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Bipolar coordinates
Bipolar coordinates
from Wikipedia
Bipolar coordinate system

Bipolar coordinates are a two-dimensional orthogonal coordinate system based on the Apollonian circles.[1] There is also a third system, based on two poles (biangular coordinates).

The term "bipolar" is further used on occasion to describe other curves having two singular points (foci), such as ellipses, hyperbolas, and Cassini ovals. However, the term bipolar coordinates is reserved for the coordinates described here, and never used for systems associated with those other curves, such as elliptic coordinates.

Geometric interpretation of the bipolar coordinates. The angle σ is formed by the two foci and the point P, whereas τ is the logarithm of the ratio of distances to the foci. The corresponding circles of constant σ and τ are shown in red and blue, respectively, and meet at right angles (magenta box); they are orthogonal.

Definition

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The system is based on two foci F1 and F2. Referring to the figure at right, the σ-coordinate of a point P equals the angle F1 P F2, and the τ-coordinate equals the natural logarithm of the ratio of the distances d1 and d2:

If, in the Cartesian system, the foci are taken to lie at (−a, 0) and (a, 0), the coordinates of the point P are

The coordinate τ ranges from (for points close to F1) to (for points close to F2). The coordinate σ is only defined modulo , and is best taken to range from −π to π, by taking it as the negative of the acute angle F1 P F2 if P is in the lower half plane.

Proof that coordinate system is orthogonal

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The equations for x and y can be combined to give

[2][3]

or

This equation shows that σ and τ are the real and imaginary parts of an analytic function of x+iy (with logarithmic branch points at the foci), which in turn proves (by appeal to the general theory of conformal mapping) (the Cauchy-Riemann equations) that these particular curves of σ and τ intersect at right angles, i.e., it is an orthogonal coordinate system.

Curves of constant σ and τ

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The curves of constant σ correspond to non-concentric circles

that intersect at the two foci. The centers of the constant-σ circles lie on the y-axis at with radius . Circles of positive σ are centered above the x-axis, whereas those of negative σ lie below the axis. As the magnitude |σ| − π/2 decreases, the radius of the circles decreases and the center approaches the origin (0, 0), which is reached when |σ| = π/2. (From elementary geometry, all triangles on a circle with 2 vertices on opposite ends of a diameter are right triangles.)

The curves of constant are non-intersecting circles of different radii

that surround the foci but again are not concentric. The centers of the constant-τ circles lie on the x-axis at with radius . The circles of positive τ lie in the right-hand side of the plane (x > 0), whereas the circles of negative τ lie in the left-hand side of the plane (x < 0). The τ = 0 curve corresponds to the y-axis (x = 0). As the magnitude of τ increases, the radius of the circles decreases and their centers approach the foci.

Inverse relations

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The passage from the Cartesian coordinates towards the bipolar coordinates can be done via the following formulas:

and

The coordinates also have the identities:

and

which can derived by solving Eq. (1) and (2) for and , respectively.

Scale factors

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To obtain the scale factors for bipolar coordinates, we take the differential of the equation for , which gives

Multiplying this equation with its complex conjugate yields

Employing the trigonometric identities for products of sines and cosines, we obtain

from which it follows that

Hence the scale factors for σ and τ are equal, and given by

Many results now follow in quick succession from the general formulae for orthogonal coordinates. Thus, the infinitesimal area element equals

and the Laplacian is given by

Expressions for , , and can be expressed obtained by substituting the scale factors into the general formulae found in orthogonal coordinates.

Applications

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The classic applications of bipolar coordinates are in solving partial differential equations, e.g., Laplace's equation or the Helmholtz equation, for which bipolar coordinates allow a separation of variables. An example is the electric field surrounding two parallel cylindrical conductors with unequal diameters.

Extension to 3-dimensions

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Bipolar coordinates form the basis for several sets of three-dimensional orthogonal coordinates.

  • The bispherical coordinates are produced by rotating the bipolar coordinates about the x-axis, i.e., the axis connecting the foci.
  • The toroidal coordinates are produced by rotating the bipolar coordinates about the y-axis, i.e., the axis separating the foci.

