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Three years statistics of simple 3 solar bursts
Authors:Oscar T Matsuura  P Marques Dos Santos
Institution:(1) Centro de Rádio Astronomia e Astrofísica, Universidade Mackenzie, São Paulo, Brasil
Abstract:A plasmoid may be ejected during a flare and condensed by a radiative instability. The spectral shape of the mean fluxes of Simple 3 (or long-enduring) solar events is interpreted in terms of a thermal emission from this transient condensation in the higher levels of the solar atmosphere. This condensation is thick enough to block the radiation from the underlying S-component. This explanation fits the observed polarization changes, as well as the thermal character of the bursts time profiles. A clue for solar activity forecasting as well as for detailed studies of active sources is indicated.
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