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81.
无人机在露天矿山监测中的应用 总被引:3,自引:0,他引:3
在露天矿山开采过程中,对矿山进行实时动态监测很有必要,它不仅能够实时掌握开采进度和开采方案实施的准确性,还有利于数字矿山建设。本文以河北省保定市涞源县某露天矿区为例,利用Pix4Dmapper软件对无人机航拍影像进行数据采集与处理,获取矿区的三维点云数据、数字正射影像和数字地表模型,并利用ArcGIS和Global Mapper软件对生产成果进行矿山开发占地分析,实现露天矿山三维可视化。本文为准确掌握矿山环境治理执行情况,把握矿山开发整体情况给予了有力的参考和借鉴作用。 相似文献
82.
Liu Shen Feng Caixia Fan Yan Chen Xiaoqing Yang Yuhong Zhao Huibo Coulson Ian M. 《中国地球化学学报》2020,39(6):862-886
Acta Geochimica - This work reports an important episode of extensional, mafic magmatism that impacted the North China Craton (NCC) during the Permo-Triassic and influenced the evolution of this... 相似文献
83.
Gang Yang Aaron Zimmerman Nicole C. Hurtig Svetoslav V. Georgiev Vineet Goswami Judith L. Hannah Holly J. Stein 《Geostandards and Geoanalytical Research》2020,44(2):231-242
Rhenium–osmium geochronometry for samples with low Re and complex matrices requires improved Re extraction methods. Here, we investigate plausible controls on efficiency and efficacy of Re extraction during our anion resin bead purification. Four different protocols are compared, each isolating a single variable to test. Rhenium concentrations for solutions at each step of each protocol document differences in chemical recovery/yield. The negative‐thermal ionisation mass spectrometry (N‐TIMS) signal intensity serves as a proxy for Re yield and purity. These data document correlations between the N‐TIMS signal intensity and (a) the duration of anion resin bead conditioning prior to loading with Re‐bearing solution, and (b) both duration and strength of nitric acid used during rinsing of the Re‐loaded anion resin bead. The optimal protocol improved Re signal intensity around fourteen times compared with our current Re extraction protocol, an aggregate of 2.4 times improvement in chemical recovery (yield) and 5.8 times improvement in emission efficiency (purity). Repeated N‐TIMS isotopic measurements on our in‐house Re standard solution (1407) verify that our optimal protocol‐3 does not fractionate Re isotopes. The improved anion resin bead method considerably lowers the Re detection limit and allows Re‐Os isotopic analysis of picogram‐level Re hosted in geological samples with complex matrices. 相似文献
84.
Interstellar graphene could be present in the interstellar medium(ISM), resulting from the photochemical processing of polycyclic aromatic hydrocarbon(PAH) molecules and/or collisional fragmentation of graphitic particles. Indeed, by comparing the observed ultraviolet(UV) extinction and infrared(IR) emission of the diffuse ISM with that predicted for graphene, as much as ~ 2% of total interstellar carbon could be locked up in graphene without violating the observational constraints. While the possible detection of planar C24, a small piece of a graphene sheet, has been reported towards several Galactic and extragalactic planetary nebulae, graphene has not yet been detected in interstellar environments. In this work, we search for the characteristic IR features of C24 at ~ 6.6, 9.8 and 20 μm toward Sgr B2, a high-mass star formation region, and find a candidate target toward R.A.(J2000) = 267.05855?and Decl.(J2000) =-28.01479?in Sgr B2 whose Spitzer/IRS spectra exhibit three bands peaking at ~ 6.637, 9.853 and 20.050 μm which appear to be coincident with those of C24. Possible features of C60 are also seen in this region. The candidate region is a warm dust environment heated by massive stars or star clusters, associated with a WISE spot(a tracer of star formation activity), close to the HII region candidate IRAS 17450–2759, and is surrounded by seven young stellar object candidates within ~ 5′, suggesting that the creation and/or excitation of C24 could be related to star formation activities. 相似文献
85.
The North China Craton(NCC)hosts some of the world-class gold deposits that formed more than 2 billion years after the major orogenic cycles and cratonization.The diverse models for the genesis of these deposits remain equivocal,and mostly focused on the craton margin examples,although synchronous deposits formed in the interior domains.Here we adopt an integrated geological and geophysical perspective to evaluate the possible factors that contributed to the formation of the major gold deposits in the NCC.In the Archean tectonic framework of the NCC,the locations of the major gold deposits fall within or adjacent to greenstone belts or the margins of micro-continents.In the Paleoproterozoic framework,they are markedly aligned along two major collisional sutures-the Trans North China Orogen and the Jiao-Liao-Ji Belt.Since the Mesozoic intrusions hosting these deposits do not carry adequate signals for the source of gold,we explore the deep roots based on available geophysical data.We show that the gold deposits are preferentially distributed above zones of uplifted MOHO and shallow LAB corresponding to thinned crust and eroded sub-lithospheric mantle,and that the mineralization is located above regions of high heat flow representing mantle upwelling.The NCC was at the center of a multi-convergent regime during the Mesozoic which intensely churned the mantle and significantly en riched it.The geophysical data on Moho and LAB upwarp from the centre towards east of the craton is more consistent with paleo-Pacific slab subduction from the east exerting the dominant control on lithospheric thinning.Based on these results,and together with an evaluation of the geochemical and isotopic features of the Mesozoic magmatic intrusions hosting the gold mineralization,we propose a genetic model that invokes reworking of ancient Au archives preserved in the lower crust and metasomatised upper mantle and which were generated through multiple subduction,underplating and cumulation events associated with cratonization of the NCC as well as the subduction-collision of Yangtze Craton with the NCC.The heat and material input along zones of heterogeneously thinned lithosphere from a rising turbulent mantle triggered by Mesozoic convergent margins surrounding the craton aided in reworking the deep roots of the ancient Au reservoirs,leading to the major gold metallogeny along craton margins as well as in the interior of the NCC. 相似文献
86.
