气象卫星观测资料的分析在城市区域气象环境研究中的应用

目前 ,我国气象部门相当普遍地拥有气象卫星观测资料 ,但是 ,这些资料如何在城市气象服务以及为城市建设规划等方面的决策研究中发挥作用 ,急待进一步研究并开展工作。本文试图通过合理的反演处理 ,给出卫星观测对地面温度的测量结果 ,由此可比较细致地分析了解地面热状况及其与土地利用类型 ,地面覆盖性质等的关系。本文利用有限的 NOAA- AVHRR气象卫星遥感资料 ,采用修正的 Ulivieri分裂窗方法反演出同期的地表温度场 ,通过对北京地区的卫星观测资料进行算例分析 ,揭示出一个 2 0 0 km× 2 0 0 km范围内的地面温度分布特征。反演结果可以明显地揭示出城市热岛现象的变化规律 ,并且能较为清楚地反映出相对的高温区和低温区     

Determination of Roughness Lengths for Heat and Momentum Over Boreal Forests

The roughness length for momentum (z_0m), zero-plane displacementheight (d), and roughness length for heat (z_0h) are importantparameters used to estimate land-atmosphere energy exchange. Although many different approaches have been developed to parameterizemomentum and heat transfer, existing parameterizations generally utilizehighly simplified representations of vegetation structure. Further, a mismatch exists between the treatments used for momentum and heat exchange and those used for radiative energy exchanges. In this paper, parameterizations are developed to estimate z_0m, d, and z_0h for forested regimes using information related to tree crown density and structure. The parameterizations provide realistic representationfor the vertical distribution of foliage within canopies, and include explicit treatment for the effects of the canopy roughness sublayer and leaf drag on momentum exchange. The proposed parameterizationsare able to realistically account for site-to-site differences in roughness lengths that arise from canopy structural properties.Comparisons between model predictions and field measurements show good agreement, suggesting that the proposed parameterizations capture the most important factors influencing turbulent exchange of momentumand heat over forests.     

A Technique for Direct Retrieval of Surface Specific Humidity Over Open Oceans from Irs-P4/Msmr Satellite Data

The Multi frequency Scanning Microwave Radiometer (MSMR) onboard Oceasat-1 was used to develop a retrieval method fornear-surface specific humidity by means of multivariate regressiontechnique. The MSMR measures the microwaveradiances in 8 channels at the frequencies of 6.6, 10.7, 18 and 21 GHzfor both vertical and horizontal polarizations. Regression coefficients were derived using the ship reports of the Comprehensive Ocean-Atmosphere Data Set (COADS) for the months of July, October and December, in 1999. Daily near-surface specific humidity data from COADS in 2° × 2° latitude/longitude bins and collocated brightness temperature data from MSMR were used to derive the coefficients. The derived coefficients werevalidated with humidity given in COADS.A linear relationship is established to determine the near-surface specifichumidity from MSMR brightness temperature (Tb) with an rms error of 1.2 g kg^-1 for individual situations and an rms errorof 0.84 g kg^-1 for monthly time scales over global oceans.The retrieval algorithm is validonly for the open sea regions.     

地表非均匀性对区域平均水分通量参数化的影响

次网格尺度地表非均匀性对于网格区平均通量具有重要影响。若将网格区视为均一地表 ,并不能真实描述地 气通量交换过程 ,且可造成很大误差。文中从理论上证明 ,区域平均水分通量的变化率可分解为两部分 :第一部分为区域水分通量的算术平均变化率 ;第二部分为非均匀性所引起的水分通量变化率扰动 ,它与区域内土壤水分空间分布的变差系数有关。数值试验表明 ,地表土壤水分的水平空间变差系数集中反映了区域内土壤水分分布的非均匀程度 ,不同土壤对同样的非均匀程度其敏感性是不同的。变差系数愈大 ,非均匀性愈强 ,在相同的土壤水分平均值下 ,不同土壤类型对地表非均匀程度的敏感性并不相同。例如沙土和粘土受非均匀性的影响就可相差数十倍。     

黄海、东海海域出海气旋发展过程中尺度数值模拟

利用MM5中尺度模式对1999年6月两个出海气旋发展过程进行 数值模拟. 数值模拟的气旋出海后移动路径与实际情况基本一致. 在数值模拟基础上重点讨 论了出海气旋发展过程潜热通量和感热通量的分布及其演变情况. 气旋出海后在气旋中心区 南方和东方存在负潜热通量和感热通量区. 出海气旋的东移和发展，其前方强大正热通量区 的存在可能是重要原因之一.     

西北地区戈壁局地陆面物理参数的研究

采用2000年8月～2001年9月在敦煌戈壁上观测的陆面过程资料，分析了敦煌地区荒漠戈壁地表反照率与太阳高度角和土壤湿度的关系以及土壤热传导率与土壤湿度的关系，初步给出了具有试验基础的戈壁局地反照率和土壤热传导率的多因子参数化公式. 并通过与观测值的比较发现试验资料拟合的参数化公式能够比较好地反映降水等气候因子引起的动态变化.     

