Classical Electrodynamics |
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Page 354
... origin ) to detect the arrival time of a light signal from the origin at various points in space . If there is a light source at rest in the system K ( and so moving with velocity v in the negative z direction in system K ' ) which is ...
... origin ) to detect the arrival time of a light signal from the origin at various points in space . If there is a light source at rest in the system K ( and so moving with velocity v in the negative z direction in system K ' ) which is ...
Page 363
... origin coincident with that of K at t = 0. An observer in K ' at the point P ' with coordinate x ' is equipped similarly to the one in K. He begins counting when the wave crest passing the origin reaches him , and con- tinues counting ...
... origin coincident with that of K at t = 0. An observer in K ' at the point P ' with coordinate x ' is equipped similarly to the one in K. He begins counting when the wave crest passing the origin reaches him , and con- tinues counting ...
Page 436
... origin O. Using the Fourier representations ( 13.16 ) and ( 13.17 ) , as well as that for a delta function ( 2.52 ) ... origin O at an impact parameter b with a velocity v , the electromagnetic fields at the origin are given by ( 11.118 ) ...
... origin O. Using the Fourier representations ( 13.16 ) and ( 13.17 ) , as well as that for a delta function ( 2.52 ) ... origin O at an impact parameter b with a velocity v , the electromagnetic fields at the origin are given by ( 11.118 ) ...
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4-vector acceleration Ampère's law angle angular distribution antenna approximation atomic axis Babinet's principle behavior boundary conditions calculate cavity Chapter charge q charged particle coefficients collisions component conducting conductor constant coordinate cross section cylinder d³x dielectric dielectric constant diffraction dipole direction discussed E₁ electric field electromagnetic fields electron electrostatic energy loss factor force equation frame frequency given Green's function impact parameter incident particle integral Kirchhoff Lagrangian Laplace's equation Lorentz force Lorentz invariant Lorentz transformation m₁ magnetic field magnetic induction magnitude Maxwell's equations meson modes momentum multipole nonrelativistic obtain oscillations P₁ P₂ parallel perpendicular phase velocity plane wave plasma polarization power radiated problem propagation radius region relativistic result scalar scattering screen shown in Fig shows sin² solution sphere spherical surface transverse unit V₁ vanishes vector potential velocity wave guide wave number wavelength ΦΩ