华北回流天气多普勒雷达径向速度分布特征

使用多普勒雷达资料对四次华北回流天气过程进行了分析,结果表明:(1)回波具有较大水平范围的、连绵成片的均匀幕状特征.回波顶较平整,回流降雨过程中还存在零度层亮带.属层状云降水回波.(2)速度图上,在零速度线两侧常分布范围较大数值不等的正负径向速度中心,低空零速度线呈"S"型,风随高度顺时针旋转,有暖平流存在.在强降水时段出现前常伴有区域性的冷平流层.(3)风廓线图上,从低层到高层由东北风转为西南风,风向发生了近180度的顺时针旋转,存在强垂直切变.降水开始与结束时分别表现为低层偏东风与中高层西南气流叠加、低层偏东风与中高层西南气流任何一者消失.边界层顶部出现浅薄的冷平流层是降水强度加强的信号.     

多普勒雷达资料在中尺度模式短时预报中的应用

将国内新一代多普勒雷达基数据Lev-Ⅱ的9个仰角的原始反射率和径向风资料应用于中尺度模式ARPS(the Advanced Regional Prediction System),通过对2007年7月18日济南短时特大暴雨过程的个例研究,分析了雷达资料对初始场的改进效果及其对模拟结果的影响。结果表明,同时利用雷达反射率和径向风资料改进过的初始场能明显改善中尺度数值模式短时定量降水预报。对比风场发现,雷达径向风调整后在初始场中出现明显的中小尺度特征,能减少模式的spin-up时间。随着积分的进行,对水汽场的调节也有一定作用,但相对于风场调节不够显著。雷达反射率主要是改进初始场中的湿度参数,增加初始场中云水等含量。积分开始后,对风场调整也很显著。此次模拟,控制试验较好地预报出雷达回波的分布和水汽中心,对应的降水落区与实况也较为接近,但对雷达回波中心强度的预报略大,相应地降水量的预报也偏大。     

High resolution spectroscopy of two young active late type stars within 20 parsecs of the Sun

We present high-resolution optical echell spectroscopy of HIP 544 and HIP 46843, two nearby solar like stars. The discovery of these young stars at such a close distance to the Sun is really a surprising phenomenon. It will help us to have a better understanding of the structure and evolutionary history of the Milky Way. The radial ve-locities (RV) of HIP 544 and HIP 46843 are measured to be -6.88±0.13km s-1 and 8.30±0.16km s-1, respectively, which are more accurate than before. The equivalent widths (EW) of the Li I 6707.8 A absorption line of HIP 544 and HIP 46843 are mea-sured to be 110±5mA and 195±5mA respectively. Based on these properties, HIP 544 is estimated to be 100-800Myr old and HIP 46843 30-100Myr old using three relatively creditable methods.     

A planetary companion orbiting the intermediate-mass G Giant HD 173416

The discovery of a planetary companion to the intermediate-mass late-type giant star HD173416 from precise Doppler surveys of G and K giants at Xingiong station and Okayama Astrophysical Observatory (OAO) is presented in this letter. The planet has a minimum mass of 2.7 MJ an eccentricity of 0.21, a semimajor axis of 1.16 AU and an orbital period of 324 days.     

Analysis of the three-dimensional stellar velocity field using vector spherical functions

We apply vector spherical functions to problems of stellar kinematics. Using these functions allows all of the systematic components in the stellar velocity field to be revealed without being attached to a specific physical model. Comparison of the theoretical decomposition coefficients of the equations for a particular kinematical model with observational data can provide precise information about whether the model is compatible with the observations and can reveal systematic components that are not described by this model. The formalism of vector spherical functions is particularly well suited for analyzing the present and future (e.g., GAIA) catalogs containing all three velocity vector components: the propermotions in both coordinates and the radial velocity. We show that there are systematic components in the proper motions of Hipparcos stars that cannot be interpreted in terms of the linear Ogorodnikov-Milne model. The same result is also confirmed by an analysis of the radial velocities for these stars.     

