All Tables

Table 1: Maximum scaled growth-rate $\zeta _{\rm I}^{\rm max}=2 \Omega \sigma _{\rm I}/\omega _a^2$ and corresponding frequency $\zeta _{\rm R}^{\rm max}=2 \Omega \sigma _{\rm R}/\omega _a^2$ , A^* and S, at given $\varepsilon A_t/A_\mu$ and for |m|=1.
Table 2: Stratification parameters and optimal conditions for the onset of instability. $A^*_{\rm max}$ is the highest value of $A^*=\varepsilon A_t+ A_\mu$ that allows for instability; $[AS]_{\rm max}$ the maximum of the product A^*S(A^*) for fixed $\varepsilon A_t/A_\mu$ , obtained at $A^*_{\rm opt}$ , from which one derives the instability threshold for the magnetic field (see text).
Table 3: Typical values of the relevant parameters in the upper radiation zone of the Sun, and values adopted for the numerical simulations (in cgs units).