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...
{"title":"Well log evaluation of the gas-bearing reservoirs in the Bombay offshore basin, Gulf of Cambay, western coast of India","authors":"Sikha Rani Mondal, Ranjana Ghosh, Maheswar Ojha, Saumen Maiti","doi":"10.1080/08123985.2023.2288958","DOIUrl":"https://doi.org/10.1080/08123985.2023.2288958","url":null,"abstract":"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...","PeriodicalId":50460,"journal":{"name":"Exploration Geophysics","volume":"7 1","pages":""},"PeriodicalIF":0.9,"publicationDate":"2023-12-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138685701","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2023-12-11DOI: 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。
{"title":"Seismic data interpolation via Unet with non-local blocks","authors":"Jiajia Cao, Lihua Fu, Wenqian Fang, Mengyi Wu","doi":"10.1080/08123985.2023.2290134","DOIUrl":"https://doi.org/10.1080/08123985.2023.2290134","url":null,"abstract":"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...","PeriodicalId":50460,"journal":{"name":"Exploration Geophysics","volume":"58 1","pages":""},"PeriodicalIF":0.9,"publicationDate":"2023-12-11","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138572736","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2023-11-29DOI: 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……
{"title":"Experimental study on various factors contributing to poor microtremor data processing results using ESAC method","authors":"Shuangcheng Ge, Gaoxiang Chen, Yonghui Zhao, Shufan Hu","doi":"10.1080/08123985.2023.2281618","DOIUrl":"https://doi.org/10.1080/08123985.2023.2281618","url":null,"abstract":"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...","PeriodicalId":50460,"journal":{"name":"Exploration Geophysics","volume":"273 1","pages":""},"PeriodicalIF":0.9,"publicationDate":"2023-11-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138540333","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2023-11-20DOI: 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...
{"title":"Quantitative measurement of the environmental disturbance caused by onshore seismic surveys","authors":"Tim Dean","doi":"10.1080/08123985.2023.2279995","DOIUrl":"https://doi.org/10.1080/08123985.2023.2279995","url":null,"abstract":"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...","PeriodicalId":50460,"journal":{"name":"Exploration Geophysics","volume":"6 1","pages":""},"PeriodicalIF":0.9,"publicationDate":"2023-11-20","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138540361","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2023-11-20DOI: 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…
{"title":"Comparative 3D inversion of magnetotelluric phase tensors and impedances reveals electrically anisotropic base of Gawler Craton, South Australia","authors":"Kristina Tietze, Stephan Thiel, Kate Brand, Graham Heinson","doi":"10.1080/08123985.2023.2281615","DOIUrl":"https://doi.org/10.1080/08123985.2023.2281615","url":null,"abstract":"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...","PeriodicalId":50460,"journal":{"name":"Exploration Geophysics","volume":"7 1","pages":""},"PeriodicalIF":0.9,"publicationDate":"2023-11-20","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138540353","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2023-11-20DOI: 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...
{"title":"Metasomatism and depletion of the southern Gawler Craton from combined mantle xenocryst and AusLAMP magnetotelluric data","authors":"Kate Selway, Sinan Özaydın, Justin Payne","doi":"10.1080/08123985.2023.2282711","DOIUrl":"https://doi.org/10.1080/08123985.2023.2282711","url":null,"abstract":"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...","PeriodicalId":50460,"journal":{"name":"Exploration Geophysics","volume":"94 1","pages":""},"PeriodicalIF":0.9,"publicationDate":"2023-11-20","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138540360","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2023-11-14DOI: 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。
{"title":"AusLAMP shines a light on space weather hazards in the Australian high-voltage power grid","authors":"Liejun Wang, Jingming Duan, Adrian P. Hitchman, Matthew G. Gard, Richard A. Marshall, Andrew M. Lewis, William V. Jones","doi":"10.1080/08123985.2023.2281617","DOIUrl":"https://doi.org/10.1080/08123985.2023.2281617","url":null,"abstract":"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","PeriodicalId":50460,"journal":{"name":"Exploration Geophysics","volume":"67 17","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"2023-11-14","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"134901593","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
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).
{"title":"Investigation of geothermal resources using a geophysical potential field in the Hurghada area, Egypt","authors":"Samah Elbarbary, Mohamed Abdel Zaher, Hossam Marzouk, Tarek Arafa-Hamed","doi":"10.1080/08123985.2023.2276403","DOIUrl":"https://doi.org/10.1080/08123985.2023.2276403","url":null,"abstract":"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).","PeriodicalId":50460,"journal":{"name":"Exploration Geophysics","volume":"52 1","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"2023-11-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"135092750","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2023-11-10DOI: 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).
{"title":"The resistive limit response of an ellipsoidal conductor: a magnetostatic formulation","authors":"Peter K. Fullagar","doi":"10.1080/08123985.2023.2275804","DOIUrl":"https://doi.org/10.1080/08123985.2023.2275804","url":null,"abstract":"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).","PeriodicalId":50460,"journal":{"name":"Exploration Geophysics","volume":"76 4","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"2023-11-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"135092851","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2023-10-11DOI: 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。
{"title":"Remote sensing campaign at the Roman Villa of Caddeddi on the Tellaro river (Noto, Italy)","authors":"D. Tanasi, R. Lanteri, S. Hassam, P. Trapani, D. Calderone, K. Kingsland, L. De Giorgi, I. Ferrari, G. Fragalá, F. Giuri, G. Leucci","doi":"10.1080/08123985.2023.2266446","DOIUrl":"https://doi.org/10.1080/08123985.2023.2266446","url":null,"abstract":"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).","PeriodicalId":50460,"journal":{"name":"Exploration Geophysics","volume":"59 1","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"2023-10-11","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"136210876","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}