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Spatial variation, sources, and trajectory of black carbon in the South Sumatra Region of Indonesia using MERRA-2 reanalysis data 利用 MERRA-2 再分析数据研究印度尼西亚南苏门答腊地区黑碳的空间变化、来源和轨迹
IF 2.3 4区 地球科学 Pub Date : 2024-09-18 DOI: 10.1007/s11600-024-01444-x
Muhammad Rendana, Novia Novia, Tuti Indah Sari, Maulana Yusuf, Idarwati

A high temperature and lack of rainfall in the South Sumatra Region during the dry season of 2019 led to an increase in intense land fires that were attributed to biomass burning and the pyrogenic combustion process. This study tried to analyze the spatiotemporal distributions of atmospheric BC (black carbon) over the South Sumatra Region during 2016–2019 land fire events using the MERRA-2 satellite images. The spatial analysis was applied to estimate the increment in black carbon concentrations during land fire episodes. Some meteorological conditions that affect black carbon diffusion and transport over the study area are explained using a backward trajectory analysis. The results exhibited that the black carbon masses mostly came from local and long-range transports (from eastern to western) over the study area. A significant percentage increment of black carbon concentration during 2016–2019 was observed at around 139%. The highest black carbon concentration recorded in October 2019 was 3.96 × 10−6 kg/m2, as hotspots were still abundant, especially on the eastern side of the study area. The black carbon trend was strongly related to total hotspots and burned areas. As a whole, this finding could be beneficial for mitigating black carbon pollution due to land fires by implementing geospatial technology for rapid monitoring of air pollution in vast areas.

2019 年旱季期间,南苏门答腊地区高温少雨,导致生物质燃烧和热源燃烧过程引起的强烈陆地火灾增加。本研究试图利用 MERRA-2 卫星图像分析 2016-2019 年陆地火灾事件期间南苏门答腊地区大气中 BC(黑碳)的时空分布。应用空间分析估算了陆火事件期间黑碳浓度的增量。利用后向轨迹分析解释了影响研究区域黑碳扩散和迁移的一些气象条件。结果表明,黑碳质量主要来自研究区域的本地和长程飘移(从东部到西部)。在 2016-2019 年期间,黑碳浓度出现了明显的百分比增长,约为 139%。2019 年 10 月记录到的最高黑碳浓度为 3.96 × 10-6 kg/m2,因为热点地区仍然很多,尤其是在研究区域的东部。黑碳趋势与热点总数和燃烧面积密切相关。总体而言,这一发现有助于通过采用地理空间技术快速监测广阔地区的空气污染,从而减轻陆地火灾造成的黑碳污染。
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引用次数: 0
3D UHR seismic and back-scattering analysis for seabed and ultra-shallow subsurface classification 用于海床和超浅层地下分类的三维 UHR 地震和反向散射分析
IF 2.3 4区 地球科学 Pub Date : 2024-09-10 DOI: 10.1007/s11600-024-01423-2
Jiho Ha, Jungkyun Shin, Kyoungmin Lim, In-Kwon Um, Boyeon Yi

Recently, the seabed classification method based on back-scattering data of multi-beam echo-sounder (MBES) is widely used to analyze the distribution of seabed sediment. Although various analysis methods for seabed classification using multi-spectral MBES have been developed, they are limited in securing penetration depth to consider the characteristics of the shallow subsurface structure. In this study, the seabed and ultra-shallow subsurface classification was performed by comparative analysis of box corer sampling, back-scattering, and 2D/3D ultra-high-resolution (UHR) seismic data obtained from Yeongil Bay, South Korea. We proposed a process for seismic ultra-shallow subsurface classification by the segmentation of the primary seabed reflection wavelet and the amplitude analysis. The seabed-reflected amplitude and back-scattering intensity showed similar mapping trends in the relatively homogeneous and thick surface sediment. On the other hand, it was confirmed that back-scattering data and seabed-reflected amplitude show different patterns when the subsurface structure is related to the seabed surface. It is presumed that because seismic data containing relatively low-frequency components have a deeper penetration depth than MBES, they contain more characteristics of the ultra-shallow subsurface than back-scattering data. These were determined that back-scattering has advantages in representing acoustic anomaly distribution by surface sediment type, and seabed-reflected amplitude is advantageous for representing sediment type by ultra-shallow subsurface. In particular, these results were well shown when the surface sediment thinly covered the rocky bottom. Therefore, it is necessary not only to analyze the back-scattering of MBES but also the ultra-shallow subsurface features through seismic data for valid seabed classification.

