MAGNETAR GIANT FLARES IN MULTIPOLAR MAGNETIC FIELDS. II. FLUX ROPE ERUPTIONS WITH CURRENT SHEETS
Huang, Lei1,2; Yu, Cong2,3
刊名ASTROPHYSICAL JOURNAL
2014-11-20
卷号796期号:1页码:3
关键词instabilities pulsars: general stars: magnetars stars: magnetic field stars: neutron
通讯作者黄磊
英文摘要We propose a physical mechanism to explain giant flares and radio afterglows in terms of a magnetospheric model containing both a helically twisted flux rope and a current sheet (CS). With the appearance of a CS, we solve a mixed boundary value problem to get the magnetospheric field based on a domain decomposition method. We investigate properties of the equilibrium curve of the flux rope when the CS is present in background multipolar fields. In response to the variations at the magnetar surface, it quasi-statically evolves in stable equilibrium states. The loss of equilibrium occurs at a critical point and, beyond that point, it erupts catastrophically. New features show up when the CS is considered. In particular, we find two kinds of physical behaviors, i.e., catastrophic state transition and catastrophic escape. Magnetic energy would be released during state transitions. This released magnetic energy is sufficient to drive giant flares, and the flux rope would, therefore, go away from the magnetar quasi-statically, which is inconsistent with the radio afterglow. Fortunately, in the latter case, i.e., the catastrophic escape, the flux rope could escape the magnetar and go to infinity in a dynamical way. This is more consistent with radio afterglow observations of giant flares. We find that the minor radius of the flux rope has important implications for its eruption. Flux ropes with larger minor radii are more prone to erupt. We stress that the CS provides an ideal place for magnetic reconnection, which would further enhance the energy release during eruptions.
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]X-RAY PULSAR ; 1998 AUGUST 27 ; MAGNETOSPHERES ; REPEATERS ; RECONNECTION ; SGR-1806-20 ; EVOLUTION ; DYNAMICS
收录类别SCI
语种英语
WOS记录号WOS:000344550300003
公开日期2015-02-14
内容类型期刊论文
源URL[http://119.78.226.72//handle/331011/15764]  
专题上海天文台_星系宇宙学重点实验室
作者单位1.Chinese Acad Sci, Shanghai Astron Observ, Key Lab Res Galaxies & Cosmol, Shanghai 200030, Peoples R China
2.Chinese Acad Sci, Key Lab Struct & Evolut Celestial Object, Kunming 650011, Peoples R China
3.Chinese Acad Sci, Yunnan Observ, Kunming 650011, Peoples R China
推荐引用方式
GB/T 7714
Huang, Lei,Yu, Cong. MAGNETAR GIANT FLARES IN MULTIPOLAR MAGNETIC FIELDS. II. FLUX ROPE ERUPTIONS WITH CURRENT SHEETS[J]. ASTROPHYSICAL JOURNAL,2014,796(1):3.
APA Huang, Lei,&Yu, Cong.(2014).MAGNETAR GIANT FLARES IN MULTIPOLAR MAGNETIC FIELDS. II. FLUX ROPE ERUPTIONS WITH CURRENT SHEETS.ASTROPHYSICAL JOURNAL,796(1),3.
MLA Huang, Lei,et al."MAGNETAR GIANT FLARES IN MULTIPOLAR MAGNETIC FIELDS. II. FLUX ROPE ERUPTIONS WITH CURRENT SHEETS".ASTROPHYSICAL JOURNAL 796.1(2014):3.
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