Strong longitudinal variations in the OH nightglow
Airglow from the hydroxyl Meinel bands, originating from about 87 km, gives a signature of the atmosphere that can be observed remotely. Analysis of long term global observations of the 2.0 μm OH Meinel brightness observed by the TIMED/SABER satellite instrument presents some striking patterns that appear in the Meinel airglow. The analysis shows that migrating and non-migrating tides have large effects on the nighttime OH airglow emission in the upper mesosphere. The OH airglow emission rate is positively correlated with temperature below 94 km and negatively correlated above. Variations with longitudinal wavenumbers 1 and 4 are shown to result from the impacts of the stationary (D0), westward wavenumber 2 (DW2), and eastward wavenumber 3 (DE3) nonmigrating diurnal tides.
document
https://n2t.org/ark:/85065/d77p8zv1
eng
geoscientificInformation
Text
publication
2016-01-01T00:00:00Z
publication
2010-11-02T00:00:00Z
An edited version of this paper was published by AGU. Copyright 2010 American Geophysical Union
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