Exploring deep and hot adiabats as a potential solution to the radius inflation problem in brown dwarfs - Long-timescale models of the deep atmospheres of KELT-1b, Kepler-13Ab, and SDSS1411B

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Fig. 11

Temporally and zonally averaged, over a period of ~3 yr, profiles of the zonal wind at 0.1 and 1 bar for deep horizontal convergence pressure models of Kepler-13Ab (green), KELT-1b (blue), and SDSS1411B (red). Here, easterly zonal winds are positive and westerly zonal winds are negative.

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