平庄凹陷烃源岩有机质成熟度评价

平庄凹陷盖层中发育九佛堂组、沙海组和阜新组3套烃源岩,虽然以往围绕煤矿生产展开了大量的煤田地质勘探工作,但石油、天然气勘探工作较少,研究程度较低。为了客观评价平庄凹陷的油气资源,需对烃源岩有机质成熟度进行评判。在对平庄凹陷烃源岩岩石热解、镜质组反射率、生物标志物参数分析的基础上,对平庄凹陷九佛堂组、沙海组烃源岩有机质热演化特征及演化阶段进行了系统研究。结果表明：平庄凹陷烃源岩各参数随埋藏深度的增加变化明显,具有纵向上的连续性和横向上的不均匀性;平庄洼陷烃源岩有机质成熟度处于未成熟—低成熟—成熟阶段,其中,九佛堂组烃源岩是盆地的主要成油岩系;四龙洼陷烃源岩有机质成熟度较低,对盆地成烃贡献不大。     

Numerical modelling of burial and temperature history as an approach for an alternative interpretation of the Bramsche anomaly, Lower Saxony Basin

The Lower Saxony Basin, Germany, is one of the several sedimentary basins within the Central European Basin system. In its southwestern part, anomalously high maturity of organic matter has been observed to reach 4.5% VRr in Upper Jurassic and Lower Cretaceous sedimentary rocks in an area which coincides with a magnetic and a positive gravimetric anomaly. This anomaly was often interpreted as the consequence of a deep-seated igneous intrusion, the so-called Bramsche Massif. However, results obtained from calibrated numerical modelling are not in accordance with this scenario. Instead, a burial by approximately 4 km of now-eroded Cretaceous rocks was revealed to be the probable cause for the anomaly. Data and modelling results from six boreholes and two pseudo-wells support this view.     

ASTER数据在深圳东部滨海地区土地利用调查中的应用

以深圳市东部滨海地区为试验区,对2004年11月21日ASTER遥感数据进行辐射和几何精校正处理,实地建立分类样地;根据多边形样地矢量数据计算分析12类地物在ASTER各波段光谱反射图和分类叠合图,同时进行植被指数和短波红外5个波段主成分分析;结合GIS并利用ASTER光谱波段、第一主成分、植被指数、立体像对生成的地形因子建立土地利用分类决策树表;再根据决策树表对ASTER影像进行土地利用分类。经验证,分类结果总体精度达到85.1%。应用效果表明,利用ASTER数据进行土地现状资源调查具有很好的性价比,能够满足土地利用现状调查的准确度和精度。     

渤海湾盆地济阳坳陷热历史及构造—热演化特征

根据镜质组反射率和磷灰石裂变径迹古温标方法模拟的济阳坳陷地温演化情况表明,地温梯度在坳陷的演化过程中是逐渐降低的。在孔店组-沙河街组沉积期间地温梯度是较高的,最高可达5.5～6.0℃/100m,但在此期间地温梯度下降较快,在东营组沉积时期降为3.5～4.5℃/100m;在馆陶组沉积时期地温梯度变化很小,至第三纪末地温梯度已降至目前的3.5℃/100m左右。济阳坳陷的构造沉降特征表现为孔店组至沙四段沉积期间(65～43Ma)的快速构造沉降阶段和沙三段沉积(43Ma)以后的热沉降阶段,盆地的地热史模拟结果和构造沉降所揭示的坳陷演化阶段具有很好的对应关系。坳陷热历史研究为渤海湾盆地的构造-热演化提供了重要的认识。     

Chromite typology and composition characterized through multispectral specular reflectance

Determination of multispectral specular reflectance is an important tool for ore identification in reflected light microscopy, and may be used for automated characterization of ores. However, reflectance values can be affected by compositional variations in a way that is seldom understood. The aim of the present work is to investigate this problem in chromite, an ore whose composition may show typically large natural variations as member of the spinel family, and whose relatively high reflectance variations are apparently unpredictable. For this research, eighteen samples of chromian spinel covering a large range of compositions in the base of the Hagerthy prism were selected for microprobe analysis and reflectance measure on polished sections. The samples belong to a variety of deposits and types (ultramafic massif, ophiolitic, and metamorphosed types: Ojén and Ronda Massifs, Spain; Mayarí, Moa-Baracoa, Camagüey and Sagua de Tánamo, Cuba; Golyamo Kemenyane, Avren and Yakovitsa, Bulgaria). The specular reflectances are characterized as multispectral values, measured at thirteen intervals (50 nm each) in the VNIR region (Visible and Near-Infrared: 400–1000 nm), using the automated CAMEVA System.The relationship between compositional and reflectance values is studied by multivariate analysis and subsequently tested on independent samples. For this purpose, the samples have been grouped in two sets: a larger population of fifteen samples constitutes the initial data set for mathematical processing, while a selection of three samples of widely differing compositions is used to test the resulting functions, so as to gain a critical appraisal of their validity.The results obtained show that the specular reflectance of chromite depends on composition and can be used to estimate compositional parameters, as #Cr = Cr/(Cr + Al) or #Mg = Mg/(Mg + Fe²⁺), but this relationship is complex and does not allow simple direct determinations, due to the multiplicity of possible changes and coupled substitutions (e.g. Al–Cr–Fe³⁺, or Mg-Fe²⁺, Ni, Zn, Ti …) in the chromian spinel family. On the other hand, the relationship of chromite composition with deposit type is also detectable through the reflectance values, but with a higher uncertainty. Reflectance increases with increasing Cr and Fe³⁺ contents in all cases, but the relationship of reflectance with Mg seems to be specific of the deposit type: while reflectance increases with increasing #Mg in the Ojén chromites, it shows the opposite behaviour in podiform chromites. Although these results should be regarded as preliminary until further studies on larger sample populations can be achieved, they are suggestive of possible practical applications for exploration, e. g. to approach Cr-spinel compositions or chromite deposit typology, early in an exploration campaign, by inexpensive reflected light determination of specular reflectance in a few samples.     

