Articles | Volume 37, issue 5
https://doi.org/10.5194/angeo-37-989-2019
https://doi.org/10.5194/angeo-37-989-2019
Regular paper
 | 
28 Oct 2019
Regular paper |  | 28 Oct 2019

Solar cycle, seasonal, and asymmetric dependencies of thermospheric mass density disturbances due to magnetospheric forcing

Andres Calabia and Shuanggen Jin

Viewed

Total article views: 1,687 (including HTML, PDF, and XML)
HTML PDF XML Total Supplement BibTeX EndNote
1,082 568 37 1,687 286 42 38
  • HTML: 1,082
  • PDF: 568
  • XML: 37
  • Total: 1,687
  • Supplement: 286
  • BibTeX: 42
  • EndNote: 38
Views and downloads (calculated since 05 Jun 2019)
Cumulative views and downloads (calculated since 05 Jun 2019)

Viewed (geographical distribution)

Total article views: 1,687 (including HTML, PDF, and XML) Thereof 1,591 with geography defined and 96 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Latest update: 23 Apr 2024
Download
Short summary
Atmospheric drag due to mass density distribution, particularly during storm-time, is of great importance for low Earth orbit precise orbit determination, and for the understanding of magnetosphere–ionosphere–thermosphere phenomena. In this paper, we investigate solar cycle, seasonal, and hemispheric asymmetry dependencies of thermospheric mass density disturbances due to magnetospheric forcing, from 10-year (2003–2013) continuous time series of GRACE estimates.