In mathematics, parabolic cylindrical coordinates are a three-dimensional orthogonal coordinate system that results from projecting the two-dimensional parabolic coordinate system in theperpendicular
z
The parabolic cylindrical coordinates are defined in terms of the Cartesian coordinates by:
\begin{align} x&=\sigma\tau\\ y&=
1 | |
2 |
\left(\tau2-\sigma2\right)\\ z&=z \end{align}
The surfaces of constant form confocal parabolic cylinders
2y=
x2 | |
\sigma2 |
-\sigma2
that open towards, whereas the surfaces of constant form confocal parabolic cylinders
2y=-
x2 | |
\tau2 |
+\tau2
that open in the opposite direction, i.e., towards . The foci of all these parabolic cylinders are located along the line defined by . The radius has a simple formula as well
r=\sqrt{x2+y2}=
1 | |
2 |
\left(\sigma2+\tau2\right)
that proves useful in solving the Hamilton–Jacobi equation in parabolic coordinates for the inverse-square central force problem of mechanics; for further details, see the Laplace–Runge–Lenz vector article.
The scale factors for the parabolic cylindrical coordinates and are:
\begin{align} h\sigma&=h\tau=\sqrt{\sigma2+\tau2}\\ hz&=1 \end{align}
The infinitesimal element of volume is
dV=h\sigmah\tauhzd\sigmad\taudz=(\sigma2+\tau2)d\sigmad\taudz
The differential displacement is given by:
dl=\sqrt{\sigma2+\tau2}d\sigma\boldsymbol{\hat{\sigma}}+\sqrt{\sigma2+\tau2}d\tau\boldsymbol{\hat{\tau}}+dz\hat{z
The differential normal area is given by:
dS=\sqrt{\sigma2+\tau2}d\taudz\boldsymbol{\hat{\sigma}}+\sqrt{\sigma2+\tau2}d\sigmadz\boldsymbol{\hat{\tau}}+\left(\sigma2+\tau2\right)d\sigmad\tau\hat{z
Let be a scalar field. The gradient is given by
\nablaf=
1 | |
\sqrt{\sigma2+\tau2 |
The Laplacian is given by
\nabla2f=
1 | \left( | |
\sigma2+\tau2 |
\partial2f | + | |
\partial\sigma2 |
\partial2f | |
\partial\tau2 |
\right)+
\partial2f | |
\partialz2 |
Let be a vector field of the form:
A=A\sigma\boldsymbol{\hat{\sigma}}+A\tau\boldsymbol{\hat{\tau}}+Az\hat{z
The divergence is given by
\nabla ⋅ A=
1 | |
\sigma2+\tau2 |
\left({\partial(\sqrt{\sigma2+\tau2}A\sigma)\over\partial\sigma}+{\partial(\sqrt{\sigma2+\tau2}A\tau)\over\partial\tau}\right)+{\partialAz\over\partialz}
The curl is given by
\nabla x A= \left(
1 | |
\sqrt{\sigma2+\tau2 |
Other differential operators can be expressed in the coordinates by substituting the scale factors into the general formulae found in orthogonal coordinates.
Relationship to cylindrical coordinates :
\begin{align} \rho\cos\varphi&=\sigma\tau\\ \rho\sin\varphi&=
1 | |
2 |
\left(\tau2-\sigma2\right)\\ z&=z\end{align}
Parabolic unit vectors expressed in terms of Cartesian unit vectors:
\begin{align} \boldsymbol{\hat{\sigma}}&=
\tau\hat{x | |
- |
\sigma\hat{y}}{\sqrt{\tau2+\sigma2}}\\ \boldsymbol{\hat{\tau}}&=
\sigma\hat{x | |
+ |
\tau\hat{y}}{\sqrt{\tau2+\sigma2}}\\ \hat{z
Since all of the surfaces of constant, and are conicoids, Laplace's equation is separable in parabolic cylindrical coordinates. Using the technique of the separation of variables, a separated solution to Laplace's equation may be written:
V=S(\sigma)T(\tau)Z(z)
and Laplace's equation, divided by, is written:
1 | \left[ | |
\sigma2+\tau2 |
\ddot{S | |
Since the equation is separate from the rest, we may write
\ddot{Z | |
where is constant. has the solution:
Zm(z)=A
imz | |
1e |
-imz | |
+A | |
2e |
Substituting for
\ddot{Z}/Z
\left[ | \ddot{S |
We may now separate the and functions and introduce another constant to obtain:
\ddot{S}-(m2\sigma2+n2)S=0
\ddot{T}-(m2\tau2-n2)T=0
The solutions to these equations are the parabolic cylinder functions
Smn(\sigma)=A3
2 | |
y | |
1(n |
/2m,\sigma\sqrt{2m})+A4
2 | |
y | |
2(n |
/2m,\sigma\sqrt{2m})
Tmn(\tau)=A5
2 | |
y | |
1(n |
/2m,i\tau\sqrt{2m})+A6
2 | |
y | |
2(n |
/2m,i\tau\sqrt{2m})
The parabolic cylinder harmonics for are now the product of the solutions. The combination will reduce the number of constants and the general solution to Laplace's equation may be written:
V(\sigma,\tau,z)=\summ,AmnSmnTmnZm
The classic applications of parabolic cylindrical coordinates are in solving partial differential equations, e.g., Laplace's equation or the Helmholtz equation, for which such coordinates allow a separation of variables. A typical example would be the electric field surrounding a flat semi-infinite conducting plate.