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  2. Zohar - Wikipedia

    en.wikipedia.org/wiki/Zohar

    The Zohar (Hebrew: זֹהַר ‎, Zōhar, lit."Splendor" or "Radiance" [a]) is a foundational work of Kabbalistic literature. [1] It is a group of books including commentary on the mystical aspects of the Torah and scriptural interpretations as well as material on mysticism, mythical cosmogony, and mystical psychology.

  3. Brightness temperature - Wikipedia

    en.wikipedia.org/wiki/Brightness_temperature

    Brightness temperature or radiance temperature is a measure of the intensity of electromagnetic energy coming from a source. [1] In particular, it is the temperature at which a black body would have to be in order to duplicate the observed intensity of a grey body object at a frequency ν {\displaystyle \nu } . [ 2 ]

  4. Riley Bloom series - Wikipedia

    en.wikipedia.org/wiki/Riley_Bloom_Series

    The Riley Bloom series is the spin-off of the fantasy series The Immortals by Alyson Noel first published in 2010 in the United States about the afterlife of Riley Bloom, the sister of Ever Bloom (lead character of The Immortals).

  5. Rayleigh–Jeans law - Wikipedia

    en.wikipedia.org/wiki/Rayleigh–Jeans_law

    Comparison of Rayleigh–Jeans law with Wien approximation and Planck's law, for a body of 5800 K temperature.. In physics, the Rayleigh–Jeans law is an approximation to the spectral radiance of electromagnetic radiation as a function of wavelength from a black body at a given temperature through classical arguments.

  6. Radiance (book) - Wikipedia

    en.wikipedia.org/wiki/Radiance_(book)

    Radiance is the first book of the Riley Bloom Series written by Alyson Noël, which is a spin-off of The Immortals. Plot. Riley Bloom crossed the bridge into the ...

  7. Stefan–Boltzmann law - Wikipedia

    en.wikipedia.org/wiki/Stefan–Boltzmann_law

    For an ideal absorber/emitter or black body, the Stefan–Boltzmann law states that the total energy radiated per unit surface area per unit time (also known as the radiant exitance) is directly proportional to the fourth power of the black body's temperature, T: =.

  8. Black-body radiation - Wikipedia

    en.wikipedia.org/wiki/Black-body_radiation

    When the body is black, the absorption is obvious: the amount of light absorbed is all the light that hits the surface. For a black body much bigger than the wavelength, the light energy absorbed at any wavelength λ per unit time is strictly proportional to the blackbody curve. This means that the blackbody curve is the amount of light energy ...

  9. Radiance - Wikipedia

    en.wikipedia.org/wiki/Radiance

    Radiance is used to characterize diffuse emission and reflection of electromagnetic radiation, and to quantify emission of neutrinos and other particles. The SI unit of radiance is the watt per steradian per square metre (W·sr −1 ·m −2). It is a directional quantity: the radiance of a surface depends on the direction from which it is ...