Parabolic cylindrical coordinates

From Wikipedia, the free encyclopedia

Coordinate surfaces of parabolic cylindrical coordinates. The red parabolic cylinder corresponds to σ=2, whereas the yellow parabolic cylinder corresponds to τ=1. The blue plane corresponds to z=2. These surfaces intersect at the point P (shown as a black sphere), which has Cartesian coordinates roughly (2, -1.5, 2).

Parabolic cylindrical coordinates are a three-dimensional orthogonal coordinate system that results from projecting the two-dimensional parabolic coordinate system in the perpendicular $z$ -direction. Hence, the coordinate surfaces are confocal parabolic cylinders. Parabolic cylindrical coordinates have found many applications, e.g., the potential theory of edges.

1 Basic definition
2 Scale factors
3 Parabolic Cylinder harmonics
4 Applications
5 See also
6 Bibliography
7 External links

[edit] Basic definition

Parabolic coordinate system showing curves of constant σ and τ the horizontal and vertical axes are the x and y coordinates respectively. These coordinates are projected along the z-axis, and so this diagram will hold for any value of the z coordinate.

The parabolic cylindrical coordinates $(σ,τ, z)$ are defined in terms of the Cartesian coordinates (x,y,z) by:

$x = \sigma \tau\,$

$y = \frac{1}{2} \left( \tau^{2} - \sigma^{2} \right)$

$z = z\,$

The surfaces of constant $σ$ form confocal parabolic cylinders

$2y = \frac{x^{2}}{\sigma^{2}} - \sigma^{2}$

that open towards $+ y$ , whereas the surfaces of constant $τ$ form confocal parabolic cylinders

$2y = -\frac{x^{2}}{\tau^{2}} + \tau^{2}$

that open in the opposite direction, i.e., towards $- y$ . The foci of all these parabolic cylinders are located along the line defined by $x = y = 0$ . The radius r has a simple formula as well

$r = \sqrt{x^{2} + y^{2}} = \frac{1}{2} \left( \sigma^{2} + \tau^{2} \right)$

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.

[edit] Scale factors

The scale factors for the parabolic cylindrical coordinates $σ$ and $τ$ are:

$h_{\sigma} = h_{\tau} = \sqrt{\sigma^{2} + \tau^{2}}$

$h_{z}=1\,$

The infinitesimal element of volume is

$dV = h_\sigma h_\tau h_z=\left( \sigma^{2} + \tau^{2} \right) d\sigma d\tau dz$

and the Laplacian equals

$\nabla^{2} \Phi = \frac{1}{\sigma^{2} + \tau^{2}} \left( \frac{\partial^{2} \Phi}{\partial \sigma^{2}} + \frac{\partial^{2} \Phi}{\partial \tau^{2}} \right) + \frac{\partial^{2} \Phi}{\partial z^{2}}$

Other differential operators such as $\nabla \cdot \mathbf{F}$ and $\nabla \times \mathbf{F}$ can be expressed in the coordinates $(σ,τ)$ by substituting the scale factors into the general formulae found in orthogonal coordinates.

[edit] Parabolic Cylinder harmonics

Since all of the surfaces of constant σ, τ and z are conicoid, 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 V , is written:

$\frac{1}{\sigma^2+\tau^2} \left[\frac{\ddot{S}}{S}+\frac{\ddot{T}}{T}\right]+\frac{\ddot{Z}}{Z}=0$

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

$\frac{\ddot{Z}}{Z}=-m^2$

where m is constant. Z(z) has the solution:

$Z_m(z)=A_1\,e^{imz}+A_2\,e^{-imz}\,$

Substituting $- m 2$ for $\ddot{Z}/Z$ , Laplace's equation may now be written:

$\left[\frac{\ddot{S}}{S}+\frac{\ddot{T}}{T}\right]=m^2(\sigma^2+\tau^2)$

We may now separate the S and T functions and introduce another constant $n 2$ to obtain:

$\ddot{S} - (m^2\sigma^2+n^2)S=0$

$\ddot{T} - (m^2\tau^2 -n^2)T=0$

The solutions to these equations are the parabolic cylinder functions

$S_{mn}(\sigma) = A_3\,y_1(n^2/2m,\sigma\sqrt{2m}) + A_4\,y_2(n^2/2m,\sigma\sqrt{2m})$

$T_{mn}(\tau) = A_5\,y_1(n^2/2m,i\tau \sqrt{2m}) + A_6\,y_2(n^2/2m,i\tau \sqrt{2m})$

The parabolic cylinder harmonics for (m,n) are now the product of the solutions. The combination will reduce the number of constants to four and the general solution to Laplace's equation may be written:

$V(\sigma,\tau,z)=\sum_{m,n} A_{mn} S_{mn} T_{mn} Z_m\,$

[edit] 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.

[edit] See also

Orthogonal coordinates
Two dimensional orthogonal coordinate systems

Three dimensional orthogonal coordinate systems

Elliptic cylindrical coordinates
Toroidal coordinates
Bispherical coordinates
Bipolar cylindrical coordinates
Conical coordinates
Flat-Ring cyclide coordinates
Flat-Disk cyclide coordinates
Bi-cyclide coordinates
Cap-cyclide coordinates

[edit] Bibliography

Morse PM, Feshbach H (1953). Methods of Theoretical Physics, Part I. New York: McGraw-Hill, p. 658. ISBN 0-07-043316-X, LCCN 52-11515.

Margenau H, Murphy GM (1956). The Mathematics of Physics and Chemistry. New York: D. van Nostrand, pp. 186–187. LCCN 55-10911.

Korn GA, Korn TM (1961). Mathematical Handbook for Scientists and Engineers. New York: McGraw-Hill, p. 181. LCCN 59-14456, ASIN B0000CKZX7.

Sauer R, Szabó I (1967). Mathematische Hilfsmittel des Ingenieurs. New York: Springer Verlag, p. 96. LCCN 67-25285.

Zwillinger D (1992). Handbook of Integration. Boston, MA: Jones and Bartlett, p. 114. ISBN 0-86720-293-9. Same as Morse & Feshbach (1953), substituting u_k for ξ_k.

Moon P, Spencer DE (1988). "Parabolic-Cylinder Coordinates (μ, ν, z)", Field Theory Handbook, Including Coordinate Systems, Differential Equations, and Their Solutions, corrected 2nd ed., 3rd print ed., New York: Springer-Verlag, pp. 21–24 (Table 1.04). ISBN 978-0387184302.