最近,基于多波束回声测深仪(MBES)反向散射数据的海底分类方法被广泛用于分析海底沉积物的分布。虽然已开发出多种利用多波束回声测深仪进行海底分类的分析方法,但这些方法在确保穿透深度方面受到限制,无法考虑浅层地下结构的特点。在本研究中,通过对从韩国永吉湾获得的箱式取样器取样、反向散射和二维/三维超高分辨率(UHR)地震数据进行对比分析,对海底和超浅表层进行了分类。我们提出了一种通过初级海底反射小波分割和振幅分析进行地震超浅层地下分类的方法。在相对均匀和较厚的表层沉积物中,海底反射振幅和反向散射强度显示出相似的映射趋势。另一方面,当地下结构与海床表面相关时,反向散射数据和海床反射振幅显示出不同的模式。据推测,由于包含相对低频成分的地震数据比 MBES 的穿透深度更深,它们比反向散射数据包含更多的超浅层次特征。经确定,反向散射在按表层沉积物类型表示声异常分布方面具有优势,而海底反射振幅在按超浅层次表层表示沉积物类型方面具有优势。特别是,当表层沉积物薄薄地覆盖在岩石底部时,这些结果得到了很好的体现。因此,不仅需要分析 MBES 的反向散射,还需要通过地震数据分析超浅亚表层特征,以进行有效的海底分类。
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引用次数: 0
Pore pressure estimation of the calcareous formations in the Middle Magdalena Valley Basin, Colombia 哥伦比亚中马格达莱纳河谷盆地钙质地层的孔隙压力估算
IF 2.3 4区 地球科学 Pub Date : 2024-09-05 DOI: 10.1007/s11600-024-01357-9
Melina Rivera, Luis Alfredo Montes, Luis Antonio Castillo

The reliable prediction of pore pressure is essential for petroleum engineering in its different stages, with the Eaton and Bowers' methods being the most used for this purpose. However, their application in carbonate rocks still needs to be improved because carbonates do not compact uniformly with depth, as shale does. This research calculated the pore pressure using the Eaton, Bowers, and Weakley methods and well logs of a carbonate formation and found that the Weakley's approach predicts pressure more accurately. The method presented uses an acoustic impedance equation derived from the Bowers' method, whose parameters were calibrated with the Weakley's pore pressure profile. The pore pressure estimated near the borehole, via the acoustic impedance provided by the pre-stack inversion, is very close to that observed during drilling, which indicates a reliable prediction. The method was applied to a seismic line and well logs in the Middle Magdalena Valley Basin—Colombia, where the overpressured well Lizama 158 caused a significant environmental disaster in 2018. The obtained subsurface pore pressure distribution is reliable, matches overpressure in calcareous rocks near the well, and estimates anomalous pressure in zones distant from the well.

可靠的孔隙压力预测对石油工程的不同阶段都至关重要,其中最常用的是伊顿和鲍尔斯方法。然而,它们在碳酸盐岩中的应用仍有待改进,因为碳酸盐岩不像页岩那样随深度均匀致密。这项研究使用伊顿、鲍尔和韦克利方法以及碳酸盐岩层的测井记录计算孔隙压力,结果发现韦克利方法预测压力更为准确。所介绍的方法使用了从 Bowers 方法中推导出的声阻抗方程,其参数根据 Weakley 的孔隙压力曲线进行了校准。通过叠前反演提供的声阻抗估算出的钻孔附近的孔隙压力与钻探过程中观测到的孔隙压力非常接近,这表明预测结果是可靠的。该方法被应用于哥伦比亚中马格达莱纳河谷盆地的地震测线和测井记录,该盆地的 Lizama 158 井超压在 2018 年造成了重大环境灾难。所获得的地下孔隙压力分布是可靠的,与油井附近钙质岩石中的超压相匹配,并估算了远离油井区域的异常压力。
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引用次数: 0
Characterization of fault-karst reservoirs based on deep learning and attribute fusion 基于深度学习和属性融合的断层喀斯特储层特征描述
IF 2.3 4区 地球科学 Pub Date : 2024-08-31 DOI: 10.1007/s11600-024-01420-5
Zhipeng Gui, Junhua Zhang, Yintao Zhang, Chong Sun

