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Well log evaluation of the gas-bearing reservoirs in the Bombay offshore basin, Gulf of Cambay, western coast of India 印度西海岸康拜湾孟买近海盆地含气储层的测井评价
IF 0.9 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2023-12-15 DOI: 10.1080/08123985.2023.2288958
Sikha Rani Mondal, Ranjana Ghosh, Maheswar Ojha, Saumen Maiti
Present study aims to locate potential reservoir zones in the Paleocene, Eocene and Oligocene sequences by analysing well log data of nine vertical wells in the exploration block MB-OSN-2004/1 in t...
本研究的目的是,通过分析渤海湾勘探区块MB-OSN-2004/1九口垂直井的测井数据,确定古新世、始新世和渐新世序列中的潜在储层带。
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引用次数: 0
Seismic data interpolation via Unet with non-local blocks 通过 Unet 对非本地块体进行地震数据插值
IF 0.9 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2023-12-11 DOI: 10.1080/08123985.2023.2290134
Jiajia Cao, Lihua Fu, Wenqian Fang, Mengyi Wu
Due to the constraints of the exploration environment, acquired seismic data are commonly irregular or incomplete, which seriously affects the quality of subsequent seismic data processing and inte...
由于勘探环境的限制,获取的地震数据通常不规则或不完整,这严重影响了后续地震数据处理和集成的质量。
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引用次数: 0
Experimental study on various factors contributing to poor microtremor data processing results using ESAC method 影响ESAC方法微震数据处理效果的各种因素的实验研究
IF 0.9 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2023-11-29 DOI: 10.1080/08123985.2023.2281618
Shuangcheng Ge, Gaoxiang Chen, Yonghui Zhao, Shufan Hu
In practical applications, microtremor data often encounter contamination from various sources of noise, leading to suboptimal processing outcomes. This study aimed to provide a comprehensive analy...
在实际应用中,微震数据经常受到各种噪声源的污染,导致处理结果不理想。本研究旨在全面分析……
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引用次数: 0
Quantitative measurement of the environmental disturbance caused by onshore seismic surveys 陆上地震测量引起的环境扰动的定量测量
IF 0.9 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2023-11-20 DOI: 10.1080/08123985.2023.2279995
Tim Dean
Environmental impact assessments are a key component of the approval process for many onshore seismic surveys. Quantifying the environmental disturbance caused by such surveys is, however, problema...
环境影响评估是许多陆上地震勘探项目审批程序的关键组成部分。然而,量化这些调查造成的环境干扰是一个问题。
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引用次数: 0
Comparative 3D inversion of magnetotelluric phase tensors and impedances reveals electrically anisotropic base of Gawler Craton, South Australia 大地电磁相张量和阻抗对比三维反演揭示了南澳大利亚高勒克拉通的电各向异性基底
IF 0.9 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2023-11-20 DOI: 10.1080/08123985.2023.2281615
Kristina Tietze, Stephan Thiel, Kate Brand, Graham Heinson
Isotropic three-dimensional (3-D) inversion has become a standard tool in the interpretation of magnetotelluric (MT) data. 3-D anisotropic inversion codes are under development, yet the number of u...
各向同性三维反演已成为大地电磁资料解释的标准工具。三维各向异性反演代码正在开发中,但u的数量…
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引用次数: 0
Metasomatism and depletion of the southern Gawler Craton from combined mantle xenocryst and AusLAMP magnetotelluric data 从地幔异种结晶和AusLAMP大地电磁资料看南高勒克拉通的交代和衰竭作用
IF 0.9 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2023-11-20 DOI: 10.1080/08123985.2023.2282711
Kate Selway, Sinan Özaydın, Justin Payne
Metasomatised mantle is considered a prerequisite for the formation of many major ore deposits. Since magnetotellurics (MT) is strongly sensitive to mantle metasomatism, MT is a useful tool for ana...
