棉田土壤热通量的计算

本文在两年棉花田间试验观测的基础上,利用土壤中热传导方程模拟5cm层土壤温度的时间变化,进而推算出其它层次的土壤温度,与实测值相比,模拟均方误最大为0．14,最大温度绝对误差为0．7℃．通过对温度方程求深度上的偏导数获得土壤热通量的计算公式,计算值与实测值比较,均方误最大为0．006,效果较好。本文还通过2cm层土壤热通量与棉花冠层净辐射之间的关系,结果表明土壤热通量与冠层净辐射有着很好的相关性。     

1998年南海季风爆发期间近海面层大气湍流结构和通量输送的观测研究

1998年5月14日至6月22日,在西沙永兴岛近海铁塔上进行了一次海-气通量观测试验,观测期包括了西南季风爆发前、爆发、爆发后风速加强等几个阶段。这次试验获得该年西南季风爆发的天气特征以及由涡度相关法、廓线法计算的动量、感热、潜热通量及湍流强度等一些统计量分布。分析结果表明,观测期湍流强度σu、σv、σw与平均风速之比为0.096、0.066、0.045;在近中性条件下（z/L≈0）,各相似函数基本为常数,σu/u＊≈3,σv/u＊≈2,σw/u＊≈1.25;在稳定条件下u、v、w三方向σ/u＊近似相等;在稳定与不稳定条件下σt/t＊随稳定度参数z/L的变化趋势相似,但符号相反。摩擦速度u＊随风速的变化接近于关系式u＊=0.029U10+0.006（U10为10m高度30min平均风速）,空气动力粗糙度长度z0变化在0.01～0.35mm之间。观测期动量通量变化在0.05～0.30N/m2之间,季风爆发期明显增大;曳力系数CD平均为1.12×10-3,它随平均风速变化可以表示为关系式103CD=0.003U210+0.020U10+0.836或103CD=0.056U10+0.732。感热通量由海洋输向大气,平均值为7.8W/m2,数值在0～15W/m2之间变化,季风爆发后明显增大;潜热通量数值一般变化于50～200W/m2,白天中午数值较高,夜间较低。季风爆发后也明显增大。观测期间鲍恩比（BowenRatio）日平均为0.05左右。     

Stratospheric Photolysis Frequencies: Impact of an Improved Numerical Solution of the Radiative Transfer Equation

Numerical schemes for the calculation of photolysis rates are usually employed in simulations of stratospheric chemistry. Here, we present an improvement of the treatment of the diffuse actinic flux in a widely used stratospheric photolysis scheme (Lary and Pyle, 1991). We discuss both the consequences of this improvement and the correction of an error present in earlier applications of this scheme on the calculation of stratospheric photolysis frequencies. The strongest impact of both changes to the scheme is for small solar zenith angles. The effect of the improved treatment of the diffuse flux is most pronounced in the lower stratosphere and in the troposphere. Overall, the change in the calculated photolysis frequencies in the region of interest in the stratosphere is below about 20%, although larger deviations are found for H₂O, O₂, NO, N₂O, and HCl.     

An OGCM Simulation of Seasonal and Interannual Variabilities in the Surface-Layer Pacific of the Equatorial Band

l. IntroductionThe physical mechanisms contro1ling t]de El Nifio event have been studied based on ob-servations in the equatorial Pacific (Weare l983; Reed l986; Hayes et al. l99l; McPhadenand Picaut l990; Frankignoul et al. 1996; Weisberg and Wang l997). One of the most impor-tant issues is whether the surface heat flux ojr ocean advective heat fluxes are dominant in con-trolling the sea surface temperature (SST). Some studies indicated that the SST is mainly con-trolled by the surface…     

卫星遥感确定沙特阿拉伯吉达地区非均匀地表区域地表参数和能量通量

对临海沙漠地区非均匀地表区域地表能量通量和蒸发(蒸散)的研究,是一个十分重要但又是一个难点问题。本文提出了1个基于卫星遥感和地面观测的参数化方案,并把其应用于沙特阿拉伯吉达地区,利用1个景的陆地资源卫星Landsat-7E^TM^ 资料进行了分析研究,得到了一些有关临海沙漠地区非均匀地表区域地表特征参数、植被参数和地表能量通量的新概念。最后讨论了所提出的参数化方案的适用范围和需改进之处。     

Effects of an Urban Park and Residential Area on the Atmospheric CO2 Concentration and Flux in Seoul, Korea