The identification of fault-karst reservoir is crucial for the exploration and development of fault-controlled oil and gas reservoirs. Traditional methods primarily rely on well logging and seismic attribute analysis for karst cave identification. However, these methods often lack the resolution needed to meet practical demands. Deep learning methods offer promising solutions by effectively overcoming the complex response characteristics of seismic wave fields, owing to their high learning capabilities. Therefore, this research proposes a method for fault-karst reservoir identification. Initially, a comparative analysis between the improved U-Net++ network and traditional deep convolutional networks is conducted to select appropriate training parameters for separate training of karst caves and faults. Subsequently, the trained models are applied to actual seismic data to predict karst caves and faults within the research area, followed by attribute fusion to acquire data on fault-karst reservoirs. The results indicate that: (1) The proposed method effectively identifies karst caves and faults, outperforming traditional seismic attribute and coherence methods in terms of identification accuracy, and slightly surpassing U-Net and FCN; (2) The fusion of predicted karst caves and faults yields clear delineation of the relationship between top karst caves and bottom fractures within the research area. In summary, the proposed method for fault-karst reservoirs identification and characterization provides valuable insights for the exploration and development of fault-controlled oil and gas reservoirs in the region.

断层岩溶储层的识别对于断层控制油气藏的勘探和开发至关重要。传统方法主要依靠测井和地震属性分析来识别岩溶洞穴。然而,这些方法往往缺乏满足实际需求所需的分辨率。深度学习方法凭借其高度的学习能力,有效克服了地震波场的复杂响应特性,提供了前景广阔的解决方案。因此,本研究提出了一种断层喀斯特储层识别方法。首先,对改进的 U-Net++ 网络和传统的深度卷积网络进行对比分析,选择合适的训练参数,分别对岩溶洞穴和断层进行训练。随后,将训练好的模型应用于实际地震数据,预测研究区域内的岩溶洞穴和断层,再通过属性融合获取断层岩溶储层数据。结果表明(1) 所提出的方法有效地识别了岩溶洞穴和断层,在识别精度方面优于传统的地震属性和相干性方法,并略高于 U-Net 和 FCN;(2) 对预测的岩溶洞穴和断层进行融合后,研究区内顶部岩溶洞穴和底部断裂之间的关系得到了清晰的划分。总之,所提出的断层岩溶储层识别和特征描述方法为该地区断层控制油气藏的勘探和开发提供了宝贵的见解。
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引用次数: 0
Increase in porosity and permeability resolution for thin-bedded Miocene formation in Carpathian Foredeep using different clustering methods 采用不同聚类方法提高喀尔巴阡山前深海中新世薄层的孔隙度和渗透率分辨率
IF 2.3 4区 地球科学 Pub Date : 2024-08-14 DOI: 10.1007/s11600-024-01409-0
Sebastian Waszkiewicz, Paulina Krakowska-Madejska

The accurate interpretation of well-logging data is a crucial stage in the exploration of gas- and oil-bearing reservoirs. Geological formations, such as the Miocene deposits, present many challenges related to thin layers, whose thickness is often less than the measurement resolution. This research emphasizes the potential of utilizing electrofacies in such challenging environments. The application of electrofacies not only allows for the grouping of intervals with similar physical characteristics but can also be useful for estimating porosity and permeability parameters. For this purpose, various clustering methods were tested, including the 2D indexed and probabilized self-organizing map (IPSOM) method with and without supervision. Subsequently, the usefulness of the obtained results to improve the estimation of porosity and permeability parameters with the help of artificial neural networks was verified. As a result of the conducted analyses, significantly better results were obtained compared to classical petrophysical interpretation. The calculated porosity and permeability parameters were characterized by much greater variability and alignment with laboratory measurements on porosity and permeability. The best results were obtained for the IPSOM method, but the other methods did not differ significantly. In conclusion, the studies have shown a positive result of applying clustering methods, including the IPSOM method, to improve the estimation of permeability and porosity parameters in complicated, thinly-layered formations.