豫西煤田构造煤反射率及其与古构造应力场的关系

为研究构造应力对煤反射率的影响,以豫西煤田不同构造区的构造煤和原生结构煤为对象,采用定向标本及反射率测定的方法作对比研究,发现构造煤的反射率比原生结构煤的反射率普遍偏高。根据反射率与构造应力的关系,求得各构造区的古构造应力场,通过与聚煤期后多次构造运动的主应力方向进行对比,可推知:影响嵩箕区二1煤变形和镜煤反射率的主要构造,是在前期断裂基础上喜山早期掀斜运动诱发的重力滑动构造,而影响崤熊区的则为燕山晚期的逆冲推覆作用。     

Maturity modelling integrated with apatite fission-track dating: Implications for the thermal history of the Mid-Polish Trough (Poland)

The Mid-Polish Trough (MPT) is situated in the easternmost part of the Central European Basin System (CEBS) and stretches NW–SE across the Polish Basin. It was characterised by pronounced subsidence and thick sediment accumulation between the Permian and the Late Cretaceous. Late Cretaceous–early Paleogene basin inversion led to the formation of the Mid-Polish Swell (MPS). The study area is located within the Pomeranian segment of the MPT/MPS (NW Poland) and experienced up to 7 km Permian-Mesozoic subsidence. PetroMod 1-D modelling was performed on several well-sections in order to study Permian to recent burial-uplift evolution. The modelling was calibrated with new vitrinite reflectance (VR_r) data and allowed to constrain the magnitude of uplift and related erosion as well as provided a first overview of the temperature history. The base of the studied Permian–Mesozoic successions attained maximum burial depths of 4800–5400 m before the onset of the inversion, less than in the axial trough area. The thickness of pre- and most probably also syn-inversion Upper Cretaceous deposits is estimated as 300 m. Erosion associated with inversion processes removed between 900 and 1400 m of the Mesozoic sediments, i.e. 1000–1500 m less than in the most inverted central part of the trough. VR_r data suggest constant Permian–Mesozoic heat flows corresponding to present-day values (40–45 mW/m²). Apatite fission-track (AFT) ages modelled with the PetroMod module PetroTracks show a good fit with AFT ages directly measured on well samples, and further support the assumption of steady heat flow in the range 40–45 mW/m². Palaeotemperatures appear to have decreased towards the East European Craton margin, which is compatible with the present day distribution of heat flow. Thermal history modelling shows a relatively simple Permian–Mesozoic heat flow pattern in the Pomeranian segment of the MPT. Such a scenario implies that the present-day heat flow distribution has not changed essentially since Mesozoic times.     

悬浮泥沙浓度遥感反演模式研究

利用野外采集的悬沙样品配置不同粒径和浓度等级的悬沙水样,进行实验室光谱测量,分析悬沙水样的光谱特征及其反射率与粒径之间的关系。根据实验结果选取泥沙浓度和粒径的敏感波段,建立了敏感波段模型和主成分模型。结果表明,主成分分析法能大量获取多通道悬沙水体光谱反射率信息,模型的反演能力优于敏感波段模型。     

水面浮油膜光谱测量及光谱特征分析

为深入解析水面浮油膜光谱特征,采用水面以上光谱测量方法,去除太阳直射和天空光两部分反射的影响,获取了珠江口水域不同厚度水面柴油膜光谱信息,对其光谱响应特征和机理进行了分析。结果表明:水面柴油膜光谱对背景水体光谱具有依赖性,但水面柴油膜光谱在可见光波段高于背景水体,且随着油膜厚度增加呈现不断增加的趋势;油膜反射光谱在蓝、紫光区域出现明显反射峰;360~500 nm区域油膜反射率与厚度相关系数大于0.8,有利于油膜厚度的遥感估算。最后指出,水面浮油膜类似于光学薄膜的单层增反膜,导致光谱反射率的增加,在360~420 nm区域的反射峰和石油类物质的荧光性有关。研究结果可为水域溢油污染遥感监测研究提供理论依据。     

影响海洋光学遥感的海面白泡云研究回顾及进展

回顾了国内外影响海洋光学遥感的白泡云的反射率和覆盖率的研究进展情况。根据海洋水色高光谱遥感发展的需要，指出应当开展海洋白泡云中信号白浪和白沫光学反射特征的测量和研究，以便评价和排除白泡云的反射分量在光学遥感中的干扰。