Ellipsoidal coordinates
In-game article clicks load inline without leaving the challenge.
Ellipsoidal coordinates are a three-dimensional orthogonal coordinate system ( λ , μ , ν ) {\displaystyle (\lambda ,\mu ,\nu )} that generalizes the two-dimensional elliptic coordinate system. Unlike most three-dimensional orthogonal coordinates that feature quadratic coordinate surfaces, the ellipsoidal coordinate system is based on confocal quadrics.
Basic formulae
The Cartesian coordinates ( x , y , z ) {\displaystyle (x,y,z)} can be produced from the ellipsoidal coordinates ( λ , μ , ν ) {\displaystyle (\lambda ,\mu ,\nu )} by the equations
x 2 = ( a 2 + λ ) ( a 2 + μ ) ( a 2 + ν ) ( a 2 − b 2 ) ( a 2 − c 2 ) {\displaystyle x^{2}={\frac {\left(a^{2}+\lambda \right)\left(a^{2}+\mu \right)\left(a^{2}+\nu \right)}{\left(a^{2}-b^{2}\right)\left(a^{2}-c^{2}\right)}}}
y 2 = ( b 2 + λ ) ( b 2 + μ ) ( b 2 + ν ) ( b 2 − a 2 ) ( b 2 − c 2 ) {\displaystyle y^{2}={\frac {\left(b^{2}+\lambda \right)\left(b^{2}+\mu \right)\left(b^{2}+\nu \right)}{\left(b^{2}-a^{2}\right)\left(b^{2}-c^{2}\right)}}}
z 2 = ( c 2 + λ ) ( c 2 + μ ) ( c 2 + ν ) ( c 2 − b 2 ) ( c 2 − a 2 ) {\displaystyle z^{2}={\frac {\left(c^{2}+\lambda \right)\left(c^{2}+\mu \right)\left(c^{2}+\nu \right)}{\left(c^{2}-b^{2}\right)\left(c^{2}-a^{2}\right)}}}
where the following limits apply to the coordinates
− λ < c 2 < − μ < b 2 < − ν < a 2 . {\displaystyle -\lambda <c^{2}<-\mu <b^{2}<-\nu <a^{2}.}
Consequently, surfaces of constant λ {\displaystyle \lambda } are ellipsoids
x 2 a 2 + λ + y 2 b 2 + λ + z 2 c 2 + λ = 1 , {\displaystyle {\frac {x^{2}}{a^{2}+\lambda }}+{\frac {y^{2}}{b^{2}+\lambda }}+{\frac {z^{2}}{c^{2}+\lambda }}=1,}
whereas surfaces of constant μ {\displaystyle \mu } are hyperboloids of one sheet
x 2 a 2 + μ + y 2 b 2 + μ + z 2 c 2 + μ = 1 , {\displaystyle {\frac {x^{2}}{a^{2}+\mu }}+{\frac {y^{2}}{b^{2}+\mu }}+{\frac {z^{2}}{c^{2}+\mu }}=1,}
because the last term in the lhs is negative, and surfaces of constant ν {\displaystyle \nu } are hyperboloids of two sheets
x 2 a 2 + ν + y 2 b 2 + ν + z 2 c 2 + ν = 1 {\displaystyle {\frac {x^{2}}{a^{2}+\nu }}+{\frac {y^{2}}{b^{2}+\nu }}+{\frac {z^{2}}{c^{2}+\nu }}=1}
because the last two terms in the lhs are negative.
The orthogonal system of quadrics used for the ellipsoidal coordinates are confocal quadrics.
