Oscillations of red giant stars with magnetic damping in the core - I. Dissipation of mode energy in dipole-like magnetic fields

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Table 2.

Initialization parameters of the ray tracing analysis for the various stellar models.

Model	r₀/R_*	r_f/R_*	$t_{int} / ω_{dyn}^{- 1}$ $t_{\mathrm{int}}/\omega_{\mathrm{dyn}}^{-1}$
1A	0.06	0.024	50
1B	0.02	0.011	200
1C	0.0021	0.0016	2000

1a	0.06	0.024	50
1b	0.02	0.011	200

2A	0.04	0.016	100
2B	0.01	0.0055	400
2C	0.0021	0.0016	2000

2a	0.04	0.016	100
2b	0.01	0.0055	400

Notes. The meaning of the parameters is described in the main text (see Sects. 2.2 and 2.4).

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