交代地幔被认为是许多主要矿床形成的先决条件。由于大地电磁对地幔交代作用非常敏感,因此大地电磁是一种非常有用的工具。
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引用次数: 0
AusLAMP shines a light on space weather hazards in the Australian high-voltage power grid AusLAMP照亮了澳大利亚高压电网的空间天气危害
4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2023-11-14 DOI: 10.1080/08123985.2023.2281617
Liejun Wang, Jingming Duan, Adrian P. Hitchman, Matthew G. Gard, Richard A. Marshall, Andrew M. Lewis, William V. Jones
AbstractA geomagnetic storm, also known as a geomagnetic disturbance (GMD), is a major disturbance of the Earth’s magnetic field caused by solar activity. A geomagnetic storm induces electric currents in the Earth that feed into power lines through substation neutral earthing, causing instabilities and even blackouts in electricity transmission systems. The intensity of geomagnetically induced currents (GICs) is closely associated with the electrical conductivity of the surrounding geology. In this paper, we analyse one of the most well-known geomagnetic storms, the 1989 “Québec storm” and 688 magnetotelluric (MT) survey sites from the Australian Lithospheric Architecture Magnetotelluric Project (AusLAMP) to gain insight into the space weather hazard posed for Australia's modern-day power grids. Transmission lines may exhibit local maxima at differing times depending on their spatial orientation and length with respect to the time-varying magnetic field. Localised peak voltages over 100 V can be observed on some individual lines. This assessment identifies the distribution of GICs in south-eastern Australia for the 1989 Québec storm and transmission lines that are more vulnerable to GICs. It is relevant to national strategies and risk assessment procedures to mitigate space weather hazards in the Australian high-voltage power grid and the design of a more resilient power transmission system. We also analyse the 2015 “St Patrick’s Day storm” to study under-estimation of the space weather hazard associated with the band-limited geomagnetic data and MT data sets.Key points The subsurface geology has a great influence on the intensity of geomagnetically induced electric fields, potentially causing up to three orders of magnitude difference between conductive basins and resistive cratonic regions in south-eastern Australia.Analysis using the 1989 “Québec geomagnetic storm” and AusLAMP magnetotelluric data shows the intensity of the geoelectric fields in south-eastern Australia could reach up to 5 [V/km].Geomagnetically induced voltages in the Australian high-voltage power grid could be in excess of 100 V in some transmission lines for a geomagnetic storm with intensity comparable with the 1989 Québec geomagnetic storm.KEYWORDS: Space weather hazardgeomagnetically induced currentshigh-voltage power gridgeomagnetic storms AcknowledgementsThe authors thank Geoscience Australia, the Geological Surveys of Victoria, South Australia, and New South Wales, the University of Adelaide and AuScope for making their MT datasets available for investigation.The geomagnetic field data can be downloaded from the Geoscience Australia Geomagnetism Program (http://www.ga.gov.au).The SECS-MT Python code of Campanyà et al. (Citation2019) has been used for computation of geoelectric field time series. The software of Wessel and Smith (Citation1998) has been used to produce some figures in this paper.We thank Dr Kate Brand, an anonymous reviewer, and editor Dr Mark Lackie for
