Abstract
The radiation emitted by self-supporting Ag foils 700 to 1700 Å in thickness was investigated as a function of angle of electron incidence, foil thickness, and degree of polarization. For a foil 700 Å in thickness, the peak at 3300 Å characteristic of transition radiation was found in the emission spectrum when the foil was bombarded by normally incident electrons (θi=0). The wavelength at which the peak appeared increased monotonically with increasing angles of electron incidence until it appeared at λ=3400 Å for θi=87. For a foil 1680 Å in thickness, the transition radiation peak at λ=3300 Å was found to decrease in intensity as θi increased from normal incidence and finally disappeared at θi=80. For θi>75, another peak appeared at 3500 Å, which increased in intensity for θi>85, and finally became an intense peak at λ=3600 Å, for θi=89. The dependence of the peak at 3500-3600 Å for large angles of electron incidence on θi, electron energy, and polarization agrees with details predicted by a model due to Howe and Ritchie based upon the production of bremsstrahlung in a semi-infinite slab, and leads to the conclusion that the optical emission observed from Ag foils bombarded by grazing-incidence electrons is bremsstrahlung, and not radiation from the decay of surface plasmons, as hypothesized by Boersch et al.