大风条件下城市冠层流场模拟

发展了基于k-ε湍流闭合方法的城市冠层流场模式,建筑群采用多孔介质来表示,对气流的阻力以形式阻力来描述,采用该模式模拟北京市一个小区的流场,并将模拟结果与北京325 m气象塔观测资料进行比较,结果表明:在大风情况下,计算风廓线与观测拟合风廓线比较吻合.该模式可以用于大风条件下城市冠层流场的模拟.     

北京海淀地区大气边界层的数值模拟研究

采用北京大学的三维复杂地形中尺度数值模式,利用Landsat-TM卫星影像图得到的地表状况计算陆气之间的能量平衡过程,模拟了北京海淀地区大气边界层的风、温场结构以及污染物浓度分布,进而模拟了由于汽车尾气的排放而转化成的气溶胶的浓度分布.模拟表明城郊之间存在热岛效应,边界层风场受到热岛的热力作用以及地形的动力作用影响.污染物及气溶胶浓度也存在城乡差别,最大浓度出现在城区的下风方向.     

Spectral dependence on the correction factor of erythemal UV for cloud,aerosol, total ozone,and surface properties: A modeling study

Radiative transfer model simulations were used to investigate the erythemal ultraviolet(EUV) correction factors by separating the UV-A and UV-B spectral ranges. The correction factor was defined as the ratio of EUV caused by changing the amounts and characteristics of the extinction and scattering materials. The EUV correction factors(CFEUV) for UV-A[CFEUV(A)] and UV-B [CFEUV(B)] were affected by changes in the total ozone, optical depths of aerosol and cloud, and the solar zenith angle. The differences between CFEUV(A) and CFEUV(B) were also estimated as a function of solar zenith angle, the optical depths of aerosol and cloud, and total ozone. The differences between CFEUV(A) and CFEUV(B) ranged from-5.0% to 25.0% for aerosols, and from-9.5% to 2.0% for clouds in all simulations for different solar zenith angles and optical depths of aerosol and cloud. The rate of decline of CFEUV per unit optical depth between UV-A and UV-B differed by up to 20% for the same aerosol and cloud conditions. For total ozone, the variation in CFEUV(A) was negligible compared with that in CFEUV(B) because of the effective spectral range of the ozone absorption band. In addition, the sensitivity of the CFEUVs due to changes in surface conditions(i.e., surface albedo and surface altitude) was also estimated by using the model in this study. For changes in surface albedo, the sensitivity of the CFEUVs was 2.9%–4.1% per 0.1 albedo change,depending on the amount of aerosols or clouds. For changes in surface altitude, the sensitivity of CFEUV(B) was twice that of CFEUV(A), because the Rayleigh optical depth increased significantly at shorter wavelengths.     

二维地形的地形阻力

讨论了在上部稳定层覆盖的不稳定大气边界层中,二维地形扰动所引起的上层波动以及扰动速度的动量通量输送,表明在大气低层层结不稳定时,波动仍可能在大气动量平衡中起明显作用。     

对流边界层中过山气流的数值模拟

采用ARPS4.0非静力中尺度气象模式模拟了对流边界层中气流过山引起的地形波,讨论了地形及大气条件改变对其的影响.模拟表明,当大气边界层是对流边界层时,气流过山引起的地形强迫,仍能在上部稳定层结中造成足够的垂直扰动,产生向上传播的重力内波,重力内波引起的波动阻力仍不可忽略.     

街谷环流和热力结构的数值模拟

文章介绍一种用于模拟街谷流场和温度场的动力学模式和热力学模式.应用动力模式模拟了方柱体塔楼和圆柱体塔楼形成的流场,应用动力和热力模式模拟了街谷中流场和温度场的日变化过程.计算实例表明,上述模式可用于城市街谷和建筑群风环境和热力环境研究以及街谷中空气污染物传输和扩散的计算.     

