Classical Electrodynamics |
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E PARALLEL TO PLANE OF INCIDENCE * = 2 Le sin 2i —o- 2 cos i sin r Eo **
sin 2r + * sin 2i o" (i + r.) cos (i — r) pr * sin 2i — sin 2r - (7.60) Eo" — 4 -> tan (i —
r) * in 2, 14 in 2: "( t ) Au Again the results on the right apply for u' = u. For normal
...
E PARALLEL TO PLANE OF INCIDENCE * = 2 Le sin 2i —o- 2 cos i sin r Eo **
sin 2r + * sin 2i o" (i + r.) cos (i — r) pr * sin 2i — sin 2r - (7.60) Eo" — 4 -> tan (i —
r) * in 2, 14 in 2: "( t ) Au Again the results on the right apply for u' = u. For normal
...
Page
E is parallel to the r axis; B is parallel to the y axis. (a) For |E| < |B make the
necessary Lorentz transformation described in Section 12.8 to obtain explicitly
parametric equations for the particle's trajectory. (b) Repeat the calculation of (a)
for |E| > ...
E is parallel to the r axis; B is parallel to the y axis. (a) For |E| < |B make the
necessary Lorentz transformation described in Section 12.8 to obtain explicitly
parametric equations for the particle's trajectory. (b) Repeat the calculation of (a)
for |E| > ...
Page
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.
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Contents
Introduction to Electrostatics | 1 |
Nš 3 | 3 |
Greens theorem | 14 |
Copyright | |
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