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

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Table A.1:

Convergence of the eigenvalues and eigenvectors of the slowest decaying poloidal and toroidal modes $^{\rm a}$ .
N	$E(\lambda)~[A]$	$E(\vec{B})~[A]$	$E(\lambda)~[B]$	$E(\vec{B})~[B]$
3	1.08e-7	3.98e-9	3.83e-5	6.849e-4
4	5.651e-11	1.255e-12	9.984e-8	4.365e-9
5	9.68e-14	2.142e-16	1.207e-10	2.497e-12
6	7.72e-14	2.136e-20	8.707e-14	9.068e-16
7	1.38e-14	1.325e-24	1.77e-14	4.80e-19
8	1.90e-14	4.427e-29	5.32e-15	6.263e-23

$^{\rm a}$ N is the number of modes in the radial basis, and $E(\lambda) [A]$ and $E(\vec{B}) [A]$ are the errors of eigenvalue and eigenvector for the poloidal mode and $E(\lambda) [B]$ and $E(\vec{B}) [B]$ the corresponding errors for the toroidal mode.

Source LaTeX | All tables | In the text

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