two-center bipolar coordinates

Image:Two-centerBipolarCoordinateSystem.JPG

In mathematics, two-center bipolar coordinates is a coordinate system based on two coordinates which give distances from two fixed centers c_1 and c_2.{{mathworld|urlname=BipolarCoordinates|title=Bipolar coordinates}} This system is very useful in some scientific applications (e.g. calculating the electric field of a dipole on a plane).[http://www.physics.utah.edu/~rprice/AREA51DOCS/paperIIa.pdf R. Price, The Periodic Standing Wave Approximation: Adapted coordinates and spectral methods.][https://arxiv.org/abs/gr-qc/0502034v1 The periodic standing-wave approximation: nonlinear scalar fields, adapted coordinates, and the eigenspectral method.]

Transformation to Cartesian coordinates

When the centers are at (+a, 0) and (-a, 0), the transformation to Cartesian coordinates (x, y) from two-center bipolar coordinates (r_1, r_2) is

:x = \frac{r_2^2-r_1^2}{4a}

:y = \pm \frac{1}{4a}\sqrt{16a^2r_2^2-(r_2^2-r_1^2+4a^2)^2}

Transformation to polar coordinates

When x > 0, the transformation to polar coordinates from two-center bipolar coordinates is

:r = \sqrt{\frac{r_1^2+r_2^2-2a^2}{2}}

:\theta = \arctan\left( \frac{\sqrt{r_1^4-8a^2r_1^2-2r_1^2r_2^2-(4a^2-r_2^2)^2}}{r_2^2-r_1^2} \right)

where 2 a is the distance between the poles (coordinate system centers).

Applications

Polar plotters use two-center bipolar coordinates to describe the drawing paths required to draw a target image.

See also

References

{{Orthogonal coordinate systems}}

Two-center bipolar coordinates

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