Oblate spheroidal coordinates

Oblate spheroidal coordinates are a three-dimensional orthogonal coordinate system that results from rotating the two-dimensional elliptic coordinate system about the non-focal axis of the ellipse, i.e., the symmetry axis that separates the foci. Thus, the two foci are transformed into a ring of radius $a$ in the ''x''-''y'' plane. (Rotation about the other axis produces prolate spheroidal coordinates.) Oblate spheroidal coordinates can also be considered as a limiting case of ellipsoidal coordinates in which the two largest semi-axes are equal in length.

Oblate spheroidal coordinates are often useful in solving partial differential equations when the boundary conditions are defined on an oblate spheroid or a hyperboloid of revolution. For example, they played an important role in the calculation of the Perrin friction factors, which contributed to the awarding of the 1926 Nobel Prize in Physics to Jean Baptiste Perrin. These friction factors determine the rotational diffusion of molecules, which affects the feasibility of many techniques such as protein NMR and from which the hydrodynamic volume and shape of molecules can be inferred. Oblate spheroidal coordinates are also useful in problems of electromagnetism (e.g., dielectric constant of charged oblate molecules), acoustics (e.g., scattering of sound through a circular hole), fluid dynamics (e.g., the flow of water through a firehose nozzle), the diffusion of materials and heat (e.g., cooling of a red-hot coin in a water bath), and relativistic physics, such as the spacetime distortion around rotating black holes.

Definition (μ,ν,φ)

The most common definition of oblate spheroidal coordinates $(\mu, \nu, \varphi)$ is
$\begin x &= a \ \cosh \mu \ \cos \nu \ \cos \varphi \\ y &= a \ \cosh \mu \ \cos \nu \ \sin \varphi \\ z &= a \ \sinh \mu \ \sin \nu \end$

where $\mu$ is a nonnegative real number and the angle \nu\in\left \pi/2,\pi/2\right/math>. The azimuthal angle $\varphi$ can fall anywhere on a full circle, between $\pm\pi$. These coordinates are favored over the alternatives below because they are not degenerate; the set of coordinates $(\mu, \nu, \varphi)$ describes a unique point in Cartesian coordinates $(x,y,z)$. The reverse is also true, except on the $z$-axis and the disk in the $xy$-plane inside the focal ring.

Coordinate surfaces

The surfaces of constant μ form oblate spheroids, by the trigonometric identity
$\frac + \frac = \cos^2 \nu + \sin^2 \nu = 1$

since they are ellipses rotated about the ''z''-axis, which separates their foci. An ellipse in the ''x''-''z'' plane (Figure 2) has a major semiaxis of length ''a'' cosh μ along the ''x''-axis, whereas its minor semiaxis has length ''a'' sinh μ along the ''z''-axis. The foci of all the ellipses in the ''x''-''z'' plane are located on the ''x''-axis at ±''a''.

Similarly, the surfaces of constant ν form one-sheet half hyperboloids of revolution by the hyperbolic trigonometric identity

$\frac - \frac = \cosh^ \mu - \sinh^ \mu = 1$

For positive , the half-hyperboloid is above the ''x''-''y'' plane (i.e., has positive ''z'') whereas for negative ν, the half-hyperboloid is below the ''x''-''y'' plane (i.e., has negative ''z''). Geometrically, the angle ν corresponds to the angle of the asymptotes of the hyperbola. The foci of all the hyperbolae are likewise located on the ''x''-axis at ±''a''.

Inverse transformation

The (μ, ν, φ) coordinates may be calculated from the Cartesian coordinates (''x'', ''y'', ''z'') as follows. The azimuthal angle φ is given by the formula
$\tan \phi = \frac$

The cylindrical radius ρ of the point P is given by
$\rho^2 = x^2 + y^2$
and its distances to the foci in the plane defined by φ is given by
$\begin d_1^2 = (\rho + a)^2 + z^2 \\ d_2^2 = (\rho - a)^2 + z^2 \end$

The remaining coordinates μ and ν can be calculated from the equations
$\begin \cosh \mu &= \frac \\ \cos \nu &= \frac \end$

where the sign of μ is always non-negative, and the sign of ν is the same as that of ''z''.

