Articles | Volume 17, issue 3
https://doi.org/10.5194/se-17-573-2026
© Author(s) 2026. This work is distributed under the Creative Commons Attribution 4.0 License.
On the criticality of return flows in viscous accretionary wedges and its implications for deep-crustal exhumation in subduction zones
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- Final revised paper (published on 25 Mar 2026)
- Supplement to the final revised paper
- Preprint (discussion started on 12 Aug 2025)
- Supplement to the preprint
Interactive discussion
Status: closed
Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor
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RC1: 'Comment on egusphere-2025-2909', Anonymous Referee #1, 09 Sep 2025
- AC1: 'Reply on RC1', Nibir Mandal, 17 Oct 2025
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RC2: 'Comment on egusphere-2025-2909', Stefan Markus Schmalholz, 11 Sep 2025
- AC2: 'Reply on RC2', Nibir Mandal, 17 Oct 2025
Peer review completion
AR – Author's response | RR – Referee report | ED – Editor decision | EF – Editorial file upload
AR by Nibir Mandal on behalf of the Authors (27 Nov 2025)
Author's response
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ED: Referee Nomination & Report Request started (08 Dec 2025) by Taras Gerya
RR by Anonymous Referee #2 (04 Jan 2026)
RR by Anonymous Referee #1 (05 Jan 2026)
ED: Publish subject to minor revisions (review by editor) (09 Jan 2026) by Taras Gerya
AR by Nibir Mandal on behalf of the Authors (16 Jan 2026)
Author's response
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ED: Publish as is (25 Feb 2026) by Taras Gerya
ED: Publish as is (07 Mar 2026) by Florian Fusseis (Executive editor)
AR by Nibir Mandal on behalf of the Authors (14 Mar 2026)
Manuscript
Patsa & Mandal present a paper to study return flow in accretionary wedges, a topic that has been widely studied in the recent decades and is still relevant today. This process has been modelled with theoretical solutions, numerical and analog models to explain field-based observations on pressure temperature conditions on metamorphic rocks along accretionary prisms. The authors provide a more generalized theoretical solution to include a non-parallel component on the slab to reproduce slab advance/rollback. In addition, they conducted analog models to enhance these results. Finally, an overview with natural observations is made.
The integration of analytical solutions with analog modelling represents a novel and valuable approach, with the potential to be further strengthened by incorporating existing numerical results. However, the current manuscript does not fully emphasize this novelty: the introductory section underplays the contribution, and the analytical and analog results are presented somewhat independently, without sufficient cross-comparison.
To improve the manuscript, I recommend (i) revising the introduction to more clearly articulate the novelty and significance of the combined approach, (ii) providing greater coverage and integration of the analog modelling, and (iii) addressing several technical issues within the analytical solution. If these major concerns are resolved, the manuscript would meet the standards for publication in Solid Earth and I look forward to see the revised version.
Major Comment 1
The use of a non-dimensional parameter to quantify the strength or weakness of return flow is both effective and intuitive. This approach allows the balance of incoming and outgoing material along the top boundary to be measured, corresponding to sediment influx and exhumed units in an accretionary wedge. In the simplest case—rigid walls with parallel subduction—the value must equal 1, as dictated by wedge geometry and mass conservation.
However, when a non-parallel component is introduced to the slab, the theoretical models also incorporate material flux along the slab boundary. This introduces bias in the calculated rates of burial and exhumation, since part of the return flow ratio (FR) is influenced by this artificial slab-sourced material. In the case of slab advance, FR appears anomalously high due to two factors: (1) the top-boundary influx of sediments, which the authors correctly identify, and (2) the additional, unaddressed influx of material along the slab boundary.
For the rollback scenario, the formulation permits material to exit through the slab boundary, which is physically unrealistic. With small rollback velocities, wedge geometry would still force material to return to the surface; however, in the present formulation, this is instead channelled out through the slab, leading to FR = 0. Furthermore, at high rollback velocities, the assumption of a downward-tapered wedge may break down, opening the system to the upper mantle. To remain consistent with the wedge geometry assumptions, I suggest restricting the analysis to small perturbations of the non-parallel component.
Finally, the comparison of slab advance, rollback, and normal subduction must be conducted under consistent assumptions regarding material influx. One possible way forward would be to fix the total incoming volume and instead vary return velocities, though I acknowledge that implementing this within the analytical framework may be non-trivial.
Major Comment 2:
I strongly recommend undertaking a systematic comparison between the analytical solution and the analog modelling, as this would greatly strengthen the validation of the theoretical framework. At present, the two sets of results are described independently, which makes the paper look unbalanced. Establishing a one-to-one correspondence between the analytical predictions and the analog experiments for identical setups would provide a more rigorous test of the model and highlight the novelty of the combined approach.
