Table 2
Global parameters for the runs presented in this paper.
Label | dim | r0 | β/ 5 | k | Σ0 | Sect. | |
|
|||||||
R1-P4 | 2 | 1 | 104 | 6 | 500 | 4.4.4 | |
R1-P4-C4 | 2 | 1 | 104 | 4 | 500 | 4.4 | |
R1-P3 | 2 | 1 | 103 | 6 | 500 | 4.2, 4.6.1 | |
R1-P2 | 2 | 1 | 102 | 6 | 500 | 4.5.3, 4.6.3 | |
R1-M3 | 2 | 1 | − 103 | 6 | 500 | 4.5 | |
|
|||||||
R10-P3 | 2 | 10 | 103 | 6 | 500 | 4.2 | |
R10-P2 | 2 | 10 | 102 | 6 | 500 | 4.6 | |
R10-M3 | 2 | 10 | − 103 | 6 | 500 | 4.3 | |
R10-M3-C2 | 2 | 10 | − 103 | 2 | 500 | 4.1 (fiducial) | |
|
|||||||
3D-R1-P4 | 3 | 1 | 104 | 6 | 500 | 4.2 | |
3D-R1-P3 | 3 | 1 | 103 | 6 | 500 | 4.6.1 | |
3D-R1-M4 | 3 | 1 | − 104 | 6 | 500 | 4.2 | |
3D-R10-P3 | 3 | 10 | 103 | 6 | 500 | 4.6.4 |
Notes. The table lists: name and dimension of the run, inner radius in astronomical units, initial plasma beta in the midplane (a minus sign corresponds to Ω·B< 0), ratio of corona over disk sound speed k (see Eq. (A.6)), mass surface density at 1 au in g cm-2, section where the run is discussed.
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