Definitions

# Cylindrical coordinate system

The cylindrical coordinate system is a three-dimensional coordinate system which essentially extends circular polar coordinates by adding a third coordinate (usually denoted $z$) which measures the height of a point above the plane.

The notation for this coordinate system is not uniform. The Standard ISO 31-11 establishes them as $\left(rho,varphi,z\right)$. Nevertheless, in many cases the azimuth $varphi$ is denoted as $theta$. Also, the radial coordinate is called $r$ while the vertical coordinate is sometimes referred as $h$.

A point P is given as $\left(rho, varphi, z\right)$. In terms of the Cartesian coordinate system:

• $rho$ is the distance from O to P', the orthogonal projection of the point P onto the XY plane. This is the same as the distance of P to the z-axis.
• $varphi$ is the angle between the positive x-axis and the line OP', measured counterclockwise.
• $z$ is the same as the Cartesian coordinate $z$.
• Thus, the conversion function $f$ from Cartesian coordinates to cylindrical coordinates is $f\left(rho,varphi,z\right)=\left(sqrt\left\{x^\left\{2\right\}+y^\left\{2\right\}\right\},operatorname\left\{atan2\right\}\left(y,x\right),z\right),$.
• The conversion function $f$ from cylindrical coordinates to Cartesian coordinates is $f\left(x,y,z\right)=\left(rhocosvarphi,rhosinvarphi,z\right),$.

Note that the atan2() function as used above is not standard: It returns a value between 0 and 2π rather than between -π and π as the standard atan2() function does.

Cylindrical coordinates are useful in analyzing surfaces that are symmetrical about an axis, with the z-axis chosen as the axis of symmetry. For example, the infinitely long circular cylinder that has the Cartesian equation $x^2+y^2=c^2$ has the very simple equation $rho = c$ in cylindrical coordinates. Hence the name "cylindrical" coordinates.

## Line and volume elements

See multiple integral for details of volume integration in cylindrical coordinates, and Del in cylindrical and spherical coordinates for vector calculus formulae.
In many problems involving cylindrical polar coordinates, it is useful to know the line and volume elements; these are used in integration to solve problems involving paths and volumes.

The line element is

$mathrm dmathbf\left\{r\right\} = mathrm drho,boldsymbol\left\{hat rho\right\} + rho,mathrm dvarphi,boldsymbol\left\{hatvarphi\right\} + mathrm dz,mathbf\left\{hat z\right\}.$

The volume element is

$mathrm dV = rho,mathrm drho,mathrm dvarphi,mathrm dz.$

The surface element is

$mathrm dS= rho,dvarphi,dz.$

The del operator in this system is written as

$nabla = boldsymbol\left\{hat rho\right\}frac\left\{partial\right\}\left\{partial rho\right\} + boldsymbol\left\{hat varphi\right\}frac\left\{1\right\}\left\{rho\right\}frac\left\{partial\right\}\left\{partial varphi\right\} + mathbf\left\{hat z\right\}frac\left\{partial\right\}\left\{partial z\right\}.$

## Cylindrical Harmonics

Cylindrical harmonics are a set of solutions to Laplace's differential equation expressed in cylindrical coordinates. Each harmonic function $V_n\left(k\right)$ consists of the product of three functions:

$V_n\left(k;rho,varphi,z\right)=P_n\left(krho\right)Phi_n\left(varphi\right)Z\left(k,z\right),$

where $\left(rho,varphi,z\right)$ are the cylindrical coordinates, and n and k are constants which distinguish the members of the set from each other. As a result of the superposition principle applied to Laplace's equation, very general solutions to Laplace's equation can be obtained by linear combinations of these functions.

Since all of the surfaces of constant ρ, φ and z  are conicoid, Laplace's equation is separable in cylindrical coordinates. Using the technique of the separation of variables, a separated solution to Laplace's equation may be written:

$V=P\left(rho\right),Phi\left(varphi\right),Z\left(z\right)$

and Laplace's equation, divided by V, is written:


frac{ddot{P}}{P}+frac{1}{rho},frac{dot{P}}{P}+frac{1}{rho^2},frac{ddot{Phi}}{Phi}+frac{ddot{Z}}{Z}=0

The Z  part of the equation is a function of z alone, and must therefore be equal to a constant:

$frac\left\{ddot\left\{Z\right\}\right\}\left\{Z\right\}=k^2$

where k  is, in general, a complex number. For a particular k, the Z(z) function has two linearly independent solutions. If k is real they are:

$Z\left(k,z\right)=cosh\left(kz\right),,,,,,mathrm\left\{or\right\},,,,,,sinh\left(kz\right),$

or by their behavior at infinity:

$Z\left(k,z\right)=e^\left\{kz\right\},,,,,,mathrm\left\{or\right\},,,,,,e^\left\{-kz\right\},$

If k is imaginary:

$Z\left(k,z\right)=cos\left(|k|z\right),,,,,,mathrm\left\{or\right\},,,,,,sin\left(|k|z\right),$

or:

$Z\left(k,z\right)=e^\left\{i|k|z\right\},,,,,,mathrm\left\{or\right\},,,,,,e^\left\{-i|k|z\right\},$

It can be seen that the Z(k,z) functions are the kernels of the Fourier transform or Laplace transform of the Z(z) function and so k may be a discrete variable for periodic boundary conditions, or it may be a continuous variable for non-periodic boundary conditions.

