基于GML的空间数据拓扑表达

拓扑关系是GIS中重要的基础理论问题之一,GML为空间数据拓扑表达提供了一种全新的手段。介绍GML及GML3.X中定义的拓扑模型,并以点线面等的表达为例阐述基于GML的空间数据拓扑表达。     

鄂陵湖湖滨地区夏季近地层微气象特征与碳通量变化分析

利用2010年夏季鄂陵湖湖滨地区试验观测资料,从中选取资料较好的5个连续晴天,分析了该地区高寒草甸夏季局地气候、辐射与能量平衡特征以及碳通量的日变化。结果表明：①夏季晴天湖滨地区近地层气象要素受到湖陆风的较大影响,风向昼夜交替变化,垂直风速和摩擦速度明显大于玛曲草原,全天盛行上升气流,昼夜温差较小;②湖滨地区日均太阳总辐射与净辐射高于玛曲草原和金塔绿洲,地表能量不平衡现象较显著,湍流输送以潜热为主,夜间近地层存在明显的逆温和逆湿现象;③夏季湖滨草甸碳吸收的日最大值出现在上午11时前后,碳吸收显著大于碳排放,其水分利用效率与海北草甸生态系统接近,总体偏低。     

黄河源区生态环境变化对湖泊效应影响的数值模拟

利用中尺度气象模式WRF,设计了陆地生态环境好转、维持现状和退化3种情境下的模拟试验,分析了夏季黄河上游鄂陵湖湖泊效应的特征和生态环境变化对该湖泊效应的影响。结果表明,夏季晴天中午至傍晚,鄂陵湖有显著的湖风环流;白天湖面感热和潜热较小,昼(夜)表现出明显的冷(暖)湖效应;湖区低层全天呈现出"湿岛"效应;受湖风作用影响,环湖陆上白天形成"湿墙"和感热高值区;随着陆地生态环境由好转到退化,湖风环流加强,环湖"湿墙"增高,湖陆边界层高度差增大,陆面感热和潜热变化显著大于湖面;陆面边界层中下部的气温和比湿主要受下垫面影响,环境退化后分别升高和减小,而在边界层顶部由于受湖风环流的作用,两者变化趋势与中下部相反。     

基于时空系统统一的北斗与GPS融合定位

我国的北斗卫星导航定位系统目前已经发射9颗“北斗”卫星,北斗区域卫星导航系统的基本系统已建设完成,正开展星地联调和测试评估工作,已经具备我国范围内的初步三维定位导航能力。本文研究了Beidou和GPS的时间系统/坐标系统的统一、卫星广播星历与卫星位置计算,以及二者的高精度定位算法,并实现了Beidou和GPS载波相位的数据融合和高精度联合定位,最后通过2011年9月29日的实测数据和处理结果证明了本文方法的正确性,同时为北斗二号系统的调试提供相关试验与结果。     

夏季绿洲气候效应的观测和数值模拟

利用“金塔绿洲能量水分循环观测试验”的资料和中尺度数值模式对绿洲小气候效应进行了17天较长序列的研究,在模拟过程中每天替换土壤湿度。研究结果表明：在分析时段内2004年7月6目前和9日后分别盛行西北风和东风两种背景风;白天,绿洲低层相对沙漠是一个冷源,随着高度的增加逐渐转为暖中心,温度场在600～700hPa之间转变。当背景风较大时,绿洲上空的温度中心会偏向绿洲中心下游。白天绿洲低层风场平均态为在东风背景场的基础上向南北两侧辐散,随着高度的增加风场逐渐由辐散转为向绿洲的辐合,转变高度在700hPa以下,且低于温度场的转变高度。白天绿洲上以下沉运动为主,绿洲风次级环流是绿洲上夏季晴天长期存在的平均态。当背景风较小时绿洲低层可形成向四周辐散的风场,当背景风场过大时,无绿洲环流生成。绿洲为高湿场,在绿洲边缘沙漠上存在的逆湿和高水汽柱,既阻止沙漠上干热气流侵入绿洲,又防止绿洲上水汽的流失。白天沙漠、绿洲的地表能量通量差异较大,绿洲上以潜热为主,沙漠上以感热为主,二者量级相当。绿洲上的边界层高度低于沙漠的,对绿洲生态系统起一定的保护作用。     

The local far-infrared galaxy colour–luminosity distribution: a reference for BLAST and Herschel/SPIRE submillimetre surveys

We measure the local galaxy far-infrared (FIR) 60 to 100 μm colour–luminosity distribution using an all-sky IRAS survey. This distribution is an important reference for the next generation of FIR–submillimetre surveys that have and will conduct deep extragalactic surveys at 250–500 μm. With the peak in dust-obscured star-forming activity leading to present-day giant ellipticals now believed to occur in submillimetre galaxies near   z ∼ 2.5  , these new FIR–submillimetre surveys will directly sample the spectral energy distributions of these distant objects at rest-frame FIR wavelengths similar to those at which local galaxies were observed by IRAS . We have taken care to correct for the temperature bias and the evolution effects in our IRAS 60-μm-selected sample. We verify that our colour–luminosity distribution is consistent with the measurements of the local FIR luminosity function, before applying it to the higher redshift Universe. We compare our colour–luminosity correlation with recent dust–temperature measurements of submillimetre galaxies and find evidence for pure luminosity evolution of the form  (1 + z )³  . This distribution will be useful for the development of evolutionary models for Balloon-borne Large Aperture Submillimeter Telescope (BLAST) and Spectral and Photometric Imaging Receiver (SPIRE) surveys as it provides a statistical distribution of the rest-frame dust temperatures for galaxies as a function of luminosity.     

