Stokes parameters

The Stokes parameters are a set of values that describe the polarization state of electromagnetic radiation (including visible light). They were defined by George Gabriel Stokes in 1852, 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. The relationship of the Stokes parameters to intensity and polarization ellipse parameters is shown in the equations and figure below.

<math> \begin{align}

S_0 &= I \\ S_1 &= I p \cos 2\psi \cos 2\chi\\ S_2 &= I p \sin 2\psi \cos 2\chi\\ S_3 &= I p \sin 2\chi \end{align} </math>

Here <math>I p</math>, <math>2\psi</math> and <math>2\chi</math> are the spherical coordinates of the polarization state in the three-dimensional space of the last three Stokes parameters. Note 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[edit | edit source]

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 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[edit | edit source]

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

<math>

\begin{pmatrix} 1 \\ 1 \\ 0 \\ 0\end{pmatrix} \quad \textrm{Linearly\ polarized\ (horizontal)} </math>

<math>

\begin{pmatrix} 1 \\ -1 \\ 0 \\ 0\end{pmatrix} \quad \textrm{Linearly \ polarized \ (vertical)} </math>

<math>

\begin{pmatrix} 1 \\ 0 \\ 1 \\ 0\end{pmatrix} \quad \textrm{Linearly \ polarized\ } (+45^\circ) </math>

<math>

\begin{pmatrix} 1 \\ 0 \\ -1 \\ 0\end{pmatrix} \quad \textrm{Linearly \ polarized\ } (-45^\circ) </math>

<math>

\begin{pmatrix} 1 \\ 0 \\ 0 \\ 1\end{pmatrix} \quad \textrm{Left-hand \ circularly \ polarized} </math>

<math>

\begin{pmatrix} 1 \\ 0 \\ 0 \\ -1\end{pmatrix} \quad \textrm{Right-hand \ circularly \ polarized} </math>

<math>

\begin{pmatrix} 1 \\ 0 \\ 0 \\ 0\end{pmatrix} \quad \textrm{Unpolarized} </math>

Alternate Explanation[edit | edit source]

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 <math>(\hat{\epsilon}_1,\hat{\epsilon}_2)</math>. Alternatively, one may specify the propagation vector, the 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 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 <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.

Definitions[edit | edit source]

The Stokes parameters are defined by

<math> \begin{matrix}

I & \equiv & |E_x|^{2}+|E_y|^{2}, \\

 &   =    & |E_a|^{2}+|E_b|^{2}, \\
 &   =    & |E_l|^{2}+|E_r|^{2}, \\

Q & \equiv & |E_x|^{2}-|E_y|^{2}, \\ U & \equiv & |E_a|^{2}-|E_b|^{2}, \\ V & \equiv & |E_l|^{2}-|E_r|^{2}, \end{matrix} </math>

where the subscripts refer to three bases: the standard 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.

Representations in fixed bases[edit | edit source]

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[edit | edit source]

For purely monochromatic 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^[1]:

<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[edit | edit source]

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[edit | edit source]

• Mueller calculus
• Jones calculus
• Polarization

References[edit | edit source]

de:Stokes-Parameter it: Parametri di Stokes ko:스토크스 변수