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At latitudes equatorward of 75°, static stability derived from the observed temperature profiles is consistent with previous <jats:italic>in-situ</jats:italic> measurements in that there is a low-stability layer at altitudes of 50–58 km and highly and moderately stratified layers above 58 km and below 50 km, respectively. Meanwhile, at latitudes poleward of 75°, a low-stability layer extends down to 42 km, which has been unreported in analyses of previous measurements. The deep low-stability layer in the polar region cannot be explained by vertical convection in the middle/lower cloud layer, and the present result thus introduces new constraints on the dynamics of the sub-cloud atmosphere. The Venusian atmosphere is in striking contrast to the Earth’s troposphere, which generally has a deeper low-stability layer at low latitudes than at mid- and high latitudes.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1381975843215420935","@type":"Researcher","foaf:name":[{"@value":"Hiroki 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