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    In situ seismic measurements in borehole LB-08A in the Bosumtwi impact structure, Ghana: Preliminary interpretation

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    Author
    Schmitt, D. R.
    Milkereit, B.
    Karp, T.
    Scholz, C.
    Danuor, S.
    Meillieux, D.
    Welz, M.
    Issue Date
    2007-01-01
    Keywords
    shock
    Ghana Impact crater
    wave
    Bosumtwi
    impacts
    geophysical signature
    structures
    
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    Citation
    Schmitt, D. R., Milkereit, B., Karp, T., Scholz, C., Danuor, S., Meillieux, D., & Welz, M. (2007). In situ seismic measurements in borehole LB‐08A in the Bosumtwi impact structure, Ghana: Preliminary interpretation. Meteoritics & Planetary Science, 42(4‐5), 755-768.
    Publisher
    The Meteoritical Society
    Journal
    Meteoritics & Planetary Science
    URI
    http://hdl.handle.net/10150/656275
    DOI
    10.1111/j.1945-5100.2007.tb01072.x
    Additional Links
    https://meteoritical.org/
    Abstract
    In order to assist in the interpretation of previous seismic refraction and reflection surveys, a vertical seismic profile was acquired in the Lake Bosumtwi (Ghana) hard-rock core hole LB-08A. No seismic reflections are seen in the up-going wave field obtained, and this observation is consistent with the lack of reflectivity observed in the corresponding 2-D surface seismic profile obtained in earlier studies. Direct down-going P-waves were found both in the cased sediment column from a depth of 73 m to 239 m below the lake surface and in the open-hole hard rock section from a depth of 239 m to 451 m of LB-08A. Analysis of the observed travel times indicates a nearly constant P-wave velocity of 1520 m/s through the soft lacustrine sediments. In the hard-rock, however, the P-wave velocity rapidly increases by nearly 30% from 2600 m/s to 3340 m/s. These values are in good agreement with the gross velocity structure obtained in the earlier joint inversion of seismic reflection and refraction data. These values are low relative to those expected for the metasedimentary protoliths, an observation that has been made at other young impact structures of similar size. The low velocities, together with the fact that they increase so rapidly, is suggestive of a decreasing density of fractures and microcracks with depth. Consequently, the seismic velocity trend may provide a proxy measure of damage, and hence, the decay of the shock pressure from the impact point. Validation of this requires additional detailed studies of the porosity structure in the core.
    Type
    Article
    text
    Language
    en
    ISSN
    1945-5100
    ae974a485f413a2113503eed53cd6c53
    10.1111/j.1945-5100.2007.tb01072.x
    Scopus Count
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    Meteoritics & Planetary Science, Volume 42, Number 4-5 (2007)

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