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Abstract


 
Chapter from: M 65:  Previous HitSaltNext Hit Tectonics: A Global Perspective
Edited By 
M.P.A. Jackson, D.G. Roberts, and S. Snelson

Author: 
C. J. Talbot

Structure, Tectonics, Paleostructure

Published 1995 as part of Memoir 65
Copyright © 1995 The American Association of Petroleum Geologists.   All Rights Reserved.
 

Talbot, C. J., 1995, Molding of Previous HitsaltNext Hit diapirs by stiff overburden, in M. P. A. Jackson, D. G. Roberts, and S. Snelson, eds., Previous HitSaltNext Hit tectonics: a global perspective: AAPG Memoir 65, p. 61-75.
Chapter 4
Molding of Previous HitSaltNext Hit Diapirs by Stiff Overburden
C. J. Talbot

Hans Ramberg Tectonic Laboratory
Institute of Earth Sciences
Uppsala University
Uppsala, Sweden


 
 

 

Abstract

 Although active diapirs must deform the overburdens they pierce, the shape of passive (downbuilt or syndepositional) diapirs is formed or molded by their overburdens. Molding of Previous HitsaltNext Hit diapirs is simplified here to profiles of diapirs entirely downbuilt in effectively rigid overburden. The dips of Previous HitsaltNext Hit-sediment contacts are shaped by the interaction of two processes: local net accumulation of overburden (A = deposition minus compaction) at rate No Disk File and the net increase in relief of Previous HitsaltNext Hit structures (R = Previous HitsaltNext Hit rise minus dissolution) at rate No Disk File. Steady kinematic molding ratios, No Disk File/No Disk File, forward model realistic dips of molded Previous HitsaltNext Hit contacts, a, at particular depths using No Disk File/No Disk File or No Disk File/No Disk File = tan a/2. Rising or falling ratios of incremental molding forward model complete diapir profiles. Conversely, molding histories can be read by backstripping profiles of downbuilt diapirs.

Previous HitSaltNext Hit diapirs are downbuilt in a field of downbuilding (100 > No Disk File/No Disk File > 0.01), that is bounded by burial and extrusion. Within this range, aggradation faster than Previous HitsaltNext Hit can rise (No Disk File/No Disk File < 1) molds tapering (narrowing-upward) top contacts of Previous HitsaltNext Hit. Accumulation of overburden slower than Previous HitsaltNext Hit rises (No Disk File/No Disk File > 1) molds flaring (widening-upward) Previous HitsaltNext Hit contacts. Below this range (where No Disk File/No Disk File < ~0.01), the top contact of the Previous HitsaltNext Hit is eclipsed (temporarily buried to depths from which it can still upbuild) or even occluded (buried below its critical roof thickness and thus unable to rise again autonomously). Occluded Previous HitsaltNext Hit is either dissolved at depth or rises in reactivated diapirs after exhumation or faulting of overburden that is not rigid. Where No Disk File/No Disk File > ~100, Previous HitsaltNext Hit emerges like a fountain and extrudes sheets of allochthonous Previous HitsaltNext Hit. Extruded Previous HitsaltTop is recycled back into the ocean by dissolution at the surface or after burial and reactivation in another cycle.

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