Atmospheric Chemistry and Physics
Atmospheric Chemistry and Physics
ACP
Articles | Volume 23, issue 11
Articles | Volume 23, issue 11
https://doi.org/10.5194/acp-23-6383-2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.
Special issue:
https://doi.org/10.5194/acp-23-6383-2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.
Articles | Volume 23, issue 11
Research article
 | 
12 Jun 2023
Research article |  | 12 Jun 2023

Simulated long-term evolution of the thermosphere during the Holocene – Part 2: Circulation and solar tides

Xu Zhou, Xinan Yue, Yihui Cai, Zhipeng Ren, Yong Wei, and Yongxin Pan

Viewed

Total article views: 3,188 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
2,105 934 149 3,188 168 261
  • HTML: 2,105
  • PDF: 934
  • XML: 149
  • Total: 3,188
  • BibTeX: 168
  • EndNote: 261
Views and downloads (calculated since 15 Feb 2023)
Cumulative views and downloads (calculated since 15 Feb 2023)

Viewed (geographical distribution)

Total article views: 3,188 (including HTML, PDF, and XML) Thereof 3,173 with geography defined and 15 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Saved (final revised paper)

Latest update: 30 May 2026
Download
Short summary
Secular variations in CO2 concentration and geomagnetic field can affect the dynamics of the upper atmosphere. We examine how these two factors influence the dynamics of the upper atmosphere during the Holocene, using two sets of ~ 12 000-year control runs by the coupled thermosphere–ionosphere model. The main results show that (a) increased CO2 enhances the thermospheric circulation, but non-linearly; and (b) geomagnetic variation induced a significant hemispheric asymmetrical effect.
Read more
Share
Special issue
Long-term changes and trends in the middle and upper...
Altmetrics
Final-revised paper
Preprint