That said, some modifications and additional discussion will be required to enable such a comparison. As noted in lines 415–416, the analog experiments allow material to exit through the bottom boundary, a feature not incorporated into the analytical solution. This discrepancy must be explicitly acknowledged and its implications discussed, since it directly affects the comparability of the results. One option is to consider modified boundary conditions in the analytical framework, or alternatively to constrain the analog results so that they are evaluated under conditions more consistent with the theoretical assumptions.
In addition, I recommend expanding the analog modelling section. At present, the manuscript dedicates considerably more space to the analytical solution, leaving the analog results underdeveloped. A more balanced treatment would not only give greater weight to the experiments but also allow for meaningful side-by-side comparisons. Importantly, you could draw inspiration from the approach of Moulas et al. (2021), who validated their analytical solution against numerical models with a similar setup. Extending your study to include a three-way comparison of analytical, analog, and numerical would significantly increase the robustness and originality of the manuscript.
To facilitate these improvements, some reorganization of the manuscript structure is advised. For example, moving Section 4 earlier in the text, immediately after the presentation of the analytical results would allow for more direct comparisons between the different methods. This restructuring would make the narrative more cohesive and highlight the integrative character of the study, which is currently one of its main strengths but not fully emphasized.
Line to Line comments:
Line 20: Delete “the” or simply state “facilitate subduction.”
Line 21: References are missing for geophysical observations; see Abers (2005).
Lines 25–28: I recommend mentioning the P–T–t path for consistency with the rest of the sentence, and introducing the concept of recycling here.
Line 33: Retain only geochronological, since this sentence refers exclusively to exhumation rates and not geochemical constraints.
Line 39: Verify the reference “?, for review.”
Line 45: A reference is required. The corner flow model also accounts for both prograde and retrograde metamorphism; please mention this. Additionally, note that the model supports the possibility of sediments reaching mantle depths where partial melting may occur.
Lines 48–49: Add one or two sentences on the thermal regime of subduction zones, as this strongly influences eclogite formation.
Lines 56–57: Clarify the rationale of this sentence, or consider removing it.
Line 59: Quantify exhumation rates, providing values from numerical models and natural estimates. Restrict the discussion to the specific tectonic setting under study (wedge geometry)
Line 61: At present, the introduction does not clearly define the scientific gap. While the questions posed are valid, they appear abruptly. The gap would be clearer if you outlined: (i) the discrepancies between modelled and observed exhumation rates, (ii) the wide variability in return-flow models, and (iii) the influence of parameters such as channel width, rheology, and boundary conditions. Emphasize the mismatch between observations and models.
Lines 62–63: Clarify whether questions (1) and (2) are essentially identical.
Line 64: Revise to “theoretical and analog study.”
Line 65: Specify the depth range of both the theoretical and analog models. Although this is mentioned later, it should also appear here. State the main assumptions explicitly—for example, that the accretionary wedge is closed and material cannot enter the mantle—since this represents a special-case scenario.
Line 70: Integrate content from later lines: prior work has already tested different boundary conditions in numerical models (e.g., Gerya et al., 2002). The novelty here lies in the analytical treatment of non-parallel slab boundary conditions, which allows replication of slab rollback and advance. When combined with analog modelling, this provides a unique contribution.
Line 76: Clarify the phrase “oblique to the slab.” If it refers to the trench, rephrase as “a non-parallel component of slab velocity.”
Lines 86–88: This is the first mention of analog experiments, which are central to the manuscript. Introduce them earlier in the introduction and highlight the novelty of combining analytical solutions with analog modelling.
Line 96: Since some material may be dragged down, this is an important limitation—discuss explicitly.
Line 107: Even if non-linearity is not first-order, note that complexity may also arise from contrasting lithologies within the accretionary wedge.
Line 117: Clarify whether this component is oblique to the trench or simply non-parallel.
Lines 120–121: If the trench-oblique component is merely a reduction of subduction velocity, avoid presenting it as a trench-oblique term, since this implies a 3D model.
Lines 127–128: Replace “trench-perpendicular vertical plane” with “non-parallel component of slab velocity.”
Line 130: In Fig. 2 it seems only the oceanic plate’s fixed wall is constrained. Confirm whether the top boundary is also fixed.
Line 181: This derivation follows Moulas et al. (2021). Add a phrase such as “Following the approach of Moulas et al. (2021)...” You may shorten this section and direct readers to that reference until the non-parallel extension is introduced.
