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Simultaneous Transverse and Longitudinal Oscillations in a Quiescent Prominence Triggered by a Coronal Jet
Zhang, Q. M.1,2; Li, D.1; Ning, Z. J.1
2017-12-10
Source PublicationASTROPHYSICAL JOURNAL
Volume851Issue:1
AbstractIn this paper, we report our multiwavelength observations of the simultaneous transverse and longitudinal oscillations in a quiescent prominence. The prominence was observed by the Global Oscillation Network Group and by the Atmospheric Imaging Assembly on board the Solar Dynamics Observatory on 2015 June 29. A GOES C2.4 flare took place in NOAA active region 12373, which was associated with a pair of short ribbons and a remote ribbon. During the impulsive phase of the flare, a coronal jet spurted out of the primary flare site and propagated in the northwest direction at an apparent speed of similar to 224 km s(-1). Part of the jet stopped near the remote ribbon. The remaining part continued moving forward before stopping to the east of the prominence. Once the jet encountered the prominence, it pushed the prominence to oscillate periodically. The transverse oscillation of the eastern part (EP) of prominence can be divided into two phases. In phase I, the initial amplitude, velocity, period, and damping timescale are similar to 4.5 Mm, similar to 20 km s(-1), similar to 25 minutes, and similar to 7.5 hr, respectively. The oscillation lasted for two cycles. In phase II, the initial amplitude increases to similar to 11.3 Mm, while the initial velocity halves to similar to 10 km s(-1). The period increases by a factor of similar to 3.5. With a damping timescale of similar to 4.4 hr, the oscillation lasted for about three cycles. The western part of prominence also experienced transverse oscillation. The initial amplitude is only similar to 2 Mm and the velocity is less than 10 km s(-1). The period (similar to 27 minutes) is slightly longer than that of the EP in phase I. The oscillation lasted for about four cycles with the shortest damping timescale (similar to 1.7 hr). To the east of prominence, a handful of horizontal threads experienced longitudinal oscillation. The initial amplitude, velocity, period, and damping timescale are similar to 52 Mm, similar to 50 km s(-1), similar to 99 minutes, and 2.5 hr, respectively. To our knowledge, this is the first report of simultaneous transverse and longitudinal prominence oscillations triggered by a coronal jet.
SubtypeArticle
KeywordSun: Flares Sun: Filaments Sun: Oscillations Prominences
WOS HeadingsScience & Technology ; Physical Sciences
Funding OrganizationInternational Space Science Institute (ISSI) ; International Space Science Institute (ISSI) ; NOAA ; NOAA ; NASA ; NASA ; USAF ; USAF ; NSFC(11333009 ; NSFC(11333009 ; Fund of Jiangsu Province(BK20161618 ; Fund of Jiangsu Province(BK20161618 ; CAS Key Laboratory of Solar Activity, National Astronomical Observatories(KLSA201716) ; CAS Key Laboratory of Solar Activity, National Astronomical Observatories(KLSA201716) ; Youth Innovation Promotion Association CAS ; Youth Innovation Promotion Association CAS ; 11773079 ; 11773079 ; BK20161095) ; BK20161095) ; 11603077 ; 11603077 ; 11573072) ; 11573072) ; International Space Science Institute (ISSI) ; International Space Science Institute (ISSI) ; NOAA ; NOAA ; NASA ; NASA ; USAF ; USAF ; NSFC(11333009 ; NSFC(11333009 ; Fund of Jiangsu Province(BK20161618 ; Fund of Jiangsu Province(BK20161618 ; CAS Key Laboratory of Solar Activity, National Astronomical Observatories(KLSA201716) ; CAS Key Laboratory of Solar Activity, National Astronomical Observatories(KLSA201716) ; Youth Innovation Promotion Association CAS ; Youth Innovation Promotion Association CAS ; 11773079 ; 11773079 ; BK20161095) ; BK20161095) ; 11603077 ; 11603077 ; 11573072) ; 11573072)
DOI10.3847/1538-4357/aa9898
WOS KeywordSOLAR PROMINENCES ; FILAMENT OSCILLATIONS ; MAGNETIC-FIELDS ; PERIODIC MOTION ; MORETON WAVE ; POLAR CROWN ; DYNAMICS ; HINODE ; MICROWAVE ; ERUPTIONS
Indexed BySCI
Language英语
Funding OrganizationInternational Space Science Institute (ISSI) ; International Space Science Institute (ISSI) ; NOAA ; NOAA ; NASA ; NASA ; USAF ; USAF ; NSFC(11333009 ; NSFC(11333009 ; Fund of Jiangsu Province(BK20161618 ; Fund of Jiangsu Province(BK20161618 ; CAS Key Laboratory of Solar Activity, National Astronomical Observatories(KLSA201716) ; CAS Key Laboratory of Solar Activity, National Astronomical Observatories(KLSA201716) ; Youth Innovation Promotion Association CAS ; Youth Innovation Promotion Association CAS ; 11773079 ; 11773079 ; BK20161095) ; BK20161095) ; 11603077 ; 11603077 ; 11573072) ; 11573072) ; International Space Science Institute (ISSI) ; International Space Science Institute (ISSI) ; NOAA ; NOAA ; NASA ; NASA ; USAF ; USAF ; NSFC(11333009 ; NSFC(11333009 ; Fund of Jiangsu Province(BK20161618 ; Fund of Jiangsu Province(BK20161618 ; CAS Key Laboratory of Solar Activity, National Astronomical Observatories(KLSA201716) ; CAS Key Laboratory of Solar Activity, National Astronomical Observatories(KLSA201716) ; Youth Innovation Promotion Association CAS ; Youth Innovation Promotion Association CAS ; 11773079 ; 11773079 ; BK20161095) ; BK20161095) ; 11603077 ; 11603077 ; 11573072) ; 11573072)
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000417808300007
Citation statistics
Cited Times:7[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/20342
Collection射电天文研究部
Affiliation1.Chinese Acad Sci, Purple Mt Observ, Key Lab Dark Matter & Space Sci, Nanjing 210008, Jiangsu, Peoples R China
2.Natl Astron Observ, CAS Key Lab Solar Act, Beijing 100012, Peoples R China
Recommended Citation
GB/T 7714
Zhang, Q. M.,Li, D.,Ning, Z. J.. Simultaneous Transverse and Longitudinal Oscillations in a Quiescent Prominence Triggered by a Coronal Jet[J]. ASTROPHYSICAL JOURNAL,2017,851(1).
APA Zhang, Q. M.,Li, D.,&Ning, Z. J..(2017).Simultaneous Transverse and Longitudinal Oscillations in a Quiescent Prominence Triggered by a Coronal Jet.ASTROPHYSICAL JOURNAL,851(1).
MLA Zhang, Q. M.,et al."Simultaneous Transverse and Longitudinal Oscillations in a Quiescent Prominence Triggered by a Coronal Jet".ASTROPHYSICAL JOURNAL 851.1(2017).
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