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Evaluation of Fluorobenzoate Tracers in Surface Soils 总被引:2,自引:0,他引:2
Dan B. Jaynes 《Ground water》1994,32(4):532-538
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In the Gyldén problem, the case of slowly changing equivalent gravitational parameter (e.g.p.) is studied. Assuming the following
law for the variation of the e.g.p.: μ (t) = μ0+ εμ (εt), ε< μ0, we obtained a) a O(ε4 T4)-approximation of the solution, on a shortened time scale (0,T), with T of order o(ε-1),for the general case (i.e. the support function μ is O(1)-valued and admits an expansion in power series of its argument),
and b) a O(ε2)-approximation of the solution, on a natural timescale of order O(1/ε), for the case of a bounded variation rate (i.e. the
support function μ and its derivative are both O(1)-valued). For the study of the first problem we introduced a type of Lissajous
variables and used the Lie-Hori normalization scheme; for the second problem we used the Delaunay variables and applied the
von Zeipel method for approximate integration. The physical interpretation of the results is in both cases the same: within
the corresponding limits of approximation, the variation of e.g.p. (i) has no effect on the size of the osculating ellipse,
(ii) it sets the pericenter in slow rotation and (iii) it introduces a secular variation in the longitudes.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
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中国虚拟天文台图像处理分析工具(VO_IMPAT),是由国家天文台虚拟天文台项目组开发的一项服务,它提供了对数字巡天图像数据(Digital Sky Survey,DSS)、天文星表以及其他数据库的交互访问。VO_IMPAT的设计目的是实现多波段天文数据的融合。可以将不同波段的星表叠加到DSS底图上,如光学波段的USNO星表、近红外波段的2MASS星表、射电波段的NVSS星表和X射线波段的RASS星表。同时VO_IMPAT还可以对图像进行放大、缩小、伪彩色、等高线、直方图、尖锐化、平滑化、旋转等处理,不同的星表数据可以采用不同的颜色和图标显示。 相似文献
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Dan Gill 《Mathematical Geology》1993,25(4):471-482
The ability of association analysis to discriminate sedimentary facies was tested on Purdy's modal analyses of modern sediments of the Great Bahama Bank. Purdy's data set has served in the past as a standard reference for evaluating various multivariate classification algorithms. In order to adapt Purdy's data to association analysis, the percent abundance of the 12 constituents was converted to binary form by dichotomizing each variable on its mean value. The results obtained by association analysis are virtually identical to those obtained by Purdy and other authors. The same four main sedimentary facies were discriminated; 86% of the samples were identically classified (97% when misclassified borderline cases are counted as matches); the total partition variance of the classification is only negligibly greater (4%); and the grouping of the variables yielded the same four groups. The rank order of the three division-attributes responsible for the sample classification is fines, oolites, and corals. Association analysis has been employed by other authors to differentiate meaningful facies groups in studies of ancient reef carbonates, modern reef sediments, and heavy minerals in stream sediments. In all these studies, the results were found to be compatible with those obtained by using the continuous quantitative measurements, indicating that qualitative binary data may often be sufficient for the purpose of facies discrimination in many branches of geology and that association analysis is an effective method for this purpose. 相似文献
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D. H. Morgan Q. A. Parker Martin Cohen 《Monthly notices of the Royal Astronomical Society》2003,346(3):719-730
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. 相似文献