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Relativistic Doppler effect
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===Motion in an arbitrary direction=== [[File:Doppler shift with source and receiver moving at arbitrary angles.svg|thumb|Figure 7. Doppler shift with source moving at an arbitrary angle with respect to the line between source and receiver.]] The analysis used in section [[#Relativistic longitudinal Doppler effect|Relativistic longitudinal Doppler effect]] can be extended in a straightforward fashion to calculate the Doppler shift for the case where the inertial motions of the source and receiver are at any specified angle.<ref name=Gill/><ref name=Brown_a> {{cite web | last=Brown |first=Kevin S. | title = Doppler Shift for Sound and Light | url = http://www.mathpages.com/rr/s2-04/2-04.htm | publisher = Mathpages | access-date = 6 August 2015 }}</ref> Fig. 7 presents the scenario from the frame of the receiver, with the source moving at speed <math>v</math> at an angle <math>\theta_r</math> measured in the frame of the receiver. The radial component of the source's motion along the line of sight is equal to <math>v \cos{\theta_r}.</math> The equation below can be interpreted as the classical Doppler shift for a stationary and moving source modified by the Lorentz factor <math>\gamma :</math> {{NumBlk||<math display="block"> f_r = \frac{f_s}{\gamma\left(1 + \beta \cos\theta_r\right)}.</math>|{{EquationRef|6|Eq. 6}}}} In the case when <math>\theta_r = 90^{\circ}</math>, one obtains the [[#Transverse Doppler effect|transverse Doppler effect]]: <math display="block">f_r = \frac {f_s} {\gamma}. </math> {{anchor|Einstein Doppler shift equation}} In his 1905 paper on special relativity,<ref group=p name=Einstein1905/> Einstein obtained a somewhat different looking equation for the Doppler shift equation. After changing the variable names in Einstein's equation to be consistent with those used here, his equation reads {{NumBlk||<math display="block"> f_r = \gamma \left( 1 - \beta \cos \theta_s \right) f_s.</math>|{{EquationRef|7|Eq. 7}}}} The differences stem from the fact that Einstein evaluated the angle <math>\theta_s</math> with respect to the source rest frame rather than the receiver rest frame. <math> \theta_s</math> is not equal to <math> \theta_r </math> because of the effect of [[relativistic aberration]]. The relativistic aberration equation is: {{NumBlk||<math display="block">\cos \theta_r=\frac{\cos \theta_s-\beta }{1-\beta \cos \theta_s} </math>|{{EquationRef|8|Eq. 8}}}} Substituting the relativistic aberration equation {{EquationNote|8|Equation 8}} into {{EquationNote|6|Equation 6}} yields {{EquationNote|7|Equation 7}}, demonstrating the consistency of these alternate equations for the Doppler shift.<ref name=Brown_a/> Setting <math>\theta_r = 0</math> in {{EquationNote|6|Equation 6}} or <math>\theta_s = 0</math> in {{EquationNote|7|Equation 7}} yields {{EquationNote|1|Equation 1}}, the expression for relativistic longitudinal Doppler shift. A four-vector approach to deriving these results may be found in Landau and Lifshitz (2005).<ref name=Landau>{{cite book| title=The Classical Theory of Fields | series=Course of Theoretical Physics: Volume 2 | last1=Landau | first1=L.D. | author-link1=Lev Landau | last2=Lifshitz | first2=E.M. | author-link2=Evgeny Lifshitz | others=Trans. Morton Hamermesh | publisher=Elsevier Butterworth-Heinemann | year=2005 | edition=Fourth revised English | pages=116β117 | isbn=9780750627689}}</ref> In electromagnetic waves both the electric and the magnetic field amplitudes ''E'' and ''B'' transform in a similar manner as the frequency:<ref>{{cite book |title=Einstein's Physics: Atoms, Quanta, and Relativity - Derived, Explained, and Appraised |author1=Ta-Pei Cheng |edition=illustrated, reprinted |publisher=OUP Oxford |year=2013 |isbn=978-0-19-966991-2 |page=164 |url=https://books.google.com/books?id=thXT19cY9jsC}} [https://books.google.com/books?id=thXT19cY9jsC&pg=PA164 Extract of page 164]</ref> <math display="block">\begin{align} E_r &= \gamma \left( 1 - \beta \cos \theta_s \right) E_s \\ B_r &= \gamma \left( 1 - \beta \cos \theta_s \right) B_s. \end{align} </math>
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