利用 PRISMA 数据划分带状赤铁矿石英岩中的蓝尘富集区:印度奥迪沙邦博拉尼地区研究

IF 2.2 4区 地球科学 Q3 ENVIRONMENTAL SCIENCES Journal of the Indian Society of Remote Sensing Pub Date : 2024-08-24 DOI:10.1007/s12524-024-01980-5
Debasis Singh, Jagadish Kumar Tripathy, Sushree Sagarika Behera
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引用次数: 0

摘要

蓝尘是一种富含马氏体的高品位矿石,常见于带状赤铁矿石英岩(BHQ)和带状赤铁矿碧玉岩中。它在前寒武纪沉积铁矿床中具有独特的地层位置,其形成归因于超生富集过程。与不纯的 BHQ 相比,蓝尘的铁含量更高,在采矿过程中与 BHQ 矿石混合,以提高低 Fe2O3 BHQ 矿石的铁品位。在这项研究中,我们利用意大利航天局提供的高光谱 PRISMA 数据,确定了印度奥迪沙邦博拉尼地区带状赤铁矿石英岩(BHQ)中的蓝色粉尘区。博拉尼铁矿位于奥迪沙邦著名的马蹄形博奈-肯杰尔铁矿带的西缘,其特点是存在相当大的蓝色粉尘区和透镜区。实验室生成的光谱特征揭示了蓝色粉尘的独特特征,包括与 BHQ 样品相比,1196 至 870 纳米光谱范围内的斜率更陡,870 纳米处的吸收极小值更大。利用这些区别,生成了相对波段深度(RBD)图像,将与在 733 纳米和 1196 纳米(肩部)以及 870 纳米(吸收极小值)观测到的蓝色尘埃诊断光谱特征相一致的 PRISMA 波段纳入其中。建议的复合图像结合了 RBD、从 350-1350 nm 光谱范围内的 PRISMA 波段得出的第一个主成分 (PC-01) 图像以及 1047 nm 波段的反射波段,有效地划分了 BHQ 的蓝色尘埃区。通过实地评估、光谱特征比较以及对采集样本的矿物学分析进行验证,提高了结果的准确性。本研究的结果凸显了 PRISMA 数据集在准确划分 BHQ 内蓝色尘埃、验证其有效性方面的巨大潜力,并为优化矿产资源勘探的未来研究开辟了道路。
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Delineating Blue-Dust Enriched Zones Within Banded Hematite Quartzite Using PRISMA Data: A Study in the Bolani Region, Odisha, India

Blue dust, a high-grade martite-rich ore commonly found in conjunction with Banded Hematite Quartzite (BHQ) and Banded Hematite Jasper. It holds a distinctive stratigraphic position within Precambrian sedimentary iron ore deposits, and its formation is attributed to the supergene enrichment process. Blue dust, with higher Fe content compared to impure BHQ, is blended during mining with BHQ ore to elevate the Fe grade of low Fe2O3 BHQ ore. In this study, we utilized hyperspectral PRISMA data provided by the Italian Space Agency to identify blue dust zones within Banded Hematite Quartzite (BHQ) in the Bolani region of Odisha, India. The Bolani iron ore deposit is situated on the western limb of the renowned horseshoe-shaped Bonai-Keonjhar iron ore belt in Odisha, characterized by the presence of blue dust in fairly large pockets and lenses. Laboratory-generated spectral signatures revealed unique characteristics in blue dust, including a steeper slope in the spectral range from 1196 to 870 nm and greater absorption minima at 870 nm compared to BHQ samples. Leveraging these distinctions, a Relative Band Depth (RBD) image was generated, incorporating PRISMA bands aligned with the diagnostic spectral feature of blue dust observed at 733 nm and 1196 nm (for shoulders) and 870 nm (for absorption minima). A proposed composite image, combining RBD, the first Principal Component (PC-01) image derived from PRISMA bands within the 350–1350 nm spectral range, and a reflectance band at 1047 nm, effectively delineates blue dust zones from BHQ. Validation through field assessments, spectral signature comparisons, and mineralogical analysis of collected samples enhances the accuracy of the results. The findings of this study highlight the substantial potential of the PRISMA dataset for accurately delineating blue dust within BHQ, validating its effectiveness, and opening avenues for future research in optimizing mineral resource exploration.

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来源期刊
Journal of the Indian Society of Remote Sensing
Journal of the Indian Society of Remote Sensing ENVIRONMENTAL SCIENCES-REMOTE SENSING
CiteScore
4.80
自引率
8.00%
发文量
163
审稿时长
7 months
期刊介绍: The aims and scope of the Journal of the Indian Society of Remote Sensing are to help towards advancement, dissemination and application of the knowledge of Remote Sensing technology, which is deemed to include photo interpretation, photogrammetry, aerial photography, image processing, and other related technologies in the field of survey, planning and management of natural resources and other areas of application where the technology is considered to be appropriate, to promote interaction among all persons, bodies, institutions (private and/or state-owned) and industries interested in achieving advancement, dissemination and application of the technology, to encourage and undertake research in remote sensing and related technologies and to undertake and execute all acts which shall promote all or any of the aims and objectives of the Indian Society of Remote Sensing.
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