MČ, June 2023: Atlas2 results for density and poloidal momentum in PLUTO simulations
of star-disk magnetospheric interactions in different points in the parameter
space. Collaborations with Ruchi Mishra (CAMK) (results with alpha_v<1),
and Aleksandra Kotek (Uni
Warsaw, NCAC) (results in a complete meridional plane, without disk
mid-plane boundary). Magnetic field strengths in the table are for YSOs
(T Tauri stars). If rescaled to white dwarfs, results are of the order of up
to million (1e6) Gauss, and if rescaled to neutron stars, of the
order of 100 million (1e8) Gauss.
  |
alphav |
0.2 |
0.2 |
0.2 |
0.2 |
0.4 |
0.4 |
0.4 |
0.4 |
1 |
1 |
1 |
1 |
alpham |
0.1 |
0.4 |
0.7 |
1 |
0.1 |
0.4 |
0.7 |
1 |
0.1 |
0.4 |
0.7 |
1 |
Pm |
1.33 |
0.33 |
0.19 |
0.13 |
2.67 |
0.67 |
0.38 |
0.63 |
6.67 |
1.67 |
0.95 |
0.67 |
B*=250 Gauss |
Omega* |
|
0.05 |
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  |
0.1 |
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  |
0.15 |
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0.2 |
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0.4 |
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0.5 |
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  |
0.8 |
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  |
  |
alphav |
0.2 |
0.2 |
0.2 |
0.2 |
0.4 |
0.4 |
0.4 |
0.4 |
1 |
1 |
1 |
1 |
alpham |
0.1 |
0.4 |
0.7 |
1 |
0.1 |
0.4 |
0.7 |
1 |
0.1 |
0.4 |
0.7 |
1 |
Pm |
1.33 |
0.33 |
0.19 |
0.13 |
2.67 |
0.67 |
0.38 |
0.63 |
6.67 |
1.67 |
0.95 |
0.67 |
B*=500 Gauss |
Omega* |
|
0.05 |
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  |
0.1 |
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  |
0.15 |
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  |
0.2 |
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  |
0.4 |
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  |
0.5 |
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  |
0.8 |
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  |
alphav |
0.2 |
0.2 |
0.2 |
0.2 |
0.4 |
0.4 |
0.4 |
0.4 |
1 |
1 |
1 |
1 |
alpham |
0.1 |
0.4 |
0.7 |
1 |
0.1 |
0.4 |
0.7 |
1 |
0.1 |
0.4 |
0.7 |
1 |
Pm |
1.33 |
0.33 |
0.19 |
0.13 |
2.67 |
0.67 |
0.38 |
0.63 |
6.67 |
1.67 |
0.95 |
0.67 |
B*=750 Gauss |
Omega* |
|
0.05 |
|
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  |
0.1 |
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  |
0.15 |
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  |
0.2 |
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  |
0.4 |
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  |
0.5 |
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  |
0.8 |
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  |
  |
alphav |
0.2 |
0.2 |
0.2 |
0.2 |
0.4 |
0.4 |
0.4 |
0.4 |
1 |
1 |
1 |
1 |
alpham |
0.1 |
0.4 |
0.7 |
1 |
0.1 |
0.4 |
0.7 |
1 |
0.1 |
0.4 |
0.7 |
1 |
Pm |
1.33 |
0.33 |
0.19 |
0.13 |
2.67 |
0.67 |
0.38 |
0.63 |
6.67 |
1.67 |
0.95 |
0.67 |
B*=1000 Gauss |
Omega* |
|
0.05 |
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  |
0.1 |
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  |
0.15 |
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  |
0.2 |
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  |
0.4 |
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  |
0.5 |
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0.8 |
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