准确解释测井数据是含气和含油储层勘探的关键阶段。中新世矿床等地质构造的薄层厚度往往小于测量分辨率,这给我们带来了许多挑战。这项研究强调了在这种具有挑战性的环境中利用电积层的潜力。电弧面的应用不仅可以将物理特征相似的区间分组,还可以用于估算孔隙度和渗透率参数。为此,对各种聚类方法进行了测试,包括有监督和无监督的二维索引和概率自组织图(IPSOM)方法。随后,在人工神经网络的帮助下,验证了所获结果对改进孔隙度和渗透率参数估算的有用性。分析结果表明,与传统的岩石物理解释相比,所获得的结果要好得多。计算出的孔隙度和渗透率参数具有更大的可变性,并与实验室测量的孔隙度和渗透率相一致。IPSOM 方法的结果最好,但其他方法的结果差异不大。总之,研究表明,应用聚类方法(包括 IPSOM 方法)来改进复杂薄层地层中渗透率和孔隙度参数的估算具有积极意义。
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引用次数: 0
Fine structures of a solar type III radio bursts observed with LOFAR 用 LOFAR 观测到的太阳 III 型射电暴的精细结构
IF 2.3 4区 地球科学 Pub Date : 2024-08-13 DOI: 10.1007/s11600-024-01421-4
Bartosz Dabrowski, Aleksandra Wolowska, Christian Vocks, Jasmina Magdalenić, Peijin Zhang, Pawel Flisek, Malte Bröse, Diana E. Morosan, Andrzej Krankowski, Adam Fron, Gottfried Mann, Pietro Zucca, Mario Bisi, Richard Fallows, Peter Gallagher, Christophe Marqué, Barbara Matyjasiak, Hanna Rothkaehl

We present spectral and imaging LOFAR (LOw-Frequency ARray) observations in the 20 – 40 MHz range of solar radio bursts fine structures, such as flag-like, sail-like, and dot-like that appeared on 8 April 2019. These structures were associated with type III solar radio bursts that occurred in the 40 – 80 MHz band. The mean duration and spectral widths of the fine structures range from 1.0 to 3.4 s and from 0.3 to 0.9 MHz, respectively. Additionally, we investigated the radio images of eight fine structures – two flags, two sails and four dots. This allowed us to determine their emission source sizes, which ranged from 240 to 392 arcmin({}^2), and their frequencies from 25.58 to 39.25 MHz as well as their location. They occurred on the east side of the Sun and were most likely associated with an emerging active region NOAA AR 12738, where a weak B1.7 flare was observed.

我们介绍了对2019年4月8日出现的太阳射电暴精细结构(如旗状、帆状和点状)在20 - 40 MHz范围内的光谱和成像LOFAR(LOw-Frequency ARray)观测结果。这些结构与发生在 40 - 80 MHz 频段的 III 型太阳射电暴有关。精细结构的平均持续时间和光谱宽度分别为 1.0 至 3.4 秒和 0.3 至 0.9 兆赫。此外,我们还研究了八个精细结构的无线电图像--两面旗、两面帆和四个点。这使我们能够确定它们的发射源大小,从 240 到 392 arcmin({}^2) 不等,频率从 25.58 到 39.25 MHz 不等,以及它们的位置。它们发生在太阳的东侧,很可能与一个新出现的活跃区域 NOAA AR 12738 有关,在那里观测到了一个微弱的 B1.7 耀斑。
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引用次数: 0
Long-term Aftershock Properties of the Catastrophic 6 February 2023 Kahramanmaraş (Türkiye) Earthquake Sequence 2023 年 2 月 6 日 Kahramanmaraş(土耳其)灾难性地震序列的长期余震特性
IF 2.3 4区 地球科学 Pub Date : 2024-08-08 DOI: 10.1007/s11600-024-01419-y
Onur Tan

