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Some Properties of Microwave Emission From Flaring Regions
Authors:V R Maksimov  VL Shchepkina  EA Chernova
Institution:Institute of Solar-Terrestrial Physics, Siberian Branch, Russian Academy of Sciences, Irkutsk 664033, Russia
Abstract:A study is made of the differences in the polarization distribution and other characteristics of microwave emission for several active regionswith high flare productivity. Conclusions are drawn about the magnetic field structure of these regions at coronal heights.
Keywords:Microwave emission  Solar activity  Solar flare prediction
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