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Crustal structure of the Mid Black Sea High from wide-angle seismic data
被引:10
|作者:
Shillington, D. J.
[1
]
Minshull, T. A.
[2
]
Edwards, R. A.
[3
]
White, N.
[4
]
机构:
[1] Columbia Univ, Lamont Doherty Earth Observ, 61 Route 9W, Palisades, NY 10964 USA
[2] Univ Southampton, Natl Oceanog Ctr Southampton, Ocean & Earth Sci, European Way, Southampton SO14 3ZH, Hants, England
[3] Natl Oceanog Ctr, European Way, Southampton SO14 3ZH, Hants, England
[4] Univ Cambridge, Bullard Labs, Madingley Rd, Cambridge CB3 0EZ, England
来源:
基金:
英国自然环境研究理事会;
关键词:
DISEQUILIBRIUM COMPACTION;
OVERPRESSURE GENERATION;
TECTONIC HISTORY;
EVOLUTION;
BASINS;
MARGIN;
TURKEY;
INVERSION;
PONTIDES;
GEOLOGY;
D O I:
10.1144/SP464.6
中图分类号:
P5 [地质学];
学科分类号:
0709 ;
081803 ;
摘要:
ridges, that separate the western and eastern Black Sea basins. The sediment cover above these ridges has been characterized by extensive seismic reflection data, but the crustal structure beneath is poorly known. We present results froma densely sampled wide-angle seismic profile, coincidentwith a pre-existing seismic reflection profile, which elucidates the crustal structure. Weshowthat the basement ridges are covered by approximately 1-2 km of pre-rift sedimentary rocks. The Archangelsky Ridge has higher pre-rift sedimentary velocities and higher velocities at the top of basement (c. 6 km s(-1)). The Andrusov Ridge has lower pre-rift sedimentary velocities and velocities less than 5 km s(-1) at the top of the basement. Both ridges are underlain by approximately 20-km-thick crust with velocities reaching around 7.2 km s(-1) at their base, interpreted as thinned continental crust. These high velocities are consistent with the geology of the Pontides, which is formed of accreted island arcs, oceanic plateaux and accretionary complexes. The crustal thickness implies crustal thinning factors of approximately 1.5-2. The differences between the ridges reflect different sedimentary and tectonic histories.
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页码:19 / 32
页数:14
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