值研究 总被引：11，自引：6，他引：11
本文利用浅水方程模式，对变分四维同化过程中模式中误差的影响进行了数值模拟实验，实验显示了模式误差被“混淆”入初始场的现象，在一些模式变量无观测时，这种混淆的后果更为严重。 相似文献
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本文对如何提高气象要素的垂直插值精度以减少数值模式中的计算误差的问题作了详细讨论。文中提出了三种温度对气压的分布关系,并检验了它们在数值模式中应用时的优劣。结果表明,温度随气压对数和随高度成线性关系的分布假设较好。试验还证明,当模式中具有高和陡的地形时,用模式大气底层的温压关系去外插地面以下的温度和位势高度时,会造成很大的不规则的误差。用等压面上局地温度相等的假定以及用水平热力结构相同的假设可大大减小外插误差并改善气压梯度力的计算方法。 相似文献
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利用ＩＡＰＧＣＭ２５年的积分结果,系统分析了模式的１、７月月平均气候,并与观测资料、ＯＳＵＧＣＭ和其它大气环流模式的模拟结果作了比较,所比较的变量包括大气基本变量即海平面气压、表面气温和降水以及与流场、加热场和水汽场有关的诸多变量。结果表明,模式成功地模拟出各种大气变量的分布特征,大多数变量的模拟结果要优于ＯＳＵＧＣＭ,从而证实模式对１、７月月平均气候有较好的模拟能力,特别是由于ＩＡＰＧＣＭ与ＯＳＵＧＣＭ两模式物理过程十分相似,这一结果还进一步证实了ＩＡＰＧＣＭ动力框架和计算方案的优良性能。模拟的主要误差包括南极槽偏浅、冰雪区表面气温偏高以及主要降雨区雨量偏大等,同时还分析了模拟误差的可能原因,提出了改进模式的一些设想。此外,计算并比较分析了模式中动量、感热和水汽的经向输送。 相似文献
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John J. Carroll Luis R-Mendez-Nuñez Saffet Tanrikulu 《Boundary-Layer Meteorology》1987,41(1-4):149-169
Most models of atmospheric flow which use the primitive equations require a diagnostic equation to determine local total pressure. In hydrostatic models, this equation is the vertically integrated hydrostatic equation. A frequently used approximation to this integration is to hold the temperature constant within model layers yielding a linear proportionality between p or (Exner's function) and z. This procedure yields static pressures with errors on the order of 10–3mb.If terrain following coordinates are used, terms arise in the horizontal momentum equations involving the gradient of total pressure along the coordinate surface, less a correction for the variation of the hydrostatic pressure along a sloped surface. Erroneous horizontal accelerations are common in these models which result from spurious pressure gradients that are due to inaccurate computation of the static pressure. This error may be amplified if the computation of the slope correction term of the horizontal pressure gradient is not consistent with the method of calculating the total pressure.We derive a methodology to be used in the vertical pressure integrations that is exact if the potential temperature lapse rate is constant between integration limits. The method is applied to both the integration of the hydrostatic equation and the computation of the slope correction term in the horizontal pressure gradient. The method employs a fixed vertical grid and a dynamic one defined by the significant levels in the vertical temperature distribution. With this methodology, the error in calculation of the horizontal pressure gradient acceleration is greatly reduced, especially in situations where the isothermal surfaces are not parallel to the vertical coordinate surfaces. The problem of aliasing and the treatment of significant temperature levels is described. 相似文献
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The albedo of snow for different cloudiness conditions is an important parameter in the Earth's radiation budget analysis and in the study of snowpack's thermal conditions. In this study an efficient approximate method is derived to calculate the incident spectral solar flux and snow-cover albedo in terms of different atmospheric, cloud, and snow parameters. The global flux under partially cloudy skies is expressed in terms of the clear sky flux and a coefficient which models the effect of scattering and absorption by cloud patches and multiple reflections between the cloud base and snowcover. The direct and the diffuse components of the clear sky flux are obtained using the spectral flux outside the atmosphere and the spectral transmission coefficients for absorption and scattering by molecules and aerosols.The spectral snow reflectance model considers both specular surface reflection and volumetric multiple scattering. The surface reflection is calculated by using a crystal-shape-dependent bidirectional reflectance distribution function; the volumetric multiple scattering is calculated by using a crystal-size-dependent approximate solution in the radiative transfer equation. The input parameters to the model are atmospheric precipitable water, ozone content, turbidity, cloud optical thickness, the size and shape of ice crystals of snow and surface pressure. The model yields spectral and integrated solar flux and snow reflectance as a function of solar elevation and fractional cloudcover.The model is illustrated using representative parameters for the Antarctic coastal regions. The albedo for a clear sky depends inversely on the solar elevation. At high elevations the albedo depends primarily upon the grain size; at low elevation the albedo depends on grain size and shape. The gradient of the albedo-elevation curve increases as the grains become larger and faceted. The albedo for a densely overcast sky is a few percent higher than the clear-sky albedo at high elevations. A simple relationship between grain size and the overcast albedo is obtained. For a set of grain size and shape, the albedo as a function of solar elevation and fractional cloud cover is tabulated. 相似文献
