Table 2
Approximate values of the scalar k3D∕1D for discrete values of αvisc.
| αvisc | k3D∕1D |
|---|---|
| 0.01 | 1.5 |
| 0.001 | 2 |
| 0.0005 | 2.5 |
| 0.0001 | 5 |
Notes. This scalar tells us that for a specific value of αvisc, say 0.01, the planetary mass required to obtain a zero pressure gradient in our 1D simulations is 1.5 times lower than the mass obtained using the equation from Bitsch et al. (2018), which was obtained using 3D simulations.
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