近岸海水质量量化方法及分类评价

近岸海域是陆地、海洋和大气之间各种过程相互作用最活跃的界面[1],沿海100km以内区域聚积着约60%的世界人口[2],其环境质量强烈受人类活动影响.对近岸海域进行水质环境管理,应依据海水物理、化学和生物学性质对海水进行分类评价[3,4].     

银河系中球状星团的空间运动

球状星团是银河系中最古老的天体类型之一,其累积光度很大,是银晕中重要的示踪天体。已以发现的银河系球状星团有１４０多个,其中１２０个银心距Ｒ〈４０Ｋｐｃ的星团已被准确地测定了视向速度。根据结数据以及球状星团金属度的统计分析,可以把球状星团次系再进一步分成某些不同的族群。目前已经测定过绝对自行的球状星团只有３８个,尽管这些自行的精度比视向速度和距离的精度差很多,然而,由此可以得出三维的空间速度,在统计     

球状星团NGC4147的绝对自行和颜色星等图

本文以上海天文台佘山40厘米折射望远镜于1958年拍摄的3张照相底片为第一期,印度Kavalur的234米VainuBappu望远镜于1996年用CCD拍摄的4幅图像为第二期,使用Brosche等1985年发表的球状星团NGC4147天区42颗恒星的位置和绝对自行作为参考架,用中心重叠法进行天体测量归算,得到了这个星团中心附近11'×11'天区内到B＝17.6为止115颗恒星的位置和绝对自行,利用这些自行对成员概率作了估计.本文还给出了用VainuBappu望远镜CCD测光结果得到的这个星因水平文和巨星支恒星V与B-V．V－R和V－I颜色星等图,并对这些颜色星等图和团自行作了讨论,得到这个星团的赤经方向绝对自行为-2.82±0.49mas／yr,赤纬方向绝对自行为2.37±0.43mas／yr.     

疏散星团NGC2244天区恒星的绝对自行研究

利用上海天文台相隔35年的两期照相底片资料,测定了疏散星团NGC2244所在天区55’×55’范围内495颗恒星基于Tycho-2星表的位置和绝对自行,并对自行精度作了初步分析。     

Numerical simulations of the Hyades dynamics and the nature of the moving Hyades cluster

We present our numerical simulations of the dynamical evolution of the Hyades open cluster. The simulations were performed usinga modified NBODY6 algorithm that included tidal forces and a realistic orbit of the cluster in a gravitational field described by the Miyamoto-Nagai potential. Our goal was to study the nature of movingclu sters. We show that the stars that were earlier cluster members could be later identified within a sphere of 50 pc in diameter around the Sun. The number of such stars for the chosen initial mass and virial radius of the cluster does not exceed ten. The maximum space velocity of these stars relative to the core of the current cluster does not exceed 3 km s^?1. Our numerical simulations confirm the assumption that some of the moving clusters near the Sun could consist of stars that have escaped from open clusters in the course of their dynamical evolution.     

Open star clusters in the spiral arms of our Galaxy

We consider the age distributions of open star clusters attributed to three segments of Galactic spiral arms. The smoothed distributions of clusters on the age-Galactocentric angle plane show a great nonuniformity. The time dependence of the formation rate of Galactic disk clusters recovered by taking into account selection effects and dynamical evolution of clusters shows that, on average, the formation rate of open star clusters decreases with time. This is in agreement with the increase in star formation rate into the past, as follows from the study of this process by the method of stellar population synthesis. The present time is the epoch of a current maximum of the cluster formation rate. In addition to the current maximum, there have been at least three more maxima with a period of 300–400 Myr and a duration of no more than 300 Myr. The age distributions are consistent with the pattern of star formation governed by the successive passages of density waves through each examined volume of the Galactic disk. The spiral structure becomes more complex when passing from the inner regions of the Galaxy to its outer regions.     

Geochemical types of pacific polymetallic nodules: An application of multivariate analysis

A total of 843 samples of Pacific Ocean polymetallic nodules (PNs) from five survey areas have been studied (metals analyzed: Mn, Fe, Ni, Cu, Co, Zn, Pb). The statistical analysis included the following techniques: factor R analysis, quick cluster Q analysis into 50 preclasses, various hierarchical cluster Q analyses (HCAs) using the preclasses (application of different HCAs to an identical set of data and of an identical HCA to two different subsets of the data), comparison of the HCA. The PNs of the survey areas can be grouped into five geochemical types (I‐V). The genesis of the PNs was interpreted as early diagenetic, hydrogenetic, and mixed (early diagenetic/hydrogenetic and hydrogenetic/hydrothermal. In addition, some further conclusions regarding the applicability of various HCA techniques depending on the structure of the data set have been drawn.     

基于系统聚类分析的西部地区环境污染程度评价

随着社会经济的不断发展,环境污染问题在西部地区经济发展中越来越凸显出来,不同省区受到不同程度的影响.同时,不同地区的环境污染问题有一定的相似性.应用系统聚类分析方法,通过提炼选取11类指标,对西部地区12省区环境污染程度的距离相似情况进行了评价.结果表明:贵州、甘肃、广西、云南、重庆和陕西等省区的距离相似归为第一类聚类;内蒙古和四川归为第二类聚类;西藏、宁夏和青海等省区的距离相似属于第三类聚类;新疆归为第四类聚类.要处理好生态系统和社会经济发展之间的关系,需要对二者进行协调,并坚持走可持续发展的道路.     

胶东山城金矿地质与地球化学变量的关系

为研究胶东地区山城金矿的控制因素和预测隐伏矿体,利用R型因子分析和聚类分析揭示了各种地质和地球化学变量的关系。同时,针对聚类分析中难以有效显示变量间负相关问题提出了反序变换的方法。结果表明,该矿的黄铜矿化、脉状黄铁矿化、Au-Ag-Cu组合与As-Sb-Hg组合相关,并受主构造面走向波动控制;而较厚石英脉、菱铁矿化、星散状黄铁矿化、Pb-Ba组合与Co-Ni组合相关,并受主构造面倾向波动控制。这些结果与地质结论一致,但研究方法更简便快捷。     

典型构造蚀变岩型金矿远景资源量数学模型与预测

数学模型是矿床深部资源量定量化预测一个重要手段,其中品位-吨位模型是一个广泛应用的数学模型,在该模型中,远景资源量为研究区源岩中成矿元素总量的函数。利用该模型,计算胶东构造蚀变岩型金矿远景资源量时,发现由于成矿源岩范围难以确定,而使模型应用准确性受到制约。基于断裂带蚀变岩型金矿的特征,修正了品位-吨位模型。在修正后的模型中,远景资源量为蚀变岩总质量的函数,另包括3个参数:蚀变区元素背景含量(由多标度分形决定)、元素工业品位及矿体品位分布分维值。利用修正后的品位-吨位模型,有效地估算了胶东大尹格庄金矿-1000m以上的理想金属量,得出远景矿石量为5.26×107t,金属量为2.89×105kg,与实际地质情况相吻合。