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  2. Radiation - Wikipedia

    en.wikipedia.org/wiki/Radiation

    Radiation, in general, exists throughout nature, such as in light and sound. In physics, radiation is the emission or transmission of energy in the form of waves or particles through space or a material medium. [1] [2] This includes:

  3. Electromagnetic radiation - Wikipedia

    en.wikipedia.org/wiki/Electromagnetic_radiation

    In electromagnetic radiation (such as microwaves from an antenna, shown here) the term radiation applies only to the parts of the electromagnetic field that radiate into infinite space and decrease in intensity by an inverse-square law of power, such that the total energy that crosses through an imaginary sphere surrounding the source is the ...

  4. Radiative transfer - Wikipedia

    en.wikipedia.org/wiki/Radiative_transfer

    Radiative transfer (also called radiation transport) is the physical phenomenon of energy transfer in the form of electromagnetic radiation. The propagation of radiation through a medium is affected by absorption, emission, and scattering processes. The equation of radiative transfer describes these interactions mathematically. Equations of ...

  5. Outline of physics - Wikipedia

    en.wikipedia.org/wiki/Outline_of_physics

    Relativity – theory of physics which describes the relationship between space and time. General Relativity – a geometric, non-quantum theory of gravitation. Special Relativity – a theory that describes the propagation of matter and light at high speeds. Other. Agrophysics – the study of physics applied to agroecosystems

  6. Light - Wikipedia

    en.wikipedia.org/wiki/Light

    Maxwell discovered that self-propagating electromagnetic waves would travel through space at a constant speed, which happened to be equal to the previously measured speed of light. From this, Maxwell concluded that light was a form of electromagnetic radiation: he first stated this result in 1862 in On Physical Lines of Force .

  7. Radiative zone - Wikipedia

    en.wikipedia.org/wiki/Radiative_zone

    where κ(r) is the opacity, ρ(r) is the matter density, L(r) is the luminosity, and σ B is the Stefan–Boltzmann constant. [1] Hence the opacity (κ) and radiation flux (L) within a given layer of a star are important factors in determining how effective radiative diffusion is at transporting energy. A high opacity or high luminosity can ...

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  9. Linear energy transfer - Wikipedia

    en.wikipedia.org/wiki/Linear_energy_transfer

    It describes the action of radiation into matter. It is identical to the retarding force acting on a charged ionizing particle travelling through the matter. [1] By definition, LET is a positive quantity. LET depends on the nature of the radiation as well as on the material traversed.