作者: G. Ya. Smol’kov , V. P. Maksimov , D. V. Prosovetskii , A. M. Uralov , I. A. Bakunina
DOI: 10.3103/S0190271710010055
关键词: Physics 、 Solar flare 、 Coronal mass ejection 、 Nanoflares 、 Astronomy 、 Microwave emission 、 Circular polarization 、 Astrophysics
摘要: An experience of radioheliographic prediction powerful solar flares using active region microwave emission intensity and circular polarization distribution is briefly described.