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Parabolic cylindrical coordinates : ウィキペディア英語版
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 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
x &= \sigma \tau \\
y &= \frac \left( \tau^2 - \sigma^2 \right) \\
z &= z
\end
The surfaces of constant form confocal parabolic cylinders
:
2 y = \frac - \sigma^2

that open towards , whereas the surfaces of constant form confocal parabolic cylinders
:
2 y = -\frac + \tau^2

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 = \frac \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.

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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