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
(4)
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(5)
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(6)
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The Laplacian is
(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
(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
(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 ,
(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.