Effect of multi-dust species on the inner rim of magnetized protoplanetary disks

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Table 2

Setup parameters for the disk models.

Stellar parameters	T_* = 8500K, R_∗ = 2.12R_⊙ M_∗ = 2.0 M_⊙
Opacity for dust species s	κ^s (λ) see Fig. 1 κ_gas = 10⁻⁶ cm²/g
N_r × N_θ	2304 x 216
R_in - R_out : Z/R	0.1-100 au : ~ ± 0.3
Ionization transition	T_MRI = 900 K
Sublimation temperature range	T_Δ = 100 K or 50 K
α viscosity	α_MRI> = 10⁻¹ for ^T > ^T_MRI α_DZ = 10⁻³ for T ≤ T_MRI
α-transition temperature range	$T_{Δ}^{α} = 100$ $T^\alpha_\Delta = 100$ K
Dust-to-gas mass ratio	see Table 1
Mass accretion rate	Ṁ = 1.0 × 10⁻⁸ M_⊙/yr

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