Lower crustal variability and the crust/mantle transition at the Atlantis Massif oceanic core complex

dc.contributor.author Blackman, Donna K.
dc.contributor.author Collins, John A.
dc.date.accessioned 2011-01-31T19:04:57Z
dc.date.available 2011-06-18T08:25:21Z
dc.date.issued 2010-12-18
dc.description Author Posting. © American Geophysical Union, 2010. This article is posted here by permission of American Geophysical Union for personal use, not for redistribution. The definitive version was published in Geophysical Research Letters 37 (2010): L2430, doi:10.1029/2010GL045165. en_US
dc.description.abstract Seismic refraction data provide new constraints on the structure of the lower oceanic crust and its variability across the Atlantis Massif oceanic core complex, ∼30°N on the Mid-Atlantic Ridge. A 40 km-long spreading-parallel profile constrains P-wave velocities to depths of up to ∼7 km beneath the seafloor. Two shorter spreading-perpendicular lines provide coverage to ∼2 km depth. The anomalous character of the massif's central dome crust is clear compared to the neighboring rift valley and similar-age crust on the opposite ridge flank. The domal core of the massif, unroofed via detachment faulting, has velocities >7.0 km/s at depths below ∼2.5 km sub-seafloor, increasing to 7.5–7.8 km/s over the depth range 4.8–6.8 km. Within the core complex, the Moho does not appear to be sharp as no PmP arrivals are observed. Within the axial valley, velocities do not reach mantle-transition zone values in the uppermost 6 km. We infer that crust there is of normal thickness but that a thinner than average mafic section is present in the central massif. Near IODP Hole U1309D, located on the central dome, there is a low velocity gradient interval at 1–3 km depth with velocities of 6.6–6.8 km/s, that coincides with a 3–5 km wide region where shallower velocities are highest. Given the predominantly gabbroic section recovered from the 1.4 km deep drillhole, this seismic structure suggests that the mafic body extends a few km both laterally and vertically. en_US
dc.description.sponsorship NSF grants provided support for the data acquisition, initial interpretation (Collins OCE‐9633114 and OCE‐ 9819297) and subsequent processing and analysis (Blackman OCE‐ 0927442). en_US
dc.format.mimetype text/plain
dc.format.mimetype application/pdf
dc.identifier.citation Geophysical Research Letters 37 (2010): L2430 en_US
dc.identifier.doi 10.1029/2010GL045165
dc.identifier.uri https://hdl.handle.net/1912/4322
dc.language.iso en_US en_US
dc.publisher American Geophysical Union en_US
dc.relation.uri https://doi.org/10.1029/2010GL045165
dc.subject Atlantis Massif en_US
dc.subject Marine refraction en_US
dc.subject Oceanic crust en_US
dc.subject Mid-Atlantic Ridge en_US
dc.title Lower crustal variability and the crust/mantle transition at the Atlantis Massif oceanic core complex en_US
dc.type Article en_US
dspace.entity.type Publication
relation.isAuthorOfPublication 0142884e-755f-40d6-80ce-fd2a03456907
relation.isAuthorOfPublication 91adcc57-3fb1-468a-aec8-b9ce0323e710
relation.isAuthorOfPublication.latestForDiscovery 0142884e-755f-40d6-80ce-fd2a03456907
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Figure S1: Details of the OBS refraction experiment at Atlantis Massif.
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Figure S2: Refracted arrivals recorded by ORB1 and OBH26 downward continued to the seafloor.
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Figure S3: Example of tests for Line 8 models with sharp Moho.
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Figure S4: Tomographic models for Lines 9a and 9b.
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