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  2. Maxwell's equations - Wikipedia

    en.wikipedia.org/wiki/Maxwell's_equations

    The net electric current I is the surface integral of the electric current density J passing through Σ: =, where dS denotes the differential vector element of surface area S, normal to surface Σ. (Vector area is sometimes denoted by A rather than S , but this conflicts with the notation for magnetic vector potential ).

  3. List of equations in wave theory - Wikipedia

    en.wikipedia.org/wiki/List_of_equations_in_wave...

    Position of a point in space, not necessarily a point on the wave profile or any line of propagation d, r: m [L] Wave profile displacement Along propagation direction, distance travelled (path length) by one wave from the source point r 0 to any point in space d (for longitudinal or transverse waves) L, d, r

  4. Critical frequency - Wikipedia

    en.wikipedia.org/wiki/Critical_frequency

    Critical Frequency changes with time of day, atmospheric conditions and angle of fire of the radio waves by antenna. The existence of the critical frequency is the result of electron limitation, i.e., the inadequacy of the existing number of free electrons to support reflection at higher frequencies.

  5. Planck's law - Wikipedia

    en.wikipedia.org/wiki/Planck's_law

    Analogous to the wave function of a particle in a box, one finds that the fields are superpositions of periodic functions. The three wavelengths λ 1 , λ 2 , and λ 3 , in the three directions orthogonal to the walls can be: λ i = 2 L n i , {\displaystyle \lambda _{i}={\frac {2L}{n_{i}}},} where the n i are positive integers.

  6. Coherence time - Wikipedia

    en.wikipedia.org/wiki/Coherence_time

    The coherence time, usually designated τ, is calculated by dividing the coherence length by the phase velocity of light in a medium; approximately given by = where λ is the central wavelength of the source, Δν and Δλ is the spectral width of the source in units of frequency and wavelength respectively, and c is the speed of light in vacuum.

  7. Sommerfeld radiation condition - Wikipedia

    en.wikipedia.org/wiki/Sommerfeld_radiation_condition

    It was introduced by Arnold Sommerfeld in 1912 [1] and is closely related to the limiting absorption principle (1905) and the limiting amplitude principle (1948). The boundary condition established by the principle essentially chooses a solution of some wave equations which only radiates outwards from known sources.

  8. Monopole antenna - Wikipedia

    en.wikipedia.org/wiki/Monopole_antenna

    The current and voltage along the element are sinusoidal waves. The current in the antenna element bounces back and forth between the ends, and the two equal but opposite current waves interfere to form a standing wave. [63] [64] The standing wave has a current node at its top and either a node or an antinode at bottom. Due to these end ...

  9. 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.