Articles | Volume 13, issue 4
https://doi.org/10.5194/esurf-13-549-2025
https://doi.org/10.5194/esurf-13-549-2025
Research article
 | 
14 Jul 2025
Research article |  | 14 Jul 2025

Computational sedimentation modelling calibration: a tool to measure the settling velocity under different gravity conditions

Nikolaus J. Kuhn and Federica Trudu

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Interactive discussion

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on esurf-2023-11', Anonymous Referee #1, 08 Nov 2023
    • AC1: 'Reply on RC1', Federica Trudu, 19 Jan 2024
  • RC2: 'Comment on esurf-2023-11', Anonymous Referee #2, 01 Dec 2023
    • AC2: 'Reply on RC2', Federica Trudu, 19 Jan 2024

Peer review completion

AR: Author's response | RR: Referee report | ED: Editor decision | EF: Editorial file upload
AR by Federica Trudu on behalf of the Authors (02 Feb 2024)  Author's response   Author's tracked changes   Manuscript 
ED: Referee Nomination & Report Request started (16 Feb 2024) by Susan Conway
RR by Anonymous Referee #1 (18 Mar 2024)
RR by Anonymous Referee #3 (04 May 2024)
ED: Publish subject to minor revisions (review by editor) (06 May 2024) by Susan Conway
AR by Nikolaus J. Kuhn on behalf of the Authors (10 Mar 2025)  Author's response   Author's tracked changes   Manuscript 
ED: Publish subject to technical corrections (02 Apr 2025) by Susan Conway
ED: Publish subject to technical corrections (07 Apr 2025) by Tom Coulthard (Editor)
AR by Nikolaus J. Kuhn on behalf of the Authors (09 Apr 2025)  Manuscript 
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Short summary
In many ways, the surface of the planet Mars is similar to that of Earth. However, Mars's lower gravity has an effect on the settling and transport of sediment particles moving in water. Using specific experimental equipment to measure settling velocity aboard a parabolic flight, it was possible to observe how sediments settled in Martian gravity. These experiments served to illustrate that parabolic flights can be used as analogue environments for surface processes on Mars.
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