Another method to compute the inverse transform is

$\begin \mu &= \operatorname \operatorname \frac \\ \nu &= \operatorname \operatorname \frac \\ \phi &= \arctan \frac \end$

where $\rho = \sqrt$

Scale factors

The scale factors for the coordinates and are equal
$h_ = h_ = a\sqrt$
whereas the azimuthal scale factor equals
$h_ = a \cosh\mu \ \cos\nu$

Consequently, an infinitesimal volume element equals
$dV = a^ \cosh\mu \ \cos\nu \ \left( \sinh^\mu + \sin^\nu \right) d\mu \, d\nu \, d\phi$
and the Laplacian can be written

\nabla^ \Phi =
\frac
\left \frac \frac
\left( \cosh \mu \frac \right) +
\frac \frac
\left( \cos \nu \frac \right)
\right+
\frac
\frac

Other differential operators such as $\nabla \cdot \mathbf$ and $\nabla \times \mathbf$ can be expressed in the coordinates (μ, ν, φ) by substituting the scale factors into the general formulae found in orthogonal coordinates.

Basis Vectors

The orthonormal basis vectors for the $\mu,\nu,\phi$ coordinate system can be expressed in Cartesian coordinates as

$\begin \hat_ &= \frac \left( \sinh \mu \cos \nu \cos \phi \boldsymbol + \sinh \mu \cos \nu \sin \phi \boldsymbol + \cosh \mu \sin \nu \boldsymbol\right) \\ \hat_ &= \frac \left( - \cosh \mu \sin \nu \cos \phi \boldsymbol - \cosh \mu \sin \nu \sin \phi \boldsymbol + \sinh \mu \cos \nu \boldsymbol \right) \\ \hat_ &= -\sin \phi \boldsymbol + \cos \phi \boldsymbol \end$

where $\boldsymbol, \boldsymbol, \boldsymbol$ are the Cartesian unit vectors. Here, $\hat_$ is the outward normal vector to the oblate spheroidal surface of constant $\mu$, $\hat_$ is the same azimuthal unit vector from spherical coordinates, and $\hat_$ lies in the tangent plane to the oblate spheroid surface and completes the right-handed basis set.

Definition (ζ, ξ, φ)

Another set of oblate spheroidal coordinates $(\zeta,\xi,\phi)$ are sometimes used where $\zeta = \sinh \mu$ and $\xi = \sin \nu$ (Smythe 1968). The curves of constant $\zeta$ are oblate spheroids and the curves of constant $\xi$ are the hyperboloids of revolution. The coordinate $\zeta$ is restricted by $0 \le \zeta < \infty$ and $\xi$ is restricted by $-1 \le \xi < 1$.

The relationship to Cartesian coordinates is
$\begin x = a\sqrt\,\cos \phi \\ y = a\sqrt\,\sin \phi \\ z = a \zeta \xi \end$

Scale factors

The scale factors for $(\zeta, \xi, \phi)$ are:
$\begin h_ &= a\sqrt \\ h_ &= a\sqrt \\ h_ &= a\sqrt \end$

Knowing the scale factors, various functions of the coordinates can be calculated by the general method outlined in the orthogonal coordinates article. The infinitesimal volume element is:
$dV = a^3 \left(\zeta^2+\xi^2\right) d\zeta\,d\xi\,d\phi$

The gradient is:
$\nabla V = \frac \frac \,\hat+ \frac \frac \,\hat+ \frac \frac \,\hat$

The divergence is:
$\nabla \cdot \mathbf = \frac \left\ +\frac \frac$

and the Laplacian equals
$\nabla^ V = \frac \left\ + \frac \frac$

Oblate spheroidal harmonics

As is the case with spherical coordinates and spherical harmonics, Laplace's equation may be solved by the method of separation of variables to yield solutions in the form of oblate spheroidal harmonics, which are convenient to use when boundary conditions are defined on a surface with a constant oblate spheroidal coordinate.

Following the technique of separation of variables, a solution to Laplace's equation is written:
$V=Z(\zeta)\,\Xi(\xi)\,\Phi(\phi)$

This yields three separate differential equations in each of the variables:
\begin
\frac\left 1+\zeta^2)\frac\right\frac-n(n+1)Z = 0 \\
\frac\left 1-\xi^2 )\frac\right\frac+n(n+1)\Xi = 0 \\
\frac=-m^2\Phi
\end
where is a constant which is an integer because the φ variable is periodic with period 2π. ''n'' will then be an integer. The solution to these equations are:
\begin
Z_ &= A_1 P_n^m(i\zeta)+A_2Q_n^m(i\zeta) \\ ex\Xi_ &= A_3 P_n^m(\xi)+A_4Q_n^m(\xi) \\ ex\Phi_m &= A_5 e^+A_6e^
\end
where the $A_i$ are constants and $P_n^m(z)$ and $Q_n^m(z)$ are associated Legendre polynomials of the first and second kind respectively. The product of the three solutions is called an ''oblate spheroidal harmonic'' and the general solution to Laplace's equation is written:
$V = \sum_^\infty\sum_^\infty\,Z_(\zeta)\,\Xi_(\xi)\,\Phi_m(\phi)$

The constants will combine to yield only four independent constants for each harmonic.

