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Two-center bipolar coordinates

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Two-center bipolar coordinates.

In mathematics, two-center bipolar coordinates is a coordinate system based on two coordinates which give distances from two fixed centers c 1 {\displaystyle c_{1}} and c 2 {\displaystyle c_{2}} . This system is very useful in some scientific applications (e.g. calculating the electric field of a dipole on a plane).

Transformation to Cartesian coordinates

When the centers are at ( + a , 0 ) {\displaystyle (+a,0)} and ( a , 0 ) {\displaystyle (-a,0)} , the transformation to Cartesian coordinates ( x , y ) {\displaystyle (x,y)} from two-center bipolar coordinates ( r 1 , r 2 ) {\displaystyle (r_{1},r_{2})} is

x = r 2 2 r 1 2 4 a {\displaystyle x={\frac {r_{2}^{2}-r_{1}^{2}}{4a}}}
y = ± 1 4 a 16 a 2 r 2 2 ( r 2 2 r 1 2 + 4 a 2 ) 2 {\displaystyle y=\pm {\frac {1}{4a}}{\sqrt {16a^{2}r_{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 = r 1 2 + r 2 2 2 a 2 2 {\displaystyle r={\sqrt {\frac {r_{1}^{2}+r_{2}^{2}-2a^{2}}{2}}}}
θ = arctan ( r 1 4 8 a 2 r 1 2 2 r 1 2 r 2 2 ( 4 a 2 r 2 2 ) 2 r 2 2 r 1 2 ) {\displaystyle \theta =\arctan \left({\frac {\sqrt {r_{1}^{4}-8a^{2}r_{1}^{2}-2r_{1}^{2}r_{2}^{2}-(4a^{2}-r_{2}^{2})^{2}}}{r_{2}^{2}-r_{1}^{2}}}\right)}

where 2 a {\displaystyle 2a} 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

  1. ^ Weisstein, Eric W. "Bipolar coordinates". MathWorld.
  2. R. Price, The Periodic Standing Wave Approximation: Adapted coordinates and spectral methods.
  3. The periodic standing-wave approximation: nonlinear scalar fields, adapted coordinates, and the eigenspectral method.
Orthogonal coordinate systems
Two dimensional
Three dimensional


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