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    The Lake Bosumtwi meteorite impact structure, Ghana—Where is the magnetic source?

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    Author
    Ugalde, H.
    Morris, W. A.
    Pesonen, L. J.
    Danuor, S. K.
    Issue Date
    2007-01-01
    Keywords
    Ghana Impact crater
    Magnetism
    geophysical signature
    Bosumtwi
    
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    Citation
    Ugalde, H., Morris, W. A., Pesonen, L. J., & Danuor, S. K. (2007). The Lake Bosumtwi meteorite impact structure, Ghana—Where is the magnetic source?. Meteoritics & Planetary Science, 42(4‐5), 867-882.
    Publisher
    The Meteoritical Society
    Journal
    Meteoritics & Planetary Science
    URI
    http://hdl.handle.net/10150/656714
    DOI
    10.1111/j.1945-5100.2007.tb01082.x
    Additional Links
    https://meteoritical.org/
    Abstract
    The Bosumtwi impact structure (Ghana) is a young and well-preserved structure where a vast amount of information is available to constrain any geophysical model. Previous analysis of the airborne magnetic data and results of numerical simulation of impact predicted a strongly magnetic impact-melt body underneath the lake. Recent drilling through the structure did not penetrate such an expected impact-melt rock magnetic source. A new 3-D magnetic model for the structure was constructed based on a newly acquired higher-resolution marine magnetic data set, with consideration of the observed gravity data on the lake, previous seismic models, and the magnetic properties and lithology identified in the two International Continental Scientific Drilling Program (ICDP) deep boreholes. The new model contains highly magnetic bodies located in the northeast sector of the structure, not centered onto the drilling sites. As in previous models, higher magnetization than that measured in outcropping impactites had to be assigned to the unexposed source bodies. Integration of the new model with the borehole petrophysics and published geology indicates that these bodies likely correspond to an extension to the south of the Kumasi batholith, which outcrops to the northeast of the structure. The possibility that these source bodies are related to the seismically identified central uplift or to an unmapped impact-melt sheet predicted by previous models of the structure is not supported. Detailed magnetic scanning of the Kumasi batholith to the north, and the Bansu intrusion to the south, would provide a test for this interpretation.
    Type
    Article
    text
    Language
    en
    ISSN
    1945-5100
    ae974a485f413a2113503eed53cd6c53
    10.1111/j.1945-5100.2007.tb01082.x
    Scopus Count
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    Meteoritics & Planetary Science, Volume 42, Number 4-5 (2007)

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