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The '''Stokes parameters''' are a set of values that describe the [[Polarization (waves)|polarization]] state of [[electromagnetic radiation]]. They were defined by [[George Gabriel Stokes]] in 1852,<ref>S. Chandrasekhar 'Radiative Transfer'', Dover Publications, New York, 1960, ISBN 0-486-60590-6, page 25</ref> as a mathematically convenient alternative to the more common description of [[coherence (physics)|incoherent]] or partially polarized radiation in terms of its total [[field strength|intensity]] (''I''), (fractional) [[degree of polarization]] (''p''), and the shape parameters of the [[polarization ellipse]].
 
==Definitions==
[[File:Poincaré sphere.svg|right|thumb|The [[Poincaré sphere]] is the parametrisation of the last three Stokes' parameters in [[spherical coordinates]]]]
The relationship of the Stokes parameters to intensity and polarization ellipse parameters is shown in the equations below and the figure at right.
 
:<math> \begin{align}
S_0 &= I \\
S_1 &= p I \cos 2\psi \cos 2\chi\\
S_2 &= p I \sin 2\psi \cos 2\chi\\
S_3 &= p I \sin 2\chi
\end{align} </math>
 
Here <math>p</math>, <math>I</math>, <math>2\psi</math> and <math>2\chi</math> are the [[spherical coordinates]] of the three-dimensional vector of [[cartesian coordinates]] <math>(S_1, S_2, S_3)</math>. <math>I</math> is the total intensity of the beam, and <math>p</math> is the degree of polarization. The factor of two before <math>\psi</math> represents the fact that any polarization ellipse is indistinguishable from one rotated by 180°, while the factor of two before <math>\chi</math> indicates that an ellipse is indistinguishable from one with the semi-axis lengths swapped accompanied by a 90° rotation. The four Stokes parameters are sometimes denoted ''I'', ''Q'', ''U'' and ''V'', respectively.
 
If given the Stokes parameters one can solve for the [[spherical coordinates]] with the following equations:
 
:<math> \begin{align}
I &= S_0 \\
p &= \frac{\sqrt{S_1^2 + S_2^2 + S_3^2}}{S_0} \\
2\psi &= \mathrm{atan} \frac{S_2}{S_1}\\
2\chi &= \mathrm{atan} \frac{S_3}{\sqrt{S_1^2+S_2^2}}\\
\end{align} </math>
 
===Stokes vectors===
The Stokes parameters are often combined into a vector, known as the '''Stokes vector''':
:<math>
\vec S \ =
\begin{pmatrix} S_0 \\ S_1 \\ S_2 \\ S_3\end{pmatrix}
=
\begin{pmatrix} I \\ Q \\ U \\ V\end{pmatrix}
</math>
 
The Stokes vector spans the [[vector space|space]] of unpolarized, partially polarized, and fully polarized light. For comparison, the [[Jones vector]] only spans the space of fully polarized light, but is more useful for problems involving [[coherence (physics)|coherent]] light. The four Stokes parameters do not form a preferred [[Basis (linear algebra)|basis]] of the space, but rather were chosen because they can be easily measured or calculated.
 
The effect of an optical system on the polarization of light can be determined by constructing the Stokes vector for the input light and applying [[Mueller calculus]], to obtain the Stokes vector of the light leaving the system.
 
====Examples====
Below are shown some Stokes vectors for common states of polarization of light.
 
