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Viewing Version 6 of 'spherical coordinates'
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Title of object: spherical coordinates
Canonical Name: SphericalCoordinates
Type: Definition

Created on: 2003-07-22 11:53:40
Modified on: 2006-10-15 16:18:11

Creator: yark
Modifier: yark
Author: yark
Author: mathcam

Classification: msc:51M05
Keywords: sphere
Defines: hyperspherical coordinates

Revision comment (for changes between this and next version):

rewording

Preamble:

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Content:

\emph{Spherical coordinates} are a system of coordinates for $\R^3$,
or more generally $\R^n$.
One coordinate is the distance from the origin,
which can be thought of as
the radius of the sphere centred at the origin on which the point lies,
and angles which specify the position of the point on this sphere.
In $\R^3$ the coordinates are given by
\begin{align*}
\left(
\begin{tabular}{c}
$x$\\
$y$\\
$z$
\end{tabular}\right)&=
\left(
\begin{tabular}{c}
$r\sin\phi\cos\theta$\\
$r\sin\phi\sin\theta$\\
$r\cos\phi$
\end{tabular}
\right),
\end{align*}
where $r$ is the distance from the origin, $\theta$ is the azimuthal angle defined for $\theta\in[0,2\pi)$, and $\phi\in[0,\pi]$ is the polar angle.
Note that $\phi=0$ corresponds to the top of the sphere and $\phi=\pi$ corresponds to the bottom of the sphere.
There is a clash between the mathematicians' and the physicists' definition of spherical coordinates, interchanging both the direction of $\phi$ and the choice of names for the two angles (physicists often use $\theta$ as the azimuthal angle and $\phi$ as the polar one).

Spherical coordinates are a generalization of polar coordinates,
and can be further generalized to $\R^n$,
with $n-2$ polar angles $\phi_i$ and one azimuthal angle $\theta$:
\begin{align*}
\left(
\begin{tabular}{c}
$x_1$\\
$x_2$\\
$\vdots$\\
$x_k$\\
$\vdots$\\
$x_{n-1}$\\
$x_n$
\end{tabular}\right)&=
\left(
\begin{tabular}{c}
$r\cos\phi_1$\\
$r\sin\phi_1\cos\phi_2$\\
$\vdots$\\
$r\left(\prod_{i=1}^{k-1}\sin\phi_i\right)\cos\phi_k$\\
$\vdots$\\
$r\sin\phi_1\sin\phi_2\cdots\cos\theta$\\
$r\sin\phi_1\sin\phi_2\cdots\sin\phi_{n-2}\sin\theta$.
\end{tabular}
\right).
\end{align*}

These are sometimes called \emph{hyperspherical coordinates} if $n>3$.