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Parabolic coordinates
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[[Image:Parabolic coords.svg|thumb|right|384px|In green, confocal parabolae opening upwards, <math>2y = \frac {x^2}{\sigma^2}-\sigma^2</math> In red, confocal parabolae opening downwards, <math>2y =-\frac{x^2}{\tau^2}+\tau^2</math>]] '''Parabolic coordinates''' are a two-dimensional [[orthogonal coordinates|orthogonal]] [[coordinate system]] in which the [[Coordinate system#Coordinate line|coordinate lines]] are [[confocal]] [[parabola]]s. [[Parabolic cylindrical coordinates|A three-dimensional version]] of parabolic coordinates is obtained by rotating the two-dimensional [[coordinate system|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 <math>(\sigma, \tau)</math> are defined by the equations, in terms of Cartesian coordinates: :<math> x = \sigma \tau </math> :<math> y = \frac{1}{2} \left( \tau^{2} - \sigma^{2} \right) </math> The curves of constant <math>\sigma</math> form confocal parabolae :<math> 2y = \frac{x^{2}}{\sigma^{2}} - \sigma^{2} </math> that open upwards (i.e., towards <math>+y</math>), whereas the curves of constant <math>\tau</math> form confocal parabolae :<math> 2y = -\frac{x^{2}}{\tau^{2}} + \tau^{2} </math> that open downwards (i.e., towards <math>-y</math>). The foci of all these parabolae are located at the origin. The Cartesian coordinates <math>x</math> and <math>y</math> can be converted to parabolic coordinates by: :<math> \sigma = \operatorname{sign}(x)\sqrt{\sqrt{x^{2} +y^{2}}-y} </math> :<math> \tau = \sqrt{\sqrt{x^{2} +y^{2}}+y} </math> ==Two-dimensional scale factors== The scale factors for the parabolic coordinates <math>(\sigma, \tau)</math> are equal :<math> h_{\sigma} = h_{\tau} = \sqrt{\sigma^{2} + \tau^{2}} </math> Hence, the infinitesimal element of area is :<math> dA = \left( \sigma^{2} + \tau^{2} \right) d\sigma d\tau </math> and the [[Laplacian]] equals :<math> \nabla^{2} \Phi = \frac{1}{\sigma^{2} + \tau^{2}} \left( \frac{\partial^{2} \Phi}{\partial \sigma^{2}} + \frac{\partial^{2} \Phi}{\partial \tau^{2}} \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>(\sigma, \tau)</math> by substituting the scale factors into the general formulae found in [[orthogonal coordinates]]. ==Three-dimensional parabolic coordinates== [[Image:Parabolic coordinates 3D.png|thumb|right|300px|[[Coordinate system#Coordinate surface|Coordinate surfaces]] of the three-dimensional parabolic coordinates. The red paraboloid corresponds to τ=2, the blue paraboloid corresponds to σ=1, and the yellow half-plane corresponds to φ=−60°. The three surfaces intersect at the point '''P''' (shown as a black sphere) with [[Cartesian coordinate system|Cartesian coordinates]] roughly (1.0, −1.732, 1.5).]] The two-dimensional parabolic coordinates form the basis for two sets of three-dimensional [[orthogonal coordinates]]. The [[parabolic cylindrical coordinates]] are produced by projecting in the <math>z</math>-direction. Rotation about the symmetry axis of the parabolae produces a set of confocal paraboloids, the coordinate system of tridimensional parabolic coordinates. Expressed in terms of cartesian coordinates: :<math> x = \sigma \tau \cos \varphi </math> :<math> y = \sigma \tau \sin \varphi </math> :<math> z = \frac{1}{2} \left(\tau^{2} - \sigma^{2} \right) </math> where the parabolae are now aligned with the <math>z</math>-axis, about which the rotation was carried out. Hence, the azimuthal angle <math>\varphi</math> is defined :<math> \tan \varphi = \frac{y}{x} </math> The surfaces of constant <math>\sigma</math> form confocal paraboloids :<math> 2z = \frac{x^{2} + y^{2}}{\sigma^{2}} - \sigma^{2} </math> that open upwards (i.e., towards <math>+z</math>) whereas the surfaces of constant <math>\tau</math> form confocal paraboloids :<math> 2z = -\frac{x^{2} + y^{2}}{\tau^{2}} + \tau^{2} </math> that open downwards (i.e., towards <math>-z</math>). The foci of all these paraboloids are located at the origin. The [[Riemannian manifold|Riemannian]] [[metric tensor]] associated with this coordinate system is :<math> g_{ij} = \begin{bmatrix} \sigma^2+\tau^2 & 0 & 0\\0 & \sigma^2+\tau^2 & 0\\0 & 0 & \sigma^2\tau^2 \end{bmatrix} </math> ==Three-dimensional scale factors== The three dimensional scale factors are: :<math>h_{\sigma} = \sqrt{\sigma^2+\tau^2}</math> :<math>h_{\tau} = \sqrt{\sigma^2+\tau^2}</math> :<math>h_{\varphi} = \sigma\tau</math> It is seen that the scale factors <math>h_{\sigma}</math> and <math>h_{\tau}</math> are the same as in the two-dimensional case. The infinitesimal volume element is then :<math> dV = h_\sigma h_\tau h_\varphi\, d\sigma\,d\tau\,d\varphi = \sigma\tau \left( \sigma^{2} + \tau^{2} \right)\,d\sigma\,d\tau\,d\varphi </math> and the Laplacian is given by :<math> \nabla^2 \Phi = \frac{1}{\sigma^{2} + \tau^{2}} \left[ \frac{1}{\sigma} \frac{\partial}{\partial \sigma} \left( \sigma \frac{\partial \Phi}{\partial \sigma} \right) + \frac{1}{\tau} \frac{\partial}{\partial \tau} \left( \tau \frac{\partial \Phi}{\partial \tau} \right)\right] + \frac{1}{\sigma^2\tau^2}\frac{\partial^2 \Phi}{\partial \varphi^2} </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>(\sigma, \tau, \phi)</math> by substituting the scale factors into the general formulae found in [[orthogonal coordinates]]. == See also == * [[Parabolic cylindrical coordinates]] * [[Orthogonal coordinate system]] * [[Curvilinear coordinates]] ==Bibliography== *{{cite book | author = [[Philip M. Morse|Morse PM]], [[Herman Feshbach|Feshbach H]] | year = 1953 | title = Methods of Theoretical Physics, Part I | publisher = McGraw-Hill | location = New York | isbn = 0-07-043316-X|lccn=52011515 | pages = 660}} *{{cite book | author = [[Henry Margenau|Margenau H]], Murphy GM | year = 1956 | title = The Mathematics of Physics and Chemistry | url = https://archive.org/details/mathematicsofphy0002marg| url-access = registration| publisher = D. van Nostrand | location = New York | pages = [https://archive.org/details/mathematicsofphy0002marg/page/185 185–186] | lccn = 55010911 }} *{{cite book | author = Korn GA, [[Theresa M. Korn|Korn TM]] |year = 1961 | title = Mathematical Handbook for Scientists and Engineers | publisher = McGraw-Hill | location = New York | id = ASIN B0000CKZX7 | pages = 180 | lccn = 59014456}} *{{cite book | author = Sauer R, Szabó I | year = 1967 | title = Mathematische Hilfsmittel des Ingenieurs | publisher = Springer Verlag | location = New York | pages = 96 | lccn = 67025285}} *{{cite book | author = Zwillinger D | year = 1992 | title = Handbook of Integration | publisher = Jones and Bartlett | location = Boston, MA | isbn = 0-86720-293-9 | pages = 114}} Same as Morse & Feshbach (1953), substituting ''u''<sub>''k''</sub> for ξ<sub>''k''</sub>. *{{cite book | author = Moon P, Spencer DE | year = 1988 | chapter = Parabolic Coordinates (μ, ν, ψ) | title = Field Theory Handbook, Including Coordinate Systems, Differential Equations, and Their Solutions | edition = corrected 2nd ed., 3rd print | publisher = Springer-Verlag | location = New York | pages = 34–36 (Table 1.08) | isbn = 978-0-387-18430-2}} ==External links== * {{springer|title=Parabolic coordinates|id=p/p071170}} *[http://mathworld.wolfram.com/ParabolicCoordinates.html MathWorld description of parabolic coordinates] {{Orthogonal coordinate systems}} [[Category:Orthogonal coordinate systems]]
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