Classical ElectrodynamicsThis edition refines and improves the first edition. It treats the present experimental limits on the mass of photon and the status of linear superposition, and introduces many other innovations. |
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Page 424
... spectrum of solar radiation ( in watts per square meter per electron volt ) as a function of photon energy ( in electron volts ) . Curve A is the incident spectrum above the atmosphere . Curve B is a typical sea - level spectrum with ...
... spectrum of solar radiation ( in watts per square meter per electron volt ) as a function of photon energy ( in electron volts ) . Curve A is the incident spectrum above the atmosphere . Curve B is a typical sea - level spectrum with ...
Page 691
... spectrum peaks at n = 1 and then falls relatively slowly as n until the value = v2 is reached . Then it falls off as n3 . For v≥1 , the spectrum peaks at n and falls at n3 for n >> 1. At n = 0 the denominator in ( 14.129 ) is ( 1 + v2 ) ...
... spectrum peaks at n = 1 and then falls relatively slowly as n until the value = v2 is reached . Then it falls off as n3 . For v≥1 , the spectrum peaks at n and falls at n3 for n >> 1. At n = 0 the denominator in ( 14.129 ) is ( 1 + v2 ) ...
Page 732
... Spectrum of photons emitted in orbital electron capture because of dis- appearance of the magnetic moment of the electron . upper end of the spectrum will be dominated by the magnetic - moment contribu- tion , unless the energy release ...
... Spectrum of photons emitted in orbital electron capture because of dis- appearance of the magnetic moment of the electron . upper end of the spectrum will be dominated by the magnetic - moment contribu- tion , unless the energy release ...
Contents
L2 The Inverse Square Law or the Mass of the Photon | 1 |
BoundaryValue Problems | 54 |
Multipoles Electrostatics | 136 |
Copyright | |
17 other sections not shown
Common terms and phrases
4-vector Ampère's law amplitude angle angular distribution angular momentum approximation atomic axis behavior boundary conditions calculate Chapter charge density charge q charged particle classical coefficients collision components conducting conductor consider coordinates cross section current density cylinder d³x defined dielectric constant diffraction dimensions dipole direction discussed electric and magnetic electric field electromagnetic fields electrons electrostatic expansion expression factor force frame frequency given Green function incident integral limit linear Lorentz transformation macroscopic magnetic field magnetic induction magnetic monopole magnitude Maxwell equations medium modes molecules motion multipole multipole expansion multipole moments nonrelativistic normal obtained oscillations parallel parameter photon Phys plane wave plasma polarization problem propagation quantum quantum-mechanical radiation radius region relativistic result scattering shown in Fig sin² solution spectrum sphere spherical surface tensor theorem transverse unit V₁ vanishes vector potential velocity volume wave guide wave number wavelength written zero ΦΩ