Nine hours apart, two catastrophic earthquakes (Mw 7.8 and 7.6) occurred on 6 February 2023, in eastern Türkiye. The mainshocks destroyed several cities and villages in 11 provinces, including Kahramanmaraş, Hatay, Adıyaman, Malatya, Adana and Gaziantep. Over about 50,000 aftershocks were detected in the nine months. Because the resolution of hypocentral locations in the Turkish national earthquake catalogs is limited, about 31,000 events are relocated using the double-difference method in this study. The aftershock distribution and its relation to energy release on the faults and Coulomb stress change areas are investigated. The improved hypocenters give a clearer image to understand the activity on the faults. The event distribution indicates that the rupture of the first mainshock in Pazarcık (Mw 7.8) propagates unilaterally on the northernmost segment of the Dead Sea Fault Zone and then transfers to the East Anatolian Fault Zone at the Maraş Triple Junction. The bilaterally extending rupture causes dense aftershock activity on the fault zone from Samandağ to Pütürge. The second mainshock in Elbistan (Mw 7.6) was triggered because of the positive Coulomb stress change on the Çardak fault, which generates dense clusters at both ends of the fault. It is observed that a high number of aftershocks occur on the low slip patches, and the high-energy release areas have low activity because of the stress equilibrium on the fault surfaces.

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引用次数: 0
Comparative assessment of gridded soil moisture data products (2000–2019) for drought detection: A study over Indian region 用于干旱探测的网格土壤水分数据产品(2000-2019 年)比较评估:印度地区研究
IF 2.3 4区 地球科学 Pub Date : 2024-08-06 DOI: 10.1007/s11600-024-01418-z
Prabir Kumar Das, Subhadip Sarkar, Rituparna Das, Dipanwita Dutta, Suparn Pathak

The soil moisture drought is an intermediate event between meteorological and agricultural droughts. The information on soil moisture droughts provides an indication about the resilience of the agricultural systems. In the present study, a comparative assessment of the monthly soil moisture gridded data products of Modern Era Retrospective analysis for Research and Applications, i.e., MERRA-2 (0.5° × 0.5°), Climate Prediction Center, i.e., CPC (0.5° × 0.5°), Global Land Data Assimilation System, i.e., GLDAS (0.25° × 0.25°), and European Space Agency Climate Change Initiative, i.e., ESA CCI (0.25° × 0.25°) during 2000 to 2019 was carried out in terms of drought occurrence and severity. The long-term soil moisture information was transformed into standardized soil moisture index (SSMI) using nonparametric distribution, followed by computation of drought duration and magnitude using thresholding approach. The long-term trends of drought parameters, i.e., duration and magnitude, were extracted using Mann–Kendall test and Sen’s Slope method, respectively. It was interesting to note that irrespective of zones, the SSMI derived from MERRA-2 and CPC have maximum coherence in terms of both pattern and intensity, followed by GLDAS. The trends of drought duration and magnitude differ based on the data products; however, frequent droughts were observed over parts of peninsular India and Indo-Gangetic plains irrespective of data products. The increased drought duration and magnitude were found over major parts of central and peninsular India, western parts of north-eastern India and eastern parts of north-western India.

