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Convective instability of thickening mantle lithosphere

Conrad, Clinton P. (2000) Convective instability of thickening mantle lithosphere. Geophysical Journal International, 143 (1). pp. 52-70. ISSN 0956-540X. http://resolver.caltech.edu/CaltechAUTHORS:20180124-104300156

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Abstract

Mantle lithosphere, being colder and therefore denser than the underlying mantle, is prone to convective instability that can be induced by horizontal shortening. Numerical experiments on a cold layer with imposed horizontal shortening are carried out to examine the relative importance of mechanical thickening, thermal diffusion and gravitational instability in deforming the layer. This analysis is then used to develop a method for determining which of these styles dominates for a layer thickening at a given rate. If viscosity is non-Newtonian, the imposition of shortening decreases the lithospheric strength, which causes perturbations to the lithosphere’s temperature structure to grow exponentially with time. Once these perturbations become sufficiently large, they then grow super-exponentially with time, eventually removing the lithospheric base. Because lithospheric viscosity is highly temperature-dependent, at most only the lower 30 per cent of the lithosphere participates in the downwelling associated with this initial super-exponential growth event. After this event, however, a downwelling develops that removes material advected into the region of downwelling by horizontal shortening. The magnitude of this persistent downwelling depends on the rate and duration of shortening. If the total amount of shortening does not exceed 50 per cent (doubling of crustal thickness), then this downwelling extends to a depth three to four times the thickness of undeformed lithosphere and forms a sheet significantly thinner than the width of the region undergoing shortening. Once shortening stops, this downwelling is no longer replenished by the shortening process, and should then detach due to its inherent gravitational instability. The hottest 60 per cent of the mantle lithosphere could be removed in such an event, which would be followed by an influx of hot, buoyant asthenosphere that causes rapid surface uplift. Because more cold material is removed after the cessation of shortening than by the initial gravitational instability, the former has a potentially greater influence on surface uplift. The Tibetan interior is thought to have been shortened by about 50 per cent in ∼30Myr and afterwards, at ∼8Ma, experienced a period of rapid uplift that may have resulted from the removal of a large downwelling ‘finger’ of cold lithosphere generated by shortening.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1046/j.1365-246x.2000.00214.xDOIArticle
https://academic.oup.com/gji/article/143/1/52/894381PublisherArticle
Additional Information:© 2000 RAS. Received: 12 April 2000; Accepted: 17 April 2000; Published: 01 October 2000. This work was supported in part by National Science Foundation grant EAR-9725648, and by a National Science Foundation Graduate Research Fellowship. I thank G. Houseman and an anonymous referee for constructive reviews, B. Hager for helpful comments and P. Molnar for suggestions and encouragement throughout the preparation of this manuscript that greatly improved its content and clarity.
Group:Seismological Laboratory
Funders:
Funding AgencyGrant Number
NSFEAR-9725648
NSF Graduate Research FellowshipUNSPECIFIED
Subject Keywords:convective instability, gravitational instability, mantle lithosphere, thermal diffusion, Tibet, viscosity
Record Number:CaltechAUTHORS:20180124-104300156
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20180124-104300156
Official Citation:Clinton P. Conrad; Convective instability of thickening mantle lithosphere, Geophysical Journal International, Volume 143, Issue 1, 1 October 2000, Pages 52–70, https://doi.org/10.1046/j.1365-246x.2000.00214.x
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:84501
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:25 Jan 2018 17:30
Last Modified:25 Jan 2018 17:30

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