Articles | Volume 18, issue 13
https://doi.org/10.5194/gmd-18-4215-2025
https://doi.org/10.5194/gmd-18-4215-2025
Model description paper
 | 
15 Jul 2025
Model description paper |  | 15 Jul 2025

A time-dependent three-dimensional dayside magnetopause model based on quasi-elastodynamic theory

Yaxin Gu, Yi Wang, Fengsi Wei, Xueshang Feng, Andrey Samsonov, Xiaojian Song, Boyi Wang, Pingbing Zuo, Chaowei Jiang, Yalan Chen, Xiaojun Xu, and Zilu Zhou

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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-2024-3012', Anonymous Referee #1, 17 Dec 2024
    • AC2: 'Reply on RC1', yi wang, 20 Mar 2025
  • RC2: 'Comment on egusphere-2024-3012', Anonymous Referee #2, 18 Feb 2025
    • AC3: 'Reply on RC2', yi wang, 20 Mar 2025
  • AC1: 'Comment on egusphere-2024-3012', yi wang, 20 Mar 2025
    • AC4: 'Reply on AC1', yi wang, 20 Mar 2025

Peer review completion

AR: Author's response | RR: Referee report | ED: Editor decision | EF: Editorial file upload
AR by yi wang on behalf of the Authors (20 Mar 2025)  Author's response   Author's tracked changes   Manuscript 
ED: Publish as is (31 Mar 2025) by Tatiana Egorova
AR by yi wang on behalf of the Authors (06 Apr 2025)  Manuscript 

Post-review adjustments

AA: Author's adjustment | EA: Editor approval
AA by yi wang on behalf of the Authors (02 Jul 2025)   Author's adjustment   Manuscript
EA: Adjustments approved (07 Jul 2025) by Tatiana Egorova
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Short summary
Understanding how solar wind interacts with Earth’s protective magnetic shield is a frontier issue in space physics, critical for predicting space weather risks. However, most existing magnetopause models cannot capture this time-dependent process, and numerical simulations demand significant computational resources. We have developed the first time-dependent 3D model capable of showing these shield changes. It is significantly more precise and performs nearly instant computations.
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