Energy and Mass Conservation
The thermodynamic equation illustrates how energy is conserved in the atmosphere, detailing the contributions from pressure, gravity, and heat transfer. Unlike the Navier-Stokes equations, it emphasizes energy transfer rather than momentum. Additionally, the continuity equation reinforces the principle of mass conservation, asserting that changes in air density correspond to the movement of air in and out of a region.In this clip
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The Science of Everything Podcast
Episode 143: Climate Modelling
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