... | ... | @@ -46,12 +46,6 @@ $`Q^+ = 2\rho \nu (D_{RR}^2+D_{\varphi \varphi}^2+D_{\theta \theta}^2 |
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We will consider in the following the heating from the central star.
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%## How we derive the equation for the internal energy
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%The equation for the internal energy is obtained from Navier-Stokes equations.
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%In many codes (mainly the ones using Rieman Solvers) the energy is treated as %the sum of kinetic plus internal energy. In the attached file we provide the %derivation of the equation for the internal energy plus some comments about %codes
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%like Jupiter [eneequa2.pdf](uploads/3f4341806d874fb2f3808712dc785418/eneequa2.pdf)
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## The contribution of the Stellar heating
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