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Parabolic coordinates : ウィキペディア英語版
Parabolic coordinates

Parabolic coordinates are a two-dimensional orthogonal coordinate system in which the coordinate lines are confocal parabolas. A three-dimensional version of parabolic coordinates is obtained by rotating the two-dimensional system about the symmetry axis of the parabolas.
Parabolic coordinates have found many applications, e.g., the treatment of the Stark effect and the potential theory of the edges.
== Two-dimensional parabolic coordinates ==

Two-dimensional parabolic coordinates (\sigma, \tau) are defined by the equations, in terms of cartesian coordinates:
:
x = \sigma \tau\,

:
y = \frac \left( \tau^ - \sigma^ \right)

The curves of constant \sigma form confocal parabolae
:
2y = \frac} - \sigma^

that open upwards (i.e., towards +y), whereas the curves of constant \tau form confocal parabolae
:
2y = -\frac} + \tau^

that open downwards (i.e., towards -y). The foci of all these parabolae are located at the origin.

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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