Articles | Volume 42, issue 2
https://doi.org/10.5194/angeo-42-419-2024
https://doi.org/10.5194/angeo-42-419-2024
Regular paper
 | 
22 Oct 2024
Regular paper |  | 22 Oct 2024

Proton plasma asymmetries between the convective-electric-field hemispheres of Venus' dayside magnetosheath

Sebastián Rojas Mata, Gabriella Stenberg Wieser, Tielong Zhang, and Yoshifumi Futaana

Viewed

Total article views: 495 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
345 103 47 495 27 34
  • HTML: 345
  • PDF: 103
  • XML: 47
  • Total: 495
  • BibTeX: 27
  • EndNote: 34
Views and downloads (calculated since 06 Dec 2023)
Cumulative views and downloads (calculated since 06 Dec 2023)

Viewed (geographical distribution)

Total article views: 495 (including HTML, PDF, and XML) Thereof 492 with geography defined and 3 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 
Latest update: 11 Dec 2024
Download
Short summary
The Sun ejects a stream of charged particles into space that have to flow around planets like Venus. We quantify how this flow varies with spatial location using spacecraft measurements of the particles and magnetic field taken over several years. We find that this flow is connected to interactions with the heavier charged particles that originate from Venus’ upper atmosphere. These interactions are not unique to Venus, so we compare our results to similar studies at Mars.