Table C.1.
Summary of the fastest parasitic modes for different initial amplitudes of the MRI modes and parasitic velocities.
NAME | B0[10−4] | v0[10−4] | q |
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θini [° ] |
![]() |
θsat [° ] | tsat [Orbits] | 𝒜 |
b0vl-dvl | 1 | 0.1 | 1.5 | 4.25 | 177.64 | 0.65 | 15.70 | 2.954 | 55.63 |
b0vl-dl | 1 | 0.5 | 1.5 | 4.50 | 177.61 | 0.70 | 15.57 | 2.927 | 48.93 |
b0vl-dm | 1 | 1 | 1.5 | 4.50 | 177.61 | 0.68 | 16.07 | 2.915 | 46.15 |
b0vl-dh | 1 | 5 | 1.5 | 4.75 | 177.59 | 0.72 | 16.25 | 2.884 | 39.93 |
b0vl-dvh | 1 | 10 | 1.5 | 4.75 | 177.59 | 0.69 | 16.90 | 2.869 | 37.24 |
b0l-dvl | 5 | 0.1 | 1.5 | 4.88 | 177.36 | 0.70 | 18.69 | 2.613 | 55.54 |
b0l-dl | 5 | 0.5 | 1.5 | 3.88 | 177.23 | 0.72 | 15.06 | 2.587 | 49.26 |
b0l-dm | 5 | 1 | 1.5 | 3.88 | 177.23 | 0.70 | 15.57 | 2.574 | 46.22 |
b0l-dh | 5 | 5 | 1.5 | 4.13 | 177.22 | 0.70 | 16.74 | 2.541 | 39.69 |
b0l-dvh | 5 | 10 | 1.5 | 4.38 | 177.22 | 0.72 | 17.22 | 2.527 | 37.10 |
b0m-dvl | 10 | 0.1 | 1.5 | 4.51 | 177.14 | 0.75 | 17.43 | 2.460 | 54.15 |
b0m-dl | 10 | 0.5 | 1.5 | 4.76 | 177.14 | 0.74 | 18.73 | 2.435 | 48.14 |
b0m-dm | 10 | 1 | 1.5 | 4.76 | 177.14 | 0.72 | 19.35 | 2.424 | 45.74 |
b0m-dh | 10 | 5 | 1.5 | 3.88 | 177.05 | 0.67 | 17.35 | 2.395 | 39.91 |
b0m-dvh | 10 | 10 | 1.5 | 3.88 | 177.05 | 0.65 | 18.00 | 2.382 | 37.56 |
b0h-dvl | 50 | 0.1 | 1.5 | 4.01 | 176.60 | 0.78 | 17.69 | 2.120 | 54.44 |
b0h-dl | 50 | 0.5 | 1.5 | 4.01 | 176.60 | 0.73 | 19.05 | 2.094 | 48.32 |
b0h-dm | 50 | 1 | 1.5 | 4.01 | 176.60 | 0.71 | 19.66 | 2.084 | 46.02 |
b0h-dh | 50 | 5 | 1.5 | 3.01 | 176.42 | 0.66 | 16.59 | 2.054 | 39.94 |
b0h-dvh | 50 | 10 | 1.5 | 3.38 | 176.40 | 0.74 | 16.77 | 2.037 | 36.91 |
b0vh-dvl | 100 | 0.1 | 1.5 | 3.51 | 176.32 | 0.71 | 18.36 | 1.970 | 53.83 |
b0vh-dl | 100 | 0.5 | 1.5 | 3.63 | 176.25 | 0.77 | 17.94 | 1.947 | 48.32 |
b0vh-dm | 100 | 1 | 1.5 | 3.63 | 176.25 | 0.75 | 18.58 | 1.935 | 45.65 |
b0vh-dh | 100 | 5 | 1.5 | 3.13 | 176.11 | 0.72 | 17.06 | 1.906 | 39.79 |
b0vh-dvh | 100 | 10 | 1.5 | 3.13 | 176.11 | 0.70 | 17.75 | 1.892 | 37.22 |
Notes. Evolutions of the fastest PIs for different initial amplitudes of the MRI modes and the parasitic velocities. We depict, from left to right: the initial MRI magnetic field, B0; the initial parasitic velocity, v0; the shear parameter, q; the modulus and angle with respect to the radial direction of the initial wavevector, , that leads to saturation; its modulus and angle at saturation; the saturation time, and the amplification factor. The runs are labeled so that vl, l, m, h, vh after b0 (MRI amplitude) and d (parasitic amplitude) stand for “very low,” “low,” “mid,” “high” and “very high,” respectively.
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