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Page 251
... dependence . Thus , using ( 8.59 ) with ( 8.62 ) and ( 8.51 ) , plus the frequency dependence of the skin depth ( 7.85 ) , we find 1/2 ( 1 ) Pi = [ + ] 1 C μ σδι 2A 21⁄2 [ & + n ( 2 ) ] ( 8.63 ) * @ 2 where σ is the conductivity ...
... dependence . Thus , using ( 8.59 ) with ( 8.62 ) and ( 8.51 ) , plus the frequency dependence of the skin depth ( 7.85 ) , we find 1/2 ( 1 ) Pi = [ + ] 1 C μ σδι 2A 21⁄2 [ & + n ( 2 ) ] ( 8.63 ) * @ 2 where σ is the conductivity ...
Page 269
... dependence ( 9.1 ) , the solution for A becomes A ( x ) = = √ J ( x ) - eikx - x ' d3x ' | x x ' | ( 9.3 ) where k = w / c is the wave number , and a sinusoidal time dependence is understood . The magnetic induction is given by B = V ...
... dependence ( 9.1 ) , the solution for A becomes A ( x ) = = √ J ( x ) - eikx - x ' d3x ' | x x ' | ( 9.3 ) where k = w / c is the wave number , and a sinusoidal time dependence is understood . The magnetic induction is given by B = V ...
Page 296
... dependence on number . But the scalar result has no azimuthal dependence ( apart from that contained in § ) , whereas the vector expression does . The azimuthal variation comes from the polarization properties of the field , and must be ...
... dependence on number . But the scalar result has no azimuthal dependence ( apart from that contained in § ) , whereas the vector expression does . The azimuthal variation comes from the polarization properties of the field , and must be ...
Contents
1 | 1 |
Greens theorem | 14 |
BoundaryValue Problems in Electrostatics I | 26 |
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4-vector acceleration Ampère's law angular distribution antenna approximation atomic axis B₁ Babinet's principle behavior boundary conditions calculate Chapter charge q charged particle classical coefficients collisions component conducting conductor constant coordinate cross section cylinder d³x dielectric diffraction dimensions dipole direction discussed E₁ effects electric field electromagnetic fields electrons electrostatic energy loss energy transfer factor force equation formula frequency given Green's function impact parameter incident particle integral Kirchhoff Lorentz invariant Lorentz transformation magnetic field magnetic induction magnitude Maxwell's equations meson modes momentum motion multipole nonrelativistic obtain oscillations P₁ parallel perpendicular plane wave plasma plasma oscillations polarization power radiated Poynting's vector problem propagation quantum quantum-mechanical radius region relativistic result scalar scattering screen shown in Fig shows sin² solid angle solution sphere spherical surface transverse unit V₁ vanishes vector potential velocity wave number wavelength ΦΩ