The general circulation of Titan's lower and middle atmosphere

S. Lebonnois; F. M. Flasar; T. Tokano; C. E. Newman

doi:10.1017/CBO9780511667398.007

4 - The general circulation of Titan's lower and middle atmosphere

Published online by Cambridge University Press: 05 January 2014

T. Tokano and

Edited by

Caitlin A. Griffith ,

Emmanuel Lellouch and

Thomas E. Cravens

Show author details

S. Lebonnois: Affiliation:
Lawrence Livermore National Laboratory
F. M. Flasar: Affiliation:
NASA/Goddard Space Flight Center
T. Tokano: Affiliation:
Universität Zu Köln
C. E. Newman: Affiliation:
Ashima Research
Ingo Müller-Wodarg: Affiliation:
Imperial College London
Caitlin A. Griffith: Affiliation:
University of Arizona
Emmanuel Lellouch: Affiliation:
Observatoire de Paris, Meudon
Thomas E. Cravens: Affiliation:
University of Kansas

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Summary

4.1 Introduction

The atmosphere of Titan shares a specific circulation feature with the atmosphere of Venus, the so-called superrotation. Most of the middle and lower atmosphere rotates significantly faster than the underlying solid body, with maximum zonal winds in the winter stratosphere of ~200 m/s. This chapter focuses on this dominant feature, through discussions of all aspects of Titan's atmospheric dynamics. In such a complex system, interactions are strong among atmospheric circulation, temperature structure, composition of the atmosphere, and clouds and haze distributions. Therefore, close links are made with other chapters of this book: Chapter 3 for temperature structure, Chapter 5 for composition, and Chapters 6 and 8 for clouds and haze distributions.

The altitude region covered by this chapter goes from the surface to the detached haze layer, a peculiar feature located at the top of the haze completely covering Titan (see Chapter 8), at an altitude of roughly 500 km. This region includes the troposphere, the stratosphere, and the lower mesosphere (see Chapter 3). The troposphere goes from the surface up to ~40 km (the tropopause), where the coldest temperatures are found on Titan. In this region, the atmospheric system includes the cycle of methane, presenting features similar to the hydrological system in the Earth atmosphere (see Chapters 5 and 6). The stratosphere goes from the tropopause to the stratopause, where temperatures peak, located at altitudes around 250 to 300 km (around 0.1 mbar).

Type: Chapter
Information: Titan
Interior, Surface, Atmosphere, and Space Environment
, pp. 122 - 157

DOI: https://doi.org/10.1017/CBO9780511667398.007 [Opens in a new window]

Publisher: Cambridge University Press

Print publication year: 2014

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