Articles | Volume 43, issue 2
https://doi.org/10.5194/angeo-43-489-2025
https://doi.org/10.5194/angeo-43-489-2025
Regular paper
 | 
08 Sep 2025
Regular paper |  | 08 Sep 2025

Effect of interplanetary shock waves on turbulence parameters

Emilia Kilpua, Simon Good, Juska Soljento, Domenico Trotta, Tia Bäcker, Julia Ruohotie, Jens Pomoell, Chaitanya Sishtla, and Rami Vainio

Viewed

Total article views: 820 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
712 85 23 820 33 49
  • HTML: 712
  • PDF: 85
  • XML: 23
  • Total: 820
  • BibTeX: 33
  • EndNote: 49
Views and downloads (calculated since 14 Jan 2025)
Cumulative views and downloads (calculated since 14 Jan 2025)

Viewed (geographical distribution)

Total article views: 820 (including HTML, PDF, and XML) Thereof 820 with geography defined and 0 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Latest update: 12 Sep 2025
Download
Short summary
Interplanetary shock waves are one of the major forms of heliospheric transients that can have a profound impact on solar wind plasma and magnetic field conditions and accelerate charged particles to high energies. This work performs an extensive statistical analysis to detail how some of the key solar wind turbulence parameters, critical for understanding particle acceleration, are modified by the interplanetary shocks waves.
Share