Three-dimensional time-dependent convection model for asteroseismology - I. Mathematical model

Open Access

Fig. 1.

Horizontal cut of the CO⁵BOLD 3D simulation box below the photosphere of the normalized temperature. Blue shades correspond to downflows while orange shades identify upflows. The snapshot shown here corresponds to a high-resolution simulation of the Sun performed with CO⁵BOLD (Grid nodes: 534 × 534 × 424).

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