Annales Geophysicae
Annales Geophysicae
ANGEO
Articles | Volume 36, issue 2
Articles | Volume 36, issue 2
https://doi.org/10.5194/angeo-36-527-2018
© Author(s) 2018. This work is distributed under
the Creative Commons Attribution 4.0 License.
https://doi.org/10.5194/angeo-36-527-2018
© Author(s) 2018. This work is distributed under
the Creative Commons Attribution 4.0 License.
Articles | Volume 36, issue 2
Regular paper
 | 
29 Mar 2018
Regular paper |  | 29 Mar 2018

Three-dimensional density and compressible magnetic structure in solar wind turbulence

Owen W. Roberts, Yasuhito Narita, and C.-Philippe Escoubet

Viewed

Total article views: 2,620 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
1,779 710 131 2,620 93 89
  • HTML: 1,779
  • PDF: 710
  • XML: 131
  • Total: 2,620
  • BibTeX: 93
  • EndNote: 89
Views and downloads (calculated since 29 Mar 2018)
Cumulative views and downloads (calculated since 29 Mar 2018)

Cited

Latest update: 01 Jun 2025
Download
Short summary
In this study we use multi-point spacecraft measurements of magnetic field and electron density derived from spacecraft potential to investigate the three-dimensional structure of solar wind plasma turbulence. We see that there is a dependence on the plasma beta (ratio of thermal to magnetic pressure) as well as a dependence on the type of wind i.e. fast or slow.
Read more
Share