基于RIA和SOA的分布式WebGIS研究

基于当前流行的RIA平台和SOA体系,以分布式WebGIS为研究对象,探讨RIA/Services架构的分布式WebGIS开发方式,并以Silverlight和ArcGIS Server为平台阐述实践方案,开发的实验系统提高了WebGIS的表现力与交互性,同时降低了开发的复杂性、缩短了产品生产周期,具有一定的理论和现实意义。     

Detection of nighttime sea fog/stratus over the Huanghai Sea using MTSAT-1R IR data

A dual channel difference (DCD) method is applied to detect nighttime sea fog/stratus over the Huanghai Sea using the infrared (IR) data of shortwave (3.5–4.0 μm) and longwave (10.3–11.3 μm) channels from the Multi-functional Transport Satellite (MTSAT)-1R, i.e., shortwave minus longwave brightness temperature difference (SLTD). Twenty-four sea fog events over the Huanghai Sea during March to July of 2006 and 2007 are chosen to determine a suitable value of SLTD for nighttime sea fog/stratus detection, and ...     

The Rumuruti chondrite group

Since 1994, the Rumuruti (R) chondrites have been recognized as a new, well-established chondrite group differing from carbonaceous, ordinary, and enstatite chondrites. The first R chondrite, Carlisle Lakes, was found in Australia in 1977. Meanwhile, the number has increased to 107 (December, 2010). This group is named after the Rumuruti meteorite, the first and so far the only R chondrite fall. Most of the R chondrites are breccias containing a variety of different clasts embedded in a clastic matrix. Some textural and mineralogical characteristics can be summarized as follows: (a) the chondrule abundance in large fragments and in unbrecciated rocks is ∼35–50 vol%; (b) Ca,Al-rich inclusions are rare; (c) the olivine abundance is typically 65–78 vol%; (d) the mean chondrule diameter is ∼400 μm; (e) in unequilibrated R chondrites, low-Ca pyroxene is dominating, whereas in equilibrated R chondrites it is Ca-rich pyroxene; (f) the typical olivine in a metamorphosed lithology is ∼Fa_38–40; (g) matrix olivine in unequilibrated, type 3 fragments and rocks has much higher Fa (∼45–60 mol%) compared to matrix olivines in type 4–6 lithologies (∼Fa_38–41); (h) spinels have a high TiO₂ of ∼5 wt%; (i) abundant different noble metal-bearing phases (metals, sulfides, tellurides, arsenides) occur. The exception is the metamorphosed, type 5/6 R chondrite La Paz Icefield 04840 which contains hornblende, phlogopite, and Ca-poor pyroxene, the latter phase typically occurring in low-grade metamorphosed R chondrites only.In bulk composition, R chondrites have some affinity to ordinary chondrites: (a) the absence of significant depletions in Mn and Na in R chondrites and ordinary chondrites is an important feature to distinguish these groups from carbonaceous chondrites; (b) total Fe (∼24 wt%) of R chondrites is between those of H and L chondrites (27.1 and 21.6 wt%, respectively); (c) the average CI/Mg-normalized lithophile element abundances are ∼0.95 × CI, which is lower than those for carbonaceous chondrites (≥1.0 × CI) and slightly higher than those for ordinary chondrites (∼0.9 × CI); (d) trace element concentrations such as Zn (∼150 ppm) and Se (∼15 ppm) are much higher than in ordinary chondrites; (e) the whole rock Δ¹⁷O of ∼2.7 for R chondrites is the highest among all meteorite groups, and the mean oxygen isotope composition is δ¹⁷O = 5.36 ± 0.43, δ¹⁸O = 5.07 ± 0.86, Δ¹⁷O = +2.72 ± 0.31; (f) noble gas cosmic ray exposure ages of R chondrites range between ∼0.1 and ∼70 Ma. More than half of the R chondrites analyzed for noble gases contain implanted solar wind and, thus, are regolith breccias. The 43 R chondrites from Northern Africa analyzed so far for noble gases seem to represent at least 16 falls. Although the data base is still scarce, the data hint at a major collision event on the R chondrite parent body between 15 and 25 Ma ago.     

里下河地区极端降水时空变化及未来趋势分析

随着全球变暖,极端天气事件逐渐增加,影响着社会经济发展,揭示区域极端降水时空变化对防洪减灾具有重要意义。基于1960—2019年的逐日降水,通过MK趋势检验、小波分析、重标极差以及克里金插值方法,从强度、频率和持续性三方面分析里下河地区的极端降水指数,并进一步探究其未来趋势变化。结果表明：（1）里下河地区多年平均降水为1017.25 mm,呈不显著增加趋势;空间分布差异明显,总体呈自西北向东南逐渐增加的分布。（2）研究区内各站点极端降水指数变化不同,总体而言,极端降水强度、频率均呈现增加趋势,持续性呈减少趋势。（3）极端降水指数变化过程中存在3类尺度的周期性变化,在整个时间尺度上存在3个偏多中心和2个偏少中心。（4）除R10mm和R20mm未来变化趋势与过去趋势相反且呈弱持续性,其他极端降水指数未来变化趋势与过去相一致,且过去总体趋势对未来趋势的影响时间长度在9~16年左右。研究结果为里下河地区科学合理应对气象灾害、合理配置水资源提供依据。     

青岛奥帆基地海域漂浮浒苔光合生理特点研究

研究了青岛奥帆基地海域漂浮浒苔Enteromorpha prolifera （Muell）J.Ag.色素组成及含量、光合放氧及呼吸耗氧速率、P／R（净光合放氧速率／净呼吸耗氧速率）、抗氰呼吸等各项生理指标。结果表明,该海域漂浮浒苔的各项生理指标都在正常范围内,且有抗氰呼吸的存在,生长状况良好。     

BVRI photometry of possible standard stars in NGC 188

CCD photometry of possible standard stars, in Cousins B, V, R and I, in a field in the region of NGC 188 is presented.     

Chandra observations of neutron stars: an overview

We present an overview of Chandra X-ray Observatory observations of neutron stars. The outstanding spatial and spectral resolution of this great observatory have allowed for observations of unprecedented clarity and accuracy. Many of these observations have provided new insights into neutron star physics. We present an admittedly biased and overly brief review of these observations, highlighting some new discoveries made possible by the Observatory’s unique capabilities. This includes our analysis of recent multiwavelength observations of the putative pulsar and its pulsar-wind nebula in the IC443 SNR.      

Methodical series tests for fuller ship hull forms

In recent years many fuller ship hull forms have been designed and constructed in various shipbuilding countries, but the data available for the development of the fuller forms are inadequate from the point of view of preliminary ship design. In this paper the authors describe how they have systematically tested vessel forms of block coefficients ranging from 0.80 to 0.90. The analysis and presentation of the test results have been made in such a manner that designers can produce hull forms like those of tankers and other bulk carriers quickly and reliably.