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• W2550249918 abstract "New X-ray and extreme ultraviolet (EUV) irradiance observations from the Solar Dynamics Observatory (SDO) EUV Variability Experiment (EVE) provide full coverage from 0.1 to 106 nm at 0.1 nm resolution and with a cadence of 10 sec. These observations during flares can usually be decomposed into four distinct characteristics. First, the emissions that dominate during the flare's impulsive phase are the transition region emissions, such as the He II 30.4 nm. Second, the hot coronal emissions above 5 MK dominate during the gradual phase and are highly correlated with the X-ray measurements. A third flare characteristic is coronal dimming, seen best in the cool coronal emissions such as the Fe IX 17.1 nm. The coronal dimming appears to be related to coronal mass ejections (CMEs), thus representing a new way to possibly estimate CME parameters from SDO observations. As the postflare loops reconnect and cool, warm coronal emissions (e.g., Fe XVI 33.5 nm) peak a few minutes after the X-ray peak and sometimes exhibit a second large peak by many minutes to hours later. We refer to this second peak as the EUV late phase (ELP), which is the fourth flare characteristic. The characterization of many flares during the SDO mission is provided, noting that only some flares have all four phases." @default.
• W2550249918 created "2016-11-30" @default.
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• W2550249918 date "2016-10-05" @default.
• W2550249918 modified "2023-09-23" @default.
• W2550249918 title "Spectrally Resolved X-Ray and Extreme Ultraviolet Irradiance Variations During Solar Flares" @default.
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• W2550249918 doi "https://doi.org/10.1002/9781118929216.ch19" @default.
• W2550249918 hasPublicationYear "2016" @default.
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