Articles | Volume 12, issue 5
https://doi.org/10.5194/esurf-12-1193-2024
https://doi.org/10.5194/esurf-12-1193-2024
Research article
 | 
22 Oct 2024
Research article |  | 22 Oct 2024

Modeling the formation of toma hills based on fluid dynamics with a modified Voellmy rheology

Stefan Hergarten

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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 egusphere-2024-1070', Anonymous Referee #1, 04 Jun 2024
    • AC2: 'Reply on RC1', Stefan Hergarten, 24 Jul 2024
  • RC2: 'Comment on egusphere-2024-1070', Martin Mergili, 14 Jun 2024
    • AC1: 'Reply on RC2', Stefan Hergarten, 22 Jul 2024

Peer review completion

AR: Author's response | RR: Referee report | ED: Editor decision | EF: Editorial file upload
AR by Stefan Hergarten on behalf of the Authors (31 Jul 2024)  Author's response   Author's tracked changes   Manuscript 
ED: Publish as is (08 Aug 2024) by Fiona Clubb
ED: Publish as is (14 Aug 2024) by Wolfgang Schwanghart (Editor)
AR by Stefan Hergarten on behalf of the Authors (30 Aug 2024)  Manuscript 
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Short summary
Toma hills are relatively isolated hills found in the deposits of rock avalanches, and their origin is still enigmatic. This paper presents the results of numerical simulations based on a modified version of a friction law that was originally introduced for snow avalanches. The model produces more or less isolated hills (which look much like toma hills) on the valley floor. The results provide, perhaps, the first explanation of the occurrence of toma hills based on a numerical model.