Paraboloidal coordinates
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Paraboloidal coordinates are three-dimensional
orthogonal coordinates In mathematics, orthogonal coordinates are defined as a set of ''d'' coordinates q = (''q''1, ''q''2, ..., ''q'd'') in which the coordinate hypersurfaces all meet at right angles (note: superscripts are indices, not exponents). A coordinate su ...
(\mu, \nu, \lambda) that generalize two-dimensional parabolic coordinates. They possess elliptic
paraboloids In geometry, a paraboloid is a quadric surface that has exactly one axis of symmetry and no center of symmetry. The term "paraboloid" is derived from parabola, which refers to a conic section that has a similar property of symmetry. Every plan ...
as one-coordinate surfaces. As such, they should be distinguished from
parabolic cylindrical coordinates In mathematics, 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 surfa ...
and parabolic rotational coordinates, both of which are also generalizations of two-dimensional parabolic coordinates. The coordinate surfaces of the former are parabolic cylinders, and the coordinate surfaces of the latter are ''circular'' paraboloids. Differently from cylindrical and rotational parabolic coordinates, but similarly to the related
ellipsoidal coordinates Ellipsoidal coordinates are a three-dimensional orthogonal coordinate system (\lambda, \mu, \nu) that generalizes the two-dimensional elliptic coordinate system. Unlike most three-dimensional orthogonal coordinate systems that feature quadratic ...
, the coordinate surfaces of the paraboloidal coordinate system are ''not'' produced by rotating or projecting any two-dimensional orthogonal coordinate system.


Basic formulas

The Cartesian coordinates (x, y, z) can be produced from the ellipsoidal coordinates (\mu, \nu, \lambda) by the equations : x^ = \frac(\mu - b)(b - \nu)(b - \lambda) : y^ = \frac(\mu - c)(c - \nu)(\lambda - c) : z = \mu + \nu + \lambda - b - c with : \mu > b > \lambda > c > \nu > 0 Consequently, surfaces of constant \mu are downward opening elliptic paraboloids: : \frac + \frac = -4 (z - \mu) Similarly, surfaces of constant \nu are ''upward'' opening elliptic paraboloids, : \frac + \frac = 4 (z - \nu) whereas surfaces of constant \lambda are hyperbolic paraboloids: : \frac - \frac = 4 (z - \lambda)


Scale factors

The scale factors for the paraboloidal coordinates (\mu, \nu, \lambda) are : h_ = \left \frac \right : h_ = \left frac \right : h_ = \left frac \right Hence, the infinitesimal volume element is : dV = \frac \ d\lambda d\mu d\nu


Differential operators

Common differential operators can be expressed in the coordinates (\mu, \nu, \lambda) by substituting the scale factors into the general formulas for these operators, which are applicable to any three-dimensional orthogonal coordinates. For instance, the
gradient operator Del, or nabla, is an operator used in mathematics (particularly in vector calculus) as a vector differential operator, usually represented by the nabla symbol ∇. When applied to a function defined on a one-dimensional domain, it denotes t ...
is : \nabla = \left frac \right \mathbf_ \frac + \left frac \right \mathbf_ \frac + \left frac \right \mathbf_ \frac and the Laplacian is : \begin \nabla^2 = &\left frac \right \frac \left \mu - b)^(\mu - c)^ \frac \right\\ &+ \left frac \right \frac \left (b - \nu)^(c - \nu)^\frac \right\\ &+ \left frac \right \frac \left b - \lambda)^(\lambda -c)^ \frac \right\end


Applications

Paraboloidal coordinates can be useful for solving certain
partial differential equations In mathematics, a partial differential equation (PDE) is an equation which imposes relations between the various partial derivatives of a multivariable function. The function is often thought of as an "unknown" to be solved for, similarly to ...
. For instance, the
Laplace equation In mathematics and physics, Laplace's equation is a second-order partial differential equation named after Pierre-Simon Laplace, who first studied its properties. This is often written as \nabla^2\! f = 0 or \Delta f = 0, where \Delta = \n ...
and Helmholtz equation are both separable in paraboloidal coordinates. Hence, the coordinates can be used to solve these equations in geometries with paraboloidal symmetry, i.e. with boundary conditions specified on sections of paraboloids. The Helmholtz equation is (\nabla^2 + k^2) \psi = 0. Taking \psi = M(\mu)N(\nu)\Lambda(\lambda), the separated equations areWillatzen and Yoon (2011), p. 227 : \begin &(\mu - b)(\mu - c) \frac + \frac\left \mu - (b + c) \right\frac + \left ^2 \mu^2 + \alpha_3 \mu - \alpha_2\rightM = 0 \\ &(b - \nu)(c - \nu) \frac + \frac\left \nu - (b + c) \right\frac + \left ^2 \nu^2 + \alpha_3 \nu - \alpha_2\rightN = 0 \\ &(b - \lambda)(\lambda - c) \frac - \frac\left \lambda - (b + c) \right\frac - \left ^2 \lambda^2 + \alpha_3 \lambda - \alpha_2\right\Lambda = 0 \\ \end where \alpha_2 and \alpha_3 are the two separation constants. Similarly, the separated equations for the Laplace equation can be obtained by setting k = 0 in the above. Each of the separated equations can be cast in the form of the Baer equation. Direct solution of the equations is difficult, however, in part because the separation constants \alpha_2 and \alpha_3 appear simultaneously in all three equations. Following the above approach, paraboloidal coordinates have been used to solve for the electric field surrounding a conducting paraboloid.


References


Bibliography

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


External links


MathWorld description of confocal paraboloidal coordinates
{{Orthogonal coordinate systems Three-dimensional coordinate systems Orthogonal coordinate systems