Fine structure and long duration of a flare coronal X-ray source with RHESSI and SDO/AIA data
Sylwester Kolomanski,
Tomasz Mrozek,
Ewa Chmielewska
Abstract:Context. Coronal X-ray sources (CXSs) are phenomenon very often occurring in solar flares regardless of a flare size, duration or power. The nature of the sources was difficult to uncover for many years. It seems that at last, combining data from RHESSI and SDO/AIA, there is a unprecedented possibility to 'look inside' CXSs and to answer the questions about their formation, evolution and structure.Aims. We present a study of a CXS of the SOL2011-10-22T11:10 long-duration flare observed simultaneously with RHES… Show more
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