中国北方干旱区感热及潜热的异常特征   总被引：7，自引：4，他引：7  

惠小英  王澄海  左洪超  董文杰 《高原气象》2005,24(3):415-421

通过对1949—1999年逐月NCEP／NCAR感热通量和潜热通量再分析资料的分析，发现在我国北方干旱区感、潜热通量的年际变化存在着2～3个敏感区，分别位于西北和华北及内蒙一带。其中以东部的华北—内蒙区最为显著。代表上述两个地区通量的平均年际变化表明，在20世纪60年代后期，感、潜热通量存在一个突变；进入70年代以后，上述两个地区的感热通量保持在一个较高的水平上，潜热通量的变化则呈现出相反的变化。  相似文献   

A Modelling Approach For Optimizing Flight Patterns In Airborne Meteorological Measurements     

Timo Vihma  Christoph Kottmeier 《Boundary-Layer Meteorology》2000,95(2):211-230

A method is presented for selecting the optimal flight patterns for airbornemeteorological measurements in various flow situations. The method is basedon systematic utilisation of mesoscale model fields. Flow overan Arctic sea-ice boundary zone is modelled, and it is assumed that the mesoscale model fields represent the true state of the atmosphere, and that each possible flight pattern yields a different sample of the true fields. A plan for the basic structure of the flight pattern is assumed, and then the unexplained variance, i.e., the difference between the true variance and the sample variance, of a quantity of interest is calculated for a variety of possible flight patterns. Different target quantities are considered, such as wind speed, air temperature, and the turbulent fluxesof momentum and sensible heat. The optimal flight pattern is defined byminimisation of the unexplained variance, and often depends on the quantitywe are interested in. For sawtooth patterns, the optimal flight pattern was sensitive to the maximum ascent angle of the aircraft. In flight patterns designed for turbulence measurements, the optimal pattern was different for the unexplained variance of the turbulent fluxes and for the unexplained total heat content of the convective layer.  相似文献   

Parameterization and Micrometeorological Measurement of Air–Sea Gas Transfer     

C. W. Fairaill  J. E. Hare  J. B. Edson  W. McGillis 《Boundary-Layer Meteorology》2000,96(1-2):63-106

Because of the combination of smallconcentrations and/or small fluxes, the determinationof air–sea gas fluxes presents unusual measurementdifficulties. Direct measurements (i.e., eddycorrelation) of the fluxes are rarely attempted. Inthe last decade, there has been an intense scientificeffort to improve measurement techniques and to placebulk parameterizations of gas transfer on firmertheoretical grounds. Oceanic tracer experiments,near-surface mean concentration profiles, eddyaccumulation, and direct eddy covariance methods haveall been used. Theoretical efforts have focusedprimarily in the realm of characterizing the transferproperties of the oceanic molecular sublayer. Recentmajor field efforts organized by the U.S.A. (GASEX-98) andthe European Union (ASGAMAGE) have yielded atmospheric-derivedresults much closer to those from oceanographicmethods. In this paper, we review the physical basisof a bulk-to-bulk gas transfer parameterization thatis generalized for solubility and Schmidt number. Wealso discuss various aspects of recent sensor andtechnique developments used for direct measurementsand demonstrate experimental progress with resultsfrom ASGAMAGE and GASEX-98. It is clear that sensornoise, sensitivity, and cross talk with other speciesand even ship motion corrections still need improvement foraccurate measurements of trace gas exchange over theocean. Significant work remains to resolve issuesassociated with the effects of waves, bubbles, andsurface films.  相似文献   

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

Gaby Becker  Jens-Uwe Grooss  Daniel S. McKenna  Rolf Müller 《Journal of Atmospheric Chemistry》2000,37(3):217-229

