Table 2
Possible scaling for the simulations.
| β | L 0 | t 0 | B 0 | P 0 | ρ 0 | T 0 | V 0 | c A | c S | E 0 | Solar layer |
|
|
|||||||||||
| 1.0 | 0.05 | 1.1 | 3 | 0.04 | 4.4 × 10-10 | 104 | 45 | 12 | 11 | 1.1 × 1014 | Chromosphere |
| 0.25 | 0.8 | 1.4 | 3.2 | 0.01 | 3.1 × 10-12 | 4.0 × 105 | 574 | 162 | 74 | 5.2 × 1017 | Transition Region |
| 0.025 | 5 | 1.7 | 5 | 0.0025 | 3.0 × 10-13 | 106 | 2873 | 810 | 117 | 3.1 × 1020 | Corona |
| 0.0025 | 25 | 1.9 | 10 | 10-3 | 6.1 × 10-14 | 2.0 × 106 | 1.3 × 104 | 3624 | 165 | 1.6 × 1023 | Corona |
Notes. Columns: characteristic length L0 (in Mm), time t0 (in s), volume magnetic field B0 (in G), pressure P0 (in Pa), density ρ0 (in kg m-3), temperature T0 (in K), velocity V0 (in km s-1), Alfvén speed cA (in km s-1), sound speed cS (in km s-1), and energy E0 (in J). The last column suggests an equivalence with different layers of the solar atmosphere.
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