Spontaneous Radiation in Relativistic Strophotron
Abstract
Spectral intensity of spontaneous radiation is calculated in relativistic strophotron. It is shown, that it in the strophotron is given by a superposition of contributions from emission at different (odd) harmonics of the main resonance frequency . The main resonance frequency is shown to depend on the initial conditions of the electron, and in particular on its initial transversal coordinate .
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