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The relationship between the duration of solar X-ray flares and the mass of associated coronal ejections
Authors:A N Shakhovskaya  Z S Akhtemov
Institution:11130. Crimean Astrophysical Observatory, National Academy of Sciences of Ukraine, Nauchnyi, Crimea, 98409, Ukraine
Abstract:The statistical relationship between the parameters of X-ray flares and coronal mass ejections on the Sun that are associated with these flares, is considered. It is shown that short X-ray flares are characterized on average by a lower mass ejection in the outer layers of the corona and interplanetary space as compared to high-energy long-duration events.
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