地磁风暴,又称地磁扰动(GMD),是由太阳活动引起的对地球磁场的重大扰动。地磁风暴在地球上产生电流,通过变电站的中性接地进入输电线,导致电力传输系统不稳定,甚至停电。地磁感应电流(gic)的强度与周围地质的导电性密切相关。在本文中,我们分析了最著名的地磁风暴之一,1989年的“qusamubec风暴”和来自澳大利亚岩石圈建筑大地电磁项目(AusLAMP)的688个大地电磁(MT)测点,以深入了解空间天气对澳大利亚现代电网构成的危害。传输线可能在不同的时间表现出局部最大值,这取决于它们相对于时变磁场的空间方向和长度。在一些单独的线路上可以观察到超过100v的局部峰值电压。这项评估确定了1989年qusamicbec风暴在澳大利亚东南部的gic分布情况,以及更容易受到gic影响的输电线路。它与国家战略和风险评估程序有关,以减轻澳大利亚高压电网中的空间天气危害,并设计更具弹性的输电系统。我们还分析了2015年“圣帕特里克节风暴”,以研究与带限地磁数据和MT数据集相关的空间天气危害的低估。地下地质对地磁感应电场的强度有很大的影响,可能导致澳大利亚东南部导电盆地和电阻克拉通区之间的差异高达3个数量级。利用1989年“qubec地磁暴”和AusLAMP大地电磁资料分析,澳大利亚东南部地电场强度可达5 [V/km]。澳大利亚高压电网中的地磁感应电压在一些输电线路中可能超过100伏,而强度可与1989年的quimadbec地磁风暴相媲美。作者感谢澳大利亚地球科学、维多利亚、南澳大利亚和新南威尔士州地质调查局、阿德莱德大学和AuScope为研究提供了MT数据集。地磁场数据可从澳大利亚地球科学地磁计划下载(http://www.ga.gov.au).The SECS-MT Python code of campany et al. (Citation2019)),用于计算地电场时间序列。本文使用Wessel和Smith (Citation1998)的软件生成了一些数据。我们感谢匿名审稿人Kate Brand博士和编辑Mark Lackie博士在审稿过程中提供的有益意见。我们也感谢澳大利亚地球科学协会的蒋文平博士和Josef Holzschuh博士审阅了我们的初稿。这篇论文是为了纪念F.E.M. (Ted) Lilley博士,他是我们从地球电导率到太空天气危害进行电磁感应研究的灵感来源。本研究已获得澳大利亚地球科学协会(Geoscience australia)首席执行官的许可发表。作者未发现潜在的利益冲突。
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引用次数: 0
Investigation of geothermal resources using a geophysical potential field in the Hurghada area, Egypt 利用地球物理势场对埃及赫尔格达地区地热资源进行调查
4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2023-11-10 DOI: 10.1080/08123985.2023.2276403
Samah Elbarbary, Mohamed Abdel Zaher, Hossam Marzouk, Tarek Arafa-Hamed
AbstractEgypt's need for clean and renewable energy is pressing for numerous reasons, such as unpredictable fuel prices, diminishing fossil fuel resources, and growing concern about environmental degradation. Harvesting untapped geothermal resources could meet domestic electricity needs besides enabling Egypt to export electricity. The location of Egypt confirms that it has suitable geothermal energy potential areas in some provinces around the country, especially along the Gulf of Suez, the Red Sea, and the Western Desert. The Red Sea coast and the coasts of the Gulf of Suez exhibit several surface manifestations (hot springs and thermal water wells), indicating the presence of geothermal systems in these areas. The objective of this paper is to investigate the geothermal resources and obtain a full image of the geothermal potential of the Hurghada area along the Red Sea coast using geophysical potential field data. Aeromagnetic and aerogravity data were used to identify the most promising target regions for geothermal potentiality. Power spectral analysis of the aeromagnetic data was utilised to appraise the Curie point depth (CPD) and obtain geothermal gradient and heat flow maps of the Hurghada area, whereas a 3-D inversion of gravity data was utilised to estimate the depths to the Precambrian basement rocks. In addition to 3-D inversion of magnetic data to evaluate the spatial distribution of magnetic susceptibility. This study found no direct relationship between basement depths and the CPD, where basement rock outcrops at some locations correlate to a decrease in the Curie surface, while at others, they correspond to an increase.KEYWORDS: aeromagneticaerogravityCurie point depthheat flowPrecambrian basement Disclosure statementNo potential conflict of interest was reported by the author(s).Additional informationFundingThis research was mainly funded by the Science and Technology Development Fund (STDF) in Egypt via a Development & Innovation Grant titled “A Prospective Study of the Geothermal Potential in Egypt.” (Project ID: 43553).
