Articles | Volume 19, issue 18
https://doi.org/10.5194/gmd-19-8839-2026
https://doi.org/10.5194/gmd-19-8839-2026
Development and technical paper
 | 
21 Sep 2026
Development and technical paper |  | 21 Sep 2026

Variational Stokes method applied to free surface boundaries in numerical geodynamical models using the staggered-grid finite-difference discretisation

Timothy S. Gray, Paul J. Tackley, and Taras V. Gerya

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Interactive discussion

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • CEC1: 'Comment on egusphere-2025-6354 - No compliance with the policy of the journal', Juan Antonio Añel, 07 Jan 2026
    • AC1: 'Reply on CEC1', Timothy Gray, 10 Jan 2026
      • CEC2: 'Reply on AC1', Juan Antonio Añel, 11 Jan 2026
        • AC2: 'Reply on CEC2', Timothy Gray, 20 Jan 2026
  • RC1: 'Comment on egusphere-2025-6354', Wolfgang Bangerth, 08 Feb 2026
    • AC3: 'Reply on RC1', Timothy Gray, 22 Mar 2026
  • RC2: 'Comment on egusphere-2025-6354', Thibault Duretz, 12 Feb 2026
    • AC4: 'Reply on RC2', Timothy Gray, 22 Mar 2026

Peer review completion

AR – Author's response | RR – Referee report | ED – Editor decision | EF – Editorial file upload
AR by Timothy Gray on behalf of the Authors (29 Mar 2026)  Author's response   Author's tracked changes   Manuscript 
ED: Referee Nomination & Report Request started (09 Apr 2026) by Mauro Cacace
RR by Wolfgang Bangerth (18 Apr 2026)
RR by Thibault Duretz (27 Apr 2026)
ED: Reconsider after major revisions (11 May 2026) by Mauro Cacace
AR by Timothy Gray on behalf of the Authors (22 Jun 2026)  Author's response   Author's tracked changes   Manuscript 
ED: Referee Nomination & Report Request started (08 Jul 2026) by Mauro Cacace
RR by Wolfgang Bangerth (09 Jul 2026)
ED: Publish as is (21 Jul 2026) by Mauro Cacace
AR by Timothy Gray on behalf of the Authors (29 Jul 2026)  Manuscript 
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Short summary
We developed a new way to model how planetary surfaces rise and sink as the deep interior slowly flows. Existing approaches are either costly or unstable. Our method represents the surface smoothly within a fixed grid, which avoids artificial air layers and numerical problems. Tests show it matches established results while running faster and working in more realistic settings, such as loaded surfaces and global models. This makes simulations of surface evolution more reliable and accessible.
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