The oxygen isotope composition of water masses within the North Sea

Based on measurements of the ¹⁸O isotope composition of 247 samples collected over a 3-year period we have assessed the oxygen isotope composition of water masses in the North Sea. This is the first δ¹⁸O data set that covers the entire North Sea basin. The waters lie on a mixing line: δ¹⁸O (‰_VSMOW) = −9.300 + 0.274(S) with North Atlantic sub-polar mode water (SPMW) and surface waters, and Baltic Sea water representing the saline and freshwater end members respectively. Patterns exhibited in surface and bottom water δ¹⁸O distributions are representative of the general circulation of the North Sea. Oxygen-18 enriched waters from the North Atlantic enter the North Sea between Scotland and Norway and to a lesser extent through the English Channel. In contrast, oxygen-18 depleted waters mainly inflow from the Baltic Sea, the rivers Rhine and Elbe, and to a lesser degree, the Norwegian Fjords and other river sources. Locally the δ¹⁸O–salinity relationship will be controlled by the isotopic composition of the freshwater inputs. However, the range of local freshwater compositions around the North Sea basin is too narrow to characterise the relative contributions of individual sources to the overall seawater composition. This dataset provides important information for a number of related disciplines including biogeochemical research and oceanographic studies.     

Repacking practice for G-3 engineering driller power unit with drive shaft of dual channel reverse circulation

In order to satisfy operating requirements for constant core drilling technology in reverse circulation with hollow-through DTH,the power unit of G-3 engineering driller was ameliorated. The new one with dual channel drive shaft, achieved the perfect assemble with transmission structure of the original power unit. It could interconvert according to need by using two sets of drive shafts with direct and reverse circulation. The repacked G-3 engineering driller carried on experiment in the field test in Luanchuan molybdenum mine of Henan, whose effect was very good.     

对地勘单位贯彻ISO9000《质量管理和质量保证》系列标准的几点认识

ISO9000系列标准是一套国际统一的质量管理标准,应用的主体内容是质量管理模式(质量体系)的建立与运行。其对地勘单位走向市场,到社会投标、承揽地勘项目,保证地勘工作成果质量,提高单位在地质市场中的信誉度具有十分重要的意义。     

广西若干重大基础地质特征

文章根据华南地区物探、化探、遥感编图广西综合解译成果,研究广西若干重大基础地质特征,着重讨论地壳结构、深部构造、主要隐伏深断裂带、基底性质等,以板块观点划分大地构造单元,提出广西地壳属陆壳型性质和扬子板块在广西的边界划在三江-大新一线的新认识.     

北部湾灯光罩网渔场时空分布与海洋环境关系分析 *

文章根据大型灯光罩网渔船调查数据和卫星遥感海面风场(Sea Surface Wind, SSW)、海表温度(Sea Surface Temperature, SST)和叶绿素a浓度(Chlorophyll a concentration, Chl a)资料, 基于广义线性模型(Generalized Linear Model, GLM)对北部湾渔业资源单位捕捞努力量渔获量(Catch Per Unit Effort, CPUE)进行标准化, 应用多元线性回归等方法, 对北部湾灯光罩网渔场的时空分布及其与海洋环境的关系进行了分析。结果表明, 北部湾灯光罩网渔场适宜SST为27~29℃, Chl a为0.5~1.5mg·m ^-3。较高资源量出现在10月份中上旬, 分布在18°—19°N及20°—21°N海域。北部湾灯光罩网渔场的时空分布与季风、19°N附近的暖水池和Chl a等环境因素有关。     