:{|
|-
| <math>\begin{pmatrix} 1 \\ 1 \\ 0 \\ 0\end{pmatrix}</math> || Linearly polarized (horizontal)
|-
| <math>\begin{pmatrix} 1 \\ -1 \\ 0 \\ 0\end{pmatrix}</math> || Linearly polarized (vertical)
|-
| <math>\begin{pmatrix} 1 \\ 0 \\ 1 \\ 0\end{pmatrix} </math> || Linearly polarized (+45°)
|-
| <math>\begin{pmatrix} 1 \\ 0 \\ -1 \\ 0\end{pmatrix}</math> || Linearly polarized (−45°)
|-
| <math>\begin{pmatrix} 1 \\ 0 \\ 0 \\ 1\end{pmatrix} </math> || Right-hand circularly polarized
|-
| <math>\begin{pmatrix} 1 \\ 0 \\ 0 \\ -1\end{pmatrix}</math> || Left-hand circularly polarized
|-
| <math>\begin{pmatrix} 1 \\ 0 \\ 0 \\ 0\end{pmatrix}</math> || Unpolarized
|}
 
==Alternate explanation==
[[File:Polarisation ellipse.svg|250px|right]]
A [[monochromatic]] [[plane wave]] is specified by its propagation vector, <math>\vec{k}</math>, and the complex amplitudes of the [[electric field]], <math>E_1</math> and <math>E_2</math>, in a [[Basis (linear algebra)|basis]] <math>(\hat{\epsilon}_1,\hat{\epsilon}_2)</math>. Alternatively, one may specify the propagation vector, the [[Phase (waves)|phase]], <math>\phi</math>, and the polarization state, <math>\Psi</math>, where <math>\Psi</math> is the curve traced out by the electric field in a fixed plane. The most familiar polarization states are linear and circular, which are [[Degeneracy (mathematics)|degenerate]] cases of the most general state, an [[ellipse]].
 
One way to describe polarization is by giving the [[Semi-major axis|semi-major]] and [[Semi-minor axis|semi-minor]] axes of the polarization ellipse, its orientation, and the sense of rotation (See the above figure). The Stokes parameters <math>I</math>, <math>Q</math>, <math>U</math>, and <math>V</math>, provide an alternative description of the polarization state which is experimentally convenient because each parameter corresponds to a sum or difference of measurable intensities. The next figure shows examples of the Stokes parameters in degenerate states.
 
[[File:StokesParameters.png|center]]
 
===Definitions===
The Stokes parameters are defined by
 
:<math> \begin{matrix}
I & \equiv & \langle E_x^{2} \rangle + \langle E_y^{2} \rangle \\
~ & = & \langle E_a^{2} \rangle + \langle E_b^{2} \rangle \\
~ & = & \langle E_l^{2} \rangle + \langle E_r^{2} \rangle, \\
Q & \equiv & \langle E_x^{2} \rangle - \langle E_y^{2} \rangle, \\
U & \equiv & \langle E_a^{2} \rangle - \langle E_b^{2} \rangle, \\
V & \equiv & \langle E_l^{2} \rangle - \langle E_r^{2} \rangle.
\end{matrix} </math>
 
where the subscripts refer to three bases: the standard [[Cartesian coordinate system|Cartesian basis]] (<math>\hat{x},\hat{y}</math>), a Cartesian basis rotated by 45° (<math>\hat{a},\hat{b}</math>), and a circular basis (<math>\hat{l},\hat{r}</math>). The circular basis is defined so that <math>\hat{l} = (\hat{x}+i\hat{y})/\sqrt{2}</math>. The next figure shows how the signs of the Stokes parameters are determined by the helicity and the orientation of the semi-major axis of the polarization ellipse.
 
[[File:StokesParamSign1.png|center]]
 
===Representations in fixed bases===
In a fixed (<math>\hat{x},\hat{y}</math>) basis, the Stokes parameters are
 
