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Fluid Equations in Cylindrical Coordinates

Let us adopt the cylindrical coordinate system, $r$, $\theta $, $z$. Making use of the results quoted in Section C.3, the components of the stress tensor are
$\displaystyle \sigma_{rr}$ $\textstyle =$ $\displaystyle -p + 2\,\mu\,\frac{\partial v_r}{\partial r},$ (142)
$\displaystyle \sigma_{\theta\theta}$ $\textstyle =$ $\displaystyle -p + 2\,\mu\left(\frac{1}{r}\frac{\partial v_\theta}{\partial \theta}+ \frac{v_r}{r}\right),$ (143)
$\displaystyle \sigma_{zz}$ $\textstyle =$ $\displaystyle -p + 2\,\mu\,\frac{\partial v_z}{\partial z},$ (144)
$\displaystyle \sigma_{r\theta}=\sigma_{\theta r}$ $\textstyle =$ $\displaystyle \mu\left(\frac{1}{r}\,\frac{\partial v_r}{\partial\theta} + \frac{\partial v_\theta}{\partial r}-\frac{v_\theta}{r}\right),$ (145)
$\displaystyle \sigma_{rz}=\sigma_{zr}$ $\textstyle =$ $\displaystyle \mu\left(\frac{\partial v_r}{\partial z} + \frac{\partial v_z}{\partial r}\right),$ (146)
$\displaystyle \sigma_{\theta z} = \sigma_{z\theta}$ $\textstyle =$ $\displaystyle \mu\left(\frac{1}{r}\,\frac{\partial v_z}{\partial\theta}+\frac{\partial v_\theta}{\partial z}\right),$ (147)

whereas the equations of compressible fluid flow become
$\displaystyle \frac{D\rho}{Dt}$ $\textstyle =$ $\displaystyle -\rho\,\Delta,$ (148)
$\displaystyle \frac{Dv_r}{Dt}-\frac{v_\theta^{\,2}}{r}$ $\textstyle =$ $\displaystyle - \frac{1}{\rho}\,\frac{\partial p}{\partial r} - \frac{\partial{\mit\Psi}}{\partial r}$  
    $\displaystyle + \frac{\mu}{\rho}\left(\nabla^2 v_r -\frac{v_r}{r^2}-\frac{2}{r^...
...\theta}{\partial\theta}+ \frac{1}{3}\,\frac{\partial\Delta}{\partial r}\right),$ (149)
$\displaystyle \frac{Dv_\theta}{Dt}+\frac{v_r\,v_\theta}{r}$ $\textstyle =$ $\displaystyle - \frac{1}{\rho\,r}\,\frac{\partial p}{\partial \theta} - \frac{1}{r}\frac{\partial{\mit\Psi}}{\partial \theta}$  
    $\displaystyle +\frac{\mu}{\rho}\left(\nabla^2 v_\theta +\frac{2}{r^2}\,\frac{\p...
...ac{v_\theta}{r^2}+ \frac{1}{3r}\,\frac{\partial\Delta}{\partial \theta}\right),$ (150)
$\displaystyle \frac{Dv_z}{Dt}$ $\textstyle =$ $\displaystyle - \frac{1}{\rho}\,\frac{\partial p}{\partial z} - \frac{\partial{...
...rho}\left(\nabla^2 v_z + \frac{1}{3}\,\frac{\partial\Delta}{\partial z}\right),$ (151)
$\displaystyle \frac{1}{\gamma-1}\left(\frac{D\rho}{Dt} - \frac{\gamma\,p}{\rho}\,\frac{D\rho}{Dt}\right)$ $\textstyle =$ $\displaystyle \chi + \frac{\kappa\,{\cal M}}{\cal R}\,\nabla^2\left(\frac{p}{\rho}\right),$ (152)

where
$\displaystyle \Delta$ $\textstyle =$ $\displaystyle \frac{1}{r}\,\frac{\partial (r\,v_r)}{\partial r} +\frac{1}{r}\, \frac{\partial v_\theta}{\partial \theta} + \frac{\partial v_z}{\partial z},$ (153)
$\displaystyle \frac{D}{Dt}$ $\textstyle =$ $\displaystyle \frac{\partial}{\partial t} + v_r\,\frac{\partial }{\partial r} +...
...theta}{r}\,\frac{\partial}{\partial \theta} + v_z\,\frac{\partial}{\partial z},$ (154)
$\displaystyle \nabla^2$ $\textstyle =$ $\displaystyle \frac{1}{r}\frac{\partial}{\partial r}\!\left(r\,\frac{\partial}{...
...1}{r^2}\, \frac{\partial^2}{\partial \theta^2}+\frac{\partial^2}{\partial z^2},$ (155)
$\displaystyle \chi$ $\textstyle =$ $\displaystyle 2\mu\left[\left(\frac{\partial v_r}{\partial r}\right)^2+\left(\f...
...\theta}+\frac{\partial v_\theta}{\partial r}-\frac{v_\theta}{r}\right)^2\right.$  
    $\displaystyle \left.+\frac{1}{2}\left(\frac{\partial v_r}{\partial z}+\frac{\pa...
...{\partial z}+\frac{1}{r}\,\frac{\partial v_z}{\partial \theta}\right)^2\right].$ (156)


next up previous
Next: Fluid Equations in Spherical Up: Mathematical Models of Fluid Previous: Fluid Equations in Cartesian
Richard Fitzpatrick 2012-04-27