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  2. 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.

  3. Electromagnetic spectrum - Wikipedia

    en.wikipedia.org/wiki/Electromagnetic_spectrum

    Frequencies observed in astronomy range from 2.4 × 10 23 Hz (1 GeV gamma rays) down to the local plasma frequency of the ionized interstellar medium (~1 kHz). Wavelength is inversely proportional to the wave frequency, [1] so gamma rays have very short wavelengths that are fractions of the size of atoms, whereas wavelengths on the opposite end ...

  4. Electromagnetic radiation - Wikipedia

    en.wikipedia.org/wiki/Electromagnetic_radiation

    Frequency is inversely proportional to wavelength, according to the equation: [26] = where v is the speed of the wave (c in a vacuum or less in other media), f is the frequency and λ is the wavelength. As waves cross boundaries between different media, their speeds change but their frequencies remain constant.

  5. Planck constant - Wikipedia

    en.wikipedia.org/wiki/Planck_constant

    The Planck constant, or Planck's constant, denoted by , [1] is a fundamental physical constant [1] of foundational importance in quantum mechanics: a photon's energy is equal to its frequency multiplied by the Planck constant, and the wavelength of a matter wave equals the Planck constant divided by the associated particle momentum.

  6. Wien approximation - Wikipedia

    en.wikipedia.org/wiki/Wien_approximation

    [1] [2] [3] The equation does accurately describe the short-wavelength (high-frequency) spectrum of thermal emission from objects, but it fails to accurately fit the experimental data for long-wavelength (low-frequency) emission. [3]

  7. Surface plasmon polariton - Wikipedia

    en.wikipedia.org/wiki/Surface_plasmon_polariton

    The E-field of an SPP at the silver-air interface, at a much lower frequency corresponding to a free-space wavelength of 10μm. At this frequency, the silver behaves approximately as a perfect electric conductor , and the SPP is called a Sommerfeld–Zenneck wave , with almost the same wavelength as the free-space wavelength.

  8. 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). For a modulated wave, wavelength may refer to the carrier wavelength of the signal.

  9. Ion acoustic wave - Wikipedia

    en.wikipedia.org/wiki/Ion_acoustic_wave

    In plasma physics, an ion acoustic wave is one type of longitudinal oscillation of the ions and electrons in a plasma, much like acoustic waves traveling in neutral gas. . However, because the waves propagate through positively charged ions, ion acoustic waves can interact with their electromagnetic fields, as well as simple col