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MINIFILAMENT ERUPTION AS THE SOURCE OF A BLOWOUT JET, C-CLASS FLARE, AND TYPE-III RADIO BURST
Hong JC(洪俊超)1,2; Jiang YC(姜云春)1,2; Yang JY(杨家艳)1,2; Li HD(李海东)1,2,3; Xu Z(徐喆)1,2,3; Hong, Junchao(Chinese Acad Sci, Yunnan Observ, 396 Yangfangwang, Guandu Dist 650216, Kunming, Peoples R China)
发表期刊ASTROPHYSICAL JOURNAL
2017-01-20
卷号835期号:1页码:35-43
DOI10.3847/1538-4357/835/1/35
产权排序第1完成单位
收录类别SCI
关键词Sun: Chromosphere Sun: Corona Sun: Filaments Prominences
摘要We report a strong minifilament eruption associated with Geostationary Operational Environmental Satellite C1.6 flare and WIND type-III radio burst. The minifilament, which lies at the periphery of active region 12259, is detected by Ha images from the. New Vacuum Solar Telescope. The minifilament undergoes a partial and then a full eruption. Simultaneously, two co-spatial jets are successively observed in extreme ultraviolet images from the Solar Dynamic Observatory. The first jet exhibits a typical fan-spine geometry, suggesting that the co-spatial minifilament is possibly embedded in magnetic fields with a fan-spine structure. However, the second jet displays blowout morphology when the entire minifilament erupts upward, leaving behind a hard X-ray emission source in the base. Differential emission measure analyses show that the eruptive region is heated up to about 4 MK during the fan-spine jet, while up to about 7 MK during the blowout jet. In particular, the blowout jet is accompanied by an interplanetary type-III radio burst observed by WIND/WAVES in the frequency range from above 10 to 0.1 MHz. Hence, the minifilament eruption is correlated with the interplanetary type-III radio burst for the first time. These results not only suggest that coronal jets can result from magnetic reconnection initiated by erupting minifilaments with open fields, but also shed light on the potential influence of minifilament eruption. on interplanetary space.
项目资助者Natural Science Foundation of China(11333007, 11403098, 11573012, 11503081, 11503082, 11633008) ; CAS "Light of West China" Program
语种英语
学科领域天文学
文章类型Article
ISSN0004-637X
URL查看原文
归档日期2017-03-06
WOS记录号WOS:000393455400035
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]X-RAY JETS ; VACUUM SOLAR TELESCOPE ; CORONAL MASS EJECTIONS ; BRIGHT POINTS ; QUIET SUN ; FILAMENT ERUPTIONS ; CHROMOSPHERIC JET ; MAGNETIC TOPOLOGY ; HIGH-RESOLUTION ; ACTIVE-REGION
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文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/9919
专题太阳物理研究组
通讯作者Hong, Junchao(Chinese Acad Sci, Yunnan Observ, 396 Yangfangwang, Guandu Dist 650216, Kunming, Peoples R China)
作者单位1.Yunnan Observatories, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming, 650216, China
2.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing, 100012, China
3.Graduate School of Chinese Academy of Sciences, Beijing, China
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Hong JC,Jiang YC,Yang JY,et al. MINIFILAMENT ERUPTION AS THE SOURCE OF A BLOWOUT JET, C-CLASS FLARE, AND TYPE-III RADIO BURST[J]. ASTROPHYSICAL JOURNAL,2017,835(1):35-43.
APA Hong JC,Jiang YC,Yang JY,Li HD,Xu Z,&Hong, Junchao.(2017).MINIFILAMENT ERUPTION AS THE SOURCE OF A BLOWOUT JET, C-CLASS FLARE, AND TYPE-III RADIO BURST.ASTROPHYSICAL JOURNAL,835(1),35-43.
MLA Hong JC,et al."MINIFILAMENT ERUPTION AS THE SOURCE OF A BLOWOUT JET, C-CLASS FLARE, AND TYPE-III RADIO BURST".ASTROPHYSICAL JOURNAL 835.1(2017):35-43.
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