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A three-dimensional model of moist convection for the giant planets II: Saturn's water and ammonia moist convective storms

✍ Scribed by Ricardo Hueso; Agustín Sánchez-Lavega


Book ID
108138561
Publisher
Elsevier Science
Year
2004
Tongue
English
Weight
869 KB
Volume
172
Category
Article
ISSN
0019-1035

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A Three-Dimensional Model of Moist Conve
✍ Ricardo Hueso; Agustı́n Sánchez-Lavega 📂 Article 📅 2001 🏛 Elsevier Science 🌐 English ⚖ 424 KB

We present a three-dimensional cloud model designed for the study of formation and evolution of moist convective storms on the giant planets. This is a finite-difference model that solves the dynamic and thermodynamic equations forward in time under the anelastic approximation including microphysics