MHD Energy Equation: Comparing Formats

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SUMMARY

The forum discussion centers on the MHD energy equation, specifically comparing two formats: the first format presented as \(\frac{\rho^\gamma}{\gamma-1}\frac{D}{Dt}\left(\frac{p}{\rho^\gamma}\right)=-L\) and the second as \(\frac{dp}{dt}+\gamma p\nabla\cdot\mathbf{v}=-L\). The participants clarify that the second equation applies when density (\(\rho\)) is constant, while the first format accommodates variable density. The discussion emphasizes the importance of understanding the implications of the convective time derivative (\(D/Dt\)) in the context of MHD equations.

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MasterD
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Is this the right format of the energy equation (equation 2.10)?

http://www-solar.mcs.st-and.ac.uk/~alan/sun_course/Chapter2/node3.html#energy

<br /> \frac{\rho^\gamma}{\gamma-1}\frac{D}{Dt}\left(\frac{p}{\rho^\gamma}\right)=-L<br />

I know it in a different format:

<br /> \frac{dp}{dt}+\gamma p\nabla\cdot\mathbf{v}=-L<br />

Where is the difference coming from?
 
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Hi MasterD! :smile:

Isn't your second equation the case for ρ = constant (and with D/Dt being the convective time derivative, ∂/∂t + v.)?
 
tiny-tim said:
Hi MasterD! :smile:

Isn't your second equation the case for ρ = constant (and with D/Dt being the convective time derivative, ∂/∂t + v.)?

Thanks for your reply Tim. \rho is not constant, however.. D/Dt is indeed the convective time derivative.
 

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