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 447
9.13 Scattering in the ShortWavelength Limit Scattering in the longwavelength
limit has been discussed in Sections 9.6 and 9.7. The opposite limit, similar to the
Kirchhoff domain of diffraction, is a scattering by obstacles large compared to a ...
9.13 Scattering in the ShortWavelength Limit Scattering in the longwavelength
limit has been discussed in Sections 9.6 and 9.7. The opposite limit, similar to the
Kirchhoff domain of diffraction, is a scattering by obstacles large compared to a ...
Page 774
We specialize now to the longwavelength limit (ka« 1) for a perfectly conducting
sphere (Z, = 0), and leave examples of slightly more complexity to the problems.
Only the 1= 1 terms in (16.147) are important. From (16.153) we find ...
We specialize now to the longwavelength limit (ka« 1) for a perfectly conducting
sphere (Z, = 0), and leave examples of slightly more complexity to the problems.
Only the 1= 1 terms in (16.147) are important. From (16.153) we find ...
Page 778
Tabulate the wavelength (defined in terms of the real part of the frequency) in
units of the radius a and the decay time (defined as the time taken for the energy
to fall to e~' of its initial value) in units of the transit time (ale) for each of the
modes.
Tabulate the wavelength (defined in terms of the real part of the frequency) in
units of the radius a and the decay time (defined as the time taken for the energy
to fall to e~' of its initial value) in units of the transit time (ale) for each of the
modes.
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Contents
Introduction and Survey  1 
Introduction to Electrostatics  27 
BoundaryValue Problems  54 
Copyright  
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