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  2. Relativistic Doppler effect - Wikipedia

    en.wikipedia.org/wiki/Relativistic_Doppler_effect

    The relativistic Doppler effect is the change in frequency, wavelength and amplitude [1] of light, caused by the relative motion of the source and the observer (as in the classical Doppler effect, first proposed by Christian Doppler in 1842 [2]), when taking into account effects described by the special theory of relativity.

  3. Doppler effect - Wikipedia

    en.wikipedia.org/wiki/Doppler_effect

    [1] [2] [3] The Doppler effect is named after the physicist Christian Doppler, who described the phenomenon in 1842. A common example of Doppler shift is the change of pitch heard when a vehicle sounding a horn approaches and recedes from an observer. Compared to the emitted frequency, the received frequency is higher during the approach ...

  4. On the coloured light of the binary stars and some other ...

    en.wikipedia.org/wiki/On_the_coloured_light_of...

    Front cover Albireo, a well-known coloured double star.Compare the colour of other stars in . On the coloured light of the binary stars and some other stars of the heavens or in the original German Über das farbige Licht der Doppelsterne und einiger anderer Gestirne des Himmels is a treatise by Christian Doppler (1842) [1] in which he postulated his principle that the observed frequency ...

  5. Relativistic beaming - Wikipedia

    en.wikipedia.org/wiki/Relativistic_beaming

    Only a single jet is visible in M87. Two jets are visible in 3C 31.. In physics, relativistic beaming (also known as Doppler beaming, Doppler boosting, or the headlight effect) is the process by which relativistic effects modify the apparent luminosity of emitting matter that is moving at speeds close to the speed of light.

  6. Black-body radiation - Wikipedia

    en.wikipedia.org/wiki/Black-body_radiation

    The relativistic Doppler effect causes a shift in the frequency f of light originating from a source that is moving in relation to the observer, so that the wave is observed to have frequency f': ′ = ⁡ /, where v is the velocity of the source in the observer's rest frame, θ is the angle between the velocity vector and the observer-source ...

  7. List of effects - Wikipedia

    en.wikipedia.org/wiki/List_of_effects

    Relativistic Doppler effect (Doppler effects) (special relativity) Renner–Teller effect (molecular physics) Reverse Cerenkov effect (physics) Reverse short-channel effect (transistors) Ringelmann effect (social psychology) Ripple effect (education) (sociology) Robin Hood effect (income distribution) (Robin Hood) (socioeconomics) (taxation)

  8. Tests of special relativity - Wikipedia

    en.wikipedia.org/wiki/Tests_of_special_relativity

    Moving magnet and conductor problem (only relative motion is relevant), the Fizeau experiment and the aberration of light (both implying modified velocity addition and no complete aether drag). The result is special relativity theory, which is based on the constancy of the speed of light in all inertial frames of reference and the principle of ...

  9. Doppler cooling - Wikipedia

    en.wikipedia.org/wiki/Doppler_cooling

    Doppler cooling involves light with frequency tuned slightly below an electronic transition in an atom. Because the light is detuned to the "red" (i.e. at lower frequency) of the transition, the atoms will absorb more photons if they move towards the light source, due to the Doppler effect. Consider the simplest case of 1D motion on the x axis.