Elliptic cylindrical coordinates: Difference between revisions

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'''Ellipsoidal coordinates''' are a three-dimensional [[orthogonal coordinates|orthogonal]] [[coordinate system]] <math>(\lambda, \mu, \nu)</math> that generalizes the two-dimensional [[elliptic coordinates|elliptic coordinate system]]. Unlike most three-dimensional [[orthogonal coordinates|orthogonal]] [[coordinate system]]s that feature [[quadratic function|quadratic]] [[Coordinate system#Coordinate surface|coordinate surfaces]], the ellipsoidal coordinate system is not produced by rotating or projecting any two-dimensional orthogonal coordinate system.
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==Basic formulae==
 
The Cartesian coordinates <math>(x, y, z)</math> can be produced from the ellipsoidal coordinates
<math>( \lambda, \mu, \nu )</math> by the equations
 
:<math>
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)}
</math>
 
:<math>
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)}
</math>
 
:<math>
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)}
</math>
 
where the following limits apply to the coordinates
 
:<math>
- \lambda < c^{2} < - \mu < b^{2} < -\nu < a^{2}.
</math>
 
 
Consequently, surfaces of constant <math>\lambda</math> are [[ellipsoid]]s
 
:<math>
\frac{x^{2}}{a^{2} + \lambda} +  \frac{y^{2}}{b^{2} + \lambda} + \frac{z^{2}}{c^{2} + \lambda} = 1,
</math>
 
whereas surfaces of constant <math>\mu</math> are [[hyperboloid]]s of one sheet
 
:<math>
\frac{x^{2}}{a^{2} + \mu} +  \frac{y^{2}}{b^{2} + \mu} + \frac{z^{2}}{c^{2} + \mu} = 1,
</math>
 
because the last term in the lhs is negative, and surfaces of constant <math>\nu</math> are [[hyperboloid]]s of two sheets
:<math>
\frac{x^{2}}{a^{2} + \nu} +  \frac{y^{2}}{b^{2} + \nu} + \frac{z^{2}}{c^{2} + \nu} = 1
</math>
 
because the last two terms in the lhs are negative.
 
==Scale factors and differential operators==
 
For brevity in the equations below, we introduce a function
 
:<math>
S(\sigma) \ \stackrel{\mathrm{def}}{=}\  \left( a^{2} + \sigma \right) \left( b^{2} + \sigma \right) \left( c^{2} + \sigma \right)
</math>
 
where <math>\sigma</math> can represent any of the three variables <math>(\lambda, \mu, \nu )</math>.
Using this function, the scale factors can be written
:<math>
h_{\lambda} = \frac{1}{2} \sqrt{\frac{\left( \lambda - \mu \right) \left( \lambda - \nu\right)}{S(\lambda)}}
</math>
 
:<math>
h_{\mu} = \frac{1}{2} \sqrt{\frac{\left( \mu - \lambda\right) \left( \mu - \nu\right)}{S(\mu)}}
</math>
 
:<math>
h_{\nu} = \frac{1}{2} \sqrt{\frac{\left( \nu - \lambda\right) \left( \nu - \mu\right)}{S(\nu)}}
</math>
 
Hence, the infinitesimal volume element equals
 
:<math>
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
</math>
 
and the [[Laplacian]] is defined by
 
:<math>
\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] \  +  \
</math>
:::::<math>
\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] \  + \ 
\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]
</math>
 
Other differential operators such as <math>\nabla \cdot \mathbf{F}</math>
and <math>\nabla \times \mathbf{F}</math> can be expressed in the coordinates <math>(\lambda, \mu, \nu)</math> by substituting
the scale factors into the general formulae
found in [[orthogonal coordinates]].
 
==See also==
* [[Focaloid]] (shell given by two coordinate surfaces)
 
==References==
{{reflist}}
 
==Bibliography==
*{{cite book | author = Morse PM, Feshbach H | year = 1953 | title = Methods of Theoretical Physics, Part I | publisher = McGraw-Hill | location = New York | page = 663}}
*{{cite book | author = Zwillinger D | year = 1992 | title = Handbook of Integration | publisher = Jones and Bartlett | location = Boston, MA | isbn = 0-86720-293-9 | page = 114}}
*{{cite book | author = Sauer R, Szabó I | year = 1967 | title = Mathematische Hilfsmittel des Ingenieurs | publisher = Springer Verlag | location = New York | pages = 101&ndash;102 | lccn = 6725285}} 
*{{cite book | author = Korn GA, Korn TM |year = 1961 | title = Mathematical Handbook for Scientists and Engineers | publisher = McGraw-Hill | location = New York | page = 176 | lccn = 5914456}}
*{{cite book | author = Margenau H, Murphy GM | year = 1956 | title = The Mathematics of Physics and Chemistry | publisher = D. van Nostrand | location = New York| pages = 178&ndash;180 | lccn = 5510911 }}
*{{cite book | author = Moon PH, Spencer DE | year = 1988 | chapter = Ellipsoidal Coordinates (η, θ, λ) | title = Field Theory Handbook, Including Coordinate Systems, Differential Equations, and Their Solutions | edition = corrected 2nd ed., 3rd print | publisher = Springer Verlag | location = New York | isbn = 0-387-02732-7 | pages = 40&ndash;44 (Table 1.10)}}
 
===Unusual convention===
*{{cite book | author = Landau LD, Lifshitz EM, Pitaevskii LP | year = 1984 | title = Electrodynamics of Continuous Media (Volume 8 of the [[Course of Theoretical Physics]]) | edition = 2nd | publisher = Pergamon Press | location = New York | isbn = 978-0-7506-2634-7 | pages = 19&ndash;29 }}  Uses (ξ, η, ζ) coordinates that have the units of distance squared.
 
==External links==
*[http://mathworld.wolfram.com/ConfocalEllipsoidalCoordinates.html MathWorld description of confocal ellipsoidal coordinates]
 
{{Orthogonal coordinate systems}}
 
[[Category:Coordinate systems]]

Latest revision as of 05:38, 25 August 2014

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