Please use this identifier to cite or link to this item: http://repository.futminna.edu.ng:8080/jspui/handle/123456789/19198
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dc.contributor.authorAlhassan, D.U-
dc.contributor.authorSalako, K.A-
dc.contributor.authorUdensi, E.E-
dc.date.accessioned2023-06-06T10:07:10Z-
dc.date.available2023-06-06T10:07:10Z-
dc.date.issued2023-01-11-
dc.identifier.citationTaiwo Adewumi, Kazeem Adeyinka Salako, Adedibu Sunny Akingboye, Nordiana Mohd Muztaza, Usman Defyan Alhassan, Emmanuel Emeka Udensi (2023): Reconstruction of the subsurface crustal and radiogenic heat models of the Bornu Basin, Nigeria, from multi-geophysical datasets: Implications for hydrocarbon prospecting .ADVANCES IN SPACE RESEARCHen_US
dc.identifier.urihttp://repository.futminna.edu.ng:8080/jspui/handle/123456789/19198-
dc.description.abstractThis study aims to reconstruct the subsurface crustal and radiogenic heat models from integrated airborne magnetic and gamma-ray spectrometric and satellite gravity methods for implications on hydrocarbon exploration in the Bornu Basin, NE Nigeria. The results revealed the basin’s lithologies and shallow-to-deep structures (faults and lineaments) and their trends, depicting contrasting magnetic intensities, gravity anomalies, and radionuclide concentrations. High magnetic anomalous zones in the southern and southeastern parts of the basin could be associated with the influence of the intrusive body (porphyritic granite) of high magnetization as observed in the 2D magnetic/gravity models. Moderate to low anomalous zones suggested thick sedimentation in the northeastern and central areas. The total horizontal derivatives (THDR) and Rose diagrams of the magnetic and Bouguer anomalies revealed major lineaments/faults in the NE-SW, NNE-SSW, and E-W directions. These structures likely serve as the migratory pathways/traps for the hydrocarbons. The structures delineated on the radioelements ratio, and composite maps also correlate with those identified on the THDR maps, especially the major SE-NW structure created by magmatic intrusion in the southeastern part of the basin. The estimated total radiogenic heat production (RHP) rates for the study area decreased in the order of 740.46 > 674.16 > 665.35 > 462.23 > 415.17, with the maximum obtained from the Yolde Formation (YF) and Pindiga Formation (PF). These are attributable to clay, limestone, shale, and ferruginized sandstone. The Chad Formation (CF), on the other hand, had thicker sediment (6.8 km) and a maximum RHP of 550 qWkg1 , which is relatively low ( 797.87 qWkg1 obtained in the PF and the YF falls within the moderate RHP windows (750–1500 qWkg1 ) for sufficient hydrocarbon maturation and accumulation in the Bornu Basin.en_US
dc.description.sponsorshipSelfen_US
dc.language.isoenen_US
dc.publisherADVANCES IN SPACE RESEARCHen_US
dc.relation.ispartofseriesdoi.org/10.1016/j.asr.2023.01.007;-
dc.subjectSubsurface crustal modelingen_US
dc.subjectMagnetic anomaly characterizationen_US
dc.subjectSatellite gravity modelingen_US
dc.subjectGamma-ray spectrometry (GRS)en_US
dc.subjectHydrocarbon prospectingen_US
dc.subjectChad (Bornu) Basinen_US
dc.titleReconstruction of the subsurface crustal and radiogenic heat models of the Bornu Basin, Nigeria, from multi-geophysical datasets: Implications for hydrocarbon prospectingen_US
dc.typeArticleen_US
Appears in Collections:Applied Geophysics

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