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From the following article:

A warm layer in Venus' cryosphere and high-altitude measurements of HF, HCl, H2O and HDO

Jean-Loup Bertaux, Ann-Carine Vandaele, Oleg Korablev, E. Villard, A. Fedorova, D. Fussen, E. Quémerais, D. Belyaev, A. Mahieux, F. Montmessin, C. Muller, E. Neefs, D. Nevejans, V. Wilquet, J. P. Dubois, A. Hauchecorne, A. Stepanov, I. Vinogradov, A. Rodin & the SPICAV/SOIR team

Nature 450, 646-649(29 November 2007)

doi:10.1038/nature05974

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Figure 1 - Unfortunately we are unable to provide accessible alternative text for this. If you require assistance to access this image, or to obtain a text description, please contact npg@nature.com

Figure 1

Night-side temperature of Venus atmosphere.

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Figure 2

Typical evolution of atmospheric spectral transmittances through one solar occultation observed by SOIR spectrometer.

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Figure 3

HF and HCl mixing ratio vertical profiles retrieved from SOIR occultations.

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Figure 4

HDO and H2O mixing ratio, HDO/ H2O vertical profiles.

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