:<math> \begin{matrix}
I&=&|E_x|^2+|E_y|^2, \\
Q&=&|E_x|^2-|E_y|^2, \\
U&=&2\mbox{Re}(E_xE_y^*), \\
V&=&-2\mbox{Im}(E_xE_y^*), \\
\end{matrix}
</math>
 
while for <math>(\hat{a},\hat{b})</math>, they are
 
:<math> \begin{matrix}
I&=&|E_a|^2+|E_b|^2, \\
Q&=&-2\mbox{Re}(E_a^{*}E_b), \\
U&=&|E_a|^{2}-|E_b|^{2}, \\
V&=&2\mbox{Im}(E_a^{*}E_b). \\
\end{matrix}
</math>
 
and for <math>(\hat{l},\hat{r})</math>, they are
 
:<math> \begin{matrix}
I &=&|E_l|^2+|E_r|^2, \\
Q&=&2\mbox{Re}(E_l^*E_r), \\
U & = &-2\mbox{Im}(E_l^*E_r), \\
V & =&|E_l|^2-|E_r|^2. \\
\end{matrix} </math>
 
==Properties==
For purely [[monochromatic]] [[Coherence (physics)|coherent]] radiation, one can show that
 
:<math>
\begin{matrix}
Q^2+U^2+V^2 = I^2,
\end{matrix}
</math>
 
whereas for the whole (non-coherent) beam radiation, the Stokes parameters are defined as averaged quantities, and the previous equation becomes an inequality:<ref>H. C. van de Hulst ''Light scattering by small particles'', Dover Publications, New York, 1981, ISBN 0-486-64228-3, page 42</ref>
 
:<math>
\begin{matrix}
Q^2+U^2+V^2 \le I^2.
\end{matrix}
</math>
 
However, we can define a total polarization intensity <math>I_p</math>, so that
 
:<math>
\begin{matrix}
Q^{2} + U^2 +V^2 = I_p^2,
\end{matrix}
</math>
 
where <math>I_p/I</math> is the total polarization fraction.
 
Let us define the complex intensity of linear polarization to be
 
:<math>
\begin{matrix}
L & \equiv & |L|e^{i2\theta} \\
& \equiv & Q +iU. \\
\end{matrix}
</math>
 
Under a rotation <math>\theta \rightarrow \theta+\theta'</math> of the polarization ellipse, it can be shown that <math>I</math> and <math>V</math> are invariant, but
 
:<math>
\begin{matrix}
L & \rightarrow & e^{i2\theta'}L, \\
Q & \rightarrow & \mbox{Re}\left(e^{i2\theta'}L\right), \\
U & \rightarrow & \mbox{Im}\left(e^{i2\theta'}L\right).\\
\end{matrix}
</math>
 
With these properties, the Stokes parameters may be thought of as constituting three generalized intensities:
 
:<math>
\begin{matrix}
I & \ge & 0, \\
V & \in & \mathbb{R}, \\
L & \in & \mathbb{C}, \\
\end{matrix}
</math>
 
where <math>I</math> is the total intensity, <math>|V|</math> is the intensity of circular polarization, and <math>|L|</math> is the intensity of linear polarization. The total intensity of polarization is <math>I_p=\sqrt{|L|^2+|V|^2}</math>, and the orientation and sense of rotation are given by
 
:<math>
\begin{matrix}
\theta &=& \frac{1}{2}\arg(L), \\
h &=& \sgn(V). \\
\end{matrix}
</math>
 
Since <math>Q=\mbox{Re}(L)</math> and <math>U=\mbox{Im}(L)</math>, we have
 
:<math>
\begin{matrix}
|L| &=& \sqrt{Q^2+U^2}, \\
\theta &=& \frac{1}{2}\tan^{-1}(U/Q). \\
\end{matrix}
</math>
 
==Relation to the polarization ellipse==
In terms of the parameters of the polarization ellipse, the Stokes parameters are
 
:<math>
\begin{matrix}
I_p & = & A^2 + B^2, \\
Q & = & (A^2-B^2)\cos(2\theta), \\
U & = & (A^2-B^2)\sin(2\theta), \\
V & = & 2ABh. \\
\end{matrix}
</math>
 
