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  2. Spectral energy distribution - Wikipedia

    en.wikipedia.org/wiki/Spectral_Energy_Distribution

    The SED of M51 (upper right) obtained by combining data at many different wavelengths, e.g. UV, visible, and infrared (left). A spectral energy distribution (SED) is a plot of energy versus frequency or wavelength of light (not to be confused with a 'spectrum' of flux density vs frequency or wavelength). [1]

  3. Air mass (solar energy) - Wikipedia

    en.wikipedia.org/wiki/Air_mass_(solar_energy)

    The air mass coefficient defines the direct optical path length through the Earth's atmosphere, expressed as a ratio relative to the path length vertically upwards, i.e. at the zenith. The air mass coefficient can be used to help characterize the solar spectrum after solar radiation has traveled through the atmosphere.

  4. Spectral power distribution - Wikipedia

    en.wikipedia.org/wiki/Spectral_power_distribution

    Mathematically, for the spectral power distribution of a radiant exitance or irradiance one may write: =where M(λ) is the spectral irradiance (or exitance) of the light (SI units: W/m 2 = kg·m −1 ·s −3); Φ is the radiant flux of the source (SI unit: watt, W); A is the area over which the radiant flux is integrated (SI unit: square meter, m 2); and λ is the wavelength (SI unit: meter, m).

  5. Spectral density - Wikipedia

    en.wikipedia.org/wiki/Spectral_density

    The value of the energy spectral density at is then estimated to be () /. In this example, since the power V ( t ) 2 / Z {\displaystyle V(t)^{2}/Z} has units of V 2 Ω −1 , the energy E ( f ) {\displaystyle E(f)} has units of V 2 s Ω −1 = J , and hence the estimate E ( f ) / Δ f {\displaystyle E(f)/\Delta f} of the energy spectral density ...

  6. Institute of Medicine Equation - Wikipedia

    en.wikipedia.org/wiki/Institute_of_Medicine_Equation

    The Estimated Energy Requirement, , is the estimated number of daily kilocalories, or Calories, an individual requires in order to maintain his or her current weight. For a person with a body mass of m {\displaystyle m} (kg), height of h {\displaystyle h} (m), age of a {\displaystyle a} (years) and Physical Activity PA {\displaystyle {\text{PA ...

  7. Solar constant - Wikipedia

    en.wikipedia.org/wiki/Solar_constant

    In 1838, Claude Pouillet made the first estimate of the solar constant. Using a very simple pyrheliometer he developed, he obtained a value of 1.228 kW/m 2 , [ 6 ] close to the current estimate. In 1875, Jules Violle resumed the work of Pouillet and offered a somewhat larger estimate of 1.7 kW/m 2 based, in part, on a measurement that he made ...

  8. Luminous intensity - Wikipedia

    en.wikipedia.org/wiki/Luminous_intensity

    Light with the same radiant intensity at other wavelengths has a lower luminous intensity. The curve which represents the response of the human eye to light is a defined standard function y (λ) or V (λ) established by the International Commission on Illumination (CIE, for Commission Internationale de l'Éclairage ) and standardized in ...

  9. Specific energy - Wikipedia

    en.wikipedia.org/wiki/Specific_energy

    Energy density is the amount of energy per mass or volume of food. The energy density of a food can be determined from the label by dividing the energy per serving (usually in kilojoules or food calories) by the serving size (usually in grams, milliliters or fluid ounces). An energy unit commonly used in nutritional contexts within non-metric ...