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

Viewed

Total article views: 1,077 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
866 95 116 1,077 62 125
  • HTML: 866
  • PDF: 95
  • XML: 116
  • Total: 1,077
  • BibTeX: 62
  • EndNote: 125
Views and downloads (calculated since 14 Nov 2024)
Cumulative views and downloads (calculated since 14 Nov 2024)

Viewed (geographical distribution)

Total article views: 1,077 (including HTML, PDF, and XML) Thereof 1,059 with geography defined and 18 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 
Latest update: 06 Dec 2025
Download
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.
Share