Articles | Volume 36, issue 1
https://doi.org/10.5194/angeo-36-13-2018
https://doi.org/10.5194/angeo-36-13-2018
Regular paper
 | Highlight paper
 | 
09 Jan 2018
Regular paper | Highlight paper |  | 09 Jan 2018

New insights for mesospheric OH: multi-quantum vibrational relaxation as a driver for non-local thermodynamic equilibrium

Konstantinos S. Kalogerakis, Daniel Matsiev, Philip C. Cosby, James A. Dodd, Stefano Falcinelli, Jonas Hedin, Alexander A. Kutepov, Stefan Noll, Peter A. Panka, Constantin Romanescu, and Jérôme E. Thiebaud

Viewed

Total article views: 2,479 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
1,740 619 120 2,479 74 87
  • HTML: 1,740
  • PDF: 619
  • XML: 120
  • Total: 2,479
  • BibTeX: 74
  • EndNote: 87
Views and downloads (calculated since 09 Jan 2018)
Cumulative views and downloads (calculated since 09 Jan 2018)

Cited

Latest update: 22 Nov 2024
Download
Short summary
The question of whether mesospheric rotational population distributions of vibrationally excited OH are in equilibrium with the local kinetic temperature has been debated over several decades. We examine the relationship of multi-quantum relaxation pathways with the behavior exhibited by OH(v) rotational population distributions and find that the effective rotational temperatures of mesospheric OH(v) deviate from local thermodynamic equilibrium for all observed vibrational levels.