Knowledge management system National Space Science Center,CAS
Spectroscopic and Stereoscopic Observations of the Solar Jets | |
Alternative Title | WOS:000506012000048 |
Lu, Lei; Feng, Li; Li, Ying; Li, Dong1; Ning, Zongjun; Gan, Weiqun | |
Source Publication | ASTROPHYSICAL JOURNAL
![]() |
2019 | |
Volume | 887Issue:2Pages:154 |
DOI | 10.3847/1538-4357/ab530c |
ISSN | 0004-637X |
Language | 英语 |
Keyword | X-RAY JETS H-ALPHA SURGES SMALL-SCALE QUIET SUN MAGNETIC RECONNECTION HINODE OBSERVATIONS FILAMENT ERUPTIONS CORONAL JETS ALFVEN WAVES ACCELERATION |
Abstract | We present a comprehensive study of a series of recurrent jets that occurred at the periphery of the NOAA active region 12114 on 2014 July 7. These jets were found to share the same source region and exhibited rotational motions as they propagated outward. The multiwavelength imaging observations made by the AIA and IRIS telescopes reveal that some of the jets contain cool plasma only, while some others contain not only cool but also hot plasma. The Doppler velocities calculated from the IRIS spectra show a continuous evolution from blue-to redshifts as the jet motions change from upward to downward. Additionally, some jets exhibit opposite Doppler shifts on both their sides, indicative of rotating motions along their axes. The inclination angle and three-dimensional velocity of the largest jet were inferred from the imaging and spectroscopic observations, which show high consistency with those derived from the stereoscopic analysis using dual-perspective observations by SDO/AIA and STEREO-B/EUVI. By relating the jets to the local UV/EUV and full-disk GOES X-ray emission enhancements, we found that the previous five small-scale jets were triggered by five bright points while the last/largest one was triggered by a C1.6 solar flare. Together with a number of type III radio bursts generated during the jet eruptions as well as a weak CME that was observed in association with the last jet, our observations provide evidence in support of multiscale magnetic reconnection processes being responsible for the production of jet events. |
Indexed By | SCI |
Citation statistics | |
Document Type | 期刊论文 |
Identifier | http://ir.nssc.ac.cn/handle/122/7624 |
Collection | 中国科学院国家空间科学中心 |
Affiliation | 1.Chinese Acad Sci, Key Lab Dark Matter & Space Astron, Purple Mt Observ, Nanjing 210033, Peoples R China 2.Chinese Acad Sci, State Key Lab Space Weather, Beijing 100190, Peoples R China |
Recommended Citation GB/T 7714 | Lu, Lei,Feng, Li,Li, Ying,et al. Spectroscopic and Stereoscopic Observations of the Solar Jets[J]. ASTROPHYSICAL JOURNAL,2019,887(2):154. |
APA | Lu, Lei,Feng, Li,Li, Ying,Li, Dong,Ning, Zongjun,&Gan, Weiqun.(2019).Spectroscopic and Stereoscopic Observations of the Solar Jets.ASTROPHYSICAL JOURNAL,887(2),154. |
MLA | Lu, Lei,et al."Spectroscopic and Stereoscopic Observations of the Solar Jets".ASTROPHYSICAL JOURNAL 887.2(2019):154. |
Files in This Item: | There are no files associated with this item. |
Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.
Edit Comment