氯化钾与硫酸钠制硫酸钾工艺的优化

根据 K+ ,Na+∥ Cl-,SO4 2 -— H2 O体系相图 ,提出了氯化钾与芒硝制备硫酸钾工艺中新的工业化生产循环和解决钾芒硝富集问题的具体方案 ,取得良好效果。     

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.     

Relative variation diagrams for describing patterns of compositional variability

In recognizing that a composition, such as a major oxide or sediment composition, provides information only about the relative, not the absolute, magnitudes of its components, this paper exposes the compositional variation array as the simplest and minimum way of summarizing the pattern of variability within a compositional data set. Such summaries are free of the notorious hazards of the constant-sum constraint and when depicted in relative variation diagrams can often provide substantial insights into the nature of the compositional variability. Concepts and practice are illustrated by reference to a number of real data sets.     

NGC 6404 and 6583: two neglected intermediate-age open clusters located in the Galactic Centre direction

We report on VI charge-coupled device photometry of two fields centred in the region of the open clusters NGC 6404 and 6583 down to   V = 22.0  . So far these clusters have never been studied, and we provide for the first time estimates of their fundamental parameters, namely, radial extent, age, distance and reddening. We find that the radius of NGC 6404 is 2.0 arcmin, as previously proposed, while the radius of NGC 6583 is 1.0 arcmin, significantly lower than previous estimates. Both clusters turn out to be of intermediate age (0.5–1.0 Gyr old), and located inside the solar ring, at a Galactocentric distance of about 6.5 kpc. These results make these objects very interesting targets for spectroscopic follow-up to measure their metallicity. In fact, they might allow us to enlarge by more than 1 kpc the baseline of the radial abundance gradient in the Galactic disc towards the Galactic Centre direction. This baseline is currently rather narrow especially for clusters of this age.     

贵州省未来气候变化(2018—2050年)预估分析

针对贵州省年平均降水量,年平均气温,年平均最高气温和年平均最低气温四个特征量,从空间分布上的定性比较,从年际、年代际的时间演变比较以及从泰勒图的定量比较来看,RegCM4模式的模拟效果优于CMIP5模式,因此本研究在RCP4.5排放情景下利用RegCM4模式数据预估未来2018—2050年贵州省年平均降水量,年平均气温,年平均最高气温和年平均最低气温。结果表明:21世纪Ⅰ阶段(2018—2028年)相对于基准期年平均降水在全省大部地区均是偏少的,偏少幅度在8.5%以内,其中贵州省北部地区偏少幅度最大;21世纪Ⅱ阶段(2029—2039年)相对于基准期贵州省中西部降水偏少东部降水偏多,变化幅度基本上在7%以内;21世纪Ⅲ阶段(2040—2050年)相对于基准期贵州省南部和东部降水偏少西北部降水偏多,变化幅度基本上在7.5%以内。贵州省21世纪Ⅰ阶段、Ⅱ阶段、Ⅲ阶段年平均气温、年平均最高气温和年平均最低气温相对于基准期均是偏暖的,偏暖幅度在0.6～1.3℃之间,越到后期,偏暖幅度越大,且空间差异不大。     

A COMPARISON AND EVALUATION OF TWO CENTENNIAL-SCALE SEA SURFACE TEMPERATURE DATASETS IN THE CHINA SEAS AND THEIR ADJACENT SEA AREAS

Two reconstructed sea surface temperature(SST) datasets(HadISST1 and COBE SST2) with centennial-scale are compared on the SST climate change over the China Seas and their adjacent sea areas. Two independent datasets show consistency in statistically significant trends, with a warming trend of 0.07—0.08 ℃ per decade from 1890 to2013. However, in shorter epochs(such as 1961—2013 and 1981—2013), HadISST1 exhibits stronger warming rates than those of COBE SST2. Both datasets experienced a sudden decrease in the global hiatus period(1998—2013), but the cooling rate of HadISST1 is lower than that of COBE SST2. These differences are possibly caused by the different observations sources which are incorporated to fill with data-sparse regions since 1982. Different data sources may lead to higher values in HadISST1 from 1981 to 2013 than that in COBE SST2. Meanwhile, the different data sources and bias adjustment before the World War II may also cause the large divergence between COBE SST2 and HadISST1,leading to lower SST from 1891 to 1930. These findings illustrate that the long-term linear trends are broadly similar in the centennial-scale in the China Seas using different datasets. However, there are large uncertainties in the estimate of warming or cooling tendency in the shorter epochs, because there are different data sources, different bias adjustment and interpolation method in different datasets.     

