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- W2018772088 abstract "A large data base on solar flares obtained during the last solar maximum years makes it necessary to revise our views on the relationship between the impulsive phase and the second phase of flares. Contrary to the view most popular before the launch of the Solar Maximum Mission, we now know that realistic electrons and γ-ray-producing protons and ions are accelerated during the impulsive phase. Because flares producing nuclear γ rays are different from ordinary flares, I conclude that additional processes take place in γ-ray-line flares. In my recent studies I have shown that flares with gradual hard X-ray time profiles not only produce nuclear γ rays during the impulsive phase but also develop full-fledged second-phase phenomena. I propose that filament eruption plays a key role in γ-ray-line flares. When an erupting filament interacts with an overlying flare loop, relativistic electrons and energetic protons are produced during the impulsive phase. When the erupting filament fully distends the overlying flare loop, full-fledged second-phase phenomena, such as shocks, interplanetary energetic particles, mass ejections and etc. are observed. When the overlying flare loop is compact and strong enough to supress the activated filament, γ-rays are emitted during the first phase but no second-phase phenomena occur." @default.
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- W2018772088 date "1986-01-01" @default.
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- W2018772088 title "Classification of solar flares and the relationship between the first and second phases" @default.
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- W2018772088 doi "https://doi.org/10.1016/0273-1177(86)90146-8" @default.
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