Line 214: Same as line 181.
Lines 229–230: Indicate that these models assume either a rigid overriding plate or very strong subduction channels, which generate extremely high overpressures.
Line 245: Clarify whether this is the discretization used to evaluate equations. If so, specify resolution and grid type.
Lines 261–263: Add references or case studies linking models to natural observations.
Line 267: In this simple case, the flow ratio (FR) should equal 1 due to mass conservation and wedge geometry. Clarify whether this depends on discretization.
Line 271: Is this because you are adding material through the slab or because of the "squeezing" of the wedge?
Line 286: Is this difference with the rigid case because of the viscosity ratio only? what if mu_r is even higher (i.e., 10^5 or 10^7), do you reach the rigid wall solution? Also, see later comments to define high/low FR.
Lines 290–291: Figures 4–5 show material still returning to the surface but further from the trench. Confirm whether FR is calculated only for the accretionary wedge (if so, specify at line 245).
Lines 292–294: Consider adding a figure similar to FR vs. obliquity (Fig. 7) to illustrate this result, and extend the same approach to other variables.
Line 323: Since deformation is not described, either remove the vorticity figures or move them to supplementary material with an explanation.
Line 344 and Fig. 7: FR = 0.5 is presented as a threshold between significant and negligible return flow. Explain how this value was determined, or move section 3.2 to the discussion. Kerswell et al. (2023) may provide guidance.
Line 351: Revise “wedge” to “downward-tapered wedge.”
Lines 356–357: Move this sentence to the discussion section.
Lines 392–395: Provide scaling for analog experiments. Do they correspond with analytical models or plate tectonic velocities? Indicate scaling parameters (e.g., Schellart & Strak, 2016) to demonstrate consistency with natural systems and analytical calculations.
Lines 411, 413: Replace “30%” with “0.3U” and “one-sixth” with “U/6” to align with line 415 (“0.6U”).
Line 413: Clarify whether oblique shortening with slab advance and oblique extension correspond to slab rollback. If so, use consistent terminology.
Line 419: Remove “grossly.” Add a one-to-one comparison with the analytical solution.
Lines 422–423: Gravity influences the analog model if the bottom boundary is open. Add a brief discussion of this effect.
Line 425: If slab rollback or oblique extension precludes return flow, clarify how comparisons were made, since the analog and analytical models differ in bottom boundary conditions.
Line 429: Change “crusts” to “crust.”
Lines 449–450: Clarify how comparisons between theoretical models and natural examples are made. Estimate taper angles and subduction dynamics (advance vs. rollback) for each exhumation case, then compare calculated FR values with reviews (e.g., Agard et al., 2009) or case studies (e.g., Franciscan Complex; Ring, 2008).
Line 453: Are there documented cases of absent accretionary wedges in modern rollback settings?
Line 454: Revise: note that HP units are present in Chile (Willner, 2005), with localized pressures of 2–2.5 GPa (González-Jiménez et al., 2017).
Lines 503–504: Mention the thermal regime, as it controls the brittle–ductile transition depth and influences viscosity.
Line 510: Replace “subduction” with “subduction zones.”
Line 519: Expand to “Multiple structural fabrics and fluid-assisted deformation (e.g., Muñoz-Montecinos & Behr, 2023).”
Lines 530–545: This section would benefit greatly from plotting the geological cases in Figure 8, enabling direct comparison between tectonic settings, model outputs, and natural data. Analog model results could also be added for completeness.
Line 590: Include rock strength in the brittle regime. In favorable conditions, rocks can sustain tens to hundreds of MPa before failure (Platt, 2019).
Line 625: Remove mu_r here, as it denotes viscosity ratio.
References in this review:
Abers (2005): https://doi.org/10.1016/j.pepi.2004.10.002
Agard et al. (2009): https://doi.org/10.1016/j.earscirev.2008.11.002
Gerya et al. (2002): https://doi.org/10.1029/2002TC001406
González-Jiménez et al. (2017): https://doi.org/10.1127/ejm/2017/0029-2668
Kerswell et al. (2023): https://doi.org/10.1029/2022GC010834
Moulas et al. (2021): https://doi.org/10.1093/gji/ggab246
Muñoz-Montecinos & Behr (2023): https://doi.org/10.1029/2023GL104244
Platt (2019): https://doi.org/10.5194/se-10-357-2019
Ring (2008): https://doi.org/10.1130/2008.2445
Schellart & Strak (2016): https://doi.org/10.1016/j.jog.2016.03.009
Willner (2005): https://doi.org/10.1093/petrology/egi035