培育密度和投饵量对长牡蛎壳黑选育品系幼虫生长存活及附着变态的影响

为探究长牡蛎(Crassostrea gigas)壳黑选育品系规模化繁育适宜的培育密度和投饵量,本研究以长牡蛎野生群体幼虫为对照组,分析了不同培育密度(3、7和15个/mL)和不同初始投饵量(0.4、0.8和1.6×10~3cells·ind^-1·d^-1)对长牡蛎壳黑选育品系幼虫生长、存活及附着的影响。研究显示,培育密度和投饵量对长牡蛎幼虫的生长速率、存活率和附着率有显著交互作用(P<0.05)。在培育密度3和7个/mL实验组,长牡蛎幼虫生长速率随投饵量增加而显著增大(P<0.05),并在培育密度7个/mL、投饵量1.6×10~3cells·ind^-1·d^-1实验组达到最大值。而在培育密度15个/mL实验组,投饵量增加对长牡蛎幼虫的生长速率无显著影响(P> 0.05)。且在培育密度15个/mL、投饵量1.6×10~3cells·ind^-1·d^-1实验组长牡蛎壳黑品系幼虫存活率和附着率最低。但在培育密度15个/mL实验组长牡蛎壳黑选育品系幼虫的壳高始终高于野生群体幼虫。且除投饵量0.4×10~3cells·ind^-1·d^-1实验组外,长牡蛎壳黑选育品系幼虫生长速率、存活率和附着率均高于野生群体幼虫。研究结果表明,长牡蛎壳黑选育品系幼虫最适培育条件为培育密度7个/mL、投饵量1.6×10~3cells·ind^-1·d^-1,增加投饵量可促进长牡蛎幼虫生长,但过高的培育密度会与投饵量产生拮抗作用,抑制幼虫生长,不利于幼虫存活和附着。与长牡蛎野生群体相比,壳黑选育品系幼虫能适应更高的培育密度环境,在饵料充足的条件下,其幼虫的生长、存活及附着性状均优于野生群体。     

机载激光点云中高压电塔自动识别方法

提出了一种基于格网特征的机载激光点云高压电塔自动识别方法。首先对机载激光点云数据进行滤波去噪处理;然后对点云数据进行规则格网化特征分析获得高压电塔粗识别区域;最后对粗识别区域进行外接邻域网格线性特征悬空点集检测以确定电塔识别结果,并以分层切片法分析获取电塔平面中心坐标。采用大型无人机实际线路巡检获取的机载点云数据对本文算法进行验证,试验结果表明本算法可实现高压电塔的快速自动识别,对无人机电力巡检智能诊断具有一定的促进作用。     

The use of cartographic control points in the harmonization and revision of MRDBs

The main purpose of the research is to achieve fully automated approach for supplying multi-resolution databases with linear objects in each scale. Moreover, the proposed solutions maintain the repeatability and accuracy of output data wherever possible according to the input scale. These properties are achieved by keeping the minimal object dimensions as well as the appropriate data pre-processing, based on the classification of source points. The classification distinguishes three classes of points: constant (unchangeable), temporary, and inherited. These classes build a structure of cartographic control points. Based on these solutions, the authors proposed an algorithm for linear object simplification based on minimal object dimensions and cartographic control points. It was also confirmed that the simplification between constant points does not cause geometry discrepancies in relation to the global simplification of the whole line.     

基于面片裁切技术的点云轮廓线生成算法

随着点云在各个领域的广泛应用,对点云处理相关技术的研究更为活跃。目前,研究的热点主要集中在点云去噪、配准、分割、增强、特征提取和重建等方面。其中,特征提取起着承前启后的作用,具有十分重要的研究价值。基于面片裁切技术的点云轮廓线生成算法。首先,对点云数据进行面片提取,通过面片生长、融合生成特征面片,并根据提出的面片双向索引法快速构造特征线,最终实现点云平面轮廓线的生成。实验证明,本算法可快速、准确、有效地实现点云轮廓线的生成。     

Transition-region explosive events produced by plasmoid instability

Magnetic reconnection is thought to be a key process in most solar eruptions. Thanks to highresolution observations and simulations, the studied scale of the reconnection process has become smaller and smaller. Spectroscopic observations show that the reconnection site can be very small, which always exhibits a bright core and two extended wings with fast speeds, i.e., transition-region explosive events.In this paper, using the PLUTO code, we perform a 2-D magnetohydrodynamic simulation to investigate small-scale reconnection in double current sheets. Based on our simulation results, such as the line-of-sight velocity, number density and plasma temperature, we can synthesize the line profile of SiIV 1402.77? which is a well known emission line used to study transition-region explosive events on the Sun. The synthetic line profile of Si IV 1402.77? is complex with a bright core and two broad wings which can extend to nearly 200 km s^-1. Our simulation results suggest that the transition-region explosive events on the Sun are produced by plasmoid instability during small-scale magnetic reconnection.