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Radiative-dynamical Model of Jupiter’s Quasi-quadrennial Oscillation

We present a simulation of Jupiter’s quasi-quadrennial oscillation (QQO) in a 2D radiative-dynamical model. Launching an eastward Kelvin wave and a westward Rossby-gravity wave in the lower boundary, we successfully generate a 4 yr-period oscillation in the equatorial stratosphere. The momentum flux...

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Hoofdauteurs: Jialin Zhang, Tao Li, Xi Zhang, Cheng Li, Yihuan Tang, Xiankang Dou
Formaat: Artigo
Taal:Inglês
Gepubliceerd in: IOP Publishing 2024-01-01
Reeks:The Astrophysical Journal
Onderwerpen:
Jupiter
Atmospheric circulation
Planetary atmospheres
Planetary science
Planetary dynamics
Solar system gas giant planets
Online toegang:https://doi.org/10.3847/1538-4357/ad47a0
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