利用小型无人机进行遥感图像配准在自然灾害损害评估、环境监测和目标检测与追踪等领域发挥着至关重要的作用,但小型无人机的图像采集过程容易受风速/风向、复杂地形、电池容量、飞行姿态、飞行高度等自然或人为因素的影响。这些问题通常会导致捕捉到的场景重叠率低与图像非刚性畸变,在特征点提取过程中产生大量冗余点,增加了图像配准的难度。本文提出一种基于特征点的小型无人机图像配准方法,该方法的核心思想是在配准过程中识别冗余点,同时最大化可用内点数量。所识别的冗余点当作控制点,用于控制网格代图像的运动。最后通过最大化内点和合理移动控制点来恢复图像变换。本文使用50对小型无人机图像进行特征匹配和图像配准的实验,其中平均配准精度可达80.38%,并且本文方法在所有的情况下都优于5种当前流行算法。 相似文献
87.
石炭纪时期有孔虫具有演化快、分布广、数量丰富、分异度高的特点,对于地层的划分对比具有极为重要的意义。与全球其他重要的石炭纪沉积区相比,华南有孔虫生物地层划分精度相对较低。本文首次较为系统地报道了华南石炭系代表性岩石地层单位旧司组和上司组下部丰富的有孔虫化石及其在剖面上的分布情况,并综合现有关于华南的有孔虫化石资料,将华南维宪阶划分为7个有孔虫化石带,自下而上分别为Eoparastaffella simplex带、Viseidiscus/Planoarchaediscus带、Paraarchaediscus带、Pojarkovella nibelis带、Koskinotextularia带、Bradyina带和Janischewskina带。这些有孔虫带可与全球其他典型的石炭纪沉积区进行很好的对比,从而为相关的研究提供一个较为精细的地层格架。通过对黔南上司地区有孔虫的研究,提议中国石炭系区域性年代地层单位上司阶底界可用有孔虫Bradyina的首现定义,并将上司阶与西欧的Warnantian亚阶中上部和俄罗斯的Aleksinian亚阶—Venevian亚阶对比,对应国际维宪阶上部,为全球石炭系年代地层对比提供了可靠的化石依据。 相似文献
88.
在对渤海滨州贝壳堤岛的自由生活海洋线虫进行分类和多样性研究中,发现2个我国新纪录种并进行了描述。其中,澳洲深咽线虫Bathylaimus australis Cobb,1894主要特征为:头刚毛长约20μm,分为4节,顶端膨大;前口腔大,无齿,后口腔小,具小齿;化感器双环形,位于口腔中部位置;交接刺细长,稍向腹面弯曲,近端膨大呈头状,长32-37μm;引带宽大,肾形,长36-40μm,末端角质化,渐尖。古氏努朵拉线虫Nudora gourbaultae Vincx,1989主要特征为:体表具12列纵向排列的V型装饰;第二体环较宽,头刚毛11-15μm(为头颈的67%-81%);化感器圆形,直径4-6μm(为相应体径的29%-38%),位于第二体环上;具双咽球;交接刺细长,弯曲呈S型,长为肛径的1.3-1.5倍;引带等于或长于交接刺,镰刀型,无肛前辅器。 相似文献
89.
干容重是沉积学研究中用于计算物质通量的一个重要参量,对于正确认识沉积物的收支平衡、源汇通量以及地貌演化等问题具有重要意义。然而,干容重的分析流程和计算方法仍然缺乏统一的规范,导致干容重的取值不尽合理,影响了沉积学研究的定量化和精准度,这个问题需要引起足够的重视。本文选取了东海内陆架的表层沉积物和柱状沉积物,运用实验测试和间接公式计算两种方法获得了沉积物的干容重,对比分析了两种方法的精准度。研究发现,东海内陆架的细颗粒沉积物的干容重的数值范围是1.1—1.5g/cm~3;影响沉积物干容重的主要因素是沉积物的成分与粒度,前者通过颗粒态物质的密度起作用,后者通过孔隙度来影响。建议:干容重的分析测试工作应在采样后尽快完成;运用干容重进行沉积通量计算时,应根据沉积物的平均粒度和孔隙度的空间变化选择合适的数值,以获得更加合理的结果。 相似文献
90.
CH3I、CHCl3、C2HCl3和CH2Br2是挥发性卤代烃4种重要成分,对大气化学产生重要影响。于2018年10月在西太平洋进行船基现场培养实验,研究微量元素Fe (50 nmol/L)、酸化(pH=7.9)、酸化(pH=7.9)和微量元素Fe (50 nmol/L)耦合作用、微量元素Fe (50 nmol/L)和N/P (16∶1)耦合作用及沙尘(4 mg/L)对浮游植物释放CH3I、CHCl3、C2HCl3和CH2Br2含量的影响。结果表明,与对照组相比,实验组CH3I、C2HCl3和CH2Br2的释放均被不同程度抑制;CHCl3的释放除添加沙尘时表现抑制作用外,其他条件下均为促进作用;实验组培养周期内叶绿素a浓度较高,而营养盐浓度变化规律不明显。总的来说,酸化和微量元素Fe可能是影响浮游植物释放挥发性卤代烃的重要限制因素,沙尘对促进浮游植物生长繁殖的影响更为显著。 相似文献