Classical Electrodynamics |
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Page 314
... perpendicular to B. From ( 10.16 ) it is apparent that flow parallel to B is governed by the nonelectromagnetic forces alone . The velocity of flow of the fluid perpendicular to B , on the other hand , decays from some initially ...
... perpendicular to B. From ( 10.16 ) it is apparent that flow parallel to B is governed by the nonelectromagnetic forces alone . The velocity of flow of the fluid perpendicular to B , on the other hand , decays from some initially ...
Page 476
John David Jackson. parallel to and perpendicular to the velocity . But we have just seen that for comparable parallel and perpendicular forces the radiation from the parallel component is negligible ( of order 1/72 ) compared to that ...
John David Jackson. parallel to and perpendicular to the velocity . But we have just seen that for comparable parallel and perpendicular forces the radiation from the parallel component is negligible ( of order 1/72 ) compared to that ...
Page 508
... perpendicular to the plane containing ẞ , and n . The direction of polarization of the radiation is given by the vector nx ( n x Aẞ ) . This is perpendicular to n ( as it must be ) and can be resolved into components along 1 , and ...
... perpendicular to the plane containing ẞ , and n . The direction of polarization of the radiation is given by the vector nx ( n x Aẞ ) . This is perpendicular to n ( as it must be ) and can be resolved into components along 1 , and ...
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