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  2. Light - Wikipedia

    en.wikipedia.org/wiki/Light

    [4] [5] In this sense, gamma rays, X-rays, microwaves and radio waves are also light. The primary properties of light are intensity, propagation direction, frequency or wavelength spectrum, and polarization. Its speed in vacuum, 299 792 458 m/s, is one of the fundamental constants of nature. [6]

  3. Optics - Wikipedia

    en.wikipedia.org/wiki/Optics

    Textbooks and tutorials. Light and Matter – an open-source textbook, containing a treatment of optics in ch. 28–32; Optics2001 – Optics library and community; Fundamental Optics – Melles Griot Technical Guide; Physics of Light and Optics – Brigham Young University Undergraduate Book; Optics for PV – a step-by-step introduction to ...

  4. List of optics equations - Wikipedia

    en.wikipedia.org/wiki/List_of_optics_equations

    Visulization of flux through differential area and solid angle. As always n ^ {\displaystyle \mathbf {\hat {n}} \,\!} is the unit normal to the incident surface A, d A = n ^ d A {\displaystyle \mathrm {d} \mathbf {A} =\mathbf {\hat {n}} \mathrm {d} A\,\!} , and e ^ ∠ {\displaystyle \mathbf {\hat {e}} _{\angle }\,\!} is a unit vector in the ...

  5. Geometrical optics - Wikipedia

    en.wikipedia.org/wiki/Geometrical_optics

    A light ray is a line or curve that is perpendicular to the light's wavefronts (and is therefore collinear with the wave vector). A slightly more rigorous definition of a light ray follows from Fermat's principle , which states that the path taken between two points by a ray of light is the path that can be traversed in the least time.

  6. Optical properties - Wikipedia

    en.wikipedia.org/wiki/Optical_properties

    The optical properties of a material define how it interacts with light. The optical properties of matter are studied in optical physics (a subfield of optics) and applied in materials science. The optical properties of matter include: Refractive index; Dispersion; Transmittance and Transmission coefficient; Absorption; Scattering; Turbidity

  7. Luminosity - Wikipedia

    en.wikipedia.org/wiki/Luminosity

    In the case above, the total power is 4×10 27 × 1.4×10 9 = 5.7×10 36 W. This is sometimes expressed in terms of the total (i.e. integrated over all wavelengths) luminosity of the Sun which is 3.86×10 26 W , giving a radio power of 1.5×10 10 L ⊙ .

  8. Transparency and translucency - Wikipedia

    en.wikipedia.org/wiki/Transparency_and_translucency

    Absorption centers are largely responsible for the appearance of specific wavelengths of visible light all around us. Moving from longer (0.7 μm) to shorter (0.4 μm) wavelengths: Red, orange, yellow, green, and blue (ROYGB) can all be identified by our senses in the appearance of color by the selective absorption of specific light wave ...

  9. Photon - Wikipedia

    en.wikipedia.org/wiki/Photon

    Later experiments showed that these light-quanta also carry momentum and, thus, can be considered particles: The photon concept was born, leading to a deeper understanding of the electric and magnetic fields themselves. The Maxwell wave theory, however, does not account for all properties of light.