A Case Study Of An On-Ice Air Flow Over The Arctic Marginal Sea-Ice Zone

A case study of warm air advection over the Arctic marginalsea-ice zone is presented, based on aircraft observations with direct flux measurements carriedout in early spring, 1998. A shallow atmospheric boundary layer (ABL) was observed, which wasgradually cooling with distance downwind of the ice edge. This process was mainly connected with astrong stable stratification and downward turbulent heat fluxes of about 10–20 W m^-2, but wasalso due to radiative cooling. Two mesoscale models, one hydrostatic and the other non-hydrostatic,having different turbulence closures, were applied. Despite these fundamental differences betweenthe models, the results of both agreed well with the observed data. Various closure assumptions had amore crucial influence on the results than the differences between the models.Such an assumption was, for example,the parameterization of the surface roughness for momentum (z₀) and heat (z_T). This stronglyaffected the wind and temperature fields not only close to the surface but also within and abovethe temperature inversion layer. The best results were achieved using a formulation for z₀ that took intoaccount the form drag effect of sea-ice ridges together withz_T = 0.1z₀. The stability within theelevated inversion strongly depended on the minimum eddy diffusivity K_min. A simple ad hocparameterization seems applicable, where K_min is calculated as 0.005 timesthe neutral eddy diffusivity. Although the longwave radiative cooling was largest within the ABL, theapplication of a radiation scheme was less important there than above the ABL. This was related to theinteraction of the turbulent and radiative fluxes. To reproduce the strong inversion, it wasnecessary to use vertical and horizontal resolutions higher than those applied in most regional andlarge-scale atmospheric models.     

Modelling of the OASIS Energy Flux Measurements Using Two Canopy Concepts

Two land surface schemes, SCAM and CSIRO9, were used to model the measured energy fluxes during the OASIS (Observations At Several Interacting Scales) field program. The measurements were taken at six sites along a 100 km rainfall gradient. Two types of simulations were conducted: (1) offline simulations forced with measured atmospheric input data at each of the six sites, and (2) regional simulations with the two land surface schemes coupled to the regional climate model DARLAM.The two land surface schemes employ two different canopy modelling concepts: in SCAM the vegetation is conceptually above the ground surface, while CSIRO9 employs the more commonly used `horizontally tiled' approach in which the vegetation cover is modelled by conceptually placing it beside bare ground. Both schemes utilize the same below-ground components (soil hydrological and thermal models) to reduce the comparison to canopy processes only. However, the ground heat flux, soil evaporation and evapotranspiration are parameterised by the two canopy treatments somewhat differently.Both canopy concepts reproduce the measured energy fluxes. SCAM has a slightly higher root-mean standard error in the model-measurement comparison for the ground heat flux. The mean surface radiative temperature simulated by SCAM is approximately 1K lower than in the CSIRO9 simulations. However, the soil and vegetation temperatures (which contribute to the radiative temperature) varied more in the CSIRO9 simulations. These larger variations are due to the absence of a representation of the aerodynamic interactions between vegetation and ground.     

1991年江淮暴雨时期的能量和水汽循环研究

通过对 1991年 5～ 7月江淮暴雨期全球范围的水汽输送和不同降水过程中江淮暴雨区及其临近区域的水汽收支和视热源和视水汽汇的计算分析得到了以下结论 :( 1)从水汽输送的机制来看 ,一方面 ,有大量的水汽以定常涡动的方式从孟加拉湾及南海输送到中国江淮地区 ;另一方面 ,江淮地区的瞬变涡动水汽向北输出 ,这可能与江淮地区频繁活动的α和β中尺度系统有关 ,它们将江淮地区汇集的充沛的水汽除了大部分以降水形式降下外 ,剩余部分继续向水汽较少的高纬地区输出 ,以维持全球水汽的平衡。( 2 )在降水过程中 ,局地蒸发项在水汽的供应中或再循环中十分重要 ,其数值一般为降水量的 13 ～ 12 ,这与1998年的降水情况相似。( 3 )在降水过程中 ,暴雨区的水汽主要是从南边界和西边界流入的 ,东边界和北边界则流出 ,并且水汽的流入、流出主要在中低层进行。 (a)在流入边界上 ,水汽通量的垂直分布存在差异 ,暴雨区西边界和南边界的水汽流入的垂直差异可能与其所在的地理位置有密切关系。 (b)对于暴雨区 ,不同强度的降水过程水汽的主要来源有所不同。( 4)在 5次降水过程中 ,视热源和视水汽汇的较大值对应降水的大值区 ,表明了水汽凝结加热对大气加热所起的主要作用。梅雨期降水 ,以对流性降水为主 ,对流活动随季节变化     

“93.5”黑风暴发展期中尺度期热量和水汽收支诊断

１９９３年５月４—６日（“９３．５”）在我国西北地区发生了一次极具破坏力的“黑风暴”。为了诊断这次黑风暴发展期的热量和水汽收支，使用了具有高分辨ＰＢＬ参数化及４０ｋｍ细网络的ＭＭ４对该例控制模拟的输出资料和热量与水汽收支方程。对视热源（Ｑ１）和视水汽汇（Ｑ２）的诊断结果指出，Ｑ１的垂直积分在黑风暴的前部和后部分别呈现一条显著的加热带和冷却带。在黑风暴区，Ｑ１和Ｑ２的区域平均垂直廓线揭示，黑风暴的Ｑ１加热主要发生在对流层的上部，而其中部加热主要出现在发展初期；与Ｑ１相应，Ｑ２在低空和中空分别发生明显的增湿变冷和变干加热。这些结果不仅与因黑风暴过程而观测到的强剧强降温率一致，而且也为改进和发展用于模拟和预报黑风暴的中尺度数值模式提供了一些物理依据