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Page 24
... equal to q1 , while the second has 92. Use symmetry arguments and Gauss's law to prove that ( a ) the surface - charge densities on the adjacent faces are equal and opposite ; ( b ) the surface - charge densities on the outer faces of ...
... equal to q1 , while the second has 92. Use symmetry arguments and Gauss's law to prove that ( a ) the surface - charge densities on the adjacent faces are equal and opposite ; ( b ) the surface - charge densities on the outer faces of ...
Page 334
... equal to vi the displacement current is unimportant . But , if va > c , then the phase velocity is equal to the velocity of light . From the point of view of electro- magnetic waves , the transverse Alfvén wave can be thought of as a ...
... equal to vi the displacement current is unimportant . But , if va > c , then the phase velocity is equal to the velocity of light . From the point of view of electro- magnetic waves , the transverse Alfvén wave can be thought of as a ...
Page 382
... equal to y times its nonrelati- vistic value . In the same limit , however , the duration of appreciable field strengths at the point P is decreased . A measure of the time interval over which the fields are appreciable is evidently b ...
... equal to y times its nonrelati- vistic value . In the same limit , however , the duration of appreciable field strengths at the point P is decreased . A measure of the time interval over which the fields are appreciable is evidently b ...
Contents
1 | 1 |
BoundaryValue Problems in Electrostatics I | 26 |
Dielectrics | 98 |
Copyright | |
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4-vector acceleration Ampère's law angle angular distribution antenna approximation atomic axis B₁ 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 diffraction dipole direction discussed E₁ electric field electromagnetic fields electron electrostatic energy loss energy transfer 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 plasma polarization power radiated problem radius region relativistic result S₁ scalar scattering screen shown in Fig shows sin² solid angle solution sphere spherical surface transverse unit V₁ vanishes vector potential velocity wave guide wave number wavelength ΦΩ