Marine Seismic Data from the Accreted Terranes of Southeast Alaska

John Diebold (1),  Lincoln Hollister (2)
(1) L-DEO, Palisades, NY 10964, USA, (914) 365-8524, (914) 365-8168, johnd@ldeo.columbia.edu
(2) Dept. Geol. & Geoph. Sci., Princeton University, Princeton, NJ 08544, USA (609) 258-4106, (609) 258-5275, linc@princeton.edu

Abstract:
R/V EWING  acquired 1700 km of deep penetration MCS data across the accreted terranes and principal terrane boundaries of SE Alaska. Narrow Fjordlike waterways and rough, shallow bottom produce artifacts which were partly removed by prestack velocity filtering and statics corrections based on a model obtained from brute stacks.  In Dixon Entrance we  have imaged crustal reflectors and Moho across the  fundamental pair of structural boundaries separating the  Alexander, Wrangellia, and North America terranes. The eastern margin of the Alexander terrane features strong  crustal reflectors, mostly dipping gently (ca. 12 degrees) WSW.  Moho reflections within this zone are stronger and  more continuous than those seen in the terranes to the east. A broad Moho arch,
about 3 km high, 100 km wide, and  striking NNE, is defined by two E-W profiles, 45 km apart. Minimum Moho two-way time is 8 seconds,  corresponding to a Moho depth of approximately 26 km.   It is likely that this crustal arching is the result  of the Tertiary extension forming Queen Charlotte Basin. The overall strike of the arch is oblique to nearby terrane boundaries, to graben and half-graben structures previously  mapped in  Dixon Entrance and Hecate Strait, and to the  trend of Queen Charlotte Basin, which
lies to the south. The zone of thin crust defined by this Moho arch is apparently discontinuous with similar zones mapped in Hecate Strait and Queen Charlotte Basin, suggesting their  creation by oblique extension (transtension). The strike of the Dixon Entrance Moho arch is  subparallel to and centered between theadjacent terrane boundaries, and similar arches are observed, centered within adjacent terranes to the east. This suggests that post-accretion crustal extension may be controlled by accretionary fabrics.


 
 

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