北京市地下水动态监测示范工程的建设和应用

北京市地下水动态监测示范工程是北京市科委的重大项目,从1999年开始建设,到2004年4月全面完成.本文详细介绍了该项目的建设及开发内容,以及在北京市地下水动态监测工作中的应用情况.     

襄樊汉江四桥大口径灌注桩成孔施工实践

介绍了使用泥浆护壁气举反循环回转钻进工艺进行襄樊汉江四桥大口径嵌岩桩的施工实践。施工中采用下置双护简隔离卵石层，合理选用钻头类型(卵砾石层采用五翼合金刮刀钻头，基岩采用球齿滚刀钻头)和钻进参数(混合器沉没深度，尾管长度，孔内空气流量与压力)，摸索与总结出一套复杂地层成孔施工经验。     

GGM02 – An improved Earth gravity field model from GRACE

A new generation of Earth gravity field models called GGM02 are derived using approximately 14 months of data spanning from April 2002 to December 2003 from the Gravity Recovery And Climate Experiment (GRACE). Relative to the preceding generation, GGM01, there have been improvements to the data products, the gravity estimation methods and the background models. Based on the calibrated covariances, GGM02 (both the GRACE-only model GGM02S and the combination model GGM02C) represents an improvement greater than a factor of two over the previous GGM01 models. Error estimates indicate a cumulative error less than 1 cm geoid height to spherical harmonic degree 70, which can be said to have met the GRACE minimum mission goals. Electronic Supplementary Material Supplementary material is available in the online version of this article at     

北京及其周边地区夏季地闪活动时空特征分析

利用M-LDARS闪电定位系统对北京及其周边地区1995～1997年6～9月的闪电观测数据, 分析闪电活动的时空分布特征。结果表明:闪电活动在时间分布上存在两个峰值时段, 13 :00～21:00和23:00～次日05 :00。通过对总地闪、分时段及峰值时段的地闪密度分析, 发现北京及周边地区闪电活动有几个明显的集中区域, 地闪高密度区主要出现在下垫面为山脉和水体的地方, 闪电活动与下垫面的水汽条件关系密切, 且正、负地闪的空间分布也呈现较大差异, 表明雷暴云的电荷结构存在一定差异。     

浅谈 714C型天气雷达的中修

2003年民航哈尔滨空管中心航务气象台对 714C型天气雷达进行中修.在中修中共发现大小故障 86例,雷达的整体性能显著下降,大部分指标值低于标准值.同时在中修过程中,技术人员全面分析雷达出现故障的原因.电子仪器设备在储存、运输和工作中受气候环境、机械环境与电磁环境等因素的影响较大,其中温度、湿度、电源品质等要素的影响在哈尔滨机场体现得较为突出,机场供电经常在 320～ 460V之间波动,给雷达设备造成很大的损害,同时,恶劣的气候条件和工作状况加快了半导体器件、电阻器、电容器、继电器、接插件、及开关等元器件表面氧化、老化的进程、导致电参数退休.根据故障情况进行了综合分析.     

领导人才资源开发经营的实践与思考

人才资源是第一资源，谁拥有人才优势，谁就能抢占事业发展的制高点，因此，对人才资源开发与经营的效益要远远大于对其他资源开发的效益。对山西省气象局近几年来领导人才资源开发与经营的实践进行了详细的探讨和总结，指出领导人才资源开发与经营的基础环节是造拔优势年轻人才，中介环节是创新人才选拔机制，关键环节是优化配置人才资源。     

An algorithm for determination of aerosol opticalthickness from AVHRR imagery over oceans

Summary The uncertainty in aerosol size distributions is a main source of errors in aerosol optical thickness determined from satellite measurements. To reduce the errors resulting from the uncertainty in aerosol size distributions, we have performed sensitivity analyses. It is found the errors resulting from the uncertainty in aerosol size distribution can be considerably reduced by using the Junge power law to approximate the aerosol size distribution in an actual atmosphere, if the exponent value is determined at the same time. An iterative algorithm is then developed for the simultaneous determination of aerosol optical thickness and the exponent of the Junge power law over ocean areas from the upwelling radiances measured in AVHRR visible and near infrared channels. A number of numerical experiments are carried out to investigate the validity of the Junge power law approximation by assuming the aerosol size distributions in an actual atmosphere are bimodal with different mode parameters, and by using the actual aerosol size distributions determined at several places by Kaufman et al. (1994). The results show that the errors in determined aerosol optical thickness resulting from the Junge power law approach are significantly reduced. The iterative algorithm is investigated further by comparing the aerosol optical thickness deduced from satellite measurement with that observed by a sun photometer. Received October 10, 2001 Revised December 28, 2001     

Simulation of the east asian summer monsoon using a variable resolution atmospheric GCM

The East Asia summer monsoon (EASM) is simulated with a variable resolution global atmospheric general circulation model (GCM) developed at the Laboratoire de Météorologie Dynamique, France. The version used has a local zoom centered on China. This study validates the model's capability in reproducing the fundamental features of the EASM. The monsoon behaviors over East Asia revealed by the ECMWF reanalysis data are also addressed systematically, providing as observational evidence. The mean state of the EASM is generally portrayed well in the model, including the large-scale monsoon airflows, the monsoonal meridional circulation, the cross-equatorial low-level jets, the monsoon trough in the South China Sea, the surface cold high in Australia, and the upper-level northeasterly return flow. While the performance of simulating large-scale monsoonal climate is encouraging, the model's main deficiency lies in the rainfall. The marked rainbelt observed along the Yangtze River Valley is missed in the simulation. This is due to the weakly reproduced monsoonal components in essence and is directly related to the weak western Pacific subtropical high, which leads to a fragile subtropical southwest monsoon on its western flank and results in a weaker convergence of the southwest monsoon flow with the midlatitude westerlies. The excessively westward extension of the high, together with the distorted Indian low, also makes the contribution of the tropical southwest monsoon to the moisture convergence over the Yangtze River Valley too weak in the model. The insufficient plateau heating and the resulting weak land-sea thermal contrast are responsible for the weakly reproduced monsoon. It is the deficiency of the model in handling the low-level cloud cover over the plateau rather than the horizontal resolution and the associated depiction of plateau topography that results in the insufficient plateau heating. Comparison with the simulation employing regular coarser mesh model reveals that the local zoom technique improves, in a general manner, the EASM simulation.     

地震勘探资源频率域叠加方法研究

在叠前共深度点道集内各地震道的动、静校正误差很小的情况下，地震资料时间域水平叠加方法有较好的叠加结果。但是，如果动、静校正的误差较大时，叠加效果将受到影响，即叠后振幅和分辨率都会降低。因此，提出一种频率域叠加方法。该方法既具有常规水平叠加方法能提高信噪比的优点，又能将共深度点道集内的走时时差消除，达到内相叠回的目的。几个比较叠加方法效果的有噪CDP道集叠加的例子证明了该方法的效果。     

Spatial structure of the old open cluster NGC 2420

The spatial structure of the intermediate and outer regions of the old open cluster NGC 2420 is analyzed using data from the catalog of Paparó. The differential and integrated distributions of the projected [ΔF(r) and F(r)] and spatial [Δf(r) and f(r)] stellar densities are obtained for various subsystems of cluster stars using Kholopov’s star-count method. Analysis of these curves shows that: (1) the cluster has at least three distinct spatial zones with different stellar-density gradients, (2) the each cluster subsystem has a layered structure, and (3) the spatial structure of the cluster changes systematically in the transition to subsystems containing fainter main-sequence stars. Empirical relations describing the structure of the cluster are also derived. Similar structural features can also be found in other globular and open clusters.