See also

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References

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
Bipolar coordinates are a two-dimensional orthogonal curvilinear coordinate system defined relative to two fixed foci, or poles, separated by a distance 2a2a, where the coordinate curves consist of circles that either pass through both poles (constant angular coordinate ξ\xi) or have the poles as inverse points (constant radial-like coordinate η\eta). The transformation from Cartesian coordinates (x,y)(x, y) to bipolar coordinates (ξ,η)(\xi, \eta) is given by x=asinhηcoshηcosξ,y=asinξcoshηcosξ,x = a \frac{\sinh \eta}{\cosh \eta - \cos \xi}, \quad y = a \frac{\sin \xi}{\cosh \eta - \cos \xi}, with ξ[0,2π)\xi \in [0, 2\pi) and η(,)\eta \in (-\infty, \infty), ensuring the system covers the entire plane except the poles themselves. The scale factors for both coordinates are equal, hξ=hη=acoshηcosξh_\xi = h_\eta = \frac{a}{\cosh \eta - \cos \xi}, confirming orthogonality and enabling the separation of variables in Laplace's equation. In three dimensions, bipolar coordinates extend to a cylindrical form (ξ,η,z)(\xi, \eta, z) by including the axial coordinate zz unchanged, with scale factor hz=1h_z = 1, resulting in coordinate surfaces that are circular cylinders and planes parallel to the xyxy-plane. This system is particularly suited for problems exhibiting around two parallel axes, such as the electrostatic potential between two charged cylindrical conductors or the due to parallel current-carrying wires. Bipolar coordinates find applications in various fields of physics and engineering, including steady-state heat conduction in regions with embedded cylindrical pipes, fluid dynamics around pairs of cylinders, and diffusion processes in domains with circular inclusions. They also appear in electromagnetic theory for analyzing transmission lines and in mathematical modeling of axisymmetric flows, such as locomotion within surfactant-laden droplets. The separability of the Helmholtz and Laplace equations in this system facilitates analytical solutions to boundary value problems that are intractable in Cartesian coordinates.

Definition and Geometry

Definition

Bipolar coordinates constitute a two-dimensional orthogonal curvilinear in the , defined relative to two fixed foci separated by a 2a2a where a>0a > 0. The foci are conventionally placed at F1=(a,0)F_1 = (-a, 0) and F2=(a,0)F_2 = (a, 0) along the x-axis in Cartesian coordinates. The coordinates are denoted by σ\sigma and τ\tau, where σ[0,2π)\sigma \in [0, 2\pi) represents the angle subtended by the segment joining the two foci at a point PP in the plane, and τ(,)\tau \in (-\infty, \infty) is the hyperbolic coordinate given by τ=ln(d1/d2)\tau = \ln(d_1 / d_2), with d1d_1 and d2d_2 being the Euclidean distances from PP to F1F_1 and F2F_2, respectively. The transformation from bipolar to Cartesian coordinates (x,y)(x, y) is expressed as: x=asinhτcoshτcosσ,y=asinσcoshτcosσ.x = \frac{a \sinh \tau}{\cosh \tau - \cos \sigma}, \quad y = \frac{a \sin \sigma}{\cosh \tau - \cos \sigma}. These relations map the entire plane excluding the foci, with the denominator ensuring the coordinates cover non-singular points. The level sets of constant σ\sigma and constant τ\tau form two families of circles known as , which are orthogonal to each other and pass through or are centered relative to the foci, providing the geometric basis for the coordinate system's utility in problems with around two points.

Coordinate Curves

In bipolar coordinates, the curves of constant σ form a family of circles that pass through the two foci located at (±a, 0) on the x-axis, where a > 0 is the . These circles, known as , have their centers on the y-axis at (0, a cot σ), with σ ranging from 0 to 2π (excluding σ = π, where the curve degenerates). The radius of each such circle is a |csc σ|. The Cartesian equation for a fixed σ is given by x2+(yacotσ)2=a2csc2σ.x^2 + (y - a \cot \sigma)^2 = a^2 \csc^2 \sigma. This family constitutes a confocal pencil of circles, where all members intersect at the foci but do not intersect elsewhere within the family. The curves of constant τ form another family of circles that are orthogonal to the constant-σ family. These circles do not pass through the foci; instead, they enclose one focus or the other depending on the sign of τ, which ranges from -∞ to +∞. The centers lie on the x-axis at (a coth τ, 0), and the radius is a |csch τ|. The Cartesian equation for a fixed τ is (xacothτ)2+y2=a2\csch2τ.(x - a \coth \tau)^2 + y^2 = a^2 \csch^2 \tau. Curves within this family do not intersect each other. Regarding asymptotic behavior, as σ approaches 0 or 2π, the constant-σ circles grow large with centers moving far along the y-axis, causing the arcs between the foci to approach the line segment on the x-axis connecting the two foci. For constant-τ curves, as τ approaches ±∞, the circles shrink toward the foci, with centers approaching (±a, 0) and radii tending to zero.

