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Information × Registration Number 0120U100278, ( 0222U000052  ) R & D request Title Possible mechanism of glow of solar flares: observation and numerical simulation Head Kostik Roman I., Доктор фізико-математичних наук Registration Date 31-01-2020 Organization Main Astronomical Observatory of the National Academy of Sciences of Ukraine popup.description1 The purpose of the project is to answer the question: solar flares are bright relative to the surrounding matter because, due to the presence of a strong magnetic field, the radiation emanates from deeper, and hence from the hotter layers of the solar atmosphere (due to the Wilson effect), as is currently considered, or is the plasma temperature in the flare really higher than the surrounding non-magnetic environment. popup.nrat_date 2024-12-10 Close