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Solar radiation is an essential and important variable to many models. However, it is measured at a very limited number of meteorological stations in the world. Developing method for accurate estimation of solar radiation from measured meteorological variables has been a focus and challenging task. This paper presents the method of solar radiation estimation using support vector machine (SVM). The main objective of this work is to examine the feasibility of SVM and explore its potential in solar radiation estimation. A total of 20 SVM models using different combinations of sunshine ratio, maximum and minimum air temperature, relative humidity, and atmospheric water vapor pressure as input attributes are explored using meteorological data at 15 stations in China. These models significantly outperform the empirical models with an average 14 % higher accuracy. When sunshine duration data are available, model SVM2 using sunshine ratio and air temperature range is proposed. It significantly outperforms the empirical models with an average 26 % higher accuracy. When sunshine duration data are not available, model SVM19 using maximum temperature, minimum temperature and atmospheric water vapor pressure is proposed. It significantly outperforms the temperature-based empirical models with an average of 18 % higher accuracy. The remarkable improvement indicates that the SVM method would be a promising alternative over traditional approaches for estimation of solar radiation at any locations. 相似文献
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A modeling system for investigating meteorological controls on glacier mass balance is described and applied to the Southern Patagonian Icefield. Output from a mesoscale atmospheric model is used to drive a glacier mass balance model using model precipitation and turbulent fluxes adjusted to account for the unrealistically low surface elevations of the icefield in the atmospheric model. Simulations of January and July conditionsproduce glacier equilibrium line altitudes (ELAs) that are higher than the observed, but the ELA gradient is realistically simulated. The high ELAs are primarily due to underestimates of vertical temperature gradients in the atmospheric model and uncertainties in the ablation season length. The model shows that both winter and summerprecipitation, as well as summer temperatures, are important determinants of the mass balance of the Southern Patagonia glaciers. The position of the icefield on the continent is also relevant. On the western side of the icefield, precipitation rates are high and dominate the mass balance calculation. In the east, ablation is much more important for determining the mass balance, and this introduces an enhanced sensitivity to atmospheric temperature, wind speed, and atmosphericmoisture levels. 相似文献
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AN IMPROVED SEMI-IMPLICIT TIME DIFFERENCE SCHEME OF SPECTRAL MODEL AND NUMERICAL APPLICATIONS 总被引：1，自引：0，他引：1
In fact,the popular semi-implicit time difference scheme of spectral model still includes someimportant linear terms using time explicit difference scheme,and the major terms are directlyrelated to fast internal-and external-gravity waves in the atmospheric forecasting equation.Additionally,due to using time difference on two terms at different time.the popular schemeartificially introduces unbalance between pressure gradient force and Coriolis force terms whilenumerically computing their small difference between large quantities.According to thecomputational stability analysis conducted to the linear term time difference scheme in simpleharmonic motion equation,one improved semi-implicit time difference scheme is also designed inour study.By adopting a kind of revised time-explicit-difference scheme to these linear terms thatstill included in spectral model governing equations,the defect of spectral model which only partlyusing semi-implicit integrating scheme can be overcome effectively.Moreover,besides all spectralcoefficients of prognostic equations,especially of Helmholtz divergence equation,can be workedout without any numerical iteration,the time-step (computation stability) can also be enlarged(enhanced) by properly introducing an adjustable coefficient. 相似文献
