Características de los estallidos solares asociados a las regiones activas BBR No. 18422 y BBR No.18474 en junio y julio 1982
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Abstract
The more important characteristics of the BBR No. 18422 and 18474 active regions in the radio, optical and X-ray ranges are compiled. An attempt to obtain a statistical description of the developrnent process for these centers was done. Sorne aspects indicate a very close magnetic structure and a lowering of the corona over the active region during its evolution.
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References
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