Table 1.
Summary of the numerical simulations performed for Sect. 1.
| Simulation # | Driver | Height cor. | B | Ampl | τR | Power peak |
|---|---|---|---|---|---|---|
| (Mm) | (G) | (m s−1) | (s) | (s) | ||
| 3.1.1 | Monochromatic | 2.0 | 0 | 10−3 | ∞ | 300.0 |
| 3.1.2 | Monochromatic | – | 0 | 10−3 | ∞ | 300.0 |
Notes. The first column indicates the number used to label the numerical simulation, the second column (Driver) is the kind of driver used at the bottom boundary (“Monochromatic” for a monochromatic acoustic wave and “Broadband” for a broadband wavelet, in both cases with the power peak at a period of 300 s), the third column (Height cor.) is the height of the bottom of the corona (a dash indicates that there is neither transition region nor corona), the fourth column (B) is the strength of the vertical magnetic field, the fifth column (Ampl) is the amplitude of the wave at the photosphere (z = 0 Mm), the sixth column (τR) is the radiative cooling time, and the last column (Power peak) is the period of the maximum chromospheric power in the vertical velocity.
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