The pulsational behaviour of the rapidly oscillating Ap star HD 122970 during two photometric multisite campaigns

We undertook two time-series photometric multisite campaigns for the rapidly oscillating Ap star HD 122970. The first one, conducted in 1998, resulted in 119 h of data and in the detection of three pulsation frequencies. The presence of possible further modes which held the promise of deriving a mode identification motivated a second worldwide campaign in the year 2001. This second campaign resulted in 203 h of measurement, but did not reveal further modes. Rather, one of the previously detected signals disappeared. The two modes common to both data sets have different spherical degree. They also showed slight frequency modulation, and one of them varied in amplitude as well. Possible causes of the latter behaviour include intrinsic instability of the pulsation spectrum or precession of the pulsational axis and orbital motion in a binary system. Frequency analysis of the Hipparcos observations of the star did not allow us to determine the stellar rotation period. The amplitude and phase behaviour of the two modes of HD 122970 in the Strömgren uvby bands is quite similar to that observed for other roAp stars.     

A conceptual–numerical model to simulate hydraulic head in aquifers that are hydraulically connected to surface water bodies

In this paper, we present a conceptual‐numerical model that can be deduced from a calibrated finite difference groundwater‐flow model, which provides a parsimonious approach to simulate and analyze hydraulic heads and surface water body–aquifer interaction for linear aquifers (linear response of head to stresses). The solution of linear groundwater‐flow problems using eigenvalue techniques can be formulated with a simple explicit state equation whose structure shows that the surface water body–aquifer interaction phenomenon can be approached as the drainage of a number of independent linear reservoirs. The hydraulic head field could be also approached by the summation of the head fields, estimated for those reservoirs, defined over the same domain set by the aquifer limits, where the hydraulic head field in each reservoir is proportional to a specific surface (an eigenfunction of an eigenproblem, or an eigenvector in discrete cases). All the parameters and initial conditions of each linear reservoir can be mathematically defined in a univocal way from the calibrated finite difference model, preserving its characteristics (geometry, boundary conditions, hydrodynamic parameters (heterogeneity), and spatial distribution of the stresses). We also demonstrated that, in practical cases, an accurate solution can be obtained with a reduced number of linear reservoirs. The reduced computational cost of these solutions can help to integrate the groundwater component within conjunctive use management models. Conceptual approximation also facilitates understanding of the physical phenomenon and analysis of the factors that influence it. A simple synthetic aquifer has been employed to show how the conceptual model can be built for different spatial discretizations, the parameters required, and their influence on the simulation of hydraulic head fields and stream–aquifer flow exchange variables. A real‐world case was also solved to test the accuracy of the proposed approaches, by comparing its solution with that obtained using finite‐difference MODFLOW code. Copyright © 2011 John Wiley & Sons, Ltd.     

基于光变曲线的空间碎片基本形状分类

将未编目的空间碎片正确分类是空间态势感知的重要组成部分. 基于光变曲线, 通过仿真和实测实验, 探讨了空间碎片基本类型的机器学习分类方法. 在数据集中的仿真光变来自形状或材料不同的4类碎片, 实测光变从Mini-Mega TORTORA (MMT)数据库中提取, 实验以深度神经网络作为分类模型, 并和其他机器学习方法进行了比较. 结果显示深度卷积网络优于其他算法, 在仿真实验中对不同材料的圆柱体都能准确识别, 对其余两类卫星的识别率在90%左右; 实测实验中对火箭体和失效卫星的2分类准确率超过99%, 然而在进一步的型号/平台分类中, 准确率有所降低.     

东川式层状铜矿40Ar-39Ar成矿年龄研究：华南地区晋宁-澄江期成矿作用新证据

本文采用^40Ar-^39Ar真空击碎技术和阶段加热技术，测定了采自落雪矿的“东川式”层状铜矿之两个石英样品的年龄，获得了810-770Ma的^40Ar-^39Ar等时线年龄，这是首次获得的“东川式”铜矿的成矿年龄。这些年龄与作者以前获得的脉状铜矿石英的年龄范围一致，远远小于赋矿围岩落雪组的年龄，研究结果表明“东川式”层状铜矿并非沉积成因，与脉状铜矿一样，也是热液成因，并且再次证实晋宁-澄江期是东川铜矿的主要成矿期。     

太阳系外行星的凌星观测研究

为对太阳系外行星的物理参数进行更精确估算,利用山东大学威海天文台/威海市天文台的1 m反射望远镜,对7颗已知具有行星系统的恒星:TrES-1、TrES-3、XO-2、WASP-1、WASP-2、WASP-3、HAT-P-7,进行了凌星现象的观测研究.介绍观测和数据处理的基本情况,给出凌星光变曲线结果及由之推算出的一些行星参数.在总结结果并加以分析的同时,展望下一步将进行的更为深入细致的研究.     