土壤水分干旱是气象干旱和农业干旱之间的一个中间事件。有关土壤水分干旱的信息可以说明农业系统的抗旱能力。本研究比较评估了现代研究与应用回顾分析(MERRA-2)(0.5° × 0.5°)、气候预测中心(CPC)(0.5° × 0.5°)和全球气候观测系统(GIS)的月度土壤水分网格数据产品、从干旱发生率和严重程度的角度,对 2000 至 2019 年期间的研究应用系统,即 MERRA-2(0.5° × 0.5°)、气候预测中心,即 CPC(0.5° × 0.5°)、全球陆地数据同化系统,即 GLDAS(0.25° × 0.25°)和欧洲航天局气候变化倡议,即 ESA CCI(0.25° × 0.25°)进行了回顾性分析。利用非参数分布将长期土壤水分信息转换为标准化土壤水分指数(SSMI),然后利用阈值法计算干旱持续时间和严重程度。利用 Mann-Kendall 检验法和 Sen's Slope 法分别提取了干旱参数的长期趋势,即干旱持续时间和干旱程度。值得注意的是,无论在哪个区,由 MERRA-2 和 CPC 得出的 SSMI 在模式和强度方面都具有最大的一致性,其次是 GLDAS。干旱持续时间和程度的趋势因数据产品而异;然而,无论数据产品如何,在印度半岛和印度-甘肃平原的部分地区都观察到了频繁的干旱。在印度中部和半岛的主要地区、印度东北部的西部地区以及印度西北部的东部地区,干旱持续时间和程度都有所增加。
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引用次数: 0
Contemporary seismic moment budget along the Nepal Himalaya derived from high-resolution InSAR and GPS velocity field 从高分辨率 InSAR 和 GPS 速度场得出的尼泊尔喜马拉雅山脉当代地震力矩预算
IF 2.3 4区 地球科学 Pub Date : 2024-07-31 DOI: 10.1007/s11600-024-01411-6
Himanshu Verma, Yogendra Sharma, Kuo-En Ching, Sumanta Pasari

Throughout history, several large-magnitude earthquakes have caused damage to the Himalayan region and humanity. To understand the present-day strain rate distribution and associated seismic moment budget, a high-resolution velocity field is an essential component. The present study estimates the contemporary seismic moment budget along three spatial sections over the Nepal Himalaya using the state-of-the-art high-resolution velocity field. For this, (1) we integrate 5 years of InSAR data with 77 available GPS observations over the Nepal Himalaya; (2) we then calculate strain rate distribution (dilatational and maximum shear strain rates) from this integrated velocity field, and (3) at last, we compare the geodetic moment accumulation rate estimated from strain rate tensors with the seismic moment release rate based on an earthquake database of 500 years. The results reveal that: (1) the geodetic strain rate is not homogeneous over the Nepal Himalaya, rather along the main central thrust, a relatively higher strain rate is observed; (2) the geodetic moment rate from west to east across three sections ranges from (23.39times 10^{18}) to (16.59times 10^{18}) Nm/yr, with the minimum of (8.05times 10^{18}) Nm/yr in central Nepal, whereas the seismic moment rate varies between (5.02times 10^{18}) and (11.41times 10^{18}) Nm/yr, with the minimum of (3.69times 10^{18}) Nm/yr in central Nepal; (3) the difference between geodetic and seismic moment rates from west to east provides a moment deficit rate of (18.37times 10^{18}) to (5.18times 10^{18}) Nm/yr, with the minimum of (4.36times 10^{18}) Nm/yr in central Nepal, and more importantly, (4) the inferred moment deficit rate suggests that the western and eastern Nepal have an earthquake potential of magnitude (M_w) 8.5 and (M_w) 8.1, respectively, whereas the central Nepal has energy budget equivalent to an (M_w) 7.9 event. In summary, the present study provides spatial distribution of earthquake potential in Nepal Himalaya using the most updated high-resolution InSAR and GPS velocity field, and the findings inevitably contribute to the time-dependent earthquake hazard analysis of the study region.