埃及对清洁和可再生能源的需求非常迫切,原因有很多,比如不可预测的燃料价格、日益减少的化石燃料资源以及对环境恶化的日益担忧。开采未开发的地热资源可以满足埃及国内的电力需求,还可以出口电力。埃及的地理位置确定了它在全国一些省份拥有合适的地热潜力区域,特别是沿着苏伊士湾、红海和西部沙漠。红海沿岸和苏伊斯湾沿岸表现出几种地表现象(温泉和热水井),表明这些地区存在地热系统。本文的目的是利用地球物理位场资料对红海沿岸赫尔格达地区的地热资源进行调查,并获得地热潜力的完整图像。利用航空磁和航空重力数据确定了最有希望的地热潜力目标区域。利用航磁数据的功率谱分析估算了赫尔格达地区的居里点深度(CPD),获得了地热梯度和热流图,利用重力数据的三维反演估算了前寒武纪基底岩的深度。此外,还对磁资料进行三维反演,评价磁化率的空间分布。这项研究没有发现基底深度和CPD之间的直接关系,在一些地方基底岩石的露头与居里表面的减少有关,而在另一些地方,它们对应于增加。关键词:航空磁学航空重力居里点深度热流前寒武纪基底披露声明作者未报告潜在利益冲突。本研究主要由埃及科学技术发展基金(STDF)通过题为“埃及地热潜力的前瞻性研究”的发展与创新基金资助。(项目ID: 43553)。
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引用次数: 0
The resistive limit response of an ellipsoidal conductor: a magnetostatic formulation 椭球导体的电阻极限响应:静磁公式
4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2023-11-10 DOI: 10.1080/08123985.2023.2275804
Peter K. Fullagar
AbstractInterpreting transient electromagnetic (TEM) anomalies in terms of conductive rectangular plates is effective in many situations. However, not all conductors are thin and planar. Triaxial ellipsoid conductors are an attractive alternative: geometrically simple (corner-free), mathematically tractable at early and late time limits, and able to encompass shapes ranging from discs to elongate lenses to equi-dimensional pods. Accordingly a fast magnetostatic algorithm has been developed to compute the resistive limit (RL) response of a ellipsoidal conductor, which may also be permeable. The algorithm has been validated against new analytic resistive limit solutions for spherical and spheroidal conductors and against 3D multigrid finite difference modelling for a triaxial ellipsoidal conductor. A uniformly conductive ellipsoid supports three fundamental current modes in the resistive limit, an independent mode for excitation parallel to each of the principal axes. The RL current density increases linearly with radial distance from the ellipsoid centre. A formula for the time constant of an oblate spheroid has been derived for excitation parallel to its rotational axis, namely τ3≈σμ0bc/(4+6c/b), where σ is the conductivity and c and b are respectively the minor and major radii.KEYWORDS: Ellipsoidresistive limitelectromagneticsmodelling AcknowledgementsI am indebted to the late Dr. Yves Lamontagne (Lamontagne Geophysics) who kindly modelled triaxial ellipsoid RL responses using his MGEM 3D multigrid finite difference program and who provided physical insights. Dr. David Clark (CSIRO/Integrated Magnetics LLC) assisted with theoretical aspects, and in particular confirmed my derivation of equation (22) for the RL field inside a spherical conductor.Disclosure statementNo potential conflict of interest was reported by the author(s).
