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

doi:doi:10.1038/nature05974

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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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Supplementary Information

The file contains Supplementary Notes and Supplementary Figure 1 with Legend. The Supplementary Notes discuss the retrieval of CO₂ density and temperature for stellar occultations in the UV, about the concept of the new SOIR spectrometer, and retrieval of atmospheric minor constituents from SOIR.
The Supplementary Figure 1 is composed of four panels, showing for a typical stellar occultation: a) the atmospheric spectral transmission at various altitudes and their best fit model; b) the derived line densities vertical profile; c) the derived densities vertical profile; d) the temperature vertical profile.

Supplementary Information - Download PDF file (155KB)

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