RECURRENT SOLAR JETS INDUCED by A SATELLITE SPOT and MOVING MAGNETIC FEATURES

Jie Chen; Jiangtao Su; Zhiqiang Yin; T. G. Priya; Hongqi Zhang; Jihong Liu; Haiqing Xu; Sijie Yu

doi:10.1088/0004-637X/815/1/71

RECURRENT SOLAR JETS INDUCED by A SATELLITE SPOT and MOVING MAGNETIC FEATURES

Jie Chen, Jiangtao Su, Zhiqiang Yin, T. G. Priya, Hongqi Zhang, Jihong Liu, Haiqing Xu, Sijie Yu

Research output: Contribution to journal › Article › peer-review

57 Scopus citations

Abstract

Recurrent and homologous jets were observed to the west edge of active region NOAA 11513 at the boundary of a coronal hole. We find two kinds of cancellations between opposite polarity magnetic fluxes, inducing the generation of recurrent jets. First, a satellite spot continuously collides with a pre-existing opposite polarity magnetic field and causes recurrent solar jets. Second, moving magnetic features, which emerge near the sunspot penumbra, pass through the ambient plasma and eventually collide with the opposite polarity magnetic field. Among these recurrent jets, a blowout jet that occurred around 21:10 UT is investigated. The rotation of the pre-existing magnetic field and the shear motion of the satellite spot accumulate magnetic energy, which creates the possibility for the jet to experience blowout right from the standard.

Original language	English (US)
Article number	71
Journal	Astrophysical Journal
Volume	815
Issue number	1
DOIs	https://doi.org/10.1088/0004-637X/815/1/71
State	Published - Dec 10 2015
Externally published	Yes

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

Keywords

Sun: activity
Sun: atmosphere
Sun: magnetic fields
magnetic reconnection

Access to Document

10.1088/0004-637X/815/1/71

Cite this

@article{81588384bb04436680ceab9504ee2baa,

title = "RECURRENT SOLAR JETS INDUCED by A SATELLITE SPOT and MOVING MAGNETIC FEATURES",

abstract = "Recurrent and homologous jets were observed to the west edge of active region NOAA 11513 at the boundary of a coronal hole. We find two kinds of cancellations between opposite polarity magnetic fluxes, inducing the generation of recurrent jets. First, a satellite spot continuously collides with a pre-existing opposite polarity magnetic field and causes recurrent solar jets. Second, moving magnetic features, which emerge near the sunspot penumbra, pass through the ambient plasma and eventually collide with the opposite polarity magnetic field. Among these recurrent jets, a blowout jet that occurred around 21:10 UT is investigated. The rotation of the pre-existing magnetic field and the shear motion of the satellite spot accumulate magnetic energy, which creates the possibility for the jet to experience blowout right from the standard.",

keywords = "Sun: activity, Sun: atmosphere, Sun: magnetic fields, magnetic reconnection",

author = "Jie Chen and Jiangtao Su and Zhiqiang Yin and Priya, {T. G.} and Hongqi Zhang and Jihong Liu and Haiqing Xu and Sijie Yu",

year = "2015",

month = dec,

day = "10",

doi = "10.1088/0004-637X/815/1/71",

language = "English (US)",

volume = "815",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "American Astronomical Society",

number = "1",

}

TY - JOUR

T1 - RECURRENT SOLAR JETS INDUCED by A SATELLITE SPOT and MOVING MAGNETIC FEATURES

AU - Chen, Jie

AU - Su, Jiangtao

AU - Yin, Zhiqiang

AU - Priya, T. G.

AU - Zhang, Hongqi

AU - Liu, Jihong

AU - Xu, Haiqing

AU - Yu, Sijie

PY - 2015/12/10

Y1 - 2015/12/10

N2 - Recurrent and homologous jets were observed to the west edge of active region NOAA 11513 at the boundary of a coronal hole. We find two kinds of cancellations between opposite polarity magnetic fluxes, inducing the generation of recurrent jets. First, a satellite spot continuously collides with a pre-existing opposite polarity magnetic field and causes recurrent solar jets. Second, moving magnetic features, which emerge near the sunspot penumbra, pass through the ambient plasma and eventually collide with the opposite polarity magnetic field. Among these recurrent jets, a blowout jet that occurred around 21:10 UT is investigated. The rotation of the pre-existing magnetic field and the shear motion of the satellite spot accumulate magnetic energy, which creates the possibility for the jet to experience blowout right from the standard.

AB - Recurrent and homologous jets were observed to the west edge of active region NOAA 11513 at the boundary of a coronal hole. We find two kinds of cancellations between opposite polarity magnetic fluxes, inducing the generation of recurrent jets. First, a satellite spot continuously collides with a pre-existing opposite polarity magnetic field and causes recurrent solar jets. Second, moving magnetic features, which emerge near the sunspot penumbra, pass through the ambient plasma and eventually collide with the opposite polarity magnetic field. Among these recurrent jets, a blowout jet that occurred around 21:10 UT is investigated. The rotation of the pre-existing magnetic field and the shear motion of the satellite spot accumulate magnetic energy, which creates the possibility for the jet to experience blowout right from the standard.

KW - Sun: activity

KW - Sun: atmosphere

KW - Sun: magnetic fields

KW - magnetic reconnection

UR - http://www.scopus.com/inward/record.url?scp=84951276440&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84951276440&partnerID=8YFLogxK

U2 - 10.1088/0004-637X/815/1/71

DO - 10.1088/0004-637X/815/1/71

M3 - Article

AN - SCOPUS:84951276440

SN - 0004-637X

VL - 815

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1

M1 - 71

ER -

RECURRENT SOLAR JETS INDUCED by A SATELLITE SPOT and MOVING MAGNETIC FEATURES

Abstract

All Science Journal Classification (ASJC) codes

Keywords

Access to Document

Other files and links

Fingerprint

Cite this