TY - JOUR
T1 - Ridge migration and asymmetric sea-floor spreading
AU - Stein, Seth
AU - Melosh, H. J.
AU - Minster, J. B.
N1 - Funding Information:
We thank Hiroo Kanamori, Robert Geller, Emile Okal, David Hadley, Carl Johnson, Dan Kosloff, Kevir Burke, and Tom Jordan for advice and assistance. Peter Molnar provided us with the South Pacific profiles. Dallas Abbott, Norm Sleep, Rob Cockerham, and Dick Hey offered us critical comments on an earlier draft. Norm Sleep also kindly allowed us to use his results prior to publication. We have benefited from reviews by Ken Macdonald and an anonymous reviewer. Seth Stein was supported by a fellowhip from the Fannie and John Hertz Foundation. This research was also supported by National Science Foundation Grant EAR76-14262. Contribution No. 2789, Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California.
Copyright:
Copyright 2014 Elsevier B.V., All rights reserved.
PY - 1977/8
Y1 - 1977/8
N2 - We propose that asymmetric sea-floor spreading occurs as a consequence of the relative motion between ridges and slow-moving mantle material below. A fluid mechanical model of asymmetric spreading predicts that the trailing flank of a ridge migrating with respect to the mantle spreads fastest. Observed asymmetries are compared to those predicted by ridge migration velocities. Although the magnitude of the asymmetry appears to depend as much on local effects as on the migration of the ridge, the direction of asymmetry agrees with our prediction in most locations. In contrast, models in which the ridge attempts to remain above a source fixed in the mantle predict the opposite direction of asymmetry. Other models, which attribute asymmetric spreading to asymmetric cooling, require large deviations from the standard depth-age relationship, while our model does not.
AB - We propose that asymmetric sea-floor spreading occurs as a consequence of the relative motion between ridges and slow-moving mantle material below. A fluid mechanical model of asymmetric spreading predicts that the trailing flank of a ridge migrating with respect to the mantle spreads fastest. Observed asymmetries are compared to those predicted by ridge migration velocities. Although the magnitude of the asymmetry appears to depend as much on local effects as on the migration of the ridge, the direction of asymmetry agrees with our prediction in most locations. In contrast, models in which the ridge attempts to remain above a source fixed in the mantle predict the opposite direction of asymmetry. Other models, which attribute asymmetric spreading to asymmetric cooling, require large deviations from the standard depth-age relationship, while our model does not.
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U2 - 10.1016/0012-821X(77)90187-X
DO - 10.1016/0012-821X(77)90187-X
M3 - Article
AN - SCOPUS:0002706402
VL - 36
SP - 51
EP - 62
JO - Earth and Planetary Sciences Letters
JF - Earth and Planetary Sciences Letters
SN - 0012-821X
IS - 1
ER -