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AN IMPROVED SEMI-IMPLICIT TIME DIFFERENCE SCHEME OF SPECTRAL MODEL AND NUMERICAL APPLICATIONS* 
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下载免费PDF全文 In fact,the popular semi-implicit time difference scheme of spectral model still includes some important linear terms using time explicit difference scheme,and the major terms are directly related to fast internal-and external-gravity waves in the atmospheric forecasting equation.Additionally,due to using time difference on two terms at different time.the popular schemear tificially introduces unbalance between pressure gradient force and Coriolis force terms while numerically computing their small difference between large quantities.According to the computational stability analysis conducted to the linear term time difference scheme in simple harmonic motion equation,one improved semi-implicit time difference scheme is also designed in our study.By adopting a kind of revised time-explicit-difference scheme to these linear terms that still included in spectral model governing equations,the defect of spectral model which only partlyusing semi-implicit integrating scheme can be overcome effectively.Moreover,besides all spectral coefficients of prognostic equations,especially of Helmholtz divergence equation,can be worked out without any numerical iteration,the time-step (computation stability) can also be enlarged (enhanced) by properly introducing an adjustable coefficient. 相似文献
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受台风鹿莎影响,处在其西侧外围下沉区域的南京地区于2002年8月31日出现了一次大气波导过程,利用大气中尺度模式WRF对其成因进行了详细的数值模拟研究。WRF数值模拟较好地再现了此次波导的演变过程,即波导在31日傍晚开始形成,次日凌晨达到最强,日出后迅速减弱消失。基于数值模拟高时空分辨率的输出结果,对波导成因进行细致分析,结果表明:湿度突变层和逆温层的同时存在导致了波导的发生,前者是其形成的关键因素,而后者的作用主要体现在增强其强度;台风前期流场从海上带来大量的水汽,台风后期流场将北方高空干空气输送到受高压下沉运动控制的南京地区,造成近地层出现下湿上干的剧烈湿度梯度;下沉运动强度并不足以直接导致南京地区的逆温层,但其控制下的晴朗天气非常有利于夜间地面长波辐射冷却而形成逆温。 相似文献
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B. A. Kader 《Boundary-Layer Meteorology》1992,61(4):323-347
Methods are studied which permit one to evaluate turbulent fluxes from the results of spectral measurements in turbulent laboratory flows and an unstable atmospheric surface layer. The well known dissipation method of flux measurements, which uses spectral data related to the inertial range, is reanalyzed. New theoretical ideas and the latest experimental data are used to specify this method in cases of moderately and very strongly unstable thermal stratifications.Moreover, it is also explained how to estimate momentum and heat fluxes from data in the low frequency parts of the velocity and temperature spectra in the low frequency ranges beyond the lower limit of the inertial range. This permits one to estimate fluxes using rather simple and cheap instruments (e.g., Pilot-tubes and thermocouples in laboratory flows or cup anemometers and crude resistance thermometers in meteorological studies). The equations for flux determination are based in such cases on the recent models by Kader (1987, 1988) and Kader and Yaglom (1990, 1991) of spectral shapes at mesoscale wave numbers; these models agree quite satisfactorily with many (though not all) data of direct spectral measurements. It is shown that estimated momentum and heat fluxes in the laboratory and in an unstably stratified atmospheric surface layer obtained by the method suggested in this paper agree satisfactorily with direct flux measurements. 相似文献
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Summary The spectral distributions of the pressure gradient force errors of the spectral and the finite-difference techniques used in combination with the vertical coordinate were examined in an idealized case of an atmosphere at rest and in hydrostatic equilibrium. The vertical temperature profile was piece-wise linear in lnp, with an inversion at the bottom. Trapezoidal mountains of different widths were used. The same amounts of input information were given to both the spectral and the finite-difference methods. In the rms sense, the spectral errors were generally much larger than those of the finite-difference method. However, on the larger and medium scales, a remarkable similarity of the error spectra of the two methods was found. The build up of the error of the spectral method occurs at the smallest scales. This may explain difficulties in documenting the error in higher resolution spectral models where the contribution to the total error in this part of the spectrum may be removed as the small-scale noise by the horizontal smoothing and/or filtering. In order to reduce the small-scale noise generation, the finite-difference pressure gradient force may be used in spectral models.With 6 Figures 相似文献
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