Mathematical Properties

Orthogonality

In curvilinear coordinate systems, requires that the basis vectors along the coordinate directions are , meaning their vanishes: eσeτ=0\mathbf{e}_\sigma \cdot \mathbf{e}_\tau = 0. This condition is equivalent to rσrτ=0\frac{\partial \mathbf{r}}{\partial \sigma} \cdot \frac{\partial \mathbf{r}}{\partial \tau} = 0, where r(σ,τ)\mathbf{r}(\sigma, \tau) is the position vector in Cartesian coordinates.$$] For bipolar coordinates, the position vector is [ \mathbf{r}(\sigma, \tau) = \left( a \frac{\sinh \tau}{\cosh \tau - \cos \sigma}, , a \frac{\sin \sigma}{\cosh \tau - \cos \sigma} \right), with foci at $(\pm a, 0)$ and parameters $\sigma \in [0, 2\pi)$ and $\tau \in (-\infty, \infty)$.$$\] To verify the condition explicitly, denote $D = \cosh \tau - \cos \sigma$. The partial derivatives are \[ \frac{\partial x}{\partial \sigma} = -\frac{a \sinh \tau \sin \sigma}{D^2}, \quad \frac{\partial y}{\partial \sigma} = \frac{a (\cosh \tau \cos \sigma - 1)}{D^2}, xτ=a(cosh2τcoshτcosσsinh2τ)D2=a(1coshτcosσ)D2,yτ=asinσsinhτD2.\frac{\partial x}{\partial \tau} = \frac{a (\cosh^2 \tau - \cosh \tau \cos \sigma - \sinh^2 \tau)}{D^2} = \frac{a (1 - \cosh \tau \cos \sigma)}{D^2}, \quad \frac{\partial y}{\partial \tau} = -\frac{a \sin \sigma \sinh \tau}{D^2}. The dot product is then xσxτ+yσyτ=a2sinhτsinσD4[(coshτDsinh2τ)+(cosσDsin2σ)].\frac{\partial x}{\partial \sigma} \frac{\partial x}{\partial \tau} + \frac{\partial y}{\partial \sigma} \frac{\partial y}{\partial \tau} = -\frac{a^2 \sinh \tau \sin \sigma}{D^4} \left[ (\cosh \tau D - \sinh^2 \tau) + (\cos \sigma D - \sin^2 \sigma) \right]. The expression in brackets simplifies to coshτD+cosσDsinh2τsin2σ=(cosh2τsinh2τ)(cos2σ+sin2σ)=11=0\cosh \tau D + \cos \sigma D - \sinh^2 \tau - \sin^2 \sigma = (\cosh^2 \tau - \sinh^2 \tau) - (\cos^2 \sigma + \sin^2 \sigma) = 1 - 1 = 0, yielding zero overall and confirming orthogonality.$$] The scale factors, which are the magnitudes of these basis vectors, are both hσ=hτ=a/Dh_\sigma = h_\tau = a / D. An alternative confirmation arises from the geometric interpretation: the curves of constant σ\sigma and constant τ\tau form two conjugate families of Apollonian circles, which intersect orthogonally by definition, as every circle in one family is perpendicular to every circle in the other.[$$ This orthogonal system covers the entire xyxy-plane except the line segment joining the foci (where τ=0\tau = 0 and σ\sigma is undefined), ensuring the coordinates are well-defined almost everywhere.$$]

Scale Factors

In orthogonal curvilinear coordinate systems, the scale factors hσh_\sigma and hτh_\tau quantify the stretching of infinitesimal displacements along the coordinate directions σ\sigma and τ\tau, respectively. They are given by hσ=rσh_\sigma = \left| \frac{\partial \mathbf{r}}{\partial \sigma} \right|
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