Articles | Volume 17, issue 16
Atmos. Chem. Phys., 17, 9751–9760, 2017
https://doi.org/10.5194/acp-17-9751-2017
Atmos. Chem. Phys., 17, 9751–9760, 2017
https://doi.org/10.5194/acp-17-9751-2017

Research article 18 Aug 2017

Research article | 18 Aug 2017

Resolving the mesospheric nighttime 4.3 µm emission puzzle: comparison of the CO2(ν3) and OH(ν) emission models

Peter A. Panka et al.

Viewed

Total article views: 1,471 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
1,023 391 57 1,471 56 69
  • HTML: 1,023
  • PDF: 391
  • XML: 57
  • Total: 1,471
  • BibTeX: 56
  • EndNote: 69
Views and downloads (calculated since 22 Nov 2016)
Cumulative views and downloads (calculated since 22 Nov 2016)

Viewed (geographical distribution)

Total article views: 1,499 (including HTML, PDF, and XML) Thereof 1,487 with geography defined and 12 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Discussed (final revised paper)

Latest update: 25 Jul 2021
Download
Short summary
Recently, theoretical and laboratory studies have suggested an additional nighttime channel of transfer of vibrational energy of OH molecules to CO2 in the mesosphere and lower thermosphere (MLT). We show that new mechanism brings modelled 4.3 μm emissions very close to the SABER/TIMED measurements. This renders new opportunities for the application of the CO2 4.3 μm observations in the study of the energetics and dynamics of the nighttime MLT.
Altmetrics
Final-revised paper
Preprint