The CO₂ concentrations and fluxes over an urban forest site (Namsan) and an urban residential region (Boramae) in Seoul, Korea, during the non-growing season (2–4 March 2011), the growing season (10–12 June 2011), and the late-growing season (22–24 September 2011) were analyzed. The CO₂ concentrations of two sites showed nearly the same diurnal variation, with a maximum value occurring during the night and a minimum value occurring during daytime, as well as the same seasonal variation, with a maximum value during the non-growing season (early spring) and a minimum value during the growing season (summer). The CO₂ flux over the urban forest did not show any typical diurnal variation during the non-growing season, but did show diurnal variation with a small positive value during the night and a large negative value during daytime in the growing and late-growing seasons due to photosynthesis in the urban forest. The CO₂ flux over the urban residential region showed a positive daily mean value for all periods, with large values during the non-growing season and small values during the growing season, and it also showed diurnal variation with two maxima at 0600–1000 LST and 1800–2400 LST, and two minima at 0300-0600 LST and 1100-1500 LST, and was strongly correlated with the use of liquefied natural gas for cooking and heating by surrounding houses.     

华北地区冬小麦光合作用的光响应曲线的特征参数

在冬小麦各生育期测定了田间叶片光合作用速率及其相应的气象要素, 拟合了各生育期的光合作用的光响应曲线.得出它们的几个特征参数:初始量子效率、最大光合速率和凸度.在华北地区冬小麦的整个生育期, 初始量子效率大多在0.050~0.075之间变化, 最大光合速率在5~25 μmol·m-2·s-1之间变化.表明初始量子效率随生育期的变化不大, 最大光合速率在营养生长期较高, 为20~25 μmol·m-2·s-1, 在生殖生长期, 随着叶片氮、磷、钾等营养元素含量的下降, 叶片的最大光合速率显著降低.     

中国东部春季极端降水与同期欧亚大陆地表感热的可能联系

利用1960~2010年ERA-20C再分析资料和中国东部站点降水观测资料,探讨了我国东部春季极端降水与欧亚大陆地表感热通量的联系和可能影响途径。结果发现,当春季欧亚大陆中纬度巴尔喀什湖以西及贝加尔湖以南区域地表感热通量偏弱（强）,我国东部沿海地区地表感热通量偏强（弱）时,我国东部春季极端降水呈现南少（多）北多（少）的反相分布特征。当春季欧亚大陆中纬度关键区地表感热偏弱,低纬度关键区地表感热通量偏强时,春季副热带西风急流偏弱、位置偏北,我国东部北方地区大气斜压不稳定和对流不稳定偏强,北方地区极端降水偏强,而南方地区大气斜压不稳定和对流不稳定偏弱,南方地区极端降水偏弱。当春季欧亚大陆中纬度关键区地表感热偏强,低纬度关键区地表感热通量偏弱,我国东部极端降水的情况大致相反。     

修正的质量通量积云对流方案及其模拟试验研究Ⅰ:方案介绍及对1991年洪涝过程的模拟

文中在综合比较各类积云对流参数化方案优缺点的基础上 ,主要参考陈伯民等修正的ECMWF质量通量积云参数化方案 ,对其进行简化和修改 ,发展了一个质量通量积云对流参数化方案 ,文中表示为 MFS(Mass Flux Scheme)。MFS是一种综合型的方案 ,既考虑了大尺度水汽辐合的重要性 ,又考虑了积云中的上升运动、下沉运动、环境中的补偿下沉运动 ,以及卷入、卷出和蒸发等 ,用总体云模式来描述积云与环境的相互作用 ,同时考虑了深对流和浅对流。将 MFS植入 NCAR区域气候模式 Reg CM2中 ,对 1 991年 5～ 7月江淮地区特大降水过程的夏季风气候特征和变化进行了模拟 ,并与 NCAR Reg CM2选用 Kuo方案 ,在同样初、边值条件和其它物理过程选择下的模拟结果进行了对比分析。分析结果表明 ,植入 MFS后的模式能够模拟这次极端的降水气候事件。在某些方面 ,如地表气温 ,降水的模拟上 ,植入 MFS后的模式的模拟结果要比原模式的结果更合理     

SPATIO-TEMPORAL VARIATION OF SENSIBLE HEAT FLUX OVER SOUTHERN CHINA

The spatio-temporal variation of surface sensible heat flux (SHF) in southern China (SC) is studied based on the data evaluated from conventional observational meteorological data. There exist prominent increasing trends in all seasonal surface sensible heat fluxes in the western SC and decreasing trends in the central-eastern part of southern China. The variations of surface sensible heat flux in all seasons are dominant on interannual time-scales. The land-air temperature difference and the near-surface wind speed are two key factors for the interannual variations of SHF, but the former is more important. The first two major anomalous patterns of SHF are presented as the region-wide in-phase anomalies and the east-west dipole anomalies, respectively, based on the EOF analysis results.