Classical Electrodynamics |
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Page 412
The motion described by (12.93) is a circular motion perpendicular to B and a
uniform translation parallel to B. The solution for the velocity is easily shown to be
v(t) = uses + ora(e) – ies)e “” (12.95) where ea is a unit vector parallel to the field,
...
The motion described by (12.93) is a circular motion perpendicular to B and a
uniform translation parallel to B. The solution for the velocity is easily shown to be
v(t) = uses + ora(e) – ies)e “” (12.95) where ea is a unit vector parallel to the field,
...
Page 476
parallel to and perpendicular to the velocity. But we have just seen that for
comparable parallel and perpendicular forces the radiation from the parallel
component is negligible (of order 1/y”) compared to that from the perpendicular
component.
parallel to and perpendicular to the velocity. But we have just seen that for
comparable parallel and perpendicular forces the radiation from the parallel
component is negligible (of order 1/y”) compared to that from the perpendicular
component.
Page 575
The uniform charge density of Problem 16.2 is replaced by a uniform density of
intrinsic magnetization parallel to the z axis and having total magnetic moment M.
With the same approximations as above calculate the nonvanishing radiation ...
The uniform charge density of Problem 16.2 is replaced by a uniform density of
intrinsic magnetization parallel to the z axis and having total magnetic moment M.
With the same approximations as above calculate the nonvanishing radiation ...
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Contents
Introduction to Electrostatics | 1 |
References and suggested reading | 23 |
Multipoles Electrostatics of Macroscopic Media | 98 |
Copyright | |
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