Voronoi tessellation on the ellipsoidal earth for vector data

Voronoi tessellation, and its dual the Delaunay triangulation, provide a cohesive framework for the study and interpretation of phenomena of geographical space in two and three dimensions. The planar and spherical solutions introduce errors in the positional accuracy of both Voronoi vertices and Voronoi edges due to errors in distance computations and the path connecting two locations with planar lines or great circle arcs instead of geodesics. For most geospatial applications the introduction of the above errors is insignificant or tolerable. However, for applications where the accuracy is of utmost importance, the ellipsoidal model of the Earth must be used. Characteristically, the introduction of any positional error in the delimitation of maritime zones and boundaries results in increased maritime space for one state at the expense of another. This is a situation that may, among others, have a serious impact on the financial activities and the relations of the states concerned. In the context of previous work on maritime delimitation we show that the Voronoi diagram constitutes the ideal solution for the development of an automated methodology addressing the problem in its entirety. Due to lack of a vector methodology for the generation of Voronoi diagram on the ellipsoid, the aforementioned solution was constrained by the accuracy of existing approaches. In order to fill this gap, in this paper we deal with the inherent attributes of the ellipsoidal model of the Earth, e.g. the fact that geodesics are open lines, and we elaborate on a methodology for the generation of the Voronoi diagram on the ellipsoid for a set of points in vector format. The resulting Voronoi diagram consists of vertices with positional accuracy that is only bounded by the user needs and edges that are comprised of geodesics densified with vertices equidistant to their generators. Finally, we present the implementation of the proposed algorithm in the Python programming language and the results of two case studies, one on the formation of closest service areas and one on maritime boundaries delimitation, with the positional accuracy set to 1 cm.     

温泉台体应变观测的影响因素及特征分析

为定量估计观测序列所包含的各种成分,评定台站的观测环境、观测质量及对地形变的监测能力,加深对观测数据的理解,准确识别震前异常,以温泉台体应变为例,选择体应变、辅助观测及气象三要素等观测数据,利用别尔采夫滤波、小波分析和相关性分析等方法,分析温泉台体应变观测各周期变化的影响因素及特征。结果表明：1）温泉台体应变年周期变化的影响因素可能为钻孔水位,体应变相位滞后水位约31 d;2）气压是温泉台体应变月波的主要影响因素;3）固体潮汐是温泉台体应变日波、半日波的主要影响因素;4）温泉台体应变与水位、气压、固体潮汐等具有较强的线性相关性。     

点状地名信息的加权泰森多边形检索法

鉴于地名库中多数地名仅以中心点坐标形式记录其空间位置信息,缺乏其空间范围的具体描述,造成地名检索中的片面性和局限性,本文在深入分析地名及其空间属性、空间关系的基础上,考虑同类型地名的不同性质在检索中的重要作用,利用泰森多边形在地名边界近似中的优势,提出了针对点状地名信息的加权泰森多边形检索法,依据同类型地名的面积属性作为权重指标构建泰森多边形,以近似表达地名的空间范围,进而描述地名间的各类空间关系;并从拓扑关系、方位关系与距离关系3个方面给出了具体公式以计算地名间的空间相似性;最后以行政区划边界近似与检索为例验证该方法。试验结果表明,该方法可较好地近似表达地名空间范围及空间关系,增强了检索词与地理信息资源在空间位置上的相似性度量,检索结果优于传统方法。     

邻接凸多边形方向关系计算及其推理

在对拓拟邻接凸多边形方向关系计算特殊性分析的基础上，提出了一个邻接凸多边形方向关系计算法和二维空间方向关系推理方法。与Voronoi图所表达的邻近拓扑关系相结合，该算法可以用于计算离散二维空间目标之间的方向关系。