Substituting $k^2$ for $ddot\left\{Z\right\}/Z$ , Laplace's equation may now be written:


frac{ddot{P}}{P}+frac{1}{rho},frac{dot{P}}{P}+frac{1}{rho^2}frac{ddot{Phi}}{Phi}+k^2=0

Multiplying by $rho^2$, we may now separate the P  and Φ functions and introduce another constant (n) to obtain:

$frac\left\{ddot\left\{Phi\right\}\right\}\left\{Phi\right\} =-n^2$

$rho^2frac\left\{ddot\left\{P\right\}\right\}\left\{P\right\}+rhofrac\left\{dot\left\{P\right\}\right\}\left\{P\right\}+k^2rho^2=n^2$

Since $varphi$ is periodic, we may take n to be a non-negative integer and accordingly, the $Phi\left(varphi\right)$ the constants are subscripted. Real solutions for $Phi\left(varphi\right)$ are

$Phi_n=cos\left(nvarphi\right),,,,,,mathrm\left\{or\right\},,,,,,sin\left(nvarphi\right)$

or, equivalently:

$Phi_n=e^\left\{invarphi\right\},,,,,,mathrm\left\{or\right\},,,,,,e^\left\{-invarphi\right\}$

The differential equation for $rho$ is a form of Bessel's equation.

If k is zero, but n is not, the solutions are:

$P_n\left(0,rho\right)=rho^n,,,,,,mathrm\left\{or\right\},,,,,,rho^\left\{-n\right\},$

If both k and n are zero, the solutions are:

$P_n\left(k,rho\right)=lnrho,,,,,,mathrm\left\{or\right\},,,,,,1,$

If k is a real number we may write a real solution as:

$P_n\left(k,rho\right)=J_n\left(krho\right),,,,,,mathrm\left\{or\right\},,,,,,Y_n\left(krho\right),$

where $J_n\left(z\right)$ and $Y_n\left(z\right)$ are ordinary Bessel functions. If k  is an imaginary number, we may write a real solution as:

$P_n\left(k,rho\right)=I_n\left(|k|rho\right),,,,,,mathrm\left\{or\right\},,,,,,K_n\left(|k|rho\right),$

where $I_n\left(z\right)$ and $K_n\left(z\right)$ are modified Bessel functions. The cylindrical harmonics for (k,n) are now the product of these solutions and the general solution to Laplace's equation is given by a linear combination of these solutions:

$V\left(rho,varphi,z\right)=sum_n int dk,, A_n\left(k\right) P_n\left(k,rho\right) Phi_n\left(varphi\right) Z\left(k,z\right),$

where the $A_n\left(k\right)$ are constants with respect to the cylindrical coordinates and the limits of the summation and integration are determined by the boundary conditions of the problem. Note that the integral may be replaced by a sum for appropriate boundary conditions. The orthogonality of the $J_n\left(x\right)$ is often very useful when finding a solution to a particular problem. The $Phi_n\left(varphi\right)$ and $Z\left(k,z\right)$ functions are essentially Fourier or Laplace expansions, and form a set of orthogonal functions. When $P_n\left(krho\right)$ is simply $J_n\left(krho\right)$ , the orthogonality of $J_n$, along with the orthogonality relationships of $Phi_n\left(varphi\right)$ and $Z\left(k,z\right)$ allow the constants to be determined.

$int_0^a J_n\left(krho\right)J_n\left(k\text{'}rho\right)rho,drho = frac\left\{1\right\}\left\{k\right\}delta_\left\{kk\text{'}\right\}$

see smythe p 185 for more orthogonality

In solving problems, the space may be divided into any number of pieces, as long as the values of the potential and its derivative match across a boundary which contains no sources.

### Example: Point source inside a conducting cylindrical box

As an example, consider the problem of determining the potential of a unit source located at $\left(rho_0,varphi_0,z_0\right)$ inside a conducting "cylindrical box" (e.g. an empty tin can) which is bounded above and below by the planes $z=-L$ and $z=L$ and on the sides by the cylinder $rho=a$ (Smythe, 1968). (In MKS units, we will assume $q/4piepsilon_0=1$ Since the potential is bounded by the planes on the z axis, the Z(k,z) function can be taken to be periodic. Since the potential must be zero at the origin, we take the $P_n\left(krho\right)$ function to be the ordinary Bessel function $J_n\left(krho\right)$, and it must be chosen so that one of its zeroes lands on the bounding cylinder. For the measurement point below the source point on the z axis, the potential will be:

