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Polarization mixing : ウィキペディア英語版
Polarization mixing
In optics, polarization mixing refers to changes in the relative strengths of the Stokes parameters caused by reflection or scattering—see vector radiative transfer—or by changes in the radial orientation of the detector.
==Example: A sloping, specular surface==

The definition of the four Stokes components
are, in a fixed basis:
:
\left (\\ Q \\ U \\ V
\end
\right
)
=
\left (+ |E_h|^2 \\
|E_v|^2 - |E_h|^2 \\
2 \mathrm*> \\
2 \mathrm*>
\end
\right
),

where ''E''v and ''E''h are the electric field components
in the vertical and horizontal directions respectively.
The definitions of the coordinate bases are
arbitrary and depend on the orientation of the instrument.
In the case of the Fresnel equations, the bases are defined in terms
of the surface, with the horizontal being parallel to
the surface and the vertical in a plane perpendicular to
the surface.
When the bases are rotated by 45 degrees around the viewing axis,
the definition of the third Stokes component becomes equivalent
to that of the second, that is the difference in field intensity
between the horizontal and vertical polarizations.
Thus, if the instrument is rotated out of plane from the
surface upon which it is looking, this will give rise to a signal. The geometry is illustrated in the above figure:
\theta is the instrument viewing angle with respect
to nadir, \theta_}=(\sin \theta, ~0, ~\cos \theta).

We define the slope of the surface in terms of the normal vector,
\mathbf}=(\cos \psi \sin \mu,~\sin \psi \cos \mu,~\cos \mu),

where \mu is the slope and \psi is the azimuth relative
to the instrument view. The effective viewing angle can be
calculated via a dot product between the two vectors:
:
\theta_=\cos^(\mathbf}),

from which we compute the reflection coefficients,
while the angle of the polarisation plane can be calculated
with cross products:
:
\alpha=\mathrm(\mathbf})

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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