PMO OpenIR  > 太阳活动的多波段观测研究团组
Observations of Electron-driven Evaporation in a Flare Precursor
Li, Dong; Li, Ying; Su, Wei; Huang, Yu; Ning, Zongjun
2018
发表期刊ASTROPHYSICAL JOURNAL
卷号854期号:1页码:26
摘要We investigate the relationship between the blueshifts of a hot emission line and the nonthermal emissions in microwave and hard X-ray (HXR) wavelengths in the precursor of a solar flare on 2014 October 27. The flare precursor is identified as a small but well-developed peak in the soft X-ray and extreme-ultraviolet passbands before the GOES flare onset, which is accompanied by a pronounced burst in microwave 17 and. 34 GHz and in HXR 25-50 keV. The slit of the Interface Region Imaging Spectrograph (IRIS) stays on one ribbon-like transient during the flare precursor phase, which shows visible nonthermal emissions in Nobeyama Radioheliograph and RHESSI images. The IRIS spectroscopic observations show that the hot line of Fe XXI 1354.09. angstrom (log T similar to 7.05) displays blueshifts, while the cool line of Si IV 1402.77 angstrom (log T similar to 4.8) exhibits redshifts. The blueshifts and redshifts are well correlated with each other, indicative of an explosive chromospheric evaporation during the flare precursor phase combining a high nonthermal energy flux with a short characteristic timescale. In addition, the blueshifts of Fe XXI 1354.09 angstrom are well correlated with the microwave and HXR emissions, implying that the explosive chromospheric evaporation during the flare precursor phase is driven by nonthermal electrons.
语种英语
WOS记录号WOS:000424758700001
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文献类型期刊论文
条目标识符http://libir.pmo.ac.cn/handle/332002/18051
专题太阳活动的多波段观测研究团组
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GB/T 7714
Li, Dong,Li, Ying,Su, Wei,et al. Observations of Electron-driven Evaporation in a Flare Precursor[J]. ASTROPHYSICAL JOURNAL,2018,854(1):26.
APA Li, Dong,Li, Ying,Su, Wei,Huang, Yu,&Ning, Zongjun.(2018).Observations of Electron-driven Evaporation in a Flare Precursor.ASTROPHYSICAL JOURNAL,854(1),26.
MLA Li, Dong,et al."Observations of Electron-driven Evaporation in a Flare Precursor".ASTROPHYSICAL JOURNAL 854.1(2018):26.
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