Structure of the Venusian atmosphere from surface up to 100 km
The goal of this paper is to summarize the experimental data on the atmosphere of Venus obtained after 1985, when the VIRA (Venus International Reference Atmosphere) or COSPAR model was published. Among the most important results that have appeared since then are the following: measurements of the v...
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Veröffentlicht in: | Cosmic research 2006-07, Vol.44 (4), p.364-383 |
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Sprache: | eng |
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