Articles | Volume 43, issue 2
https://doi.org/10.5194/angeo-43-593-2025
https://doi.org/10.5194/angeo-43-593-2025
Regular paper
 | 
09 Oct 2025
Regular paper |  | 09 Oct 2025

Comparing Monte Carlo simulations, mean particle theory estimates, and observations of H+ and O+ outflows at high altitudes and latitudes

Imad A. Barghouthi and May R. Halaika

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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 angeo-2024-24', Anonymous Referee #1, 06 Feb 2025
  • AC1: 'Comment on angeo-2024-24', Imad Barghouthi, 14 Mar 2025
  • AC2: 'Comment on angeo-2024-24', Imad Barghouthi, 14 Mar 2025
  • RC2: 'Comment on angeo-2024-24', Anonymous Referee #2, 17 Mar 2025

Peer review completion

AR: Author's response | RR: Referee report | ED: Editor decision | EF: Editorial file upload
ED: Publish subject to revisions (further review by editor and referees) (28 Mar 2025) by Elias Roussos
AR by Imad Barghouthi on behalf of the Authors (06 May 2025)  Author's response   Author's tracked changes   Manuscript 
ED: Publish subject to minor revisions (review by editor) (01 Jul 2025) by Elias Roussos
AR by Imad Barghouthi on behalf of the Authors (07 Jul 2025)  Author's response   Author's tracked changes   Manuscript 
ED: Publish as is (14 Jul 2025) by Elias Roussos
AR by Imad Barghouthi on behalf of the Authors (16 Jul 2025)  Manuscript 
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Short summary
This research explores how hydrogen ions and oxygen ions move and gain energy in Earth’s magnetosphere at high altitudes and latitudes. Using Monte Carlo simulations, predictions of mean particle theory, and corresponding observations, we compared different energy profiles of hydrogen and oxygen ions across polar-wind, aurora, cusp, and central-polar-cap regions. Our findings reveal that unique interactions in each area affect energy gain differently, with implications for future space weather models.
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