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- W2893032161 abstract "For brightness classes this trend is less pronounced. We have found that flares with explosive phase and flares with one brilliant point have the shortest flash phases; two-ribbon flares and flares with several intensity maxima, the longest ones. We have separated 572 cases when the brightness rise time was more than 60 min; 80 % of such ultra-long flares have a shorter brightness decay time (main phase). We have established that low-power flares in terms of developmental features do not differ from large flares. Low-power solar flares, as well as large flares, can be followed by filament activation or disappearance, and can have an explosive phase and several intensity maxima. Two-ribbon flares, white-light flares, and flares covering sunspot umbra can also have low power." @default.
- W2893032161 created "2018-10-05" @default.
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- W2893032161 date "2018-09-28" @default.
- W2893032161 modified "2023-09-27" @default.
- W2893032161 title "Distribution of low-power solar flares by brightness rise time" @default.
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- W2893032161 doi "https://doi.org/10.12737/stp-43201801" @default.
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