Articles | Volume 23, issue 2
https://doi.org/10.5194/acp-23-1705-2023
https://doi.org/10.5194/acp-23-1705-2023
Research article
 | 
31 Jan 2023
Research article |  | 31 Jan 2023

Aura/MLS observes and SD-WACCM-X simulates the seasonality, quasi-biennial oscillation and El Niño–Southern Oscillation of the migrating diurnal tide driving upper mesospheric CO primarily through vertical advection

Cornelius Csar Jude H. Salinas, Dong L. Wu, Jae N. Lee, Loren C. Chang, Liying Qian, and Hanli Liu

Viewed

Total article views: 2,142 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
1,683 409 50 2,142 38 31
  • HTML: 1,683
  • PDF: 409
  • XML: 50
  • Total: 2,142
  • BibTeX: 38
  • EndNote: 31
Views and downloads (calculated since 04 Oct 2022)
Cumulative views and downloads (calculated since 04 Oct 2022)

Viewed (geographical distribution)

Total article views: 2,142 (including HTML, PDF, and XML) Thereof 2,135 with geography defined and 7 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Latest update: 20 Nov 2024
Download
Short summary
Upper mesospheric carbon monoxide's (CO) photochemical lifetime is longer than dynamical timescales. This work uses satellite observations and model simulations to establish that the migrating diurnal tide and its seasonal and interannual variabilities drive CO primarily through vertical advection. Vertical advection is a transport process that is currently difficult to observe. This work thus shows that we can use CO as a tracer for vertical advection across seasonal and interannual timescales.
Altmetrics
Final-revised paper
Preprint