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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 6.

Contours of horizontal flow convergence (in lavender) and divergence (in yellow) plotted over the temperature (in K) and wind map at the 150 mbar pressure level. The convergence/divergence contour levels are set at ±1 × 10 −4, 1.5 × 10 −4, 2 × 10 −4, and 2.5 × 10 −4 s −1. Clearly, the bulk of the flow has |∇ · v| < 1 × 10 −4 s −1. The narrow region of strong convergence around longitude +135° is what we refer to as a shock-like feature. An increase in temperature around longitude +135° seen in the bottom panel of Figure  1, just one model level below the one shown here, is consistent with adiabatic heating by a downward flow associated with this shock-like feature.

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