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  2. Inverse-square law - Wikipedia

    en.wikipedia.org/wiki/Inverse-square_law

    The divergence of a vector field which is the resultant of radial inverse-square law fields with respect to one or more sources is proportional to the strength of the local sources, and hence zero outside sources. Newton's law of universal gravitation follows an inverse-square law, as do the effects of electric, light, sound, and radiation ...

  3. Distance modulus - Wikipedia

    en.wikipedia.org/wiki/Distance_modulus

    This definition is convenient because the observed brightness of a light source is related to its distance by the inverse square law (a source twice as far away appears one quarter as bright) and because brightnesses are usually expressed not directly, but in magnitudes.

  4. Cosmic distance ladder - Wikipedia

    en.wikipedia.org/wiki/Cosmic_distance_ladder

    Just as with standard candles, given the emitted and received amplitudes, the inverse-square law determines the distance to the source. There are some differences with standard candles, however. Gravitational waves are not emitted isotropically, but measuring the polarisation of the wave provides enough information to determine the angle of ...

  5. Luminosity distance - Wikipedia

    en.wikipedia.org/wiki/Luminosity_distance

    Calculating the relation between the apparent and actual luminosity of an object requires taking all of these factors into account. The object's actual luminosity is determined using the inverse-square law and the proportions of the object's apparent distance and luminosity distance.

  6. Near and far field - Wikipedia

    en.wikipedia.org/wiki/Near_and_far_field

    By contrast, the near-field ' s E and B strengths decrease more rapidly with distance: The radiative field decreases by the inverse-distance squared, the reactive field by an inverse-cube law, resulting in a diminished power in the parts of the electric field by an inverse fourth-power and sixth-power, respectively. The rapid drop in power ...

  7. Luminosity - Wikipedia

    en.wikipedia.org/wiki/Luminosity

    Luminosity is an intrinsic measurable property of a star independent of distance. The concept of magnitude, on the other hand, incorporates distance. The apparent magnitude is a measure of the diminishing flux of light as a result of distance according to the inverse-square law. [17]

  8. Intensity (physics) - Wikipedia

    en.wikipedia.org/wiki/Intensity_(physics)

    This is an example of the inverse-square law. Applying the law of conservation of energy, if the net power emanating is constant, =, where P is the net power radiated; I is the intensity vector as a function of position; the magnitude | I | is the intensity as a function of position;

  9. Attenuation - Wikipedia

    en.wikipedia.org/wiki/Attenuation

    Therefore, calculation of the total change in intensity involves both the inverse-square law and an estimation of attenuation over the path. The primary causes of attenuation in matter are the photoelectric effect , Compton scattering , and, for photon energies of above 1.022 MeV, pair production .