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Observation of night OH in the mesosphere
Author(s) -
Pickett H. M.,
Read W. G.,
Lee K. K.,
Yung Y. L.
Publication year - 2006
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/2006gl026910
Subject(s) - mesosphere , lidar , altitude (triangle) , atmospheric sciences , excited state , infrared , environmental science , stratosphere , mesopause , physics , remote sensing , atomic physics , geology , optics , geometry , mathematics
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 HO x 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 HO x chemistry. The model predicts that ground state OH represents 99% of the total OH up to 84 km.