Characteristics of the escape of quasi-trapped electrons from the atmosphere

Physics

Scientific paper

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Electron Precipitation, High Energy Electrons, Magnetically Trapped Particles, Particle Motion, Secondary Emission, Upper Atmosphere, Albedo, Atmospheric Radiation, Cosmos Satellites, Electron Mobility, Electron Scattering, Forbidden Transitions, Longitude

Scientific paper

Previous studies have indicated the existence of high-energy (exceeding 100 MeV) electrons in a cone of pitch angles forbidden for direct-albedo particles at heights of 200-500 km above the earth's surface. The cone of forbidden angles can be filled by albedo electrons, having arrived at a given longitude due to longitudinal drift (such electrons are called quasi-trapped). This paper presents calculations which make it possible to determine the initial conditions under which the quasi-trapped electrons can escape from the atmosphere in order to be registered by satellites at the above-mentioned heights. Particular attention is given to conditions at the Brasilian anomaly, where the most efficient escape of quasi-trapped electrons due to longitudinal drift occurs.

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