A conservative orbital advection scheme for simulations of magnetized shear flows with the PLUTO code

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Table 2

Growth rates of the linear MRI mode.

N_z/mode	γ^MRI (std 2nd)	γ^MRI (Fargo 2nd)	γ^MRI (Fargo 3rd)

16	0.70	0.71	0.74
8	0.57	0.59	0.69
4	0.00	0.14	0.14

Notes. The first column gives the resolution per wavelength, while Cols. 2 to 4 show, respectively, the MRI growth rates obtained using the standard scheme, FARGO-MHD with linear reconstruction (Eq. (29)) and FARGO-MHD with parabolic reconstruction (PPM, Eq. (30)).

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