Elliptic cylindrical coordinates

Elliptic cylindrical coordinates

Elliptic cylindrical coordinates are a three-dimensional orthogonal coordinate system that results from projecting the two-dimensional elliptic coordinate system in theperpendicular z-direction. Hence, the coordinate surfaces are prisms of confocal ellipses and hyperbolae. The two foci F_{1} and F_{2} are generally taken to be fixed at -a and+a, respectively, on the x-axis of the Cartesian coordinate system.

Basic definition

The most common definition of elliptic cylindrical coordinates (mu, u, z) is

:x = a cosh mu cos u

:y = a sinh mu sin u

:z = z!

where mu is a nonnegative real number and u in [0, 2pi).

These definitions correspond to ellipses and hyperbolae. The trigonometric identity

:frac{x^{2{a^{2} cosh^{2} mu} + frac{y^{2{a^{2} sinh^{2} mu} = cos^{2} u + sin^{2} u = 1

shows that curves of constant mu form ellipses, whereas the hyperbolic trigonometric identity

:frac{x^{2{a^{2} cos^{2} u} - frac{y^{2{a^{2} sin^{2} u} = cosh^{2} mu - sinh^{2} mu = 1

shows that curves of constant u form hyperbolae.

cale factors

The scale factors for the elliptic cylindrical coordinates mu and u are equal

:h_{mu} = h_{ u} = asqrt{sinh^{2}mu + sin^{2} u}

whereas the remaining scale factor h_{z}=1. Consequently, an infinitesimal volume element equals

:dV = a^{2} left( sinh^{2}mu + sin^{2} u ight) dmu d u dz

and the Laplacian equals

: abla^{2} Phi = frac{1}{a^{2} left( sinh^{2}mu + sin^{2} u ight)} left( frac{partial^{2} Phi}{partial mu^{2 + frac{partial^{2} Phi}{partial u^{2 ight) + frac{partial^{2} Phi}{partial z^{2

Other differential operators such as abla cdot mathbf{F} and abla imes mathbf{F} can be expressed in the coordinates (mu, u, z) by substituting the scale factors into the general formulae found in orthogonal coordinates.

Alternative definition

An alternative and geometrically intuitive set of elliptic coordinates (sigma, au, z) are sometimes used, where sigma = cosh mu and au = cos u. Hence, the curves of constant sigma are ellipses, whereas the curves of constant au are hyperbolae. The coordinate au must belong to the interval [-1, 1] , whereas the sigma coordinate must be greater than or equal to one. The coordinates (sigma, au, z) have a simple relation to the distances to the foci F_{1} and F_{2}. For any point in the (x,y) plane, the "sum" d_{1}+d_{2} of its distances to the foci equals 2asigma, whereas their "difference" d_{1}-d_{2} equals 2a au.Thus, the distance to F_{1} is a(sigma+ au), whereas the distance to F_{2} is a(sigma- au). (Recall that F_{1} and F_{2} are located at x=-a and x=+a, respectively.)

A drawback of these coordinates is that they do not have a 1-to-1 transformation to the Cartesian coordinates:x = asigma au !

:y^{2} = a^{2} left( sigma^{2} - 1 ight) left(1 - au^{2} ight)

Alternative scale factors

The scale factors for the alternative elliptic coordinates (sigma, au, z) are

:h_{sigma} = asqrt{frac{sigma^{2} - au^{2{sigma^{2} - 1

:h_{ au} = asqrt{frac{sigma^{2} - au^{2{1 - au^{2}

and, of course, h_{z}=1. Hence, the infinitesimal volume element becomes

:dV = a^{2} frac{sigma^{2} - au^{2{sqrt{left( sigma^{2} - 1 ight) left( 1 - au^{2} ight) dsigma d au dz

and the Laplacian equals

: abla^{2} Phi = frac{1}{a^{2} left( sigma^{2} - au^{2} ight) }left [sqrt{sigma^{2} - 1} frac{partial}{partial sigma} left( sqrt{sigma^{2} - 1} frac{partial Phi}{partial sigma} ight) + sqrt{1 - au^{2 frac{partial}{partial au} left( sqrt{1 - au^{2 frac{partial Phi}{partial au} ight) ight] + frac{partial^{2} Phi}{partial z^{2

Other differential operators such as abla cdot mathbf{F} and abla imes mathbf{F} can be expressed in the coordinates (sigma, au) by substituting the scale factors into the general formulae found in orthogonal coordinates.

Applications

The classic applications of elliptic cylindrical coordinates are in solving partial differential equations, e.g., Laplace's equation or the Helmholtz equation, for which elliptic cylindrical coordinates allow a
separation of variables. A typical example would be the electric field surrounding a flat conducting plate of width 2a.

The three-dimensional wave equation, when expressed in elliptic cylindrical coordinates, may be solved by separation of variables, leading to the Mathieu differential equations.

The geometric properties of elliptic coordinates can also be useful. A typical example might involve an integration over all pairs of vectors mathbf{p} and mathbf{q} that sum to a fixed vector mathbf{r} = mathbf{p} + mathbf{q}, where the integrand was a function of the vector lengths left| mathbf{p} ight| and left| mathbf{q} ight|. (In such a case, one would position mathbf{r} between the two foci and aligned with the x-axis, i.e., mathbf{r} = 2a mathbf{hat{x.) For concreteness, mathbf{r}, mathbf{p} and mathbf{q} could represent the momenta of a particle and its decomposition products, respectively, and the integrand might involve the kinetic energies of the products (which are proportional to the squared lengths of the momenta).

See also

Bibliography

* | pages = p. 657

* | pages = pp. 182–183

*, ASIN B0000CKZX7 | pages = p. 179

* | pages = p. 97

* Same as Morse & Feshbach (1953), substituting "u""k" for ξ"k".

*

External links

* [http://mathworld.wolfram.com/EllipticCylindricalCoordinates.html MathWorld description of elliptic cylindrical coordinates]


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