WASP-3b: a strongly irradiated transiting gas-giant planet

We report the discovery of WASP-3b, the third transiting exoplanet to be discovered by the WASP and SOPHIE collaboration. WASP-3b transits its host star USNO-B1.0 1256−0285133 every  1.846 834 ± 0.000 002  d. Our high-precision radial velocity measurements present a variation with amplitude characteristic of a planetary-mass companion and in phase with the light curve. Adaptive optics imaging shows no evidence for nearby stellar companions, and line-bisector analysis excludes faint, unresolved binarity and stellar activity as the cause of the radial velocity variations. We make a preliminary spectroscopic analysis of the host star and find it to have   T _eff= 6400 ± 100 K  and  log   g = 4.25 ± 0.05  which suggests it is most likely an unevolved main-sequence star of spectral type F7-8V. Our simultaneous modelling of the transit photometry and reflex motion of the host leads us to derive a mass of  1.76^+0.08_−0.14 M _J  and radius  1.31^+0.07_−0.14 R _J  for WASP-3b. The proximity and relative temperature of the host star suggests that WASP-3b is one of the hottest exoplanets known, and thus has the potential to place stringent constraints on exoplanet atmospheric models.     

论珠江三角洲河网的人为影响

文章论述了珠江三角洲河网的发育、演变过程和整治方案。由于人类活动影响,珠江三角洲河网区西、北两江下游放射状河系支汊淤断及消亡,使西、北两江正干均成为单一水道;在两江汇流区内又受绥江三角洲南展而分离开来,只留一条狭窄的小河涌(思贤)连接;由于北江正干的淤积、西江正干刷深,使古代(唐代以前)西江合北江同流向东流入番禺(广州)的形势大变,形成江水反向西流入西江,西江水不能过入广州。由此,西、北两江合成的珠江三角洲主体网河区成为浅水狭窄的小河区,以往主要干流多不复存在,生态环境日益变劣。因此,需要修复河网。关键是把西江大量优质水源(沙少、污染少)引回,过入珠江三角洲网河区,北江水源也需截流使其不再西流入西江;开通北江大堤沿途防西水的闸门(如芦苞、西南、沙口等闸),以便通水通航;在思贤建立新型分水闸,可将西、北两江正干水源恢复到良好生态环境     

易坍塌地层双管水平定向钻进工艺研究

水平定向钻进技术已被广泛地用于铺设各种管线,具有施工速度快,对地面破坏小,不会影响已有管线的正常使用等优点。但是,在砂卵石和粉细砂类易坍塌地层中,常规的单钻杆水平定向钻进常会出现导向偏差和钻孔坍塌等事故。在已有技术的基础上,开发出了一套双管水平定向钻进系统,包括双回转动力头钻机、内外钻杆、双管导向节。通过现场应用证明了该双管系统具有导向精度高、调整方向灵敏等优点,能克服易坍塌地层带来的导向精度差和钻孔坍塌等难题。     

ICP-AES双向测定土壤中铜、锰、钒、锌金属元素的对比研究

本文采用电感耦合等离子体发射光谱法(ICP-AES)轴向和径向测定土壤中铜、锰、钒、锌四种金属元素的含量,比较分析了在不同三酸[硝酸(HNO3)、氢氟酸(HF)、高氯酸(HCLO4)]用量(配比)下对5种国家标准物质的消解性差异和对四种元素轴向和径向测定结果的影响。结果表明:(1)消解过程中f、g、h配比的三酸消解速度较快,d、e次之,a、b、c相对较慢。(2)对于低含量试样径向观测对轴向观测灵敏度较高;同时三酸消解用量不同,其结果差异性不明显,而发现中高含量范围内横向观测比径向观测相对偏差较小,说明了轴向观测效果较好。(3)通过采用f配比的三酸经过前处理进行稳定性分析,结果可知标准偏差(SD)均小于10,相对标准偏差(RSD)均小于5%,对于高含量锰元素横向观测较径向观测稳定性高,其余元素差异性不明显。     

考虑径向渗透系数变化的真空预压竖井地基固结解析解

针对真空预压条件下竖井地基固结问题,考虑竖井地基扰动区土体径向渗透系数变化的3种模式(扰动区渗透系数为常数、线性变化、抛物线变化)和竖井井阻随时间变化等因素影响;建立数学计算模型,采用解析解法,推导了考虑径向渗透系数因施工扰动而变化的真空预压竖井地基固结问题的解析解。基于此解,编制了计算程序,绘制出了考虑扰动区土体径向渗透系数变化和竖井井阻随时间变化影响的真空预压竖井地基固结曲线图。研究表明:井阻变化率对固结速率有较大影响;在土体扰动区径向渗透系数变化的3种模式中,渗透系数为抛物线变化时固结速率最快,渗透系数为线性时次之,渗透系数为常数时固结速率最慢。