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 -direction. Hence, the coordinate surfaces are confocal parabolic cylinders. Parabolic cylindrical coordinates have found many applications, e.g., the potential theory of edges.
The parabolic cylindrical coordinates (σ, τ, z) are defined in terms of the Cartesian coordinates (x, y, z) by:
The surfaces of constant σ form confocal parabolic cylinders
that open towards +y, whereas the surfaces of constant τ form confocal parabolic cylinders
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
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 σ and τ are:
The infinitesimal element of volume is
The differential displacement is given by:
The differential normal area is given by:
Let f be a scalar field. The gradient is given by
The Laplacian is given by
Let A be a vector field of the form:
The divergence is given by
The curl is given by
Other differential operators can be expressed in the coordinates (σ, τ) by substituting the scale factors into the general formulae found in orthogonal coordinates.
Relationship to other coordinate systems
Relationship to cylindrical coordinates (ρ, φ, z):
Parabolic unit vectors expressed in terms of Cartesian unit vectors:
Parabolic cylinder harmonics
Since all of the surfaces of constant σ, τ and z 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:
and Laplace's equation, divided by V, is written:
Since the Z equation is separate from the rest, we may write
where m is constant. Z(z) has the solution:
Substituting −m2 for , Laplace's equation may now be written:
We may now separate the S and T functions and introduce another constant n2 to obtain:
The solutions to these equations are the parabolic cylinder functions
The parabolic cylinder harmonics for (m, n) 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:
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.
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