Classical ElectrodynamicsProblems after each chapter |
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Page 222
... propagating is a conductor , there are characteristic differences in the propagation , when compared with non- conducting media . If the medium is characterized by a conductivity σ , as well as a dielectric constante and permeability μ ...
... propagating is a conductor , there are characteristic differences in the propagation , when compared with non- conducting media . If the medium is characterized by a conductivity σ , as well as a dielectric constante and permeability μ ...
Page 229
... propagate differently . The ionosphere is birefringent . For propagation in directions other than parallel to the static field Bo it is straightforward to show that , if terms of the order of 2 are neglected compared to @ 2 and wwp ...
... propagate differently . The ionosphere is birefringent . For propagation in directions other than parallel to the static field Bo it is straightforward to show that , if terms of the order of 2 are neglected compared to @ 2 and wwp ...
Page 233
... propagation with different phase velocities v = w / k which satisfy the Fresnel equation , 3 n , 2 = 0 v2 vi where v1 = c / V , is called a principal velocity , and n , is the component of n along the ith principal axis . • ( c ) Show ...
... propagation with different phase velocities v = w / k which satisfy the Fresnel equation , 3 n , 2 = 0 v2 vi where v1 = c / V , is called a principal velocity , and n , is the component of n along the ith principal axis . • ( c ) Show ...
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4-vector Ampère's law angle angular distribution approximation atomic axis boundary conditions calculate Chapter charge density charge q charged particle coefficients collisions component conductor consider coordinates cross section current density cylinder d³x delta function dielectric constant diffraction dimensions dipole direction discussed E₁ electric field electromagnetic fields electron electrostatic energy loss expansion expression factor frequency given Green's function impact parameter incident particle inside integral inversion Laplace's equation linear Lorentz transformation macroscopic magnetic field magnetic induction magnetic moment magnitude Maxwell's equations meson modes molecules momentum motion multipole nonrelativistic normal obtain oscillations P₁ parallel plasma point charge Poisson's equation polarization problem radiation radius region relativistic result scalar scalar potential scattering shown in Fig shows solution spherical surface surface-charge density theorem transverse unit V₁ vanishes vector potential velocity volume wave equation wave number wavelength written zero ΦΩ