Articles | Volume 33, issue 7
https://doi.org/10.5194/angeo-33-829-2015
https://doi.org/10.5194/angeo-33-829-2015
ANGEO Communicates
 | 
08 Jul 2015
ANGEO Communicates |  | 08 Jul 2015

Estimating along-track plasma drift speed from electron density measurements by the three Swarm satellites

J. Park, H. Lühr, C. Stolle, G. Malhotra, J. B. H. Baker, S. Buchert, and R. Gill

Viewed

Total article views: 1,550 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
867 632 51 1,550 62 51
  • HTML: 867
  • PDF: 632
  • XML: 51
  • Total: 1,550
  • BibTeX: 62
  • EndNote: 51
Views and downloads (calculated since 08 Jul 2015)
Cumulative views and downloads (calculated since 08 Jul 2015)

Cited

Latest update: 27 Mar 2024
Download
Short summary
Though high-latitude plasma convection has been monitored with a number of methods, more independent measurements are still warranted. In this study we introduce an automatic method to estimate along-track plasma drift velocity in the high-latitude ionosphere using the Swarm constellation. The obtained velocity is in qualitative agreement with Super Dual Auroral Radar Network (SuperDARN) data. The method can be generalized to any satellite constellations in pearls-on-a-string configurations.