Seismic and magnetic constraints on the structure of upper oceanic crust at fast and slow spreading ridges
Seismic and magnetic constraints on the structure of upper oceanic crust at fast and slow spreading ridges
Date
1998-09
Authors
Hussenoeder, Stefan A.
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Date Created
Location
East Pacific Rise
Mid-Atlantic Ridge
Mid-Atlantic Ridge
DOI
10.1575/1912/4780
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Keywords
Mid-ocean ridges
Seismic prospecting
Sea-floor spreading
Robert D. Conrad (Ship) Cruise RC2908
Charles Darwin (Ship) Cruise CD57
Seismic prospecting
Sea-floor spreading
Robert D. Conrad (Ship) Cruise RC2908
Charles Darwin (Ship) Cruise CD57
Abstract
The upper ocean crust contains a comprehensive record of the shallow geological processes
active along the world's mid-ocean ridge system. This thesis examines the
magnetic and seismic structure of the upper crust at two contrasting ridges-the
fast spreading East Pacific Rise (EPR) and the slow spreading Mid-Atlantic Ridge
(MAR)-to build a more complete understanding about the roles of volcanic emplacement,
tectonic disruption and hydrothermal alteration in the near-ridge environment.
A technique that inverts potential field measurements. directly from an uneven
observation track is developed and applied to near-bottom magnetic data from the
spreading segments north of the Kane transform on the MAR. It is concluded that
the central anomaly magnetization high marks the locus of focused volcanic emplacement.
A cyclic faulting model is proposed to explain the oscillatory magnetization
pattern associated with discrete blocks of crust being transported out of the rift valley
between intensely altered fault zones. Seismic waveform and amplitude analyses
of the magma sill along the EPR reveal it to be a thin (<100 m) body of partial
melt. These characteristics have important implications for melt availability and
transport within the cycle of eruption and replenishment. A genetic algorithm-based
seismic waveform inversion technique is developed and applied to on- and near-axis
multichannel data from 17°20'S on the EPR and the spreading segment south of the
Oceanographer transform (MAR) to map and compare for the first time the detailed
velocity structure of the upper crust at two different spreading rates. Combined with
conventionally processed seismic profiles, our results show that, while final extrusive
thickness is comparable at all spreading ridges (300-500 m), the style of thickening
may vary. While a thin (≤100 m) extrusive carapace quadruples in thickness within
1-4 km of the EPR crest, the extrusive section at the MAR achieves its final thickness
within the inner valley. Both show evidence for a narrow zone of volcanic emplacement.
Vigorous hydrothermalism at the EPR may produce a more rapid increase in
basement velocities relative to the MAR. Rapid modification of the extrusive/dike
transition at both ridges indicates that hydrothermalism is enhanced in this interval.
Along-axis transport of lavas may thicken the extrusive pile at slow spreading segment
ends, strengthening the magnetic highs generated by lava chemistry.
Description
Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy at the Massachusetts Institute of Technology and the Woods Hole Oceanographic Institution September 1998
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Citation
Hussenoeder, S. A. (1998). Seismic and magnetic constraints on the structure of upper oceanic crust at fast and slow spreading ridges [Doctoral thesis, Massachusetts Institute of Technology and Woods Hole Oceanographic Institution]. Woods Hole Open Access Server. https://doi.org/10.1575/1912/4780