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List of canonical coordinate transformations

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This is a list of canonical coordinate transformations.

2-Dimensional

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

To Cartesian coordinates from polar coordinates

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

To polar coordinates from Cartesian coordinates

[r=\sqrt]
[\theta = \arctan\frac]
Note: the result is an angle over 2π or 360° (0° to 360°, −180° to +180°, etc.) As the main value of the arctangent is defined only to be from −90° to +90°, one should add or subtract 180° when x<0. In addition when x=0 the division is undefined; yet the angle exists and is ±90° depending on the sign of y. Alternatively one could take the arccotangent of x/y in this case. Another special case to be aware of is the case when both x and y are zero.

Anyhow these special exceptions, although easily allowed for when calculated by hand, make the writing of a general computer program quite a task. Luckily most computer languages provide in addition to the normal arctangent, also an arctangent with 2 arguments with exactly the wanted behaviour. On electronic pocket calculators that function is usually called R->P (rectangular to polar).

3-Dimensional

Let (x, y, z) be the standard Cartesian coordinates, and (r, θ, φ) the spherical coordinates, with φ the angle measured away from the +Z axis. As θ has a range of 360° the same considerations as in polar (2 dimensional) coordinates apply whenever an arctangent of it is taken. φ 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, φ is chosen to run from −90° to +90°, in opposite direction of the earlier defintion, it can be found uniquely from an arcsine, but beware of an arccotangent. In this case in all formulas below all arguments in φ 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 mainaxes and are in practice most easily solved by observation.

To Cartesian coordinates

From spherical coordinates

[=\rho \, \sin\phi \, \cos\theta \quad ]
[=\rho \, \sin\phi \, \sin\theta \quad ]
[=\rho \, \cos\phi \quad ]
[\frac =\begin\sin\phi\cos\theta & -\rho\sin\phi\sin\theta & \rho\cos\phi\cos\theta \\\sin\phi\sin\theta & \rho\sin\phi\cos\theta & \rho\cos\phi\sin\theta \\\cos\phi & 0 & -\rho\sin\phi\end]
[\det} =\rho^2 \sin\phi \; d\rho \; d\theta \; d\phi \;]

From cylindrical coordinates

[= \,\cos\theta]
[= \, \sin\theta]
[= \,]
[\frac =\begin\cos\theta & -r\sin\theta & 0 \\\sin\theta & r\cos\theta & 0 \\ 0 & 0 & 1\end]
[\det} =\; dr \; d\theta \; dh \;]

To Spherical coordinates

From Cartesian coordinates

[ = \sqrt]
[ = \arccos \frac} = \arcsin \frac} = \arctan\frac]
[ = \arccos\frac} = \arctan\frac}]
[\frac =\begin \frac & \frac & \frac \\ \frac & \frac & 0 \\\frac} & \frac} & \frac}\end]

From cylindrical coordinates

[=\sqrt]
[=\theta \quad]
[=\arctan\frac]
[\frac =\begin\frac} & 0 & \frac} \\0 & 1 & 0 \\\frac & 0 & \frac \end]
[ \det \frac = \frac}]

To cylindrical coordinates

From Cartesian coordinates

[r=\sqrt]
[\theta=\arctan\frac + \pi u_0(-x) \, \operatorname y ]
[h=z \quad]
[\frac =\begin\frac}&\frac}&0\\\frac&\frac&0\\0&0&1\end]

From spherical coordinates

[ r = \rho \sin \phi ]
[ \theta = \theta ]
[ h = \rho \cos \phi ]
[\frac =\begin\sin\phi & 0 & \rho\cos\phi \\0 & 1 & 0 \\\cos\phi & 0 & -\rho\sin\phi\end]
[ \det\frac = - \rho ]

 


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