新疆哈密坡子泉地区首次发现隐爆角砾岩筒     

白云山  彭湘萍 《新疆地质》1999,(2)

新疆哈密坡子泉地区首次发现的隐爆角砾岩筒处在塔里木板块北缘活动带卡瓦布拉克微板块之上,基底地层为前寒武系,盖层主要为石炭系,受ＮＥ向断裂带控制。隐爆角砾岩特征及产出环境相似于金伯利岩。  相似文献   

同波束干涉测量在月面相对定位中的应用     

黄岸毅  谢鑫  张智斌  李恒年 《测绘学报》2015,44(9):973-979

基于同波束干涉测量原理和观测模型,针对月面目标特性,推导了给定着陆器先验位置的差分时延、差分时延率观测方程。引入指定高程约束、月球数字地形模型等约束方程,提出巡视器相对位置确定的卡尔曼滤波算法。通过仿真数据进行了验证和评估,表明该算法可快速、较高精度地确定月面巡视器相对着陆器的位置。  相似文献   

青海克停哈尔铜锌矿床隐爆角砾岩地球化学及地质意义     

刘国燕  李泽峰  张勇  何书跃  林贵  张来平  王磷  张鹏 《矿床地质》2019,38(1):197-210

克停哈尔铜锌矿床是近年来在东昆仑造山带西段新发现的一处矿床,并且在隐爆角砾岩中发现了锌矿体,为查明隐爆角砾岩成因及与成矿的关系,对隐爆角砾岩进行了主量、微量及稀土元素的分析和研究。研究结果显示,w(SiO_2)为64.13%～66.54%,w(Al_2O_3)为14.55%～15.59%,w(Na_2O+K_2O)为6.29%～7.24%,K_2O/Na_2O比值为0.87～1.17,A/CNK比值为0.971～1.121,属于过铝质高钾钙碱性岩石系列;稀土元素总量中等,轻稀土元素富集,中等负铕异常;富集大离子亲石元素(Rb、K)、活泼不相容元素(Th)和轻稀土元素,相对亏损高场强元素(Ta、Nb、Ti、P、HREE),总体反映具壳源为主的花岗岩特征,形成于碰撞造山晚期并开始向陆内造山伸展环境转变,至少存在2期爆破3期成矿,第二期爆破是铅锌矿的主要成矿期。  相似文献   

福建政和县东际金（银）矿床黄铁矿微量元素和硫-铅同位素及锆石年龄研究          下载免费PDF全文

肖凡  班宜忠  范飞鹏  许乃岑  毛光武  李凤春 《中国地质》2020,47(2):375-393

东际金(银)矿床赋存于燕山晚期南园组火山岩中,是东南沿海地区一个隐爆角砾岩型贵金属矿床,已探明金资源量达12.5 t,银资源量135.9 t。通过开展主要金属硫化物黄铁矿电子探针和硫-铅同位素分析,讨论了成矿作用和成矿物质来源等问题。研究表明,东际金(银)矿床黄铁矿Co/Ni值3～94(平均值23)且Co含量为500×10-6～1070×10-6(均值799×10-6),Fe/(S+As)值0.827～0.871(均值0.860),Au/Ag值0.9～5.5(均值2.6),反映该矿床是与陆相火山作用有关的浅成中低温热液型矿床。黄铁矿δ34S在-6.6‰～-0.7‰,206Pb/204Pb为17.9801～18.4303,207Pb/204Pb为15.2689～15.9397,208Pb/204Pb为37.9052～38.7871,指示成矿物质主要来源于具有壳幔混源性质的花岗质岩浆,此外含矿热液也活化萃取了部分基底变质岩和火山岩围岩的金属元素。通过锆石U-Pb年代学研究和区域成矿资料对比,东际金(银)矿床成矿时代可被限定于早白垩世晚期。  相似文献   

Formation of mud clast breccias and the process of sedimentary autobrecciation in the hominin-bearing (Homo naledi) Rising Star Cave system,South Africa     