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.  相似文献   

华北地区冬小麦光合作用的光响应曲线的特征参数   总被引：33，自引：1，他引：32       下载免费PDF全文

陆佩玲  罗毅  刘建栋  于强 《应用气象学报》2000,11(2):236-241

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.  相似文献   

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   总被引：28，自引：1，他引：27  

闫俊岳  姚华栋  李江龙  王强  杨志勇 《气候与环境研究》2000,5(4):447-458

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。  相似文献   

关于棉田感热通量和潜热通量的几种计算方法   总被引：8，自引：1，他引：7  

吴洪颜  申双和 《气象科学》2000,20(4):537-542

根据棉田的实测资料,选用四种常用的计算感染热通量的潜热通量的方法进行分析,发现空气动力学方法Ｉ和伯温比－能量平衡法的计算结果较一致,梯度扩散法略小,而布德科方法计算的潜热通量偏高、感热通量过低,因此得出结论：在计算棉花等作物的冠层通量时,选用空气动力学方法Ｉ最合适,其次是梯度扩散法。  相似文献   

海气陆相互作用的准四年振荡机制     

陈隆勋  赵平 《气象科学》2000,21(3):249-259

目前有关Ｅｌ Ｎｉｎｏ（Ｌａ Ｎｉｎａ）形成机制的讨论,大多是强调海气的相互作用。实际上地气互作用过程中形成的异常气流对于Ｅｌ Ｎｉｎｏ／Ｌａ Ｎｉｎａ的形成也是必不可少的,海气和地气相互作用过程应该是耦合的,不应该加以分离。本文综合了近年来我们得到的有关研究结果,提出了一个海气陆相互作用过程的准四年振荡过程,用来解释Ｅｌ Ｎｉｎａ形成机制和亚洲大陆气候年际变化机制。  相似文献   

动态地幔柱尾管结构   总被引：2，自引：0，他引：2       下载免费PDF全文

李荫亭 《地球物理学报》2000,43(1):30-36

动态地幔柱模式被广泛用于讨论地球科学中的一些重要课题,如巨大火成区的成因,冈瓦纳古陆解体的原因,板块内中小尺度动力过程的驱动因素等．但是这个基于实验研究而建立的模式中,忽略了地幔柱尾管特征及其作用．地幔柱尾管内温度和速度分布是研究地幔柱上升过程的必要条件．本文从控制尾管结构的基本方程出发,给出了一个定常轴对称地幔柱温度和速度分布的近似分析解．从而得到尾管结构的基本特征：影响尾管内温度分布的主导因素是地幔柱的热流通量,而尾管内上涌速度的大小则不仅取决于热流通量,主要是取决于地幔粘度随深度的变化方式．结果表明,对弱地幔柱,尾管的热损失可能是不可忽略的,而对强地幔柱,径向质量传递可能是不可忽略的.  相似文献   

磁通量浮现驱动磁场重联的数值研究   总被引：1，自引：0，他引：1       下载免费PDF全文

苏守军  王水 《地球物理学报》2000,43(1):1-10

应用二维时变可压缩磁流体动力学数值模拟,研究了双极－单极磁场中由于磁通量浮现驱动的磁场重联过程．结果表明,双极场与单极场间磁力线的重联形成上升的冷而密的等离子体团,磁场演变成鞭状结构．向上运动的等离子体团到达其最大高度后将回落和弥散.等离子体团最大上升速度达０．１４ＶＡ,等离子体最大上升速度达０．２７ＶＡ,ＶＡ为下边界处的Ａｌｆｖｅｎ速度．随着磁通量浮现幅度的增大,等离子体上升速度增加,重联过程发展得较快．背景等离子体β１值（β１为等离子体压力与磁压之比）越小,等离子体团中密度增量越大．磁Ｌｕｎｄｑｕｉｓｔ数Ｓ在１０３－１０６之间的改变对等离子体的速度和密度增量影响并不明显．与电阻撕裂模不稳定性引起的自发重联相比,磁通量浮现会更有效地驱动双极－单极场中的磁场重联过程,寻致日冕Ｈα冲浪和Ｘ射线喷流的形成．  相似文献