An advective solar-type dynamo without the effect | Astronomy & Astrophysics (A&A)

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Table A.2:

Test case B of Jouve et al. (2008) $^{\rm a}$ .
Resolution	$C_{\alpha}^{{\rm crit}}$	$\omega$
$8\times8$	0.443	180.5
$10\times10$	0.4175	175.1
$12\times12$	0.4095	172.2
$13\times13$	0.411	172.4
$14\times14$	0.4122	172.7
$16 \times 16$	0.4125	172.9

$^{\rm a}$ Critical values of the dynamo number, $C_{\alpha}^{{\rm crit}}$ , and the oscillation frequency at the dynamo onset, $\omega$ , for different radial and latitudinal spectral resolutions. $\omega$ is measured in units of the inverse magnetic diffusion time.

Source LaTeX | All tables | In the text

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