Abstract
Satellite measurements from the Aura MLS instrument show a layer of OH near 82 km in the night. This layer confirms earlier measurements by ground-based LIDAR. The MLS and LIDAR observations measure OH in the lowest vibrational state and are distinct, but related chemically, from vibrationally-excited emission from the OH Meinel bands in the near infrared. The Caltech 1-D model has been extended to include vibrational dependence of OH reactions and shows good agreement with MLS OH data and with observations of the Meinel bands. The model shows a chemical lifetime of HOx that increases from less than a day at 80 km to over a month at 87 km. Above this altitude transport processes become an important part of HOx chemistry. The model predicts that ground state OH represents 99% of the total OH up to 84 km. Copyright 2006 by the American Geophysical Union.
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CITATION STYLE
Pickett, H. M., Read, W. G., Lee, K. K., & Yung, Y. L. (2006). Observation of night OH in the mesosphere. Geophysical Research Letters, 33(19). https://doi.org/10.1029/2006GL026910
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