Late Pleistocene sea-level oscillations (MIS 10–2) recorded in shallow marine and coastal plain sediments of the southern Wanganui Basin, New Zealand

The northern Wanganui Basin, New Zealand, is one of the key global sites for understanding marine cyclic sedimentation during the Quaternary. This paper presents the first evidence of marine cyclic sedimentation from its central-southern parts. Sedimentological, micropalaeontological and palynological analyses on a 280-m-deep borehole encountered units dating back to MIS 10. The sequence includes four marine cycles spanning MIS 9–5, which are overlain by terrestrial fluvial aggradation surfaces dating from MIS 4–2. Each marine unit represents a progressively shallowing depositional environment from the mid-shelf to coastal plain. This is overlain by a terrestrial sequence of lowstand fluvial terraces. Localized fault movements appear to have influenced the sedimentary character of the sequence during MIS 7a and 5e producing basement highs which provided protection to the shoreline. The cyclothems described in this paper now extend the already extensive, previously described record from MIS 17–10 to produce a combined eustatic record of Quaternary sea level change within the basin to MIS 5. They also provide an excellent example of the sedimentary response of a coastal basin to a progressive loss of sedimentation accommodation space.     

AzTEC millimetre survey of the COSMOS field – I. Data reduction and source catalogue

We present a 1.1 mm wavelength imaging survey covering 0.3 deg² in the COSMOS field. These data, obtained with the AzTEC continuum camera on the James Clerk Maxwell Telescope, were centred on a prominent large-scale structure overdensity which includes a rich X-ray cluster at z ≈ 0.73. A total of 50 mm-galaxy candidates, with a significance ranging from 3.5 to 8.5σ, are extracted from the central 0.15 deg² area which has a uniform sensitivity of ∼1.3 mJy beam⁻¹. 16 sources are detected with S/N ≥ 4.5, where the expected false-detection rate is zero, of which a surprisingly large number (9) have intrinsic (deboosted) fluxes ≥5 mJy at 1.1 mm. Assuming the emission is dominated by radiation from dust, heated by a massive population of young, optically obscured stars, then these bright AzTEC sources have far-infrared luminosities  >6 × 10¹² L_⊙  and star formation rates  >1100 M_⊙ yr⁻¹  . Two of these nine bright AzTEC sources are found towards the extreme peripheral region of the X-ray cluster, whilst the remainder are distributed across the larger scale overdensity. We describe the AzTEC data reduction pipeline, the source-extraction algorithm, and the characterization of the source catalogue, including the completeness, flux deboosting correction, false-detection rate and the source positional uncertainty, through an extensive set of Monte Carlo simulations. We conclude with a preliminary comparison, via a stacked analysis, of the overlapping MIPS 24-μm data and radio data with this AzTEC map of the COSMOS field.     

贵州黔东南坑头蚀变岩型金矿的发现及意义

坑头金矿位于贵州黔东南金矿带,前人对该金矿带石英脉型金矿进行了广泛研究,认为深部可能有蚀变岩型金矿存在,但都未证实。近期经综合研究,在坑头金矿施工钻孔发现坑头金矿的深部存在蚀变岩型矿体,含金量最高达6. 65 g/t。蚀变岩型金矿矿石中金的赋存状态以裂隙金为主,主要载金矿物为毒砂。硅化蚀变及断层与金矿化关系密切,金矿体位于硅化蚀变发育的构造破碎带中。目前,黔东南金矿的开采目标多为300 m以浅的石英脉型金矿体,因此该发现对黔东南地区金矿深部勘查工作具有重要意义。     

Effects of the peat acid digestion protocol on geochemically and morphologically diverse tephra deposits

Tephra shards for electron probe microanalysis are most efficiently extracted from peat using acid digestion, which removes organic material that hinders density separation methods. However, strong acids are known to alter glass chemical compositions, and several studies have examined how acid digestion affects rhyolitic volcanic glass. The focus on rhyolitic tephra in these studies leaves considerable uncertainty, as the dissolution rates of natural glasses (including tephra) are determined by the chemical composition and surface area/volume ratio, both of which vary in tephra deposits. Here, we use duplicate samples of basaltic, trachydacitic and rhyolitic tephra to examine physical and geochemical alteration following acid digestion. Scanning electron microscope imagery reveals no discernible degradation of glass surfaces, and electron probe microanalysis results from duplicate samples are statistically indistinguishable. These findings suggest the acid digestion protocol for organic peats does not significantly alter glass geochemistry regardless of shard morphologies or geochemical compositions.