Jelle P. Wiersma  Eric M. Roberts  Paul H. G. M. Dirks 《Sedimentology》2020,67(2):897-919

Unconsolidated mud clast breccia facies in the hominin-bearing (Homo naledi) Rising Star Cave, Cradle of Humankind, South Africa, are interpreted to have formed through a process termed sedimentary autobrecciation in this study. This process, by which most of the angular mud clast breccia deposits are thought to have formed autochthonously to para-autochthonously via a combination of erosion, desiccation, diagenesis and microbial alteration of laminated mud deposits, is thought to have taken place under relatively dry (i.e. non-flooded) conditions inside the cave. Subsequently, gravitational slumping and collapse was the dominant mechanism that produced the mud clast breccia deposits, which commonly accumulate into debris aprons. The mud clast breccia is typically associated with (micro) mammal fossils and is a common facies throughout the cave system, occurring in lithified and unlithified form. This facies has not been described from other cave localities in the Cradle of Humankind. Additionally, sedimentary autobrecciation took place during the deposition of some of the fossils within the Rising Star Cave, including the abundant Homo naledi skeletal remains found in the Dinaledi Subsystem. Reworking of the mud clast breccia deposits occurs in some chambers as they slump towards floor drains, resulting in the repositioning of fossils embedded in the breccias as evidenced by cross-cutting manganese staining lines on some Homo naledi fossil remains. The formation of the unlithified mud clast breccia deposits is a slow process, with first order formation rates estimated to be ca 8 × 10⁻⁴ mm year⁻¹. The slow formation of the unlithified mud clast breccia facies sediments and lack of laminated mud facies within these deposits, indicates that conditions in the Dinaledi Chamber were probably stable and dry for at least the last ca 300 ka, meaning that this study excludes Homo naledi being actively transported by fluvial mechanisms during the time their remains entered the cave.  相似文献   

Radiolarian‐based study on the fabric and the formation process of the Early Cretaceous mélange near Zhongba,Yarlung–Tsangpo Suture Zone,southern Tibet     

Xin Li  Atsushi Matsuoka  Yalin Li  Yushuai Wei  Chengshan Wang 《Island Arc》2019,28(1)

The Yarlung–Tsangpo Suture Zone (YTSZ), as the southernmost and youngest among the sutures that subdivides the Tibetan Plateau into several east–west trending blocks, marks where the Neo‐Tethys was consumed as the Indian continent moved northward and collided against the Eurasian continent. Mélanges in the YTSZ represent the remnants of the oceanic plate through subduction and collision. Mélanges are characterized by a highly sheared volcanoclastic or siliceous mudstone matrix including blocks of chert, claystone, and basalt. Detailed radiolarian analyses are conducted on the mélange near Zhongba County. Macroscopic, mesoscopic, and microscopic observations are combined in order to elucidate the relationships among age, lithology, and structure of blocks in the mélange. Reconstructed ocean plate stratigraphy includes Lower Jurassic limestone within the chert sequence accumulated at a depth near the CCD (Unit 2), Upper Jurassic thin‐bedded chert interbedded with claystone deposited in the wide ocean basin (Unit 3), and Lower Cretaceous chert with siliceous mudstone (Units 4 and 5), representing the middle parts of ocean plate stratigraphy. The results highlight the fabric of brecciated chert on mesoscopic scale, which is thought to be due to localized overpressure. The formation of mesoscopic and microscopic block‐in‐matrix fabrics in the mélange is proposed for the chert and siliceous mudstone bearing different extents of consolidation and competence during the progressive deformation of accreted sediments at shallow‐level subduction.  相似文献   

再论盐源模范村喜马拉雅期斑岩铜矿床地质特征及找矿前景     

李立主  赵支刚  贺金良  杨泽湘 《四川地质学报》2005,25(4):215-223

该矿床具有典型斑岩铜矿特征,成岩的多期次构成复式岩体,断裂构造控制的隐爆碎裂岩筒为成矿提供了通道和沉积场所.多期次成矿,特别是次生富集作用形成达中型规模的Ⅰ号矿体,影响次生富集带发育的F7断裂带起了重要作用.总结出适合本区斑岩群特点的找矿标志和提出的找矿靶区,对开展新一轮普查找矿具有现实意义.  相似文献   

