4.7 Article

Simultaneous Retrievals of Nighttime O(3P) and Total OH Densities From Satellite Observations of Meinel Band Emissions

期刊

GEOPHYSICAL RESEARCH LETTERS
卷 48, 期 1, 页码 -

出版社

AMER GEOPHYSICAL UNION
DOI: 10.1029/2020GL091053

关键词

atmospheric retrievals; mesosphere-lower thermosphere; Meinel band emissions; non-LTE; remote sensing

资金

  1. NSF [1301762, AGS-1441896]
  2. NASA [NNX15AN08G, 80NSSC17K0638]
  3. NASA/TIMED project
  4. Specialized Research Fund for State Key Laboratories
  5. NSSC Research Fund for key development directions
  6. Directorate For Geosciences
  7. Div Atmospheric & Geospace Sciences [1301762] Funding Source: National Science Foundation
  8. NASA [800109, NNX15AN08G] Funding Source: Federal RePORTER

向作者/读者索取更多资源

This study presents a novel approach for retrieving atomic oxygen and total hydroxyl densities in the middle and upper atmosphere from nighttime observations, showing good agreement in atomic oxygen densities obtained from different instruments but large discrepancies in hydroxyl densities.
Retrieving the total number density [OH], which is used in the chemical balance equations and is the sum of both ground and excited vibrational state populations, is a challenging problem to such a degree there exist no such estimates from recent space observations. We present a novel retrieval approach to simultaneously and self-consistently derive both [O(P-3)] and total [OH] in the nighttime mesosphere and lower thermosphere which operates with the Meinel band volume emission rates and their ratios. Its application to the Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) and Scanning Imaging Absorption spectroMeter for Atmospheric CHartographY (SCIAMACHY) observations shows a good agreement of the retrieved [O(P-3)] taking into account the measurement uncertainties and variation of model inputs used. However, retrieved [OH] show a large discrepancy, mainly above 90 km. SCIAMACHY [OH] is generally in good agreement with WACCM [OH] after accounting for uncertainties, while SABER OH is larger than WACCM [OH] by up to a factor of 2. Plain Language Summary The hydroxyl molecule plays an important role in the physics, chemistry, and dynamics of the middle and upper atmosphere region (60-120 km). Obtaining total hydroxyl density from its molecular emissions is a challenging problem to such a degree there exist no such estimates from the recent space observations. We present a novel approach to obtain both atomic oxygen and total hydroxyl densities in the middle and upper atmosphere from nighttime observations of the hydroxyl molecular emissions. We apply the new approach to two different space-based instrument observations of hydroxyl emissions at multiple infrared wavelengths. The atomic oxygen densities obtained from the two instruments using our new approach are in good agreement after taking into account uncertainties, while the hydroxyl densities show a large discrepancy.

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