Unpolarized Light

Unpolarized light is light with a random, time-varying polarization.
Natural light, like most other common sources of visible light, produced independently by a large number of atoms or molecules whose emissions are uncorrelated.
This term is somewhat inexact, since at any instant of time at one location there is a definite plane of polarization; however, it implies that the polarization changes so quickly in time that it will not be measured or relevant to the outcome of an experiment.

Unpolarized light can be produced from the incoherent combination of vertical and horizontal linearly polarized light, or right- and left-handed circularly polarized light.
Conversely, the two constituent linearly polarized states of unpolarized light cannot form an interference pattern, even if rotated into alignment ( Fresnel–Arago 3rd law).

A so-called ''depolarizer'' acts on a polarized beam to create one in which the polarization varies so rapidly across the beam that it may be ignored in the intended applications.
Conversely, a ''polarizer'' acts on an unpolarized beam or arbitrarily polarized beam to create one which is polarized.

Unpolarized light can be described as a mixture of two independent oppositely polarized streams, each with half the intensity. Light is said to be ''partially polarized'' when there is more power in one of these streams than the other. At any particular wavelength, partially polarized light can be statistically described as the superposition of a completely unpolarized component and a completely polarized one. One may then describe the light in terms of the degree of polarization and the parameters of the polarized component. That polarized component can be described in terms of a Jones vector or polarization ellipse. However, in order to also describe the degree of polarization, one normally employs Stokes parameters to specify a state of partial polarization.

Motivation

The transmission of plane waves through a homogeneous medium are fully described in terms of Jones vectors and 2×2 Jones matrices. However, in practice there are cases in which all of the light cannot be viewed in such a simple manner due to spatial inhomogeneities or the presence of mutually incoherent waves. So-called depolarization, for instance, cannot be described using Jones matrices. For these cases it is usual instead to use a 4×4 matrix that acts upon the Stokes 4-vector. Such matrices were first used by Paul Soleillet in 1929, although they have come to be known as Mueller matrices. While every Jones matrix has a Mueller matrix, the reverse is not true. Mueller matrices are then used to describe the observed polarization effects of the scattering of waves from complex surfaces or ensembles of particles, as shall now be presented.

Coherency matrix

The Jones vector perfectly describes the state of polarization ''and phase'' of a single monochromatic wave, representing a pure state of polarization as described above. However any mixture of waves of different polarizations (or even of different frequencies) do ''not'' correspond to a Jones vector. In so-called partially polarized radiation the fields are stochastic, and the variations and correlations between components of the electric field can only be described statistically. One such representation is the coherency matrix:
: $\begin \mathbf &= \left\langle \mathbf\mathbf^\dagger \right\rangle \\ &= \left\langle\begin e_1 e_1^* & e_1 e_2^* \\ e_2 e_1^* & e_2 e_2^* \end\right\rangle \\ &= \left\langle\begin a_1^2 & a_1 a_2 e^ \\ a_1 a_2 e^ & a_2^2 \end\right\rangle \end$

where angular brackets denote averaging over many wave cycles. Several variants of the coherency matrix have been proposed: the Wiener coherency matrix and the spectral coherency matrix of Richard Barakat measure the coherence of a spectral decomposition of the signal, while the Wolf coherency matrix averages over all time/frequencies.

The coherency matrix contains all second order statistical information about the polarization. This matrix can be decomposed into the sum of two idempotent matrices, corresponding to the eigenvectors of the coherency matrix, each representing a polarization state that is orthogonal to the other. An alternative decomposition is into completely polarized (zero determinant) and unpolarized (scaled identity matrix) components. In either case, the operation of summing the components corresponds to the incoherent superposition of waves from the two components. The latter case gives rise to the concept of the "degree of polarization"; i.e., the fraction of the total intensity contributed by the completely polarized component.

Stokes parameters

The coherency matrix is not easy to visualize, and it is therefore common to describe incoherent or partially polarized radiation in terms of its total intensity (''I''), (fractional) degree of polarization (''p''), and the shape parameters of the polarization ellipse. An alternative and mathematically convenient description is given by the Stokes parameters, introduced by George Gabriel Stokes in 1852. The relationship of the Stokes parameters to intensity and polarization ellipse parameters is shown in the equations and figure below.

: $S_0 = I \,$
: $S_1 = Ip \cos 2\psi \cos 2\chi\,$
: $S_2 = Ip \sin 2\psi \cos 2\chi\,$
: $S_3 = Ip \sin 2\chi\,$

Here ''Ip'', 2ψ and 2χ are the spherical coordinates of the polarization state in the three-dimensional space of the last three Stokes parameters. Note the factors of two before ψ and χ corresponding respectively to the facts that any polarization ellipse is indistinguishable from one rotated by 180°, or one with the semi-axis lengths swapped accompanied by a 90° rotation. The Stokes parameters are sometimes denoted ''I'', ''Q'', ''U'' and ''V''.

The four Stokes parameters are enough to describe 2D polarization of a paraxial wave, but not the 3D polarization of a general non-paraxial wave or an evanescent field.

Poincaré sphere

Neglecting the first Stokes parameter ''S''₀ (or ''I''), the three other Stokes parameters can be plotted directly in three-dimensional Cartesian coordinates. For a given power in the polarized component given by
: $P = \sqrt$

the set of all polarization states are then mapped to points on the surface of the so-called Poincaré sphere (but of radius ''P''), as shown in the accompanying diagram.

Often the total beam power is not of interest, in which case a normalized Stokes vector is used by dividing the Stokes vector by the total intensity ''S''₀:
:$\mathbf = \frac \beginS_0\\S_1\\S_2\\S_3\end.$

The normalized Stokes vector $\mathbf$ then has unity power ($S'_0 = 1$) and the three significant Stokes parameters plotted in three dimensions will lie on the unity-radius Poincaré sphere for pure polarization states (where $P'_0 = 1$). Partially polarized states will lie ''inside'' the Poincaré sphere at a distance of $P' = \sqrt$ from the origin. When the non-polarized component is not of interest, the Stokes vector can be further normalized to obtain
:$\mathbf = \frac \begin 1\\S'_1\\S'_2\\S'_3 \end = \frac \begin S_0\\S_1\\S_2\\S_3 \end.$

When plotted, that point will lie on the surface of the unity-radius Poincaré sphere and indicate the state of polarization of the polarized component.

Any two antipodal points on the Poincaré sphere refer to orthogonal polarization states. The overlap between any two polarization states is dependent solely on the distance between their locations along the sphere. This property, which can only be true when pure polarization states are mapped onto a sphere, is the motivation for the invention of the Poincaré sphere and the use of Stokes parameters, which are thus plotted on (or beneath) it.

Note that the IEEE defines RHCP and LHCP the opposite as those used by Physicists. The IEEE 1979 Antenna Standard will show RHCP on the South Pole of the Poincare Sphere. The IEEE defines RHCP using the right hand with thumb pointing in the direction of transmit, and the fingers showing the direction of rotation of the E field with time. The rationale for the opposite conventions used by Physicists and Engineers is that Astronomical Observations are always done with the incoming wave traveling toward the observer, where as for most engineers, they are assumed to be standing behind the transmitter watching the wave traveling away from them. This article is not using the IEEE 1979 Antenna Standard and is not using the +t convention typically used in IEEE work.

See also

* Coherence (physics)#Polarization and coherence
*Photon polarization

References

{{reflist

Polarization (waves)