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- W3099967879 abstract "We present different signatures of chromospheric evaporation in two solar flares observed by the Interface Region Imaging Spectrograph (IRIS). In the B1.6 flare on 2016 December 6 (SOL2016-12-06T10:40), the transition region Si IV line and the chromospheric C II and Mg II lines show blueshifts with low velocities up to 20 km/s at the flare loop footpoints in the rise phase, indicative of a gentle chromospheric evaporation. While in the C1.6 flare on 2015 December 19 (SOL2015-12-19T10:51), the Si IV, C II, and Mg II lines exhibit redshifts with velocities from several to tens of km/s at the footpoints, which might suggest an explosive chromospheric evaporation. Explosive evaporation has been observed in many flares that were captured by IRIS; however, gentle evaporation, especially manifested as blueshifts in the cool Si IV, C II, and Mg II lines, has scarcely been reported. Our results bring some new insights into chromospheric evaporation in the IRIS era." @default.
- W3099967879 created "2020-11-23" @default.
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- W3099967879 date "2019-07-01" @default.
- W3099967879 modified "2023-10-10" @default.
- W3099967879 title "Different Signatures of Chromospheric Evaporation in Two Solar Flares Observed with IRIS" @default.
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- W3099967879 doi "https://doi.org/10.3847/1538-4357/ab245a" @default.
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