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  2. Polarization (waves) - Wikipedia

    en.wikipedia.org/wiki/Polarization_(waves)

    Polarization is an important parameter in areas of science dealing with transverse waves, such as optics, seismology, radio, and microwaves. Especially impacted are technologies such as lasers, wireless and optical fiber telecommunications, and radar.

  3. Polarizability - Wikipedia

    en.wikipedia.org/wiki/Polarizability

    The polarization is proportional to the macroscopic field by = = where is the electric permittivity constant and is the electric susceptibility. Using this proportionality, we find the local field as F = 1 3 ( ε r + 2 ) E {\displaystyle \mathbf {F} ={\tfrac {1}{3}}(\varepsilon _{\mathrm {r} }+2)\mathbf {E} } which can be used in the definition ...

  4. Polarization - Wikipedia

    en.wikipedia.org/wiki/Polarization

    Polarization (physics), the ability of waves to oscillate in more than one direction; polarization of light allows the glare-reducing effect of polarized sunglasses Polarization (antenna), the state of polarization (in the above sense) of electromagnetic waves transmitted by or received by a radio antenna

  5. Polarimetry - Wikipedia

    en.wikipedia.org/wiki/Polarimetry

    Polarimetry is the measurement and interpretation of the polarization of transverse waves, most notably electromagnetic waves, such as radio or light waves. Typically polarimetry is done on electromagnetic waves that have traveled through or have been reflected, refracted or diffracted by some material in order to characterize that object. [1] [2]

  6. Physical optics - Wikipedia

    en.wikipedia.org/wiki/Physical_optics

    Physical optics is used to explain effects such as diffraction. In physics, physical optics, or wave optics, is the branch of optics that studies interference, diffraction, polarization, and other phenomena for which the ray approximation of geometric optics is not valid.

  7. Polarization (cosmology) - Wikipedia

    en.wikipedia.org/wiki/Polarization_(cosmology)

    Observation of these primordial photons is meant to reveal the two polarization patterns E and B modes which help to understand the physics of the early universe and its late-time evolution. Unfortunately, galactic nuclei and dust emit very strongly in the wavelength < 3 x 10^-2 cm, completely swamping the primordial signal .

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  9. Plane of polarization - Wikipedia

    en.wikipedia.org/wiki/Plane_of_polarization

    [1] [11] Hence D, E, the wave-normal direction, and the ray direction are all in the same plane, and it is all the more natural to define that plane as the "plane of polarization". This "natural" definition, however, depends on the theory of EM waves developed by James Clerk Maxwell in the 1860s — whereas the word polarization was coined ...