从PM10的测量推测成都市区汞污染的来源     

李奕霖  ;张成江  ;施泽明  ;郭亚杰 《辽宁气象》2007,(6):68-71

通过2007年5—6月期间测量成都市若干条剖面上大气可吸入颗粒物（PM10）中的汞含量，来推测成都市大气中汞的来源。结果表明：在12个点的测量范围内，成都市PM10的质量平均浓度为210．8μg／m^3；PM10中汞的质量平均浓度为0．36ng／m^3。公园和郊区PM10浓度和其中汞浓度均较少，可能与植被茂盛有关。由PM10中汞的分布可知，在热电厂、停用的生活垃圾堆放场和寺庙附近出现最高值。说明热电厂和生活垃圾堆放场是大气汞污染的重要次生来源。寺庙附近出现的高汞值，推测与寺庙的礼仪活动如香烛燃烧有关。  相似文献   

地铁隧洞带水作业施工技术          下载免费PDF全文

罗启录 《探矿工程》2007,34(3):58-60

以在建的北京地铁十号线双井一劲松区间暗挖隧道为例，通过分析北京特殊地层在带水条件下单洞结构单线隧道台阶法的施工工艺，洞悉浅埋暗挖正台阶法施工中超前预加固、开挖时空顺序、台阶长度等工艺对围岩稳定性的影响程度。  相似文献   

兰州市取暖期可吸入颗粒物中单颗粒矿物组成特征   总被引：1，自引：1，他引：1  

肖正辉  邵龙义  孙珍全  张宁  李卫军 《矿物岩石地球化学通报》2007,26(1):64-69

为研究兰州市2005年冬季大气可吸入颗粒物(PM10)中单颗粒的矿物组成,用能谱扫描电镜识别和统计了兰州市区(东方红广场)和郊区(榆中县)两个采样点的单矿物颗粒。结果在市区样品中识别出方解石、伊/蒙混层、石英、斜长石、伊利石、石膏、绿泥石、高岭石、浊沸石和钾长石等21种矿物,前7种占统计总量的75%以上;郊区样品中识别出20种矿物,以方解石、石英、伊利石、绿泥石、斜长石和伊/蒙混层为主(占70%以上),与市区相比缺少钾石膏、金红石和水铝酸钙而增加了硫酸镁和磷灰石。总体来看,大气PM10中的矿物颗粒可分为粘土类、长石类、碳酸盐类、硫酸盐类、氧化物类和其他六类,以粘土类和碳酸盐类矿物为主(约占60%);冬季市区颗粒物表面的“硫化”现象较郊区严重;这些矿物颗粒主要来自地表土,人为排放和大气中二次化学反应生成的矿物的贡献较小。  相似文献   

2004年春季中国沙尘天气特征分析          下载免费PDF全文

周自江  牛若芸 《气象科学》2007,27(1):69-75

利用全国681个站的沙尘天气观测资料分析得出,2004年春季中国北方的沙尘天气明显偏少、偏弱,主要表现在：（1）2004年春季681个站累计的沙尘天气日数2 080 d,相当于历史平均值的46.9%,是近四十余年中第三个偏少年份。沙尘暴的总面积约190万km2,仅为历史平均值的37.3%。（2）危害性较大的沙尘暴和强沙尘暴过程6次,不足2001年的一半。（3）4月和5月沙尘天气明显偏少导致整个春季显著偏少。沙尘天气出现时,PM10浓度相对增加,空气质量恶化,但与历史上较典型的强沙尘暴个例相比,PM10浓度增加的幅度不大。进一步分析表明,2004年春季沙尘天气偏少、偏弱的主要原因是大气动力条件不足,是比较特殊的一个年份。  相似文献   

The complex gravitational lens system B1933+503     

C. M. Sykes  I. W. A. Browne  N. J. Jackson  D. R. Marlow  S. Nair  P. N. Wilkinson  R. D. Blandford  J. Cohen  C. D. Fassnacht  D. Hogg  T. J. Pearson  A. C. S. Readhead  D. S. Womble  S. T. Myers  A. G. de Bruyn  M. Bremer  G. K. Miley  & R. T. Schilizzi 《Monthly notices of the Royal Astronomical Society》1998,301(2):310-314

We report the discovery of the most complex arcsec-scale radio gravitational lens system yet known. B1933+503 was found during the course of the CLASS survey and MERLIN and VLA radio maps reveal up to 10 components. Four of these are compact and have flat spectra; the rest are more extended and have steep spectra. The background lensed object appears to consist of a flat-spectrum core (quadruply imaged) and two compact 'lobes' symmetrically disposed relative to the core. One of the lobes is quadruply imaged while the other is doubly imaged. An HST observation of the system with the WFPC2 shows a galaxy with an axial ratio of 0.5, but none of the images of the background object is detected. A redshift of 0.755 has been measured for the lens galaxy.  相似文献   

