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AMT | Articles | Volume 12, issue 1
Atmos. Meas. Tech., 12, 585–598, 2019
https://doi.org/10.5194/amt-12-585-2019
© Author(s) 2019. This work is distributed under
the Creative Commons Attribution 4.0 License.
Atmos. Meas. Tech., 12, 585–598, 2019
https://doi.org/10.5194/amt-12-585-2019
© Author(s) 2019. This work is distributed under
the Creative Commons Attribution 4.0 License.

Research article 28 Jan 2019

Research article | 28 Jan 2019

High-resolution temperature profiles retrieved from bichromatic stellar scintillation measurements by GOMOS/Envisat

Viktoria F. Sofieva et al.
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Cited articles  
Allen, S. J. and Vincent, R. A.: Gravity wave activity in the lower atmosphere: Seasonal and latitudinal variations, J. Geophys. Res., 100, 1327–1350, 1995. 
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Dalaudier, F., Sofieva, V. F., Hauchecorne, A., Kyrölä, E., Blanot, L., Guirlet, M., Retscher, C., and Zehner, C.: High-resolution density and temperature profiling in the stratosphere using bi-chromatic scintillation measurements by GOMOS, in: Proceedings of the First Atmospheric Science Conference, 8–12 May 2006, ESA ESRIN Frascati, Italy, European Space Agency, 2006. 
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This paper describes the temperature profiles in the stratosphere obtained from unique stellar scintillation measurements by the GOMOS instrument operated on board Envisat in 2002–2012. The high-resolution temperature profiles (HRTPs) are retrieved with a very good vertical resolution of ~ 200 m and a high accuracy of ~ 1–3 K for altitudes 15–32 km as well as a global coverage. HRTPs can be assimilated into atmospheric models and used in analyses of internal gravity wave activity.
This paper describes the temperature profiles in the stratosphere obtained from unique stellar...
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