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  2. Wien's displacement law - Wikipedia

    en.wikipedia.org/wiki/Wien's_displacement_law

    Using Wien's law, one finds a peak emission per nanometer (of wavelength) at a wavelength of about 500 nm, in the green portion of the spectrum near the peak sensitivity of the human eye. [3] [4] On the other hand, in terms of power per unit optical frequency, the Sun's peak emission is at 343 THz or a wavelength of 883 nm in the near infrared ...

  3. Electromagnetic spectrum - Wikipedia

    en.wikipedia.org/wiki/Electromagnetic_spectrum

    In frequency (and thus energy), UV rays sit between the violet end of the visible spectrum and the X-ray range. The UV wavelength spectrum ranges from 399 nm to 10 nm and is divided into 3 sections: UVA, UVB, and UVC. UV is the lowest energy range energetic enough to ionize atoms, separating electrons from them, and thus causing chemical reactions.

  4. Wavelength - Wikipedia

    en.wikipedia.org/wiki/Wavelength

    Wavelength is a characteristic of both traveling waves and standing waves, as well as other spatial wave patterns. [3] [4] The inverse of the wavelength is called the spatial frequency. Wavelength is commonly designated by the Greek letter lambda (λ).

  5. Visible spectrum - Wikipedia

    en.wikipedia.org/wiki/Visible_spectrum

    The LWS opsin of birds is sometimes reported to have a peak wavelength above 600 nm, but this is an effective peak wavelength that incorporates the filter of avian oil droplets. [34] The peak wavelength of the LWS opsin alone is the better predictor of the long-wave limit.

  6. Electromagnetic radiation - Wikipedia

    en.wikipedia.org/wiki/Electromagnetic_radiation

    A monochromatic electromagnetic wave can be characterized by its frequency or wavelength, its peak amplitude, its phase relative to some reference phase, its direction of propagation, and its polarization. Interference is the superposition of two or more waves resulting in a new wave pattern.

  7. Planck's law - Wikipedia

    en.wikipedia.org/wiki/Planck's_law

    The 41.8% point is the wavelength-frequency-neutral peak (i.e. the peak in power per unit change in logarithm of wavelength or frequency). These are the points at which the respective Planck-law functions ⁠ 1 / λ 5 ⁠ , ν 3 and ⁠ ν 2 / λ 2 ⁠ , respectively, divided by exp ( ⁠ hν / k B T ⁠ ) − 1 attain their maxima.

  8. Wien approximation - Wikipedia

    en.wikipedia.org/wiki/Wien_approximation

    The peak value of this curve, as determined by setting the derivative of the equation equal to zero and solving, [7] occurs at a wavelength = , and frequency = . Relation to Planck's law [ edit ]

  9. Spectral density - Wikipedia

    en.wikipedia.org/wiki/Spectral_density

    The spectral centroid of a signal is the midpoint of its spectral density function, i.e. the frequency that divides the distribution into two equal parts. The spectral edge frequency (SEF), usually expressed as "SEF x", represents the frequency below which x percent of the total power of a given signal are located; typically, x is in the range ...