2014
DOI: 10.1002/2013jb010359
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The Coulomb critical taper theory applied to gravitational instabilities

Abstract: The critical Coulomb wedge theory has been widely applied to the structural evolution of accretionary wedges and fold and thrust belts, but it also predicts the spreading of a wedge under gravity. This solution may be applied to the formation of gravitational spreading and gliding along passive margins, where elevated pore fluid pressure is common. Following the initial hypotheses of the theory, we provide an alternative expression of the exact solution for a noncohesive wedge, better suited to slope instabili… Show more

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Cited by 19 publications
(13 citation statements)
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References 48 publications
(112 reference statements)
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“…In our numerical models we observe shallow gravity instabilities /similar to slope aprons/ for simulations in mechanical modes II and III. This result is consistent with the prediction of Mourgues et al (). In their analysis, they use the concept of the safety factor ( FS=tanfalse(αfalse)false/tanfalse(αmaxfalse)) often used in engineering and which varies very similarly to trueα¯.…”
Section: Discussionsupporting
confidence: 94%
See 1 more Smart Citation
“…In our numerical models we observe shallow gravity instabilities /similar to slope aprons/ for simulations in mechanical modes II and III. This result is consistent with the prediction of Mourgues et al (). In their analysis, they use the concept of the safety factor ( FS=tanfalse(αfalse)false/tanfalse(αmaxfalse)) often used in engineering and which varies very similarly to trueα¯.…”
Section: Discussionsupporting
confidence: 94%
“…When those numbers are close to 1, shallow gravity sliding occurs. When FS or trueα¯ decreases, Mourgues et al () suggest that deep normal faults reaching the décollement are expected. This theoretical prediction is consistent with the transition that we observe from shallow gravity sliding in Style 2 to deep normal faulting in Style 3.…”
Section: Discussionmentioning
confidence: 99%
“…The lower boundary of this domain corresponds to the stability limit of accretionary wedges in the compressive regime. Of more interest here is the upper boundary of the grey domain corresponding to gravity instability (Mourgues et al 2014). This upper limit is very close to our predictions (dash-dotted curve) for β larger than 25…”
Section: Stability Conditionssupporting
confidence: 85%
“…It complements the derivation found in Wang et al [2006] and Mourgues et al [2014], by providing the complete expression of the implicit solution in terms of the critical taper + as function of the fluid overpressures and friction angles. This expression is valid for any permissible value of the slopes and , thus the proposed name ECCW theory.…”
Section: Appendix A: Different Fluid Pressure Parametrizationsmentioning
confidence: 65%
“…The solution in the last two references is nevertheless approximate in the sense that its validity is limited to low topographic slopes and pore pressures. It is only recently that the CCW theory was amended by Wang et al [2006] to produce an exact solution (called the exact critical Coulomb wedge (ECCW) theory in this contribution) that was applied to sandbox experiments [Mourgues et al, 2014].…”
Section: Introductionmentioning
confidence: 99%