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- W4252183831 abstract "A stellar flare model in which the main energy release is located above the chromosphere based on a set of elementary acts of the electron acceleration or impulsive heating of plasma is discussed. The response of the chromosphere to impulsive heating for both a single burst and the simultaneous effect of a set of the bursts is considered. The results of numerical modeling of the process of explosive evaporation of the stellar chromosphere allow us to select 3 classes of EUV emission source: (1) the bursts of the EUV emission in the temperature range of 3 · 10 4 – 3 · 10 5 K at the beginning of each of elementary act of the energy release; (2) the bursts of the EUV emission at temperatures T ≈ 10 6 K, accompanied by outflow of heated plasma; (3) the EUV emission, caused by new features of the process, namely, when the maxima of the distribution of the pressure are forming in the region of the downward-moving thermal front. The properties of the EUV sources, velocities of the plasma motions therein, and possible behaviour of the light curve for an elementary burst are discussed." @default.
- W4252183831 created "2022-05-12" @default.
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- W4252183831 date "1996-01-01" @default.
- W4252183831 modified "2023-09-30" @default.
- W4252183831 title "EUV Emission Sources in Gas-Dynamic Models of Stellar Flares" @default.
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- W4252183831 cites W2027607094 @default.
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- W4252183831 doi "https://doi.org/10.1017/s0252921100035922" @default.
- W4252183831 hasPublicationYear "1996" @default.
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