Articles | Volume 40, issue 3
https://doi.org/10.5194/angeo-40-281-2022
https://doi.org/10.5194/angeo-40-281-2022
Regular paper
 | 
09 May 2022
Regular paper |  | 09 May 2022

Menura: a code for simulating the interaction between a turbulent solar wind and solar system bodies

Etienne Behar, Shahab Fatemi, Pierre Henri, and Mats Holmström

Viewed

Total article views: 3,874 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
2,507 1,255 112 3,874 131 153
  • HTML: 2,507
  • PDF: 1,255
  • XML: 112
  • Total: 3,874
  • BibTeX: 131
  • EndNote: 153
Views and downloads (calculated since 03 Jan 2022)
Cumulative views and downloads (calculated since 03 Jan 2022)

Viewed (geographical distribution)

Total article views: 3,874 (including HTML, PDF, and XML) Thereof 3,732 with geography defined and 142 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Saved (final revised paper)

Latest update: 09 Jun 2026
Download
Short summary
Despite the solar wind being turbulent in nature, numerical models of its interaction with obstacles have until now assumed it to be laminar. The code \textit{Menura} allows for the global simulation of the interaction between a fully turbulent solar wind and various bodies of the solar system. The code is illustrated by a first example: the interaction between a turbulent solar wind and a comet.
Share