Univ California Berkeley Wiggler Radiation At very high K 1 the radiated energy appears in very high harmonics and at rather large ex03C4 521 Because the emission angles are large on ID: 217600
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For Very Large K >> 1, and Large Dτ, Univ. California, Berkeley Wiggler Radiation At very high K >> 1, the radiated energy appears in very high harmonics, and at rather large (eτ. 5.21). Because the emission angles are large, one tends to use larger collection angles, which tends to spectrally merge nearby harmonics. The result is a continuum at very high photon energies, similar to that of bending magnet radiation, Univ. California, Berkeley StanfordWiggler.aiStanford Permanent Magnet Wiggler LBNL/E;;2N/SSRL (1982), SSRL Beamline V, Univ. California, Berkeley Ch05_TimeStruc.ai Time Structure of Synchrotron RadiationThe axial electric field within the RF cavity, used to replenish lost (radiated) energy, forms a potential well “bucket” system that forces electrons into axial Time Time Univ. California, Berkeley Ch05_VariablePolar.ai Variable Polarization Undulator Radiation Variable phase delay Univ. California, Berkeley