Modelling the 10-image lensed system B1933+503     

S. Nair 《Monthly notices of the Royal Astronomical Society》1998,301(2):315-322

A gravitational lens model is presented for the newly discovered 10-image system B1933+503. The underlying object, revealed by modelling, is a triple radio source on the scale of a couple of hundred mas that is well-aligned along the line of sight with a foreground and somewhat flattened lensing galaxy, the orientation and location of which match those of an observed galaxy, known to be at a redshift of 0.755. Uncertainties in the modelling are obtained by a Monte Carlo exercise. Observational tests of the lens model are proposed, and the time delays between various pairs of images are determined, as the core of the source is known to be significantly variable. Future observations of the lens hold the key to using B1933+503 to constrain Hubble's constant. Despite the absence of a source redshift, the utility of the system as a probe of the structure of the lens galaxy is unparalleled as it provides a surfeit of easily identifiable constraints for modelling the system.  相似文献   

A timing formula for main-sequence star binary pulsars     

Norbert Wex 《Monthly notices of the Royal Astronomical Society》1998,298(1):67-77

In binary radio pulsars with a main-sequence star companion, the spin-induced quadrupole moment of the companion gives rise to a precession of the binary orbit. As a first approximation one can model the secular evolution caused by this classical spin-orbit coupling by linear-in-time changes of the longitude of periastron and the projected semi-major axis of the pulsar orbit. This simple representation of the precession of the orbit neglects two important aspects of the orbital dynamics of a binary pulsar with an oblate companion. First, the quasiperiodic effects along the orbit, owing to the anisotropic 1/ r ³ nature of the quadrupole potential. Secondly, the long-term secular evolution of the binary orbit, which leads to an evolution of the longitude of periastron and the projected semi-major axis, which is non-linear in time.   In this paper a simple timing formula for binary radio pulsars with a main-sequence star companion is presented which models the short-term secular and most of the short-term periodic effects caused by the classical spin-orbit coupling. I also give extensions of the timing formula that account for long-term secular changes in the binary pulsar motion. It is shown that the short-term periodic effects are important for the timing observations of the binary pulsar PSR B1259–63. The long-term secular effects are likely to become important in the next few years of timing observations of the binary pulsar PSR J0045–7319. They could help to restrict or even determine the moments of inertia of the companion star and thus probe its internal structure.   Finally, I reinvestigate the spin-orbit precession of the binary pulsar PSR J0045–7319 since the analysis given in the literature is based on an incorrect expression for the precession of the longitude of periastron. A lower limit of 20° for the inclination of the B star with respect to the orbital plane is derived.  相似文献   

参数调整对气象预测的B-P网络模型性能的影响     

邓新民  顾永刚 《成都信息工程学院学报》1998,(1)

为了探索ＢＰ网络的参数调整特性,进行了参数α、β的选取对ＢＰ算法的收敛速度和模型的稳定性的影响研究。通过ＢＰ网络用于气象预测建模的参数调整个例分析表明：参数α、β的取值对ＢＰ模型的稳定性无显著影响,但参数值的调整尤其是β值的调整对建模的收敛速度有明显的影响。  相似文献   

Mathematical Modelling and Accuracy Testing of Spot Level 1B Stereopairs     

M. J. Valadan Zoej  & G. Petrie 《The Photogrammetric Record》1998,16(91):67-82

During a project concerned with DEM generation using SPOT stereoscopic imagery, difficulties were experienced when using Level 1B stereopairs for the task. This paper presents a mathematical solution to overcome this problem which has been implemented at the University of Glasgow. Results are included from experimental tests which were carried out over a test field in Jordan using this solution. These tests used five SPOT Level 1B stereopairs together with a single SPOT Level 1A stereopair for comparative purposes. The residual errors at the ground control points and independent check points are given and show that a satisfactory solution was achieved.  相似文献   

陕西段家坡黄土剖面中布容／松山古地磁界线附近铱异常的发现及其启示   总被引：3，自引：0，他引：3  

马配学  侯泉林 《地质学报》1998,72(2):173-177

利用高灵敏度放射化学中子活化分析方法,对我国陕西段家坡黄土剖面早－中更新统（约０．７３Ｍａ）沉积界线附近铱和其它元素的丰度进行了测定。结果表明,在布容／松山（Ｂ／Ｍ）古地磁界线附近铱的含量明显增大,最大值为４６．３ｐｇ／ｇ。相对于整个剖面的平均背景值（约１５ｐｇ／ｇ）大约富集了３倍。用地壳元素钪进行标准化之后,铱异常十分明显,而其它元素在界线附近则没有变化。黄土剖面上铱异常的赋存层位与西南太平洋钻  相似文献