Parabolic cylindrical coordinates explained

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

-direction. Hence, the coordinate surfaces are confocal parabolic cylinders. Parabolic cylindrical coordinates have found many applications, e.g., the potential theory of edges.

Basic definition

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.

Scale factors

The scale factors for the parabolic cylindrical coordinates and are:

\begin{align} h\sigma&=h\tau=\sqrt{\sigma2+\tau2}\\ hz&=1 \end{align}

Differential elements

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

}

Del

Let be a scalar field. The gradient is given by

\nablaf=

1
\sqrt{\sigma2+\tau2
} \boldsymbol + \frac \boldsymbol + \mathbf

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

\nablaA=

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
} \frac - \frac \right) \boldsymbol- \left(\frac \frac - \frac \right) \boldsymbol+ \frac \left(\frac - \frac \right) \mathbf

Other differential operators can be expressed in the coordinates by substituting the scale factors into the general formulae found in orthogonal coordinates.

Relationship to other coordinate systems

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

} &= \mathbf\end

Parabolic cylinder harmonics

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
} + \frac\right] + \frac = 0

Since the equation is separate from the rest, we may write

\ddot{Z
}=-m^2

where is constant. has the solution:

Zm(z)=A

imz
1e
-imz
+A
2e

Substituting for

\ddot{Z}/Z

, Laplace's equation may now be written:
\left[\ddot{S
} + \frac\right] = m^2 (\sigma^2 + \tau^2)

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

Applications

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.

See also

Bibliography

External links