Articles | Volume 20, issue 9
Atmos. Chem. Phys., 20, 5269–5292, 2020
https://doi.org/10.5194/acp-20-5269-2020
Atmos. Chem. Phys., 20, 5269–5292, 2020
https://doi.org/10.5194/acp-20-5269-2020
Research article
06 May 2020
Research article | 06 May 2020

OH level populations and accuracies of Einstein-A coefficients from hundreds of measured lines

Stefan Noll et al.

Viewed

Total article views: 1,496 (including HTML, PDF, and XML)
HTML PDF XML Total Supplement BibTeX EndNote
1,033 432 31 1,496 74 22 18
  • HTML: 1,033
  • PDF: 432
  • XML: 31
  • Total: 1,496
  • Supplement: 74
  • BibTeX: 22
  • EndNote: 18
Views and downloads (calculated since 18 Dec 2019)
Cumulative views and downloads (calculated since 18 Dec 2019)

Viewed (geographical distribution)

Total article views: 1,318 (including HTML, PDF, and XML) Thereof 1,317 with geography defined and 1 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Latest update: 08 Aug 2022
Download
Short summary
Line emission from hydroxyl (OH) molecules at altitudes of about 90 km strongly contributes to the Earth's night-sky brightness and is therefore used as an important indicator of atmospheric chemistry and dynamics. However, interpreting the measurements can be ambiguous since necessary molecular parameters and the internal state of OH are not well known. Based on high-quality spectral data, we investigated these issues and found solutions for a better understanding of the OH line intensities.
Altmetrics
Final-revised paper
Preprint