历史上,数次大震级地震给喜马拉雅地区和人类造成了破坏。要了解当今的应变率分布和相关的地震力矩预算,高分辨率速度场是必不可少的组成部分。本研究利用最先进的高分辨率速度场估算了尼泊尔喜马拉雅山脉三个空间断面的当代地震力矩预算。为此,(1) 我们整合了尼泊尔喜马拉雅山脉 5 年的 InSAR 数据和 77 个可用的 GPS 观测数据;(2) 然后,我们根据整合后的速度场计算应变率分布(扩张应变率和最大剪切应变率);(3) 最后,我们将应变率张量估算出的大地力矩累积率与基于 500 年地震数据库的地震力矩释放率进行比较。结果显示(1) 尼泊尔喜马拉雅山脉的大地应变率并不均匀,相反,在中央主推线上,应变率相对较高;(2) 三个地段的大地力矩率从西向东从 23.39times 10^{18} 到 (16.59times 10^{18} Nm/yr),尼泊尔中部的最小值为 (8.05times 10^{18} Nm/yr),而地震力矩率在(5.02times 10^{18} 和 (11.41times 10^{18} Nm/yr)之间变化,最小值为 (3.69times 10^{18} Nm/yr)。69times 10^{18}) Nm/yr;(3) 大地测量和地震力矩率之间的差异自西向东提供了(18.37times 10^{18}) to(5.18times 10^{18}) Nm/yr的力矩亏损率,最小值为(4.36times 10^{18}) Nm/yr,更重要的是,(4)推断出的力矩亏损率表明,尼泊尔西部和东部的地震潜力分别为(M_w )8.5级和(M_w )8.1级,而尼泊尔中部的能量预算相当于(M_w )7.9级事件。总之,本研究利用最新的高分辨率 InSAR 和 GPS 速度场提供了尼泊尔喜马拉雅地区潜在地震的空间分布情况,研究结果必然有助于对研究区域进行随时间变化的地震灾害分析。
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引用次数: 0
Application of airborne gamma-ray spectrometry in geological lithology mapping—a case study of a region in the Qinling Mountains, China 机载伽马射线光谱仪在地质岩性测绘中的应用--中国秦岭地区案例研究
IF 2.3 4区 地球科学 Pub Date : 2024-07-31 DOI: 10.1007/s11600-024-01408-1
Yongzai Xi, Guixiang Liao, Yongbo Li, Junjie Liu, Shan Wu, Ning Lu, Peng He

Different types of rocks have different content and distribution characteristics of radioactive uranium, potassium, and thorium elements. Even for rocks of the same lithology, the content of radioactive elements varies due to different ages of formation, different origins, and different geological evolution processes. However, in various rocks and formations, the distribution of radioactive elements follows the general rule that the content of radioactive elements in igneous rocks is higher than that in sedimentary rocks, and increases with the acidity of the rocks. The younger the age of the rocks formed by the same type, the higher the content of radioactive elements. Based on this characteristic of radioactive elements in rocks, the author takes a region in the Qinling Mountains of China as an example. By using high-precision airborne gamma-ray spectrometry measurement data and existing geological information, the total content, K, eU, and eTh content, variation coefficient, ternary colour image, and other parameters of airborne gamma-ray spectrometry measurement are statistically analysed. The distribution characteristics of radioactive elements in various lithologies and formations in the area are studied, and the distribution rules are summarized. The rocks and formations in the research area are reclassified, and the typical fault structures in the area are analysed. The well-developed structural zone is mainly oriented in the northeast–southwest or north–northeast direction in the northern part and in the northwest–southeast direction in the southern part, which controls the favourable uranium mineralization zones in the research area.

不同类型的岩石具有不同的放射性铀、钾和钍元素含量和分布特征。即使是同一岩性的岩石,由于形成年代不同、成因不同、地质演化过程不同,放射性元素的含量也不尽相同。然而,在不同的岩石和岩层中,放射性元素的分布遵循着一个普遍规律,即火成岩中的放射性元素含量高于沉积岩中的放射性元素含量,并随着岩石酸度的增加而增加。同一类型岩石形成的年龄越小,放射性元素的含量就越高。根据岩石中放射性元素的这一特征,作者以中国秦岭地区为例。利用高精度机载伽马射线光谱仪测量数据和已有的地质资料,对机载伽马射线光谱仪测量的总含量、K、eU、eTh 含量、变异系数、三元彩色图像等参数进行了统计分析。研究了放射性元素在该地区不同岩性和地层中的分布特征,总结了其分布规律。对研究区内的岩石和地层进行了重新分类,并分析了区内典型的断层构造。构造带发育,北部以东北-西南或北-东北走向为主,南部以西北-东南走向为主,控制了研究区的有利铀成矿带。
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Acta Geophysica
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