Fig. 9

Upper panels: heat transport for a 1.1
M⊙ star
(Z = Z⊙) at three different epochs
indicated in each panel with the terms non-stationary
(; magenta solid
line), barotropic (
; blue dashed
line), baroclinic (
; red dotted
line), and advective (
; black long
dashed line), and the contribution due to nuclear and gravitational energy
variations (
;
green dashed-dotted line). Lower panels: similar to the upper panel
with a zoom on the small amplitude components. Hatched areas indicate the convective
envelope.
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