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Variability and trends in the OH airglow layer observed by GOMOS/ENVISAT

Alain Hauchecorne 1 Laurent Blanot 2 Christophe Bellisario 3 Philippe Keckhut 1 Pierre Simoneau 4 Jean-Loup Bertaux 1
1 STRATO - LATMOS
LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales
2 ACRI-ST - Analytic and Computational Research, Inc. - Earth Sciences
3 ONERA - The French Aerospace Lab [Châtillon]
4 ONERA - The French Aerospace Lab [Palaiseau]
Abstract : The OH near-infrared nigthglow emission in the upper mesosphere is a marker of the chemistry and dynamics occurring at this level. The stellar occultation spectrometer GOMOS on board ENVISAT allowed to observe the OH(8-4) Meinel band in the spectral range 930-955 nm with a spectrometer dedicated to the observation of the water vapour. Climatology of OH emission has been established for the period 2002-2012. It allowed to confirm already published results as the maximum of intensity and semi-annual variation at the equator. The causes of variability and trends in the brightness and maximum altitude of the OH layer will be discussed. A new result concerns the apparent correlation of the emission rate with the solar activity.
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Conference papers
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https://hal-insu.archives-ouvertes.fr/insu-01303872
Contributor : Catherine Cardon <>
Submitted on : Monday, April 18, 2016 - 5:07:24 PM
Last modification on : Friday, January 10, 2020 - 3:42:30 PM

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  • HAL Id : insu-01303872, version 1

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INSU | CNRS | UPMC | UVSQ | LATMOS | ONERA | UNIV-PARIS-SACLAY | SORBONNE-UNIVERSITE | SU-SCIENCES

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Alain Hauchecorne, Laurent Blanot, Christophe Bellisario, Philippe Keckhut, Pierre Simoneau, et al.. Variability and trends in the OH airglow layer observed by GOMOS/ENVISAT. European Geosciences Union General Assembly 2016, Apr 2016, Vienna, Austria. pp. EGU2016-17349. ⟨insu-01303872⟩

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