Explosive Chromospheric Evaporation Driven by Nonthermal Electrons around One Footpoint of a Solar Flare Loop | |
Li, D.1,2,3; Ning, Z. J.1; Huang, Y.1; Zhang, Q. M.1,2 | |
刊名 | ASTROPHYSICAL JOURNAL LETTERS |
2017-05-20 | |
卷号 | 841期号:1页码:6 |
关键词 | line: profiles Sun: flares Sun: radio radiation Sun: UV radiation Sun: X-rays, gamma rays |
ISSN号 | 2041-8205 |
DOI | 10.3847/2041-8213/aa71b0 |
英文摘要 | We explore the temporal relationship between microwave/hard X-ray (HXR) emission and Doppler velocity during the impulsive phase of a solar flare on 2014 October 27 (SOL2014-10-27) that displays a pulse on the light curves in the microwave (34 GHz) and HXR (25-50 keV) bands before the flare maximum. Imaging observation shows that this pulse mainly comes from one footpoint of a solar flare loop. The slit of the Interface Region Imaging Spectrograph (IRIS) stays at this footpoint during this solar flare. The Doppler velocities of Fe XXI. 1354.09 angstrom and Si IV. 1402.77. angstrom are extracted from the Gaussian fitting method. We find that the hot line of Fe XXI. 1354.09 angstrom (log T similar to 7.05) in the corona exhibits blueshift, while the cool line of Si IV. 1402.77 angstrom (log T similar to 4.8) in the transition region exhibits redshift, indicating explosive chromospheric evaporation. Evaporative upflows along the flare loop are also observed in the AIA 131 angstrom image. To our knowledge, this is the first report of chromospheric evaporation evidence from both spectral and imaging observations in the same flare. Both microwave and HXR pulses are well correlated with the Doppler velocities, suggesting that the chromospheric evaporation is driven by nonthermal electrons around this footpoint of a solar flare loop. |
WOS关键词 | ULTRAVIOLET IMAGING SPECTROMETER ; OBSERVATIONAL EVIDENCE ; IMPULSIVE PHASE ; IRIS ; RESOLUTION ; HINODE ; SPECTROSCOPY ; MICROFLARE ; CONVERSION ; EVOLUTION |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | IOP PUBLISHING LTD |
WOS记录号 | WOS:000402563400007 |
内容类型 | 期刊论文 |
源URL | [http://libir.pmo.ac.cn/handle/332002/23054] |
专题 | 中国科学院紫金山天文台 |
通讯作者 | Li, D. |
作者单位 | 1.Chinese Acad Sci, Purple Mt Observ, Key Lab Dark Matter & Space Astron, Nanjing 210008, Jiangsu, Peoples R China 2.Natl Astron Observ, CAS Key Lab Solar Act, Beijing 100012, Peoples R China 3.Nanjing Univ, Minist Educ, Key Lab Modern Astron & Astrophys, Nanjing 210023, Jiangsu, Peoples R China |
推荐引用方式 GB/T 7714 | Li, D.,Ning, Z. J.,Huang, Y.,et al. Explosive Chromospheric Evaporation Driven by Nonthermal Electrons around One Footpoint of a Solar Flare Loop[J]. ASTROPHYSICAL JOURNAL LETTERS,2017,841(1):6. |
APA | Li, D.,Ning, Z. J.,Huang, Y.,&Zhang, Q. M..(2017).Explosive Chromospheric Evaporation Driven by Nonthermal Electrons around One Footpoint of a Solar Flare Loop.ASTROPHYSICAL JOURNAL LETTERS,841(1),6. |
MLA | Li, D.,et al."Explosive Chromospheric Evaporation Driven by Nonthermal Electrons around One Footpoint of a Solar Flare Loop".ASTROPHYSICAL JOURNAL LETTERS 841.1(2017):6. |
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