List of common coordinate transformations

From Wikipedia, the free encyclopedia
Jump to: navigation, search

This is a list of some of the most commonly used coordinate transformations.

2-Dimensional[edit]

Let (x, y) be the standard Cartesian coordinates, and r and θ the standard polar coordinates.

To Cartesian coordinates from polar coordinates[edit]

x=r\,\cos\theta \quad
y=r\,\sin\theta \quad

\frac{\partial(x, y)}{\partial(r, \theta)} =
\begin{pmatrix}
\cos\theta & -r\,\sin\theta  \\
\sin\theta & r\,\cos\theta
\end{pmatrix}

\det{\frac{\partial(x, y)}{\partial(r, \theta)}} =
r

To polar coordinates from Cartesian coordinates[edit]

r=\sqrt{x^2 + y^2}
\theta^\prime = \arctan\left|\frac{y}{x}\right|

Note: solving for \theta^\prime returns the resultant angle in the first quadrant (0<\theta<\frac{\pi}{2}). To find \theta, one must refer to the original Cartesian coordinate, determine the quadrant in which \theta lies (ex (3,-3) [Cartesian] lies in QIV), then use the following to solve for \theta:

For \theta^\prime in QI:
\theta = \theta^\prime
For \theta^\prime in QII:
\theta= \pi - \theta^\prime
For \theta^\prime in QIII:
\theta = \pi + \theta^\prime
For \theta^\prime in QIV:
\theta = 2\pi - \theta^\prime

The value for \theta must be solved for in this manner because for all values of \theta, \tan\theta is only defined for -\frac{\pi}{2}<\theta<+\frac{\pi}{2}, and is periodic (with period \pi). This means that the inverse function will only give values in the domain of the function, but restricted to a single period. Hence, the range of the inverse function is only half a full circle.

Note that one can also use

r=\sqrt{x^2 + y^2}
\theta^\prime = 2 \arctan \frac{y}{x+r}

To Cartesian coordinates from log-polar coordinates[edit]

Main article: Log-polar coordinates
\begin{cases}x = e^\rho\cos\theta, \\ y = e^\rho\sin\theta.\end{cases}

By using complex numbers (x,y)=x+iy', the transformation can be written as

 x + iy = e^{\rho+i\theta} \,

i.e. it is given by the complex exponential function.

To log-polar coordinates from Cartesian coordinates[edit]

\begin{cases} \rho = \log\sqrt{ x^2 + y^2}, \\ \theta = \arctan \frac{y}{x}.  \end{cases}

To Cartesian coordinates from bipolar coordinates[edit]

Main article: bipolar coordinates

x = a \ \frac{\sinh \tau}{\cosh \tau - \cos \sigma}

y = a \ \frac{\sin \sigma}{\cosh \tau - \cos \sigma}

To Cartesian coordinates from two-center bipolar coordinates[edit]


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

y = \pm \frac{1}{4c}\sqrt{16c^2r_1^2-(r_1^2-r_2^2+4c^2)^2}
[1]

To polar coordinates from two-center bipolar coordinates[edit]


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

\theta = \arctan \left[ \sqrt{\frac{8c^2(r_1^2+r_2^2-2c^2)}{r_1^2-r_2^2}-1}\right]

Where 2c is the distance between the poles.

To Cartesian coordinates from Cesàro equation[edit]

Main article: Cesàro equation

x = \int \cos \left[\int \kappa(s) \,ds\right] ds

y = \int \sin \left[\int \kappa(s) \,ds\right] ds

Arc length and curvature from Cartesian coordinates[edit]

\kappa = \frac{x'y''-y'x''}{(x'^2+y'^2)^{3/2}}

s = \int_a^t \sqrt { x'^2 + y'^2 }\, dt

Arc length and curvature from polar coordinates[edit]

\kappa=\frac{r^2+2r'^2-rr''}{(r^2+r'^2)^{3/2}}

s = \int_a^\phi \sqrt { 1 + y'^2 }\, d\phi

3-Dimensional[edit]

Let (x, y, z) be the standard Cartesian coordinates, and (ρ, θ, φ) the spherical coordinates, with θ the angle measured away from the +Z axis. As φ has a range of 360° the same considerations as in polar (2 dimensional) coordinates apply whenever an arctangent of it is taken. θ has a range of 180°, running from 0° to 180°, and does not pose any problem when calculated from an arccosine, but beware for an arctangent. If, in the alternative definition, θ is chosen to run from −90° to +90°, in opposite direction of the earlier definition, it can be found uniquely from an arcsine, but beware of an arccotangent. In this case in all formulas below all arguments in θ should have sine and cosine exchanged, and as derivative also a plus and minus exchanged.

All divisions by zero result in special cases of being directions along one of the main axes and are in practice most easily solved by observation.

