ERUPTIVE PHENOMENA IN THE SOLAR ATMOSPHERE: RADIATION-MHD MODELING AND CODE DEVELOPMENT
A bewildering variety of eruptive and ejective phenomena continually take place in the solar atmosphere on a wide range of space and time scales. Particular attention was devoted in the past decades to those associated with the reconnection of magnetic field lines of separate plasma systems that come into contact in the atmosphere, especially when
Daniel Nóbrega Siverio
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2018