Navier-Stokes-ligningene
Fra Wikipedia, den frie encyklopedi
Navier–Stokes-ligningene, oppkalt etter Claude-Louise Navier og George Gabriel Stokes, er ligninger som beskriver bevegelse av viskøse væsker og gasser. Som oftest gir ligningene opphav til ikke-lineære differentialligninger som demonstrerer fenomenet kaos.
Vektorligningen er

For en newtonsk fluid kan leddet
erstattes med
, der
er den dynamiske viskositetskonstanten for fluiden.
[rediger] Kartesiske koordinater
Ved å skrive ut komponentene i vektorligningen over får vi følgende ligninger for impulsen i 3-D,
Kontinuitetsligningen gir:
[rediger] Sylinderkoordinater
Et variabelskifte på ligningssettet i kartesiske koordinater gir impulsligningene for r, θ, og z:
Kontinuitetsligningen gir:
[rediger] Kulekoordinater
Kontinuitetsligningen gir:




![\rho \left(\frac{\partial u_r}{\partial t} + u_r \frac{\partial u_r}{\partial r} + \frac{u_{\theta}}{r} \frac{\partial u_r}{\partial \theta} + u_z \frac{\partial u_r}{\partial z} - \frac{u_{\theta}^2}{r}\right) =
-\frac{\partial p}{\partial r} +
\mu \left[\frac{1}{r}\frac{\partial}{\partial r}\left(r \frac{\partial u_r}{\partial r}\right) + \frac{1}{r^2}\frac{\partial^2 u_r}{\partial \theta^2} + \frac{\partial^2 u_r}{\partial z^2} - \frac{u_r}{r^2} - \frac{2}{r^2}\frac{\partial u_{\theta}}{\partial \theta}\right] + \rho g_r](http://upload.wikimedia.org/wikipedia/no/math/f/e/5/fe5c63677802bd79a4eb7273814487a6.png)
![\rho \left(\frac{\partial u_{\theta}}{\partial t} + u_r \frac{\partial u_{\theta}}{\partial r} + \frac{u_{\theta}}{r} \frac{\partial u_{\theta}}{\partial \theta} + u_z \frac{\partial u_{\theta}}{\partial z} + \frac{u_r u_{\theta}}{r}\right) =
-\frac{1}{r}\frac{\partial p}{\partial \theta} +
\mu \left[\frac{1}{r}\frac{\partial}{\partial r}\left(r \frac{\partial u_{\theta}}{\partial r}\right) + \frac{1}{r^2}\frac{\partial^2 u_{\theta}}{\partial \theta^2} + \frac{\partial^2 u_{\theta}}{\partial z^2} + \frac{2}{r^2}\frac{\partial u_r}{\partial \theta} - \frac{u_{\theta}}{r^2}\right] + \rho g_{\theta}](http://upload.wikimedia.org/wikipedia/no/math/1/c/4/1c4d779ed7b3291b9fe2af81a28109b0.png)
![\rho \left(\frac{\partial u_z}{\partial t} + u_r \frac{\partial u_z}{\partial r} + \frac{u_{\theta}}{r} \frac{\partial u_z}{\partial \theta} + u_z \frac{\partial u_z}{\partial z}\right) =
-\frac{\partial p}{\partial z} + \mu \left[\frac{1}{r}\frac{\partial}{\partial r}\left(r \frac{\partial u_z}{\partial r}\right) + \frac{1}{r^2}\frac{\partial^2 u_z}{\partial \theta^2} + \frac{\partial^2 u_z}{\partial z^2}\right] + \rho g_z](http://upload.wikimedia.org/wikipedia/no/math/f/c/b/fcb392feda195f51b477d9acf15ee057.png)

![\mu \left[
\frac{1}{r^2} \frac{\partial}{\partial r}\left(r^2 \frac{\partial u_r}{\partial r}\right) +
\frac{1}{r^2 \sin(\theta)^2} \frac{\partial^2 u_r}{\partial \phi^2} +
\frac{1}{r^2 \sin(\theta)} \frac{\partial}{\partial \theta}\left(\sin(\theta) \frac{\partial u_r}{\partial \theta}\right) -
2 \frac{u_r + \frac{\partial u_{\theta}}{\partial \theta} + u_{\theta} \cot(\theta)}{r^2} +
\frac{2}{r^2 \sin(\theta)} \frac{\partial u_{\phi}}{\partial \phi}
\right]](http://upload.wikimedia.org/wikipedia/no/math/7/9/9/799b364bf8140fad3913b0fe83682f47.png)
![\mu \left[
\frac{1}{r^2} \frac{\partial}{\partial r}\left(r^2 \frac{\partial u_{\theta}}{\partial r}\right) +
\frac{1}{r^2 \sin(\theta)^2} \frac{\partial^2 u_{\theta}}{\partial \phi^2} +
\frac{1}{r^2 \sin(\theta)} \frac{\partial}{\partial \theta}\left(\sin(\theta) \frac{\partial u_{\theta}}{\partial \theta}\right) +
\frac{2}{r^2} \frac{\partial u_r}{\partial \theta} -
\frac{u_{\theta} + 2 \cos(\theta) \frac{\partial u_{\phi}}{\partial \phi}}{r^2 \sin(\theta)^2}
\right]](http://upload.wikimedia.org/wikipedia/no/math/9/5/d/95de34b6bf200842039d744583662ecf.png)
![\mu \left[
\frac{1}{r^2} \frac{\partial}{\partial r}\left(r^2 \frac{\partial u_{\phi}}{\partial r}\right) +
\frac{1}{r^2 \sin(\theta)^2} \frac{\partial^2 u_{\phi}}{\partial \phi^2} +
\frac{1}{r^2 \sin(\theta)} \frac{\partial}{\partial \theta}\left(\sin(\theta) \frac{\partial u_{\phi}}{\partial \theta}\right) +
\frac{2 \frac{\partial u_r}{\partial \phi} + 2 \cos(\theta) \frac{\partial u_{\theta}}{\partial \phi} - u_{\phi}}{r^2 \sin(\theta)^2}
\right]](http://upload.wikimedia.org/wikipedia/no/math/d/8/8/d885abc6e2ba775041543b00dde16a6b.png)