Inverting the previous equation gives
 
:<math>
\begin{matrix}
A & = & \sqrt{\frac{1}{2}(I_p+|L|)} \\
B & = & \sqrt{\frac{1}{2}(I_p-|L|)} \\
\theta & = & \frac{1}{2}\arg(L)\\
h & = & \sgn(V). \\
\end{matrix}
</math>
 
==See also==
* [[Mueller calculus]]
* [[Jones calculus]]
* [[Polarization (waves)]]
* [[Rayleigh Sky Model]]
* [[Stokes operators]]
* [[Polarization mixing]]
 
==Notes==
<references />
 
==References==
* E. Collett, ''Field Guide to Polarization'', SPIE Field Guides vol. '''FG05''', SPIE (2005). ISBN 0-8194-5868-6.
* E. Hecht, ''Optics'', 2nd ed., Addison-Wesley (1987). ISBN 0-201-11609-X.
* {{cite journal | author  = William H. McMaster
      | title  = Polarization and the Stokes Parameters
      | journal = Am. J. Phys.
      | page    = 351
      | volume  = 22
      | year    = 1954
      | doi    = 10.1119/1.1933744|bibcode = 1954AmJPh..22..351M }}
* {{cite journal | author  = William H. McMaster
      | title  = Matrix representation of polarization
      | journal = Rev. Mod. Phys.
      | page    = 33
      | volume  = 8
      | year    = 1961
      | doi    = 10.1103/RevModPhys.33.8|bibcode = 1961RvMP...33....8M }}
 
==External links==
*[http://www.atnf.csiro.au/computing/software/atca_aips/node11.html Stokes parameters and polarisation]
 
{{DEFAULTSORT:Stokes Parameters}}
[[Category:Polarization (waves)]]
[[Category:Radiometry]]

Revision as of 04:26, 14 March 2013

The Stokes parameters are a set of values that describe the polarization state of electromagnetic radiation. They were defined by George Gabriel Stokes in 1852,[1] as a mathematically convenient alternative to the more common description of 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.

Definitions

The Poincaré sphere is the parametrisation of the last three Stokes' parameters in spherical coordinates

The relationship of the Stokes parameters to intensity and polarization ellipse parameters is shown in the equations below and the figure at right.

S0=IS1=pIcos2ψcos2χS2=pIsin2ψcos2χS3=pIsin2χ

Here p, I, 2ψ and 2χ are the spherical coordinates of the three-dimensional vector of cartesian coordinates (S1,S2,S3). I is the total intensity of the beam, and p is the degree of polarization. The factor of two before ψ represents the fact that any polarization ellipse is indistinguishable from one rotated by 180°, while the factor of two before χ indicates that an ellipse is indistinguishable from one with the semi-axis lengths swapped accompanied by a 90° rotation. The four Stokes parameters are sometimes denoted I, Q, U and V, respectively.

If given the Stokes parameters one can solve for the spherical coordinates with the following equations:

I=S0p=S12+S22+S32S02ψ=atanS2S12χ=atanS3S12+S22

Stokes vectors

The Stokes parameters are often combined into a vector, known as the Stokes vector:

S =(S0S1S2S3)=(IQUV)

The Stokes vector spans the space of unpolarized, partially polarized, and fully polarized light. For comparison, the Jones vector only spans the space of fully polarized light, but is more useful for problems involving coherent light. The four Stokes parameters do not form a preferred basis of the space, but rather were chosen because they can be easily measured or calculated.

The effect of an optical system on the polarization of light can be determined by constructing the Stokes vector for the input light and applying Mueller calculus, to obtain the Stokes vector of the light leaving the system.

Examples

Below are shown some Stokes vectors for common states of polarization of light.

(1100) Linearly polarized (horizontal)
(1100) Linearly polarized (vertical)
(1010) Linearly polarized (+45°)
(1010) Linearly polarized (−45°)
(1001) Right-hand circularly polarized
(1001) Left-hand circularly polarized
(1000) Unpolarized

Alternate explanation

A monochromatic plane wave is specified by its propagation vector, k, and the complex amplitudes of the electric field, E1 and E2, in a basis (ϵ̂1,ϵ̂2). Alternatively, one may specify the propagation vector, the phase, ϕ, and the polarization state, Ψ, where Ψ is the curve traced out by the electric field in a fixed plane. The most familiar polarization states are linear and circular, which are degenerate cases of the most general state, an ellipse.

