Diagram of the electric field of a light wave (blue), linear-polarized along a plane (purple line), and consisting of two orthogonal, in-phase components (red and green waves) In electrodynamics , linear polarization or plane polarization of electromagnetic radiation is a confinement of the electric field vector or magnetic field vector to a given plane along the direction of propagation. See polarization for more information.
Historically, the orientation of a polarized electromagnetic wave has been defined in the optical regime by the orientation of the electric vector, and in the radio regime, by the orientation of the magnetic vector.
Mathematical description of linear polarization
The classical sinusoidal plane wave solution of the electromagnetic wave equation for the electric and magnetic fields is (cgs units)
E
(
r
,
t
)
=∣
E
∣
R
e
{
|
ψ
⟩
exp
[
i
(
k
z
−
ω
t
)
]
}
{\displaystyle \mathbf {E} (\mathbf {r} ,t)=\mid \mathbf {E} \mid \mathrm {Re} \left\{|\psi \rangle \exp \left[i\left(kz-\omega t\right)\right]\right\}}
B
(
r
,
t
)
=
z
^
×
E
(
r
,
t
)
/
c
{\displaystyle \mathbf {B} (\mathbf {r} ,t)={\hat {\mathbf {z} }}\times \mathbf {E} (\mathbf {r} ,t)/c}
for the magnetic field, where k is the wavenumber ,
ω
=
c
k
{\displaystyle \omega _{}^{}=ck}
is the angular frequency of the wave, and
c
{\displaystyle c}
speed of light .
Here
∣
E
∣
{\displaystyle \mid \mathbf {E} \mid }
is the amplitude of the field and
|
ψ
⟩
=
d
e
f
(
ψ
x
ψ
y
)
=
(
cos
θ
exp
(
i
α
x
)
sin
θ
exp
(
i
α
y
)
)
{\displaystyle |\psi \rangle \ {\stackrel {\mathrm {def} }{=}}\ {\begin{pmatrix}\psi _{x}\\\psi _{y}\end{pmatrix}}={\begin{pmatrix}\cos \theta \exp \left(i\alpha _{x}\right)\\\sin \theta \exp \left(i\alpha _{y}\right)\end{pmatrix}}}
is the Jones vector in the x-y plane.
The wave is linearly polarized when the phase angles
α
x
,
α
y
{\displaystyle \alpha _{x}^{},\alpha _{y}}
α
x
=
α
y
=
d
e
f
α
{\displaystyle \alpha _{x}=\alpha _{y}\ {\stackrel {\mathrm {def} }{=}}\ \alpha }
This represents a wave polarized at an angle
θ
{\displaystyle \theta }
|
ψ
⟩
=
(
cos
θ
sin
θ
)
exp
(
i
α
)
{\displaystyle |\psi \rangle ={\begin{pmatrix}\cos \theta \\\sin \theta \end{pmatrix}}\exp \left(i\alpha \right)}
The state vectors for linear polarization in x or y are special cases of this state vector.
If unit vectors are defined such that
|
x
⟩
=
d
e
f
(
1
0
)
{\displaystyle |x\rangle \ {\stackrel {\mathrm {def} }{=}}\ {\begin{pmatrix}1\\0\end{pmatrix}}}
and
|
y
⟩
=
d
e
f
(
0
1
)
{\displaystyle |y\rangle \ {\stackrel {\mathrm {def} }{=}}\ {\begin{pmatrix}0\\1\end{pmatrix}}}
then the polarization state can written in the "x-y basis" as
|
ψ
⟩
=
cos
θ
exp
(
i
α
)
|
x
⟩
+
sin
θ
exp
(
i
α
)
|
y
⟩
=
ψ
x
|
x
⟩
+
ψ
y
|
y
⟩
{\displaystyle |\psi \rangle =\cos \theta \exp \left(i\alpha \right)|x\rangle +\sin \theta \exp \left(i\alpha \right)|y\rangle =\psi _{x}|x\rangle +\psi _{y}|y\rangle }
References
Jackson, John D. (1998). Classical Electrodynamics (3rd ed.) . Wiley. ISBN 0-471-30932-X
See also
public domain material from Federal Standard 1037C General Services Administration . Archived from the original on 2022-01-22.
![{\displaystyle \mathbf {E} (\mathbf {r} ,t)=\mid \mathbf {E} \mid \mathrm {Re} \left\{|\psi \rangle \exp \left[i\left(kz-\omega t\right)\right]\right\}}](/media/api/rest_v1/media/math/render/svg/1f76514bed697200b46c30726b957614f01994ae)
This article incorporates public domain material from Federal Standard 1037C. General Services Administration. Archived from the original on 2022-01-22.