The terms toroidal and poloidal refer to directions relative to a torus of reference. They describe a three-dimensional coordinate system in which the poloidal direction follows a small circular ring around the surface, while the toroidal direction follows a large circular ring around the torus, encircling the central void.
The earliest use of these terms cited by the Oxford English Dictionary is by Walter M. Elsasser (1946) in the context of the generation of the Earth's magnetic field by currents in the core, with "toroidal" being parallel to lines of constant latitude and "poloidal" being in the direction of the magnetic field (i.e. towards the poles).
The OED also records the later usage of these terms in the context of toroidally confined plasmas, as encountered in magnetic confinement fusion. In the plasma context, the toroidal direction is the long way around the torus, the corresponding coordinate being denoted by in the slab approximation or or in magnetic coordinates; the poloidal direction is the short way around the torus, the corresponding coordinate being denoted by in the slab approximation or in magnetic coordinates. (The third direction, normal to the magnetic surfaces, is often called the "radial direction", denoted by in the slab approximation and variously,,,, or in magnetic coordinates.)
As a simple example from the physics of magnetically confined plasmas, consider an axisymmetric system with circular, concentric magnetic flux surfaces of radius
r
\zeta
\theta
x=(R0+r\cos\theta)\cos\zeta
y=s\zeta(R0+r\cos\theta)\sin\zeta
z=s\thetar\sin\theta.
where
s\theta=\pm1,s\zeta=\pm1
The natural choice geometrically is to take
s\theta=s\zeta=+1
r,\theta,\zeta
r,\theta,\zeta
\nablar ⋅ \nabla\theta x \nabla\zeta>0
s\theta=-1,s\zeta=+1
s\theta=+1,s\zeta=-1
To study single particle motion in toroidally confined plasma devices, velocity and acceleration vectors must be known. Considering the natural choice
s\theta=s\zeta=+1
\left(r,\theta,\zeta\right)
er=\begin{pmatrix} \cos\theta\cos\zeta\\ \cos\theta\sin\zeta\\ \sin\theta \end{pmatrix} e\theta=\begin{pmatrix} -\sin\theta\cos\zeta\\ -\sin\theta\sin\zeta\\ \cos\theta \end{pmatrix} e\zeta=\begin{pmatrix} -\sin\zeta\\ \cos\zeta\\ 0 \end{pmatrix}
according to Cartesian coordinates. The position vector is expressed as:
r=\left(r+R0\cos\theta\right)er-R0\sin\thetae\theta
The velocity vector is then given by:
|
=
r |
er+r
\theta |
e\theta+
\zeta |
\left(R0+r\cos\theta\right)e\zeta
and the acceleration vector is:
\begin{align} \ddot{r