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====Hybrid Scheme==== In our ''hybrid scheme,'' we will continue to use <math>~\mathcal{L}_u</math> — that is, an advection operator that incorporates the rotating-frame velocity, <math>~\bold{u}</math> — but we will switch all other velocity references to the inertial-frame velocity, <math>~\bold{v}</math>, and its components. This will be done via the [[#Rotating_Frame|above-declared mapping]], <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\bold{u}</math> </td> <td align="center"> <math>~~\rightarrow~~</math> </td> <td align="left"> <math>~[\bold{v} - \bold{\hat{e}}_\varphi \varpi \Omega_f] \, ,</math> </td> </tr> </table> that is, <math>~u_\varpi ~\rightarrow~ v_\varpi</math>, <math>~u_z ~\rightarrow~ v_z</math>, and <math>~u_\varphi ~\rightarrow~ (v_\varphi - \varpi \Omega_f)</math>. The Euler equation becomes, <table border="0" cellpadding="5" align="center"> <tr> <td align="right" colspan="1"> <math>~\frac{\partial [\bold{v} - \bold{\hat{e}}_\varphi \varpi \Omega_f]}{\partial t} + \bold{\hat{e}}_\varpi \biggl[ \mathcal{L}_u v_\varpi \biggr] + \bold{\hat{e}}_\varphi \biggl[ \mathcal{L}_u (v_\varphi - \varpi \Omega_f)\biggr] + \bold{\hat{e}}_z \biggl[ \mathcal{L}_u v_z \biggr] </math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \bold{a} + \bold{\hat{e}}_\varpi \biggl[ \frac{v_\varphi^2}{\varpi} \biggr] - \bold{\hat{e}}_\varphi \biggl[ \varpi \Omega_f + v_\varphi \biggr] \frac{v_\varpi}{\varpi} \, , </math> </td> </tr> </table> where we recognize that, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\mathcal{L}_u v_i</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~(\bold{u}\cdot \bold\nabla) v_i \, .</math> </td> </tr> </table> Now, given that, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\frac{\partial}{\partial t} \biggl[ \bold{\hat{e}}_\varphi \varpi \Omega_f \biggr]</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~0 \, ,</math> </td> </tr> </table> and, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\mathcal{L}_u (\varpi \Omega_f)</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\biggl[ u_\varpi \frac{\partial }{\partial \varpi} + \frac{u_\varphi }{\varpi}\frac{\partial }{\partial \varphi} + u_z \frac{\partial }{\partial z} \biggr] (\varpi \Omega_f) = u_\varpi \Omega_f = v_\varpi \Omega_f \, , </math> </td> </tr> </table> the Euler equation becomes, <table border="0" cellpadding="5" align="center"> <tr> <td align="right" colspan="1"> <math>~\frac{\partial \bold{v} }{\partial t} + \bold{\hat{e}}_\varpi \biggl[ \mathcal{L}_u v_\varpi \biggr] + \bold{\hat{e}}_\varphi \biggl[ \mathcal{L}_u v_\varphi - v_\varpi \Omega_f \biggr] + \bold{\hat{e}}_z \biggl[ \mathcal{L}_u v_z \biggr] </math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \bold{a} + \bold{\hat{e}}_\varpi \biggl[ \frac{v_\varphi^2}{\varpi} \biggr] - \bold{\hat{e}}_\varphi \biggl[ \varpi \Omega_f + v_\varphi \biggr] \frac{v_\varpi}{\varpi} </math> </td> </tr> <tr> <td align="right" colspan="1"> <math>~\Rightarrow ~~~ \frac{\partial \bold{v} }{\partial t} + \bold{\hat{e}}_\varpi \biggl[ \mathcal{L}_u v_\varpi \biggr] + \bold{\hat{e}}_\varphi \biggl[ \mathcal{L}_u v_\varphi \biggr] + \bold{\hat{e}}_z \biggl[ \mathcal{L}_u v_z \biggr] </math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \bold{a} + \bold{\hat{e}}_\varpi \biggl[ \frac{v_\varphi^2}{\varpi} \biggr] - \bold{\hat{e}}_\varphi \biggl[ \frac{v_\varpi v_\varphi}{\varpi} \biggr] \, . </math> </td> </tr> </table> Also, if we multiply the [[PGE/ConservingMass#Various_Forms|standard Lagrangian representation of the continuity equation]] through by <math>~v_i</math>, we have, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~0</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ v_i \biggl[\frac{d \rho}{dt} + \rho \bold\nabla \cdot \bold{v} \biggr] = v_i \biggl[\frac{d \rho}{dt} + \rho \bold\nabla \cdot \bold{u} + \rho \cancelto{0}{\bold\nabla \cdot (\bold{\hat{e}}_\varphi \varpi \Omega_f)} \biggr] </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~v_i \biggl[\frac{\partial \rho}{\partial