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dc.contributor.authorSchmitt, D. R.
dc.contributor.authorMilkereit, B.
dc.contributor.authorKarp, T.
dc.contributor.authorScholz, C.
dc.contributor.authorDanuor, S.
dc.contributor.authorMeillieux, D.
dc.contributor.authorWelz, M.
dc.date.accessioned2021-02-12T21:41:39Z
dc.date.available2021-02-12T21:41:39Z
dc.date.issued2007-01-01
dc.identifier.citationSchmitt, 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.
dc.identifier.issn1945-5100
dc.identifier.doi10.1111/j.1945-5100.2007.tb01072.x
dc.identifier.urihttp://hdl.handle.net/10150/656275
dc.description.abstractIn 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.
dc.language.isoen
dc.publisherThe Meteoritical Society
dc.relation.urlhttps://meteoritical.org/
dc.rightsCopyright © The Meteoritical Society
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/
dc.subjectshock
dc.subjectGhana Impact crater
dc.subjectwave
dc.subjectBosumtwi
dc.subjectimpacts
dc.subjectgeophysical signature
dc.subjectstructures
dc.titleIn situ seismic measurements in borehole LB-08A in the Bosumtwi impact structure, Ghana: Preliminary interpretation
dc.typeArticle
dc.typetext
dc.identifier.journalMeteoritics & Planetary Science
dc.description.collectioninformationThe Meteoritics & Planetary Science archives are made available by the Meteoritical Society and the University of Arizona Libraries. Contact lbry-journals@email.arizona.edu for further information.
dc.eprint.versionFinal published version
dc.description.admin-noteMigrated from OJS platform February 2021
dc.source.volume42
dc.source.issue4-5
dc.source.beginpage755
dc.source.endpage768
refterms.dateFOA2021-02-12T21:41:39Z


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