Definition (σ, τ, φ)

An alternative and geometrically intuitive set of oblate spheroidal coordinates (σ, τ, φ) are sometimes used, where σ = cosh μ and τ = cos ν.Abramowitz and Stegun, p. 752. Therefore, the coordinate σ must be greater than or equal to one, whereas τ must lie between ±1, inclusive. The surfaces of constant σ are oblate spheroids, as were those of constant μ, whereas the curves of constant τ are full hyperboloids of revolution, including the half-hyperboloids corresponding to ±ν. Thus, these coordinates are degenerate; ''two'' points in Cartesian coordinates (''x'', ''y'', ±''z'') map to ''one'' set of coordinates (σ, τ, φ). This two-fold degeneracy in the sign of ''z'' is evident from the equations transforming from oblate spheroidal coordinates to the Cartesian coordinates
$\begin x &= a\sigma\tau \cos \phi \\ y &= a\sigma\tau \sin \phi \\ z^2 &= a^2 \left( \sigma^2 - 1 \right) \left(1 - \tau^2 \right) \end$

The coordinates $\sigma$ and $\tau$ have a simple relation to the distances to the focal ring. For any point, the ''sum'' $d_1 + d_2$ of its distances to the focal ring equals $2a\sigma$, whereas their ''difference'' $d_1 - d_2$ equals $2a\tau$. Thus, the "far" distance to the focal ring is $a(\sigma+\tau)$, whereas the "near" distance is $a(\sigma-\tau)$.

Coordinate surfaces

Similar to its counterpart μ, the surfaces of constant σ form oblate spheroids
$\frac + \frac = 1$

Similarly, the surfaces of constant τ form full one-sheet hyperboloids of revolution
$\frac - \frac = 1$

Scale factors

The scale factors for the alternative oblate spheroidal coordinates $(\sigma, \tau, \phi)$ are
$\begin h_\sigma = a\sqrt \\ h_\tau = a\sqrt \end$
whereas the azimuthal scale factor is $h_ = a \sigma \tau$.

Hence, the infinitesimal volume element can be written
$dV = a^3 \sigma \tau \frac \, d\sigma \, d\tau \, d\phi$
and the Laplacian equals
$\nabla^2 \Phi = \frac \left\ + \frac \frac$

Other differential operators such as $\nabla \cdot \mathbf$ and $\nabla \times \mathbf$ can be expressed in the coordinates $(\sigma, \tau)$ by substituting the scale factors into the general formulae found in orthogonal coordinates.

As is the case with spherical coordinates, Laplaces equation may be solved by the method of separation of variables to yield solutions in the form of oblate spheroidal harmonics, which are convenient to use when boundary conditions are defined on a surface with a constant oblate spheroidal coordinate (See Smythe, 1968).

See also

* Ellipsoidal coordinates (geodesy)

References

Bibliography

No angles convention

* Uses ξ₁ = a sinh μ, ξ₂ = sin ν, and ξ₃ = cos φ.
* Same as Morse & Feshbach (1953), substituting ''u''_''k'' for ξ_''k''.
*
* Uses hybrid coordinates ξ = sinh μ, η = sin ν, and φ.

Angle convention

* Korn and Korn use the (μ, ν, φ) coordinates, but also introduce the degenerate (σ, τ, φ) coordinates.
* Like Korn and Korn (1961), but uses colatitude θ = 90° - ν instead of latitude ν.
* Moon and Spencer use the colatitude convention θ = 90° - ν, and rename φ as ψ.

Unusual convention

* Treats the oblate spheroidal coordinates as a limiting case of the general ellipsoidal coordinates. Uses (ξ, η, ζ) coordinates that have the units of distance squared.

External links

MathWorld description of oblate spheroidal coordinates

{{Orthogonal coordinate systems

Three-dimensional coordinate systems
Orthogonal coordinate systems