Classical Electrodynamics |
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Page 169
... magnetic phenomena disappears when we consider time - dependent problems . Time - varying magnetic fields give rise to electric fields and vice - versa . We then must speak of electromagnetic fields , rather than electric or magnetic fields ...
... magnetic phenomena disappears when we consider time - dependent problems . Time - varying magnetic fields give rise to electric fields and vice - versa . We then must speak of electromagnetic fields , rather than electric or magnetic fields ...
Page 189
... electromagnetic fields E and B is qv . E , where v is the velocity of the charge . The magnetic field does no work , since the magnetic force is perpendicular to the velocity . If there exists a continuous distribution of charge and ...
... electromagnetic fields E and B is qv . E , where v is the velocity of the charge . The magnetic field does no work , since the magnetic force is perpendicular to the velocity . If there exists a continuous distribution of charge and ...
Page 380
... Electromagnetic Fields Since the fields E and B are elements of the field - strength tensor F their transformation properties can be found from = F'Av Fuvaμavo Fi μες ( 11.113 ) With transformation ( 11.75 ) from a system K to K ...
... Electromagnetic Fields Since the fields E and B are elements of the field - strength tensor F their transformation properties can be found from = F'Av Fuvaμavo Fi μες ( 11.113 ) With transformation ( 11.75 ) from a system K to K ...
Common terms and phrases
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