Classical Electrodynamics |
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Page 313
... fields occur . The time dependence of the magnetic field can be written , using ( 10.8 ) to eliminate E , in the form : дв at = ▽ x ( v x B ) + c2 Απσ V2B ( 10.10 ) Here it is assumed that σ is constant in space . For a fluid at rest ...
... fields occur . The time dependence of the magnetic field can be written , using ( 10.8 ) to eliminate E , in the form : дв at = ▽ x ( v x B ) + c2 Απσ V2B ( 10.10 ) Here it is assumed that σ is constant in space . For a fluid at rest ...
Page 382
John David Jackson. induction in the x2 direction . This magnetic field becomes almost equal to the transverse electric field E1 as ẞ - > 1. Even at nonrelativistic velocities where y 1 , this magnetic induction is equivalent to B с ...
John David Jackson. induction in the x2 direction . This magnetic field becomes almost equal to the transverse electric field E1 as ẞ - > 1. Even at nonrelativistic velocities where y 1 , this magnetic induction is equivalent to B с ...
Page 419
... field . Consequently they experience no net drift , at least to first order in 1 / R . This method of eliminating drifts due to spatial variations of the magnetic field is used in the Stellarator type of thermonuclear machine , in which ...
... field . Consequently they experience no net drift , at least to first order in 1 / R . This method of eliminating drifts due to spatial variations of the magnetic field is used in the Stellarator type of thermonuclear machine , in which ...
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