Matteo Cantiello edited Gradients.tex  over 9 years ago

Commit id: 33961bd8d62c3db374cb79f2bcab3dcf3b0cebc5

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F = F_{c} + F_{r} \equiv \frac{4ac}{3}\frac{T^4}{\kappa \rho}\frac{\nabla_r}{\hp}.  \end{equation}  In a stellar convection zone where no energy is produced by nuclear reactions, the following hierarchy holds: $\nabla_r > \nabla > \nabla' > \gradad$ \adgrad$