Abstract
Velocity distribution functions of both the electron and the proton component of the magnetospheric plasma are measured in 62 logarithmically spaced steps from 50 eV to 50 keV by an instrument carried upon the ATS-5 spacecraft in circular synchronous orbit (6.6 earth radii). Oscillations which appear to be collisionless drift waves having periods of several minutes or longer are found in this data. Linearized wave theory can be use to predict the theoretical perturbation distribution function fT in terms of the perturbing fields and the equilibrium distribution function F. The functional dependence of the theoretical perturbation distribution function fT upon particle energy can then be compared with that of the measured perturbation fM. The linear wave theory is found to predict correctly a change in the sign of fM which occurs at a critical particle energy E* and the relative magnitude of fM over the entire energy range.
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