$V\left(rho,varphi,z\right)=sum_\left\{n=0\right\}^infty sum_\left\{r=0\right\}^infty, A_\left\{nr\right\} J_n\left(k_\left\{nr\right\}rho\right)cos\left(n\left(varphi-varphi_0\right)\right)sinh\left(k_\left\{nr\right\}\left(L+z\right)\right),,,,,zle z_0$

where $k_\left\{nr\right\}a$ is the r-th zero of $J_n\left(z\right)$ and, from the orthogonality relationships for each of the functions:

$A_\left\{nr\right\}=frac\left\{4\left(2-delta_\left\{n0\right\}\right)\right\}\left\{a^2\right\},,frac\left\{sinh k_\left\{nr\right\}\left(L-z_0\right)\right\}\left\{sinh 2k_\left\{nr\right\}L\right\},,frac\left\{J_n\left(k_\left\{nr\right\}rho_0\right)\right\}\left\{k_\left\{nr\right\}\left[J_\left\{n+1\right\}\left(k_\left\{nr\right\}a\right)\right]^2\right\},$

Above the source point:

$V\left(rho,varphi,z\right)=sum_\left\{n=0\right\}^infty sum_\left\{r=0\right\}^infty, A_\left\{nr\right\} J_n\left(k_\left\{nr\right\}rho\right)cos\left(n\left(varphi-varphi_0\right)\right)sinh\left(k_\left\{nr\right\}\left(L-z\right)\right),,,,,zge z_0$

$A_\left\{nr\right\}=frac\left\{4\left(2-delta_\left\{n0\right\}\right)\right\}\left\{a^2\right\},,frac\left\{sinh k_\left\{nr\right\}\left(L+z_0\right)\right\}\left\{sinh 2k_\left\{nr\right\}L\right\},,frac\left\{J_n\left(k_\left\{nr\right\}rho_0\right)\right\}\left\{k_\left\{nr\right\}\left[J_\left\{n+1\right\}\left(k_\left\{nr\right\}a\right)\right]^2\right\}.,$

It is clear that when $rho=a$ or $|z|=L$, the above function is zero. It can also be easily shown that the two functions match in value and in the value of their first derivatives at $z=z_0$.

#### Point source inside cylinder

Removing the plane ends (i.e. taking the limit as L approaches infinity) gives the field of the point source inside a conducting cylinder:

$V\left(rho,varphi,z\right)=sum_\left\{n=0\right\}^infty sum_\left\{r=0\right\}^infty, A_\left\{nr\right\} J_n\left(k_\left\{nr\right\}rho\right)cos\left(n\left(varphi-varphi_0\right)\right)e^\left\{-k_\left\{nr\right\}|z-z_0|\right\}$

$A_\left\{nr\right\}=frac\left\{2\left(2-delta_\left\{n0\right\}\right)\right\}\left\{a^2\right\},,frac\left\{J_n\left(k_\left\{nr\right\}rho_0\right)\right\}\left\{k_\left\{nr\right\}\left[J_\left\{n+1\right\}\left(k_\left\{nr\right\}a\right)\right]^2\right\}.,$

#### Point source in open space

As the radius of the cylinder (a) approaches infinity, the sum over the zeroes of J_n(z) becomes an integral, and we have the field of a point source in infinite space:

$V\left(rho,varphi,z\right)$
=frac{1}{R}

# sum_{n

0}^infty int_0^infty dk, A_n(k) J_n(krho)cos(n(varphi-varphi_0))e^{-k|z-z_0|}

$A_n\left(k\right)=\left(2-delta_\left\{n0\right\}\right)J_n\left(krho_0\right),$

and R is the distance from the point source to the measurement point:

$R=sqrt\left\{\left(z-z_0\right)^2+rho^2+rho_0^2-2rhorho_0cos\left(varphi-varphi_0\right)\right\}.,$

#### Point source in open space at origin

Finally, when the point source is at the origin, $rho_0=z_0=0$

$V\left(rho,varphi,z\right)=frac\left\{1\right\}\left\{sqrt\left\{rho^2+z^2\right\}\right\}=int_0^infty J_0\left(krho\right)e^\left\{-k|z|\right\},dk.$

## Bibliography

• Morse PM, Feshbach H (1953). Methods of Theoretical Physics, Part I. New York: McGraw-Hill. ISBN 0-07-043316-X,
• Margenau H, Murphy GM (1956). The Mathematics of Physics and Chemistry. New York: D. van Nostrand.
• Korn GA, Korn TM (1961). Mathematical Handbook for Scientists and Engineers. New York: McGraw-Hill.
• Sauer R, Szabó I (1967). Mathematische Hilfsmittel des Ingenieurs. New York: Springer Verlag.
• Zwillinger D (1992). Handbook of Integration. Boston, MA: Jones and Bartlett.
• Moon P, Spencer DE (1988). Field Theory Handbook, Including Coordinate Systems, Differential Equations, and Their Solutions. corrected 2nd ed., 3rd print ed., New York: Springer-Verlag.