Table 1.
64 star-disk magnetospheric interaction simulations in a setup detailed in Čemeljić (2019).
| αm= | 0.1 | 0.4 | 0.7 | 1 |
|---|---|---|---|---|
| Pm= | 6.7 | 1.67 | 0.95 | 0.67 |
| Ω⋆/Ωbr | ||||
| B⋆ = 250 G | ||||
| 0.05 | a1(DCE1) | a2(DC) | a3(DC) | a4(DC) |
| 0.1 | a5(DCE1) | a6(DC) | a7(DC) | a8(DC) |
| 0.15 | a9(DCE1) | a10(DC) | a11(DC) | a12(DC) |
| 0.2 | a13(DCE1) | a14(DC) | a15(DC) | a16(DC) |
| B⋆ = 500 G | ||||
| 0.05 | b1(DCE1) | b2(DC) | b3(DC) | b4(DC) |
| 0.1 | b5(DCE1) | b6(DC) | b7(DC) | b8(DC) |
| 0.15 | b9(DCE1) | b10(DC) | b11(DC) | b12(DC) |
| 0.2 | b13(DCE1) | b14(DC) | b15(DC) | b16(DC) |
| B⋆ = 750 G | ||||
| 0.05 | c1(DCE1) | c2(DC) | c3(DC) | c4(DC) |
| 0.1 | c5(DCE1) | c6(DC) | c7(DC) | c8(DC) |
| 0.15 | c9(DCE2) | c10(DC) | c11(DC) | c12(DC) |
| 0.2 | c13(DCE2) | c14(DC) | c15(DC) | c16(DC) |
| B⋆ = 1000 G | ||||
| 0.05 | d1(DCE1) | d2(DC) | d3(DC) | d4(DC) |
| 0.1 | d5(DCE1) | d6(DC) | d7(DC) | d8(DC) |
| 0.15 | d9(DCE2) | d10(D) | d11(D) | d12(D) |
| 0.2 | d13(DCE2) | d14(D) | d15(D) | d16(D) |
Notes. There are all together 64 runs with all the combinations of parameters as listed in the table. The magnetic Prandtl number 
is also listed – in all the cases the anomalous viscosity parameter is αv = 1. The four simulations shown in Fig. 1 are highlighted with boxed letters. Simulations in which 
are marked in bold. Annotated type of solution for each combination of parameters are shown in brackets, as illustrated in Fig. 1.
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