A Three-Dimensional Model of Moist Conve
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Ricardo Hueso; AgustΔ±́n SΓ‘nchez-Lavega
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Article
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2001
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Elsevier Science
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English
β 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