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Abstract
Journal of Sedimentary Research, Section
A: Sedimentary Petrology and Processes
Vol. 66 (1996)No.
5. (September), Pages 916-927
Sediment Mass-Flow Processes on a Depositional Lobe, Outer Mississippi
Fan
William C. Schwab (1), Homa J. Lee (2), David C. Twichell
(1), Jacques Locat (3), C. Hans Nelson (2), William G. McArthur (2), Neil
H. Kenyon (4)
ABSTRACT
SeaMARC 1A sidescan-sonar imagery and cores from the distal reaches
of a depositional lobe on the Mississippi Fan show that channelized mass
flow was the dominant mechanism for transport of silt and sand during the
formation of this part of the fan. Sediments in these flows were rapidly
deposited once outside of their confining channels. The depositional lobe
is formed of a series of long, narrow sublobes composed of thin-bedded
turbidites (normally graded siliciclastic sand and silt, 20 cm thick on
average), debris-flow deposits (soft clay clasts up to 5 cm in diameter
in a siliciclastic silt matrix, 48 cm thick on average), and background-sedimentation
hemipelagic muds. The mass flows most likely originated from slope failure
at the head of the Mississippi Canyon or on the outer ontinental shelf
and flowed approximately 500 km to the distal reaches of the fan, with
debris flow being the dominant flow type. An analysis that uses the geometry
of the confining channels and strength properties of the debris-flow material
shows that these thin debris flows could have traveled hundreds of kilometers
on extremely small sea-floor slopes at low velocities if the flowing medium
behaved as Bingham fluids and were steady-state phenomena.
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