CE3玉兔号月球车APXS特征X射线能谱信息分析     

刘菁华  王文华  陈圣波  周大鹏 《吉林大学学报(地球科学版)》2018,48(2):445-450

通过对CE3玉兔号月球车粒子激发X射线谱仪（APXS）获取的数据进行处理,获得测点的累积特征X荧光计数率谱线,经小波滤波,消除放射性涨落对X荧光谱线的影响。由能量刻度获得了月球车着陆点月壤元素X射线特征能量峰,由此分析了着陆点月壤元素的成分,得知测量点月壤元素成分包括Si、Ca、Al、Mg、K、P、S、Fe、Ti、Ni、Cr、Mo、Sr、Y、Zr、Nb。研究结果为月陆地质演化提供了有利的参数制约。  相似文献   

Influence of lunar phases,winds and seasonality on the stranding of mesopelagic fish in the Strait of Messina (Central Mediterranean Sea)          下载免费PDF全文

Pietro Battaglia  Giovanni Ammendolia  Mauro Cavallaro  Pierpaolo Consoli  Valentina Esposito  Danilo Malara  Ignazio Rao  Teresa Romeo  Franco Andaloro 《Marine Ecology》2017,38(5)

The shore stranding of mesopelagic fauna is a recurrent phenomenon in the Strait of Messina (Central Mediterranean Sea). The aim of this paper is to test the influence of lunar phases, winds and seasons upon the frequency of occurrence of strandings of mesopelagic fish. Species abundance in relation to these factors was quantified for the first time. Specimens were collected stranded on the shore along the Sicilian coast of the Strait of Messina between 2008 and 2016. Overall 32 species belonging to seven families (Gonostomatidae, Microstomatidae, Myctophidae, Paralepididae, Phosichthyidae, Sternoptychidae, Stomiidae) were found stranded. Myctophidae was the family including the highest number of species (16), whereas Gonostomatidae was the most abundant in terms of total number of individuals (47.2%), mainly thanks to the species Cyclothone braueri. The moon, which influences the strength of currents (highest during full and new moon phases) and irradiance (higher in some lunar phases, such as the full moon), affected the abundance of stranded mesopelagic fish in the study area. The highest number of stranding events was recorded during the new moon: 34.6% of the total relative abundance of stranded mesopelagic fish. Wind blowing from the sea towards the coastline (southeasterly and easterly winds) created the best conditions for strandings. The highest abundance of stranded specimens was recorded during the winter season.  相似文献   

Automatic mapping of lunar landforms using DEM-derived geomorphometric parameters   总被引：1，自引：0，他引：1  

Jiao Wang  Weiming Cheng  Chenghu Zhou  Xinqi Zheng 《地理学报(英文版)》2017,27(11):1413-1427

Developing approaches to automate the analysis of the massive amounts of data sent back from the Moon will generate significant benefits for the field of lunar geomorphology. In this paper, we outline an automated method for mapping lunar landforms that is based on digital terrain analysis. An iterative self-organizing (ISO) cluster unsupervised classification enables the automatic mapping of landforms via a series of input raster bands that utilize six geomorphometric parameters. These parameters divide landforms into a number of spatially extended, topographically homogeneous segments that exhibit similar terrain attributes and neighborhood properties. To illustrate the applicability of our approach, we apply it to three representative test sites on the Moon, automatically presenting our results as a thematic landform map. We also quantitatively evaluated this approach using a series of confusion matrices, achieving overall accuracies as high as 83.34% and Kappa coefficients (K) as high as 0.77. An immediate version of our algorithm can also be applied for automatically mapping large-scale lunar landforms and for the quantitative comparison of lunar surface morphologies.  相似文献