Influence of South China Sea SST and the ENSO on Winter Rainfall over South China

The present study investigates the influence of South China Sea (SCS) SST and ENSO on winter (January--February--March; JFM) rainfall over South China and its dynamic processes by using station observations for the period 1951--2003, Met Office Hadley Center SST data for the period 1900--2008, and ERA-40 reanalysis data for the period 1958--2002. It is found that JFM rainfall over South China has a significant correlation with Nino-3 and SCS SST. Analyses show that in El Nino or positive SCS SST anomaly years, southwesterly anomalies at 700 hPa dominate over the South China Sea, which in turn transports more moisture into South China and favors increased rainfall. A partial regression analysis indicates that the independent ENSO influence on winter rainfall occurs mainly over South China, whereas SCS SST has a larger independent influence on winter rainfall in northern part of South China. The temperature over South China shows an obvious decrease at 300 hPa and an increase near the surface, with the former induced by Nino-3 and the latter SCS SST anomalies. This enhances the convective instability and weakens the potential vorticity (PV), which explains the strengthening of ascending motion and the increase of JFM rainfall over South China.     

氩-氩定年法国际标准物质BSP-1角闪石的研制

BSP-1角闪石选自中国吉林省桦甸县老牛沟的角闪石岩。~(40)Ar-~(39)Ar分析和均匀性检查表明:此角闪石结晶以后未受过热扰动,~(40)Ar~*保存性好,谱线平坦,K/Ca和Cl/K比值稳定。定值结果显示,在置信概率为0.95时,~(40)Ar~*和K含量的相对偏差均<5‰,是目前最理想的Ar-Ar和K-Ar法国际标准物质,可供全世界Ar-Ar实验室使用80年以上。     

沁水盆地南部煤层气井增产的储层生产控制探讨

以沁水盆地南部区块煤层气生产井的工程、测试、监测数据为依据,对影响煤层气井产能的储层生产控制因素进行了分析,探讨了优化储层生产控制、提高煤层气井产能的工程措施,重点研究了水力压裂工艺施工参数与煤层气井产能的关系,提出了有利于提高煤层气井产能的水力压裂工艺施工参数。结果表明：合理控制钻井液的密度与粘度,可提高煤层气井的产能;煤层气井的产能与固井工艺中的水泥浆密度与用量呈现负相关关系;水力压裂采用变砂比、控制压裂液、变排量等施工工艺和优化的工艺参数值可有效提高煤层气井气产量。     

油气藏全空间磁学、地球化学与矿物学结构及意义--检验"烟筒效应"的形成机理

位于松辽盆地南部某油气田边缘一个油气显示井的磁性测量结果表明,岩石具有明显的磁性变异结构特征.以磁化率(κ)为例,在低缓的背景磁性上主要呈现高强度与中等强度的2类异常:大于400×10-5为强磁性,100×10-5～150×10-5为中等强度磁性.结合录井资料与地球化学分析解释可知,强磁性异常主要位于取样间隔的底部干层区,少数样品位于浅部油气显示层;中等强度异常主要位于2 700 m附近的油气显示层.岩石磁性与地球化学成分对应分析表明,油气显示层岩石的C1和C2成分与磁化率 (κ)、饱和磁化强度 (Js) 和饱和等温剩余磁化强度(SIRM)之间呈明显的正相关,与内禀矫顽力(Hc)为逆相关,而干层岩石相关性不明显.矿物成分分析显示,岩石中主要含铁矿物为磁铁矿、磁赤铁矿、赤铁矿、黄铁矿和菱铁矿.其中磁赤铁矿主要分布在具有中等磁性强度的油气显示层,而高含量(最高含量达12.5%)的磁铁矿主要位于底部干层.磁赤铁矿与赤铁矿、黄铁矿及菱铁矿含量之间相关特征初步表明,自生磁赤铁矿可能主要来源于原地赤铁矿与黄铁矿.推测油气显示层岩石中磁性偏软的磁赤铁矿属于烃蚀变的产物,为烃微渗漏效应(或烟筒效应)的全空间形成机理提供了新证据.