巴基斯坦雷克迪克斑岩型Cu Au矿集区典型矿床闪长岩Pb、Sr、Nd同位素组成特征及其示踪意义

雷克迪克斑岩型Cu-Au矿集区是巴基斯坦最重要的斑岩型Cu-Au矿产地之一,发育20个斑岩型Cu-Au矿床(点),其中包括世界级的H14、H15矿床。本文在前人研究基础上重新分析探讨了Pb、Sr、Nd同位素的组成特征,计算了铅同位素的H-H单阶段演化模式年龄,以及Pb、Sr、Nd同位素的μ、ω、Th/U、△α、△β、εSr、εNd等重要参数。研究结果表明,雷克迪克矿集区成矿物质主要来源于受岩浆作用控制的壳幔混合物质,是新特提斯洋岩石圈俯冲及再循环或幔源岩浆注入地壳的结果。该矿集区的含矿斑岩可能是在岛弧碰撞造山带演化过程中伴随着特提斯构造域的演化而形成的,属于洋壳俯冲消减和大陆碰撞过程中导致地壳增生加厚的结果,它们与扬子地块具有亲缘关系,属于特提斯构造区,构成了特提斯构造域多岛洋体系的组成部分之一。该矿集区的铅主要为混入了放射性成因Pb的混合铅,具有典型DUPAL异常的特征。其中,异常铅(放射性铅)来源于富含U、Th的上地壳物质,而DUPAL异常可能直接产生于欧亚大陆南缘EMII与DM的混合源区,并以异常铅的形式表现出来。     

在线示踪试验在隧道建设前期勘察中的应用研究以重庆城开高速公路拟建旗杆山隧道为例

由于岩溶含水介质具有高度不均一性和复杂性,给隧道建设带来很多不确定因素。本文以城开高速公路城口拟建旗杆山隧道为例,利用在线示踪技术,获取高分辨率示踪数据,结合定量解译的方法,分析隧址区岩溶地下水潜在的流向及其流场情况。本次在钻孔内注入投放示踪剂,开展示踪工作,通过试验结果查清了投放示踪剂位置地下水与水文单元内几个大型暗河的水力联系,为划分地下水分水岭和计算隧址区岩溶管道流水力梯度提供了有力依据,该成果极大地提高了隧址区水文地质调查工作的精度。通过本例,表明在线示踪技术在我国西南岩溶区的地下含水介质研究及相关的勘察中具有较大的推广和应用价值。     

福建惠安沿海大气扩散特性的数值分析与模拟

用福建惠安地区的实测气象资料,结合风场诊断、轨迹分析和随机游走模拟方法,分析惠安核电厂所在地小尺度(40 km×40 km)范围内的大气扩散特性,并与现场扩散示踪实验数据比较.结果表明,该地区的扩散输送总体受天气系统和海陆风环流二因子影响.研究范围内的风场,在水平方向的空间变化不大,扩散烟流基本平直.海陆风环流因子所致的风场时间变化和风向摆动对当地扩散有重要意义.随机游走模拟方法较好地反映出当地大气扩散的定量特征,但复杂地形与海岸气象条件的联合作用,仍使模拟结果与示踪实验结果的统计比较显得离散.     

重庆市金佛山台原岩溶地下水系统结构特征分析

为了查明金佛山各洞穴之间的地下水力联系,探讨岩溶地下水系统结构特征,于2016年12月进行了多元示踪试验。将罗丹明B作为示踪剂,从药池坝附近消水洞（S01）投入,验证消水洞与北坡水源（水房泉）（S02）之间存在水力联系。结果显示,示踪剂历时曲线为多峰型,推测地下过水通道可能由单管道型演变为多管道型通道;将荧光素钠投入金佛洞地下水流动处（S05）和将罗丹明B、荧光增白剂投入羊口洞地下水流动处（S03）,利用高分辨率荧光光度计,于燕子洞（S04）在线监测。结果显示,金佛洞、羊口洞分别与燕子洞之间存在水力联系,且示踪剂历时曲线均为跳跃型,推测地下过水通道可能为发育有一定规模溶潭的多管道型。