The confocal ellipsoidal coordinates, called simply "ellipsoidal coordinates" by Morse and Feshbach (1953) and "elliptic coordinates" by Hilbert and Cohn-Vossen (1999, p. 22), are given by the equations
|
(1)
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|
(2)
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(3)
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where ,
,
and
.
These coordinates correspond to three confocal quadrics
all sharing the same pair of foci. Surfaces of constant
are confocal ellipsoids, surfaces
of constant
are one-sheeted hyperboloids,
and surfaces of constant
are two-sheeted hyperboloids
(Hilbert and Cohn-Vossen 1999, pp. 22-23). For every
, there is a unique set of ellipsoidal coordinates. However,
specifies eight points symmetrically located in octants.
Solving for ,
, and
gives
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(4)
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(5)
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(6)
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The Laplacian is
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(7)
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where
|
(8)
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Another definition is
|
(9)
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(10)
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(11)
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where
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(12)
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(Arfken 1970, pp. 117-118). Byerly (1959, p. 251) uses a slightly different definition in which the Greek variables are replaced by their squares, and . Equation (9) represents an ellipsoid,
(10) represents a one-sheeted hyperboloid,
and (11) represents a two-sheeted hyperboloid.
In terms of Cartesian coordinates,
|
(13)
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(14)
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(15)
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The scale factors are
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(16)
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(17)
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(18)
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The Laplacian is
|
(19)
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Using the notation of Byerly (1959, pp. 252-253), this can be reduced to
|
(20)
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where
|
(21)
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(22)
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(23)
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(24)
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(25)
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(26)
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Here,
is an elliptic integral of the first
kind. In terms of
,
, and
,
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(27)
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(28)
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(29)
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where ,
and
are Jacobi elliptic functions. The Helmholtz differential equation is
separable in confocal ellipsoidal coordinates.