3D anelastic simulations find that both convective zone Busse columns and weather-layer PV homogenization produce Jupiter-like jets, with the weather layer causing deviations in thermal wind balance and long-term high-latitude jet migration.
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Early Venus experienced large seasonal and latitudinal insolation redistribution but only modest orbit-averaged flux changes, making atmospheric opacity the dominant control on surface temperature rather than orbital forcing.
citing papers explorer
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Superrotation and Jet Migration in Simulations of Jupiter's Convective Zone and Weather Layer
3D anelastic simulations find that both convective zone Busse columns and weather-layer PV homogenization produce Jupiter-like jets, with the weather layer causing deviations in thermal wind balance and long-term high-latitude jet migration.
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Seasonal Insolation Variability on Early Venus: Implications for Energy Budget
Early Venus experienced large seasonal and latitudinal insolation redistribution but only modest orbit-averaged flux changes, making atmospheric opacity the dominant control on surface temperature rather than orbital forcing.