parabolic coordinates
Parabolic coordinates are a two-dimensional orthogonal coordinate system in which the coordinate lines are confocal parabolas. A three-dimensional version of parabolic coordinates is obtained by rotating the two-dimensional 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 are defined by the equations, in terms of Cartesian coordinates:
:
x = \sigma \tau
:
y = \frac{1}{2} \left( \tau^{2} - \sigma^{2} \right)
The curves of constant form confocal parabolae
:
2y = \frac{x^{2}}{\sigma^{2}} - \sigma^{2}
that open upwards (i.e., towards ), whereas the curves of constant form confocal parabolae
:
2y = -\frac{x^{2}}{\tau^{2}} + \tau^{2}
that open downwards (i.e., towards ). The foci of all these parabolae are located at the origin.
The Cartesian coordinates and can be converted to parabolic coordinates by:
:
\sigma = \operatorname{sign}(x)\sqrt{\sqrt{x^{2} +y^{2}}-y}
:
\tau = \sqrt{\sqrt{x^{2} +y^{2}}+y}
Two-dimensional scale factors
The scale factors for the parabolic coordinates are equal
:
h_{\sigma} = h_{\tau} = \sqrt{\sigma^{2} + \tau^{2}}
Hence, the infinitesimal element of area is
:
dA = \left( \sigma^{2} + \tau^{2} \right) d\sigma d\tau
and the Laplacian equals
:
\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)
Other differential operators such as
and can be expressed in the coordinates by substituting
the scale factors into the general formulae
found in orthogonal coordinates.
Three-dimensional parabolic coordinates
Image:Parabolic coordinates 3D.png 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 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 -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:
:
x = \sigma \tau \cos \varphi
:
y = \sigma \tau \sin \varphi
:
z = \frac{1}{2} \left(\tau^{2} - \sigma^{2} \right)
where the parabolae are now aligned with the -axis,
about which the rotation was carried out. Hence, the azimuthal angle is defined
:
\tan \varphi = \frac{y}{x}
The surfaces of constant form confocal paraboloids
:
2z = \frac{x^{2} + y^{2}}{\sigma^{2}} - \sigma^{2}
that open upwards (i.e., towards ) whereas the surfaces of constant form confocal paraboloids
:
2z = -\frac{x^{2} + y^{2}}{\tau^{2}} + \tau^{2}
that open downwards (i.e., towards ). The foci of all these paraboloids are located at the origin.
The Riemannian metric tensor associated with this coordinate system is
:
Three-dimensional scale factors
The three dimensional scale factors are:
:
:
:
It is seen that the scale factors and are the same as in the two-dimensional case. The infinitesimal volume element is then
:
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
and the Laplacian is given by
:
\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}
Other differential operators such as
and can be expressed in the coordinates by substituting
the scale factors into the general formulae
found in orthogonal coordinates.
See also
Bibliography
- {{cite book | author = Morse PM, 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 = 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, 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 uk for ξk.
- {{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}}