One way to describe polarization is by giving the semi-major and semi-minor axes of the polarization ellipse, its orientation, and the sense of rotation (See the above figure). The Stokes parameters I, Q, U, and V, provide an alternative description of the polarization state which is experimentally convenient because each parameter corresponds to a sum or difference of measurable intensities. The next figure shows examples of the Stokes parameters in degenerate states.

Definitions

The Stokes parameters are defined by

IEx2+Ey2=Ea2+Eb2=El2+Er2,QEx2Ey2,UEa2Eb2,VEl2Er2.

where the subscripts refer to three bases: the standard Cartesian basis (x̂,ŷ), a Cartesian basis rotated by 45° (â,b̂), and a circular basis (l̂,r̂). The circular basis is defined so that l̂=(x̂+iŷ)/2. The next figure shows how the signs of the Stokes parameters are determined by the helicity and the orientation of the semi-major axis of the polarization ellipse.

Representations in fixed bases

In a fixed (x̂,ŷ) basis, the Stokes parameters are

I=|Ex|2+|Ey|2,Q=|Ex|2|Ey|2,U=2Re(ExEy),V=2Im(ExEy),

while for (â,b̂), they are

I=|Ea|2+|Eb|2,Q=2Re(EaEb),U=|Ea|2|Eb|2,V=2Im(EaEb).

and for (l̂,r̂), they are

I=|El|2+|Er|2,Q=2Re(ElEr),U=2Im(ElEr),V=|El|2|Er|2.

Properties

For purely monochromatic coherent radiation, one can show that

Q2+U2+V2=I2,

whereas for the whole (non-coherent) beam radiation, the Stokes parameters are defined as averaged quantities, and the previous equation becomes an inequality:[2]

Q2+U2+V2I2.

However, we can define a total polarization intensity Ip, so that

Q2+U2+V2=Ip2,

where Ip/I is the total polarization fraction.

Let us define the complex intensity of linear polarization to be

L|L|ei2θQ+iU.

Under a rotation θθ+θ of the polarization ellipse, it can be shown that I and V are invariant, but

Lei2θL,QRe(ei2θL),UIm(ei2θL).

With these properties, the Stokes parameters may be thought of as constituting three generalized intensities:

I0,V,L,

where I is the total intensity, |V| is the intensity of circular polarization, and |L| is the intensity of linear polarization. The total intensity of polarization is Ip=|L|2+|V|2, and the orientation and sense of rotation are given by

θ=12arg(L),h=sgn(V).

Since Q=Re(L) and U=Im(L), we have

|L|=Q2+U2,θ=12tan1(U/Q).

Relation to the polarization ellipse

In terms of the parameters of the polarization ellipse, the Stokes parameters are

Ip=A2+B2,Q=(A2B2)cos(2θ),U=(A2B2)sin(2θ),V=2ABh.

Inverting the previous equation gives

A=12(Ip+|L|)B=12(Ip|L|)θ=12arg(L)h=sgn(V).

See also

Notes

  1. S. Chandrasekhar 'Radiative Transfer, Dover Publications, New York, 1960, ISBN 0-486-60590-6, page 25
  2. H. C. van de Hulst Light scattering by small particles, Dover Publications, New York, 1981, ISBN 0-486-64228-3, page 42

References

  • E. Collett, Field Guide to Polarization, SPIE Field Guides vol. FG05, SPIE (2005). ISBN 0-8194-5868-6.
  • E. Hecht, Optics, 2nd ed., Addison-Wesley (1987). ISBN 0-201-11609-X.
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