The paper deals with a coupled model of the upper atmosphere and ionosphere of Titan. The neutral atmosphere is described by a comprehensive photochemical model for 30 โข solar zenith angle with molecular and turbulent diffusive transport taken into account. At the upper boundary (1430 km) escaping f
A model of Triton's atmosphere and ionosphere
โ Scribed by E. Lellouch; M. Blanc; J. Oukbir; P.-Y. Longaretti
- Publisher
- Elsevier Science
- Year
- 1992
- Tongue
- English
- Weight
- 548 KB
- Volume
- 12
- Category
- Article
- ISSN
- 0273-1177
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
The atmospheric structure of Triton in the altitude range 25-150 km shows an unexpectedly steep thermal gradient of 0.26 K km -1 above 50 km altitude, with a nearly isothermal profile below. The upper part of the profile can be explained by downward conduction of heat deposited by magnetospheric ele
## I. INTRODUCTION We present an updated model for the photochemistry of Io's The structure of Io's SO 2 atmosphere has long been a atmosphere and ionosphere and use this model to investigate the sensitivity of the chemical structure to vertical transport subject of considerable debate, especiall