Turbulence destroys thermal lobes around Mars-sized planetary embryos

Open Access

Fig. 1

Perturbation of density arising from heat release obtained by subtracting a hot run (L = L_c) and a cold run (L = 0) for the case ß = 50 at t = 1 orbit. The perturbation was integrated over colatitude and normalized to $γ (γ - 1) L / χ c_{s}^{2}$ $Mathematical equation: $\gamma \left( {\gamma - 1} \right)L/\chi c_s^2$$ . The solid purple line indicates the corotation radius.

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