TBP－（X－5）反相色谱分离m－NPF分光光度法测定铀

本文研究了以磷酸三丁酯为固定相，大孔聚乙烯苯（Ｘ－５型）为担体的浸渍树脂、垂直型反相色谱柱，对铀分离富集的基本性能，以及铀（Ⅳ）－间硝基苯基萤光酮（ｍ－ＮＰＦ）一氨三乙酸（ＮＴＡ）－吐温－８０显色体系的反应条件，提出了ＴＢＰ（Ｘ－５）分离，ｍ－ＮＰＦ－ＮＴＡ－吐温－８０光度法测定铀，经标准样品验证，结果满意。     

采用小径密抗桩一条龙抢治滑坡的方法及效果

以往整治滑坡,较多地使用大口径挖孔桩或钻孔灌注抗滑桩,周期长、成本高。川地208队在治理重庆制药五厂已处于危急态势的滑坡中,采用“天平式”控制、勘治结合、快速抢险,用三排小径密抗桩(300mm口径)整治,取得明显成效。实践表明:浅层滑坡采用较小口径的密抗桩,并辅以排水,能达到事半功倍的效果。     

When are relative variograms useful in geostatistics?

The relative variogram has been employed as a tool for correcting a simple kind of nonstationarity, namely that in which local variance is proportional to local mean squared. In the past, this has been linked in a vague way to the lognormal distribution, although if {Z_t; t D}is strongly stationary and normal over a domain D,then clearly {exp (Z_t); t D}will stillbe stationary, but lognormal. The appropriate link is made in this article through a universal transformation principle. More general situations are considered, leading to the use of a scaled variogram.     

A Discrete Wavenumber Boundary Element Method for study of the 3-D response 2-D scatterers

A mathematical formulation of the 2·5D elastodynamic scattering problem is presented and validated. The formulation is a straightforward extension of the Discrete Wave number Boundary Integral Equation Method (DWBIEM) originally proposed by Kawase¹ for 2D scattering problems and subsequently extended to the 3D problem by Kim and Papageorgiou.² It is demonstrated that the Green's function which is appropriate for a boundary formulation of the 2·5D elastodynamic scattering problem is the one corresponding to a unit force moving on a straight line with constant velocity. Such a Green's function is derived in the present study. The formulation may be used to study the wavefields in models of sedimentary deposits (e.g. valleys) or topography (e.g. canyons or ridges) with a 2D variation in structure but obliquely incident plane waves. The advantage of a 2·5D formulation is that it provides the means for calculations of 3D wavefields in scattering problems by requiring a storage comparable to that of the corresponding 2D calculations. © 1998 John Wiley & Sons, Ltd.     

A unique Galactic planetary nebula with a [WN] central star

We report the discovery of the first probable Galactic [WN] central star of a planetary nebula (CSPN). The planetary nebula candidate was found during our systematic scans of the AAO/UKST Hα Survey of the Milky Way. Subsequent confirmatory spectroscopy of the nebula and central star reveals the remarkable nature of this object. The nebular spectrum shows emission lines with large expansion velocities exceeding 150 km s⁻¹, suggesting that perhaps the object is not a conventional planetary nebula. The central star itself is very red and is identified as being of the [WN] class, which makes it unique in the Galaxy. A large body of supplementary observational data supports the hypothesis that this object is indeed a planetary nebula and not a Population I Wolf–Rayet star with a ring nebula.     

用MM5模式Reisner霰方案对华南暴雨的数值模拟

利用MM5中尺度数值模式对1998年6月8～9日华南暴雨进行了模拟，用Re—isner在方案模拟了可分辨尺度降水，详细分析了暴雨的微物理过程。结果表明，Re—isner在方案对华南暴雨具有较好的模拟能力。在降水最大时段，霰和云水是形成雨水的主要来源，云水的碰冻是产生霰的主要微物理过程。     

基于定向片模型的SPOT-5遥感影像自检校光束法平差

本文通过建立内方位自检校模型,利用定向片模型对外方位元素进行内插建模,建立了基于定向片模型的自检校光束法平差,研究不同控制点数量和不同定向片间隔对定位精度的影响,并利用河南嵩山地区SPOT-5遥感影像数据对模型进行了实验验证和分析,结果表明,平面精度可以达到10.06m,高程精度可以达到8.84m.     

基于再分析资料ERA5的对流层延迟估计方法及精度评估

提出基于再分析资料ERA5的天顶对流层延迟计算方法,使用中国大陆构造环境监测网络提供的26个GNSS测站2017年全年数据,评估由该方法计算的天顶对流层延迟的精度,并与前一代再分析资料ERA-Interim的计算结果进行对比分析。结果显示,ERA5计算的天顶对流层延迟均方根误差比ERA-Interim计算结果低,表明新一代产品的精度有明显提升。