t} + \bold\nabla \cdot (\rho \bold{u}) \biggr]</math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \frac{\partial \rho v_i}{\partial t} - \rho \frac{\partial v_i}{\partial t} + \bold\nabla \cdot (\rho v_i \bold{u}) - \rho (\bold{u}\cdot \bold\nabla) v_i </math> </td> </tr> <tr> <td align="right"> <math>~\Rightarrow~~~ \rho \frac{\partial v_i}{\partial t} + \rho \biggl[ \mathcal{L}_u v_i \biggr] </math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \frac{\partial \rho v_i}{\partial t} + \bold\nabla \cdot (\rho v_i \bold{u}) \, . </math> </td> </tr> </table> ---- <font color="red">'''Vertical Component:'''</font> Multiplying the <math>~\bold{\hat{k}}</math> component of our modified Euler equation through by <math>~\rho</math>, then incorporating this version of the continuity equation, gives, <table border="0" cellpadding="5" align="center"> <tr> <td align="right" colspan="1"> <math>~\rho \frac{\partial v_z}{\partial t} + \rho \biggl[ \mathcal{L}_u v_z \biggr] </math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\rho a_z </math> </td> </tr> <tr> <td align="right"> <math>~\Rightarrow~~~ \frac{\partial \rho v_z}{\partial t} + \bold\nabla \cdot (\rho v_z \bold{u}) </math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\rho a_z \, .</math> </td> </tr> </table> <font color="red">'''Radial Component:'''</font> Multiplying the <math>~\bold{\hat{e}}_\varpi</math> component of our modified Euler equation through by <math>~\rho</math>, then incorporating the continuity equation, gives, <table border="0" cellpadding="5" align="center"> <tr> <td align="right" colspan="1"> <math>~\rho \frac{\partial v_\varpi}{\partial t} + \rho \biggl[ \mathcal{L}_u v_\varpi \biggr] </math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\rho a_\varpi + \frac{v_\varphi^2}{\varpi} </math> </td> </tr> <tr> <td align="right"> <math>~\Rightarrow~~~ \frac{\partial \rho v_\varpi}{\partial t} + \bold\nabla \cdot (\rho v_\varpi \bold{u}) </math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\rho a_\varpi + \frac{v_\varphi^2}{\varpi} \, .</math> </td> </tr> </table> <font color="red">'''Azimuthal Component:'''</font> Multiplying the <math>~\bold{\hat{e}}_\varphi</math> component of our modified Euler equation through by <math>~\rho</math>, then incorporating the continuity equation, gives, <table border="0" cellpadding="5" align="center"> <tr> <td align="right" colspan="1"> <math>~\rho \frac{\partial v_\varphi}{\partial t} + \rho \biggl[ \mathcal{L}_u v_\varphi \biggr] </math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\rho a_\varphi - \frac{\rho v_\varphi v_\varpi}{\varpi} </math> </td> </tr> <tr> <td align="right"> <math>~\Rightarrow~~~ \frac{\partial \rho v_\varphi}{\partial t} + \bold\nabla \cdot (\rho v_\varphi \bold{u}) </math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\rho a_\varphi - \frac{\rho v_\varphi v_\varpi}{\varpi} \, .</math> </td> </tr> </table> Then, multiplying through by <math>~\varpi</math>, we have, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\rho \varpi a_\varphi - \rho v_\varphi v_\varpi</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \varpi \frac{\partial \rho v_\varphi}{\partial t} + \varpi \bold\nabla \cdot (\rho v_\varphi \bold{u}) </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \frac{\partial(\rho \varpi v_\varphi )}{\partial t} - (\rho v_\varphi )\cancelto{0}{\frac{\partial \varpi}{\partial t}} + \bold\nabla \cdot (\rho \varpi v_\varphi \bold{u}) - \rho v_\varphi (\bold{u}\cdot \bold\nabla) \varpi </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \frac{\partial(\rho \varpi v_\varphi )}{\partial t} + \bold\nabla \cdot (\rho \varpi v_\varphi \bold{u}) - \rho v_\varphi \biggl[ \cancelto{v_\varpi}{\mathcal{L}_u \varpi} \biggr] </math> </td> </tr> <tr> <td align="right"> <math>~ \Rightarrow~~~ \frac{\partial(\rho \varpi v_\varphi )}{\partial t} + \bold\nabla \cdot (\rho \varpi v_\varphi \bold{u}) </math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\rho \varpi a_\varphi \, .</math> </td> </tr> </table>
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