摘要用导电矩形板解释瞬变电磁(TEM)异常在许多情况下是有效的。然而,并不是所有的导体都是薄而平面的。三轴椭球导体是一种有吸引力的替代方案:几何上简单(无角),在早期和晚期的时间限制下在数学上易于处理,并且能够涵盖从圆盘到拉长透镜到等维吊舱的各种形状。因此,我们开发了一种快速的静磁算法来计算椭球导体的电阻极限(RL)响应,这种椭球导体也可能是可渗透的。该算法已通过球面和球面导体的新的解析电阻极限解和三轴椭球导体的三维多网格有限差分模型进行了验证。一个均匀导电的椭球体在电阻极限下支持三种基本电流模式,一种与每个主轴平行的独立激励模式。RL电流密度随距椭球中心径向距离的增加而线性增加。推导了平行于其旋转轴的椭球的时间常数公式τ3≈σμ0bc/(4+6c/b),其中σ为电导率,c和b分别为小半径和大半径。感谢已故的Yves Lamontagne博士(Lamontagne地球物理学),他用他的MGEM 3D多网格有限差分程序模拟了三轴椭球体RL响应,并提供了物理见解。David Clark博士(CSIRO/Integrated Magnetics LLC)在理论方面提供了帮助,特别是证实了我对球形导体内RL场的推导公式(22)。披露声明作者未报告潜在的利益冲突。
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引用次数: 0
Remote sensing campaign at the Roman Villa of Caddeddi on the Tellaro river (Noto, Italy) 在Tellaro河上的卡迪迪罗马别墅的遥感活动(诺托,意大利)
4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2023-10-11 DOI: 10.1080/08123985.2023.2266446
D. Tanasi, R. Lanteri, S. Hassam, P. Trapani, D. Calderone, K. Kingsland, L. De Giorgi, I. Ferrari, G. Fragalá, F. Giuri, G. Leucci
AbstractThe Villa of Caddeddi, in the territory of Noto (Siracusa) is located on the south bank of the Tellaro river, about 3 km from its mouth. The site, interpreted as a rural luxury residence dated to the fourth–fifth century CE, was first discovered in 1972 and intermittently investigated in the subsequent decades and mostly studied from the perspectives of the splendid mosaic floors there uncovered. The excavated structure accounts for just a portion of the complex, which is partially covered by an eighteenth–nineteenth century farmhouse. After a long period of neglect, the villa, mainly known in literature for its exquisite mosaic floors, has been recently restored and opened to the public and become subject of new studies by the University of South Florida’s Institute for Digital Exploration (IDEx) and the Institute of Heritage Science – CNR which between 2019 and 2022 conducted a remote sensing, using ground penetrating radar method, campaign in partnership with the Parco Archeologico e Paesaggistico di Siracusa, Eloro, Villa del Tellaro e Akrai. The results related to the digital exploration and ground penetrating radar allow new knowledge relating to the Roman villa and allows a scientific reconstruction of the villa.KEYWORDS: Roman Sicilyground penetrating radargeophysical surveyRoman Villa Disclosure statementNo potential conflict of interest was reported by the author(s).
【摘要】卡迪迪别墅位于诺托(锡拉库萨)境内,位于特拉罗河南岸,距离河口约3公里。该遗址被认为是一座可追溯到公元4 - 5世纪的乡村豪华住宅,于1972年首次被发现,在随后的几十年里,人们对它进行了断断续续的调查,主要是从那里发现的华丽马赛克地板的角度进行研究。挖掘出的结构只是建筑群的一部分,建筑群部分被一座18 - 19世纪的农舍所覆盖。经过长时间的忽视,别墅主要以其精美的马赛克地板在文学中闻名,最近已被修复并向公众开放,并成为南佛罗里达大学数字探索研究所(IDEx)和遗产科学研究所(CNR)的新研究对象,该研究所在2019年至2022年期间与Eloro的Parco Archeologico e Paesaggistico di Siracusa合作,使用探地雷达方法进行遥感活动。Villa del Tellaro e Akrai。与数字探测和探地雷达相关的结果提供了与罗马别墅有关的新知识,并允许对别墅进行科学重建。关键词:罗马西西里探地雷达地球物理测量罗马别墅披露声明作者未报告潜在的利益冲突。
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Exploration Geophysics
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