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===Principal Governing Equations=== Quoting from [Ref01] … Among the [[PGE#Principal_Governing_Equations|principal governing equations]] we have included the ''inertial-frame'', <div align="center"> <span id="ConservingMomentum:Lagrangian"><font color="#770000">'''Lagrangian Representation'''</font></span><br /> of the Euler Equation, {{Math/EQ_Euler01}} [<b>[[Appendix/References#EFE|<font color="red">EFE</font>]]</b>], Chap. 2, §11, p. 20, Eq. (38)<br /> [<b>[[Appendix/References#BLRY07|<font color="red">BLRY07</font>]]</b>], p. 13, Eq. (1.55) </div> Shifting into a rotating frame characterized by the angular velocity vector, <div align="center"> <math>~\vec{\Omega}_f \equiv \hat\mathbf{k} \Omega_f \, ,</math> </div> and applying the operations that are specified in the first few subsections of [Ref02], we recognize the following relationships … <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\vec{v}_\mathrm{inertial}</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\vec{v}_\mathrm{rot} + {\vec\Omega}_f \times \vec{x} \, ,</math> </td> </tr> <tr> <td align="right"> <math>~\biggl[ \frac{d \vec{v}}{dt} \biggr]_\mathrm{inertial}</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \biggl[ \frac{d \vec{v}}{dt} \biggr]_\mathrm{rot} + 2{\vec\Omega}_f \times {\vec{v}}_\mathrm{rot} + {\vec\Omega}_f \times ({\vec\Omega}_f \times \vec{x}) </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \biggl[ \frac{d \vec{v}}{dt} \biggr]_\mathrm{rot} + 2{\vec\Omega}_f \times {\vec{v}}_\mathrm{rot} - \frac{1}{2} \nabla | {\vec\Omega}_f \times \vec{x}|^2 </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \biggl[ \frac{\partial \vec{v}}{\partial t} \biggr]_\mathrm{rot} + ({\vec{v}}_\mathrm{rot} \cdot \nabla){\vec{v}}_\mathrm{rot} + 2{\vec\Omega}_f \times {\vec{v}}_\mathrm{rot} - \frac{1}{2} \nabla | {\vec\Omega}_f \times \vec{x}|^2 \, .</math> </td> </tr> </table> Making this substitution on the left-hand-side of the above-specified "<font color="maroon">Lagrangian Representation</font> of the Euler Equation," we obtain what we have referred to [[PGE/RotatingFrame#Euler_Equation_.28rotating_frame.29|also in [Ref02]]] as the, <div align="center"> <font color="#770000">'''Eulerian Representation'''</font><br /> of the Euler Equation <br /> <font color="#770000">'''as viewed from a Rotating Reference Frame'''</font> <math>\biggl[\frac{\partial\vec{v}}{\partial t}\biggr]_\mathrm{rot} + ({\vec{v}}_\mathrm{rot}\cdot \nabla) {\vec{v}}_\mathrm{rot}= - \frac{1}{\rho} \nabla P - \nabla \biggl[\Phi - \frac{1}{2}|{\vec{\Omega}}_f \times \vec{x}|^2 \biggr] - 2{\vec{\Omega}}_f \times {\vec{v}}_\mathrm{rot} \, .</math> </div> This form of the Euler equation also appears early in [Ref05], where we set up a discussion of the paper by [http://adsabs.harvard.edu/abs/1996ApJS..105..181K Korycansky & Papaloizou] (1996, ApJS, 105, 181; hereafter KP96). But, for now, let's back up a couple of steps and retain the ''total'' time derivative on the left-hand-side. That is, let's select as the foundation expression the, <div align="center"> <font color="#770000">'''Lagrangian Representation'''</font><br /> of the Euler Equation <br /> <font color="#770000">'''as viewed from a Rotating Reference Frame'''</font> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\biggl[ \frac{d \vec{v}}{dt} \biggr]_\mathrm{rot} </math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~- \frac{1}{\rho} \nabla P - \nabla \Phi - 2{\vec\Omega}_f \times {\vec{v}}_\mathrm{rot} - {\vec\Omega}_f \times ({\vec\Omega}_f \times \vec{x}) \, ,</math> </td> </tr> <tr><td align="center" colspan="3"> [<b>[[Appendix/References#EFE|<font color="red">EFE</font>]]</b>], Chap. 2, §12, p. 25, Eq. (62) </td> </tr> </table> </div> which also serves as the foundation of most of our [Ref03] discussions.
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