Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
8143278 | Planetary and Space Science | 2015 | 15 Pages |
Abstract
The thermal structure of Venus upper atmosphere (90-140Â km) was investigated using stellar occultation measurements acquired by the SPICAV experiment on board Venus Express. The SPICAV ultraviolet channel provides CO2 local density and temperature vertical profiles with a vertical resolution of <7km of both the southern and the northern hemispheres on the nightside (18:00-06:00Â h local time). A permanent layer of warm air is observed at the mesopause in the altitude range 90-100Â km. Temperature then decreases with increasing altitude reaching a minimum value around 125Â km. Spatial and temporal changes in the thermal structure have been analyzed. Local time variations dominate the structure of Venus atmosphere at these altitudes: temperatures show an increase of ~20K on the morning side compared to the evening side. The homopause altitude was also determined; it varies between 119 and 138Â km of altitude, increasing from the evening side to the morning side. SPICAV temperature profiles were compared to several literature results from ground-based observations, previous spacecraft missions and the Venus Express mission.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geophysics
Authors
A. Piccialli, F. Montmessin, D. Belyaev, A. Mahieux, A. Fedorova, E. Marcq, J.-L. Bertaux, S. Tellmann, A.C. Vandaele, O. Korablev,