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Table 1

List of runs discussed in this paper.

Simulation R 0 Ohmic Hall Ambipolar β 0 α Ṁ outflow
1-O-5 1 au × 105 2.5 × 10-3 1.3 × 10-4 N/A
1-OH-5 1 au × × 105 4.5 × 10-1 2.0 × 10-2 N/A
1-OA-5 1 au × × 105 5.9 × 10-4 5.8 × 10-5 1.5 × 10-4
1-OHA-5 1 au × × × 105 5.0 × 10-2 1.4 × 10-3 6.5 × 10-4
1-OHA-mB 1 au × × × −105 3.9 × 10-4 3.8 × 10-5 N/A
1-OHA-znf 1 au × × × ∞ 5.4 × 10-6 1.7 × 10-7 N/A
1-OA-5-e 1 au × × 105 4.7 × 10-4 4.6 × 10-5 1.3 × 10-4
1-O-3 1 au × 103 2.4 × 10-1 9.3 × 10-3 1.6 × 10-2
1-OH-3 1 au × × 103 1.5 9.7 × 10-2 4.7 × 10-2
1-OA-3 1 au × × 103 2.4 × 10-2 8.4 × 10-4 4.3 × 10-3
1-OHA-3 1 au × × × 103 3.1 × 10-1 5.5 × 10-3 1.2 × 10-2
5-OHA-5 5 au × × × 105 2.3 × 10-2 4.6 × 10-4 4.0 × 10-4
10-OA-5 10 au × × 105 1.3 × 10-3 1.3 × 10-4 2.5 × 10-4
10-OHA-5 10 au × × × 105 1.0 × 10-2 2.4 × 10-4 3.5 × 10-4
10-OA-gr 10 au × × 105 7.8 × 10-4 8.7 × 10-5 1.7 × 10-4
10-OHA-gr 10 au × × × 105 2.4 × 10-3 8.7 × 10-5 1.9 × 10-4

Notes. Each simulation is of a stratified shearing box of size 4 × 8 × 12 located a radial distance R0 from the central protostellar object. The plasma β0 is given in the initial state (see Eq. (5)). The effective (radial) transport parameter α, the mass-loss rate due to outflows Ṁoutflow, and the (dimensionless) surface magnetic stress are defined by Eqs. (8)–(10), respectively.

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