Two-dimensional simulations of solar-like models with artificially enhanced luminosity - I. Impact on convective penetration

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Table 2.

Summary of the 2D simulations.

Model	L/L_star	τ_conv^(a) (s)	N_conv^(b)	t_steady^(c) (s)	t_sim^(d) (s)
ref	1	8 × 10⁵	565	1.3 × 10⁸	6.1 × 10⁸
boost1d1	10¹	3.6 × 10⁵	375	3 × 10⁷	1.72 × 10⁸
boost1d2	10²	1.7 × 10⁵	450	2.44 × 10⁷	9.9 × 10⁷
boost1d4	10⁴	3.5 × 10⁴	530	1.5 × 10⁶	2 × 10⁷

Notes.

^(a)

Convective turnover time. See Sect. 3.1 for its definition.

^(b)

Number of convective turnover times covered by the simulation once steady state convection is reached.

^(c)

Physical time to reach a steady state for convection.

^(d)

Total physical runtime of the simulation.

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