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81.
黑龙江嘉荫连珠山金矿床成岩成矿年代学及其地质意义   总被引:2,自引:0,他引:2  
连珠山矿床位于小兴安岭北麓,是一个产于花岗岩内部断裂体系的蚀变岩型金矿床。为了限定其成矿时代与成矿地质背景,本文对其赋矿围岩黑云母二长花岗岩和石英闪长岩进行了岩石地球化学、锆石U-Pb和绢云母40Ar/39Ar年代学的系统研究。定年结果表明黑云母二长花岗岩形成时代为中三叠世(243.7±1.3Ma,MSWD=0.77,n=12),岩浆上侵过程中受到早古生代(474~438Ma)和中二叠世(267~261Ma)的岩浆混染,而石英闪长岩形成于晚三叠世(215.3±1.3Ma,MSWD=0.35,n=17);黄铁绢英岩化矿石中的绢云母40Ar/39Ar坪年龄为194.2±2.0Ma,指示为早侏罗世成矿;元素地球化学特征显示连珠山侵入岩为准铝质-弱过铝质、高钾钙碱性岩石系列,具有I型花岗岩的地球化学属性;轻稀土元素富集,相对亏损重稀土元素,且具有弱的负Eu异常;富集大离子亲石元素(LILE),亏损高场强元素(HFSE)。结合小兴安岭-张广才岭地区已有年代学资料和区域构造演化特征,认为其成矿地质背景为兴蒙造山晚期与古太平洋板块俯冲转换期,或成矿发生在兴蒙造山期后的伸展阶段。  相似文献   
82.
RAPD分析中最适样本量和位点数的研究   总被引:2,自引:0,他引:2  
用25个引物,对40个样本扩增,研究了勒氏笛鲷随机扩增多态性DNA(RAPD)分析中的最适样本量和位点数。结果显示:在样本量达到20且位点数达到70个以上时,遗传距离趋于一个稳定的数值,即在RAPD分析中,样本数应达到20且位点数应达到70才能保证结果的可靠性。  相似文献   
83.
One of the major application areas of factor analysis, multivariate calibration and quantitation, is coveredin this review. The algorithms, methodologies and applications covered include principal componentregression, target transformation factor analysis, singular value decomposition and rank annihilationfactor analysis. Many important areas of research having relevance to multivariate calibration andquantitation problems are also covered in this review, including background correction, measurementerror, rank determination, cross-validation, figures of merit, detection of invalid samples, experimentaldesign, sample selection, statistical inference and wavelength selection.  相似文献   
84.
The Sample Catchment Basin (SCB) mapping technique extends the representativeness of the geochemical features of stream sediments to the surface of the whole upstream drainage basin. SCB boundaries clash with the water divides traced from each sampling point and are limited upstream by the presence of further SCBs. They are also assumed to represent the elementary map unit. The rank of SCBs can be defined counting the number of upstream SCBs along the branches of a fluvial network. The presence of low rank SCBs minimizes the statistical redundancy of measures. The SCB technique is particularly suitable for the geochemical mapping of mountainous or hilly areas and to correctly display the information into a morphological context. This approach can be also valuable in the case of low sampling density, inhomogeneous sampling schemes, and especially when very accurate evaluations of the spatial distribution of chemicals (with natural or anthropogenic origin) are required.  相似文献   
85.
In the light of progressive depletion of groundwater reservoir and water quality deterioration of the Independence aquifer, an investigation on chemical data of dissolved major and minor constituents in 246 recent groundwater samples was performed. The main objective was the detection of processes responsible for the geochemical evolution and mineralization throughout the area. Multivariate techniques revealed different sources of solutes (a) dissolution of calcium and magnesium carbonate minerals, (b) weathering of acid volcanic minerals, (c) alteration of manganese containing alkaline silicates, (d) leaching of halite deposits of meteoric origin, (e) contamination from agricultural and urban wastewaters, and (f) evaporative effects due to intensive irrigation. Although nitrate contamination is associated with pollution from intensive cultivated areas, natural contamination plays an important role in the study area. The investigation reveals that weathering of acid volcanic rocks (rhyolite) and oxidation of arsenic bearing sulfide minerals are the responsible processes for high fluorine (up to 16 mg/l) and arsenic (up to 0.12 mg/l) contents, respectively, exceeding the Mexican maximum admissible concentration for drinking water. Except for kaolinite, all recharge processes are dissolution oriented (CO2, calcite, dolomite, K-feldspar, plagioclase). Silicate precipitation (amorphous silica and chalcedony) is of growing importance in discharge zones. Cation exchange is not an important issue in the whole study area.  相似文献   
86.
