Table 1.
Boundaries for the integration of the power spectral density.
| νinf(n, ℓ) | νsup(n, ℓ) | |
|---|---|---|
| ℓ = 0 | (νn, 0 + νn − 1, 2)/2 | (3 νn − 1, 3 + νn, 0)/4 |
| ℓ = 3 | (3 νn − 1, 3 + νn, 0)/4 | (7 νn − 1, 3 − νn, 0)/6 |
| ℓ = 1 | (7 νn − 1, 3 − νn, 0)/6 | (4 νn − 1, 2 − νn, 0)/3 |
| ℓ = 2 | (4 νn − 1, 2 − νn, 0)/3 | (νn, 0 + νn − 1, 2)/2 |
Notes. The boundaries are equivalent to the mid-point between consecutive modes, except when ℓ = 1 and ℓ = 3 modes are involved. This is illustrated in Fig. 2. The boundary between the ℓ = 1 and the ℓ = 3 modes is chosen close to the ℓ = 3 mode frequency. We made this choice to avoid any confusion between a ℓ = 3 mode and the neighbouring dipole mixed-modes because the dipole mixed-modes extend up to the ℓ = 3 modes.
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