Scale factors and differential operators
For brevity in the equations below, we introduce a function
S ( σ ) = d e f ( a 2 + σ ) ( b 2 + σ ) ( c 2 + σ ) {\displaystyle S(\sigma )\ {\stackrel {\mathrm {def} }{=}}\ \left(a^{2}+\sigma \right)\left(b^{2}+\sigma \right)\left(c^{2}+\sigma \right)}
where σ {\displaystyle \sigma } can represent any of the three variables ( λ , μ , ν ) {\displaystyle (\lambda ,\mu ,\nu )}. Using this function, the scale factors can be written
h λ = 1 2 ( λ − μ ) ( λ − ν ) S ( λ ) {\displaystyle h_{\lambda }={\frac {1}{2}}{\sqrt {\frac {\left(\lambda -\mu \right)\left(\lambda -\nu \right)}{S(\lambda )}}}}
h μ = 1 2 ( μ − λ ) ( μ − ν ) S ( μ ) {\displaystyle h_{\mu }={\frac {1}{2}}{\sqrt {\frac {\left(\mu -\lambda \right)\left(\mu -\nu \right)}{S(\mu )}}}}
h ν = 1 2 ( ν − λ ) ( ν − μ ) S ( ν ) {\displaystyle h_{\nu }={\frac {1}{2}}{\sqrt {\frac {\left(\nu -\lambda \right)\left(\nu -\mu \right)}{S(\nu )}}}}
Hence, the infinitesimal volume element equals
d V = ( λ − μ ) ( λ − ν ) ( μ − ν ) 8 − S ( λ ) S ( μ ) S ( ν ) d λ d μ d ν {\displaystyle dV={\frac {\left(\lambda -\mu \right)\left(\lambda -\nu \right)\left(\mu -\nu \right)}{8{\sqrt {-S(\lambda )S(\mu )S(\nu )}}}}\,d\lambda \,d\mu \,d\nu }
and the Laplacian is defined by
∇ 2 Φ = 4 S ( λ ) ( λ − μ ) ( λ − ν ) ∂ ∂ λ [ S ( λ ) ∂ Φ ∂ λ ] + 4 S ( μ ) ( μ − λ ) ( μ − ν ) ∂ ∂ μ [ S ( μ ) ∂ Φ ∂ μ ] + 4 S ( ν ) ( ν − λ ) ( ν − μ ) ∂ ∂ ν [ S ( ν ) ∂ Φ ∂ ν ] {\displaystyle {\begin{aligned}\nabla ^{2}\Phi ={}&{\frac {4{\sqrt {S(\lambda )}}}{\left(\lambda -\mu \right)\left(\lambda -\nu \right)}}{\frac {\partial }{\partial \lambda }}\left[{\sqrt {S(\lambda )}}{\frac {\partial \Phi }{\partial \lambda }}\right]\\[1ex]&+{\frac {4{\sqrt {S(\mu )}}}{\left(\mu -\lambda \right)\left(\mu -\nu \right)}}{\frac {\partial }{\partial \mu }}\left[{\sqrt {S(\mu )}}{\frac {\partial \Phi }{\partial \mu }}\right]\\[1ex]&+{\frac {4{\sqrt {S(\nu )}}}{\left(\nu -\lambda \right)\left(\nu -\mu \right)}}{\frac {\partial }{\partial \nu }}\left[{\sqrt {S(\nu )}}{\frac {\partial \Phi }{\partial \nu }}\right]\end{aligned}}}
Other differential operators such as ∇ ⋅ F {\displaystyle \nabla \cdot \mathbf {F} } and ∇ × F {\displaystyle \nabla \times \mathbf {F} } can be expressed in the coordinates ( λ , μ , ν ) {\displaystyle (\lambda ,\mu ,\nu )} by substituting the scale factors into the general formulae found in orthogonal coordinates.
Angular parametrization
An alternative (but non-orthogonal) parametrization exists that closely follows the angular parametrization of spherical coordinates:
x = a s sin θ cos ϕ , {\displaystyle x=as\sin \theta \cos \phi ,}
y = b s sin θ sin ϕ , {\displaystyle y=bs\sin \theta \sin \phi ,}
z = c s cos θ . {\displaystyle z=cs\cos \theta .}
Here, s > 0 {\displaystyle s>0} parametrizes the concentric ellipsoids around the origin and θ ∈ [ 0 , π ] {\displaystyle \theta \in [0,\pi ]} and ϕ ∈ [ 0 , 2 π ] {\displaystyle \phi \in [0,2\pi ]} are the usual polar and azimuthal angles of spherical coordinates, respectively. The corresponding volume element is
d x d y d z = a b c s 2 sin θ d s d θ d ϕ . {\displaystyle dx\,dy\,dz=abc\,s^{2}\sin \theta \,ds\,d\theta \,d\phi .}
See also
- Ellipsoidal latitude
- Focaloid (shell given by two coordinate surfaces)
- Map projection of the triaxial ellipsoid
Bibliography
- Morse PM, Feshbach H (1953). Methods of Theoretical Physics, Part I. New York: McGraw-Hill. p. 663.
- Zwillinger D (1992). Handbook of Integration. Boston, MA: Jones and Bartlett. p. 114. ISBN 0-86720-293-9.
- Sauer R, Szabó I (1967). Mathematische Hilfsmittel des Ingenieurs. New York: Springer Verlag. pp. 101–102. LCCN .
- Korn GA, Korn TM (1961). . New York: McGraw-Hill. p. . LCCN .
- Margenau H, Murphy GM (1956). . New York: D. van Nostrand. pp. –180. LCCN .
- Moon PH, Spencer DE (1988). "Ellipsoidal Coordinates (η, θ, λ)". (corrected 2nd, 3rd print ed.). New York: Springer Verlag. pp. –44 (Table 1.10). ISBN 0-387-02732-7.
Unusual convention
- Landau LD, Lifshitz EM, Pitaevskii LP (1984). Electrodynamics of Continuous Media (Volume 8 of the Course of Theoretical Physics) (2nd ed.). New York: Pergamon Press. pp. 19–29. ISBN 978-0-7506-2634-7. Uses (ξ, η, ζ) coordinates that have the units of distance squared.