The Moon 35 years after Apollo: What's left to learn?   总被引:1,自引:0,他引:1  
With the cancellation of the Apollo program after Apollo 17 returned from the Moon in 1972, the focus of NASA switched to other areas of the Solar System. Study of the Moon did continue through analysis of the returned samples and remotely sensed data sets (both orbital and surface), as well as through Earth-based telescopic studies. In the 1990s, new orbital data were obtained from several missions (fly-by and orbital), the first being Galileo that allowed the lunar farside to be mapped, followed by global mapping by the Clementine and Lunar Prospector missions.Interest in the Moon started to increase at the beginning of the 21st century as other nations focused their space exploration programs on the Moon. The speech by President Bush in January 2004 put the Moon back into the critical exploration path for NASA, paving the way for humans to return to the lunar surface by 2020. This return will be critical for developing technologies and protocols for the eventual human exploration of other parts of the solar system. At the time of writing (June 2008), the SELENE/Kaguya mission (Japan and Chang’e-1 (China) are orbiting the Moon, with Chandrayaan-1 (India) and Lunar Reconnaissance Orbiter (USA) being scheduled to launch later in 2008.The past (and present) exploration of the Moon begs the question “what's left to be done?” With the renewed focus on the Moon, now that it is on the pathway for the exploration of Mars (and beyond) a similar question has been raised - what should the astronauts do on the Moon? The publication of the New Views of the Moon book [Jolliff et al., 2006. New Views of the Moon, Reviews in Mineralogy, vol. 60. American Mineralogical Society, 721pp] highlighted a number of important scientific questions that remain unanswered as well as posing many more on the basis of the currently available data. These questions resonated in three Lunar Exploration Analysis Group (LEAG) reports pertinent to this discussion, which were also published (on line) during 2006 (http://www.lpi.usra.edu/leag), and in the National Research Council of the National Academies [2007. The Scientific Context for Exploration of the Moon. National Academies Press, Washington, DC, 112pp] report entitled “The Scientific Context for Exploration of the Moon”. This paper synthesizes these recent studies, along with those from the 1980s and 1990s, to emphasize the lunar science questions that remain unanswered. In addition, it summarizes the missions already flown to the Moon along with those that are planned in order to give the reader an idea of exactly what lunar science has been and will be conducted in the hope that it will inspire proposals for missions to address the outstanding science questions.  相似文献   
87.
山阳色河花岗岩地球化学特征和锆石SHRIMP U Pb年代学   总被引:6,自引:0,他引:6  
王涛  王宗起  闫臻  闫全人  张英利  向忠金 《地质学报》2009,83(11):1657-1666
山阳色河二长花岗岩出露于泥盆纪地层中,并与泥盆纪地层呈断层接触关系.花岗岩主要由钾长石、斜长石和石英组成,其SiO_2含量介于71%~77%之间、高碱(K_2O+Na_2O=7.43%~8.50%),低CaO(0.25%~2.81%),为高钾钙碱性花岗岩,A/CNK的平均值为<1.05,属弱过铝质岩石;较强的轻、重稀土元素分馏程度[(La/Yb)_N=4.23],明显的Eu负异常(δEu=0.511),富集Rb、Th、K、La和Cs等大离子亲石元素,亏损Ba、Nb、Sr、P和Ti元素为特征,属后碰撞花岗岩类.在泥盆纪地层中的花岗岩砾石的岩石地球化学与色河二长花岗岩具有形似性质,高精度的锆石SHRIMPⅡU-Pb定年获得花岗岩与花岗岩砾石形成时代相一致,分别为709±5Ma和700±11Ma.山阳后碰撞花岗岩的发现,标志着新元古代在东秦岭地区表现为造山后伸展拉张阶段,从而为东秦岭造山带从元古代到古生代的构造体制转换提供证据.  相似文献   
88.
由相对地热梯度推断的腾冲火山区现存岩浆囊   总被引:15,自引:6,他引:15  
为利用温泉来研究和监测腾冲火山区的现今岩浆分布并探讨其活动性,提出相对地热梯度的概念:假设各热田或水热活动区的热储深度相等,则热储温度与地表温泉温度之差为该地相对地热梯度。通过对前人在该地区获得的温泉的基本要素和温泉水化学分析数据分析,选取了159个温泉计算相对地热梯度。用这159个数据,通过克里金插值方法获得了腾冲火山区的相对地热梯度平面分布。结果发现腾冲火山区有3个相对地热梯度在100℃以上的高值区域。结合其他资料,认为腾冲火山区现今存在3个岩浆囊,它们的几何尺度为19~28kin,深度为4~12km或更深,并且目前的活动性各不相同。  相似文献   
89.
则不吓铅锌矿床为冈底斯成矿带中部西段新发现的热液脉型铅锌矿床。依据成矿地质条件、地球化学异常、高磁异常和激电异常、矿体特征等综合分析,区内成矿元素以Pb、Zn、Ag等元素为主,是寻找中低温热液型铅锌银多金属矿的有利地区,并指示其深部可能存在隐伏岩体,地表出露的断裂构造很可能是岩浆侵入在顶部引爆形成的裂隙,而各类岩脉为深部岩体向上延伸的分支。综合认为,该矿床找矿前景很好,后续通过进一步勘查可望取得更大的找矿突破,同时应注意在热液脉型铅锌矿体深部对斑岩型钨钼铜矿或隐爆角砾岩型铅锌银矿的识别和寻找,以拓展区内找矿空间和矿种类型。  相似文献   
90.
中国东部中生代发生的大规模岩浆活动是地学界长期以来关注的课题之一。本文通过对浙东地区晚中生代火山岩锆石U-Pb年代学、主量、稀土及微量元素地球化学的研究,讨论其岩石成因及形成的构造环境。研究表明,大爽组底部火山岩年龄为155.2±1.4 Ma(MSWD=0.83),显示浙东地区晚中生代火山岩的形成时代并不限于白垩纪,火山喷发至少于晚侏罗世就已经开始;岩石总体属高钾钙碱性系列,少量属钾玄岩系列;基性岩石、中性岩石与中酸性(酸性)岩之间不具有同源演化关系,基性岩石来源于富集地幔,并受到了不同程度的地壳混染,中性岩石可能来源于先存于下地壳深部的新元古代岛弧岩石,中酸性(酸性)岩石来源于地壳,中酸性岩浆与酸性岩浆之间存在演化关系;岩石总体形成于地壳幕式减薄环境,而其弧岩浆岩特征主要反映源岩属性。  相似文献   
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