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2D photochemical modeling of Saturn's stratosphere. Part II: Feedback between composition and temperature

Authors :
Franck Hersant
Michel Dobrijevic
Vincent Hue
Thomas K. Greathouse
Thibault Cavalié
ASP 2016
Laboratoire d'Astrophysique de Bordeaux [Pessac] (LAB)
Université de Bordeaux (UB)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Bordeaux (UB)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Southwest Research Institute [San Antonio] (SwRI)
ECLIPSE 2016
Source :
Icarus, Icarus, Elsevier, 2016, 267, pp.334-343. ⟨10.1016/j.icarus.2015.12.007⟩
Publication Year :
2015

Abstract

Saturn's axial tilt produces seasons in a similar way as on Earth. Both the stratospheric temperature and composition are affected by this latitudinally varying insolation along the seasons. The thermal structure is controlled and regulated by the amount of hydrocarbons in the stratosphere, which act as absorbers and coolants from the UV to the far-IR spectral range, and this structure influences the amount of hydrocarbons. We study here the feedback between the chemical composition and the thermal structure by coupling a latitudinal and seasonal photochemical model with a radiative seasonal model. Our results show that the seasonal temperature peak in the higher stratosphere, associated with the seasonal increase of insolation, is shifted earlier than the maximum insolation peak. This shift is increased with increasing latitudes and is caused by the low amount of stratospheric coolants in the spring season. At 80$^{\circ}$ in both hemispheres, the temperature peak at 1d-2mbar is seen to occur half a season earlier than was previously predicted by radiative seasonal models that assumed spatially and temporally uniform distribution of coolants. This shift progressively decreases with increasing pressure, up to around the 0.5mbar pressure level where it vanishes. However, the thermal field has a small feedback on the abundance distributions. This feedback modifies the predicted equator-to-pole temperature gradient. The meridional gradients of temperature at the mbar pressure levels are better reproduced when this feedback is accounted for. At lower pressure levels, the thermal structure seems to depart from pure radiative seasonal equilibrium as previously suggested by Guerlet et al. (2014). Although the agreement with the absolute value of the stratospheric temperature observed by Cassini is moderate, it is a mandatory step toward a fully coupled GCM-photochemical model.<br />23 pages, 8 figures, accepted for publication in Icarus

Details

Language :
English
ISSN :
00191035 and 10902643
Database :
OpenAIRE
Journal :
Icarus, Icarus, Elsevier, 2016, 267, pp.334-343. ⟨10.1016/j.icarus.2015.12.007⟩
Accession number :
edsair.doi.dedup.....272b526d1c768579e5d508a6291207f7
Full Text :
https://doi.org/10.1016/j.icarus.2015.12.007⟩