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Three-dimensional Modeling of Hot Jupiter Atmospheric Flows

  • Authors: Emily Rauscher and Kristen Menou

RAUSCHER & MENOU 2010 The Astrophysical Journal 714 1334.

  • Provider: AAS Journals

Caption: Figure 3.

Zonal average of the zonal wind in m s −1, as a function of latitude and depth in the atmosphere. Yellow lines separate regions of positive (eastward) flow and negative (westward) flow. A strong super-rotating equatorial jet descends through much of the atmosphere. At the equator the maximum (eastward) zonal-average wind speed occurs where the radiative and advective timescales are comparable. Deep in the atmosphere, the minimum (peak westward) zonal-average wind speed occurs at the transition between radiatively forced and inert layers.

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