To Cartesian coordinates[edit]

From spherical coordinates[edit]

Main article: spherical coordinates
{x}=\rho \, \sin\theta \, \cos\phi \quad
{y}=\rho \, \sin\theta \, \sin\phi \quad
{z}=\rho \, \cos\theta\quad

\frac{\partial(x, y, z)}{\partial(\rho, \theta, \phi)} =
\begin{pmatrix}
\sin\theta\cos\phi & \rho\cos\theta\cos\phi & -\rho\sin\theta\sin\phi  
\\
\sin\theta\sin\phi & \rho\cos\theta\sin\phi & \rho\sin\theta\cos\phi   
\\
\cos\theta           & -\rho\sin\theta          & 0
\end{pmatrix}

So for the volume element:


dx\;dy\;dz=\det{\frac{\partial(x, y, z)}{\partial(\rho, \theta, \phi)}} d\rho\;d\theta\;d\phi =
\rho^2 \sin\theta \; d\rho \; d\theta \; d\phi \;

From cylindrical coordinates[edit]

{x}={r} \,\cos\theta
{y}={r} \, \sin\theta
{z}={h} \,

\frac{\partial(x, y, z)}{\partial(r, \theta, h)} =
\begin{pmatrix}
\cos\theta & -r\sin\theta & 0 \\
\sin\theta &  r\cos\theta & 0 \\
         0 &            0 & 1
\end{pmatrix}

So for the volume element:


dx\;dy\;dz=\det{\frac{\partial(x, y, z)}{\partial(r, \theta, h)}} dr\;d\theta\;dh =
{r}\; dr \; d\theta \; dh \;

To Spherical coordinates[edit]

From Cartesian coordinates[edit]

{\rho}=\sqrt{x^2 + y^2 + z^2}
{\phi}=\arctan \left( {\frac{y}{x}} \right)= \arccos \left( \frac{x}{\sqrt{x^2+y^2}}\right) = \arcsin \left( \frac{y}{\sqrt{x^2+y^2}}\right)
{\theta}=\arctan \left( \frac{\sqrt{x^2 + y^2}}{z} \right)=\arccos \left( {\frac{z}{\sqrt{x^2 + y^2 + z^2}}} \right)

\frac{\partial(\rho, \theta, \phi)}{\partial(x, y, z)} =
\begin{pmatrix}
\frac{x}{\rho} &                  \frac{y}{\rho} & \frac{z}{\rho} \\
\frac{xz}{\rho^2\sqrt{x^2+y^2}} & \frac{yz}{\rho^2\sqrt{x^2+y^2}} & -\frac{\sqrt{x^2+y^2}}{\rho^2}\\
\frac{-y}{x^2+y^2} &               \frac{x}{x^2+y^2} & 0\\
\end{pmatrix}

So for the volume element:

d\rho\ d\theta\ d\phi=\det\frac{\partial(\rho,\theta,\phi)}{\partial(x,y,z)}dx\ dy\ dz=\frac{1}{\sqrt{x^2+y^2}\sqrt{x^2+y^2+z^2}}dx\ dy\ dz

From cylindrical coordinates[edit]

{\rho}=\sqrt{r^2+h^2}
{\phi}=\phi \quad
{\theta}=\arctan\frac{r}{h}

\frac{\partial(\rho, \theta, \phi)}{\partial(r, \phi, h)} =
\begin{pmatrix}
\frac{r}{\sqrt{r^2+h^2}} & 0 & \frac{h}{\sqrt{r^2+h^2}} \\
\frac{-r}{r^2+h^2} & 0 & \frac{h}{r^2+h^2} \\
0 & 1 & 0 
\end{pmatrix}
 \det \frac{\partial(\rho, \theta, \phi)}{\partial(r, \phi, h)} = \frac{1}{\sqrt{r^2+h^2}}

To Cylindrical Coordinates[edit]

From Cartesian Coordinates[edit]

r=\sqrt{x^2 + y^2}
\theta = 
  \begin{cases}
   0 & \mbox{if } x = 0 \mbox{ and } y = 0\\
    \arcsin(\frac{y}{r}) & \mbox{if } x \geq 0 \\
    -\arcsin(\frac{y}{r}) + \pi & \mbox{if } x < 0\\
  \end{cases}
h=z \quad

Note that many computer systems may offer a more concise function for computing \theta, such as atan2(y,x) in the C language.


\frac{\partial(r, \theta, h)}{\partial(x, y, z)} =
\begin{pmatrix}
\frac{x}{\sqrt{x^2+y^2}}&\frac{y}{\sqrt{x^2+y^2}}&0\\
\frac{-y}{x^2+y^2}&\frac{x}{x^2+y^2}&0\\
0&0&1
\end{pmatrix}

From Spherical Coordinates[edit]

 r = \rho \sin \phi \,
 \theta  = \theta \,
 h  = \rho \cos \phi \,

\frac{\partial(r, \theta, h)}{\partial(\rho, \theta, \phi)} =
\begin{pmatrix}
\sin\phi & 0 & \rho\cos\phi  \\
0        & 1 &   0           \\
\cos\phi & 0 & -\rho\sin\phi
\end{pmatrix}
 \det\frac{\partial(r, \theta, h)}{\partial(\rho, \theta, \phi)} = - \rho

Arc length, curvature and torsion from cartesian coordinates[edit]

s = \int_0^t \sqrt { x'^2 + y'^2 + z'^2 }\, dt
\kappa=\frac{\sqrt{(z''y'-y''z')^2+(x''z'-z''x')^2+(y''x'-x''y')^2}}{(x'^2+y'^2+z'^2)^{3/2}}
\tau=\frac{z'''(x'y''-y'x'')+z''(x'''y'-x'y''')+z'(x''y'''-x'''y'')}{(x'^2+y'^2+z'^2)(x''^2+y''^2+z''^2)}

References[edit]

  1. ^ Weisstein, Eric W.. "Bipolar Coordinates." Treasure Troves. 26 May 1999. Sociology and Anthropology China. 14 February 2007 [1]