Three-dimensional Separator Reconnection – How Does It Occur?

被引:0
|
作者
K. Galsgaard
E.R. Priest
Å. Nordlund
机构
[1] University of St. Andrews,School of Mathematics and Statistics
[2] University of St. Andrews,School of Mathematics and Statistics
[3] NBIfAFG,Astronomical Observatorium
来源
Solar Physics | 2000年 / 193卷
关键词
Advection; Magnetic Flux; Field Line; Current Sheet; Magnetic Field Strength;
D O I
暂无
中图分类号
学科分类号
摘要
In two dimensions magnetic energy release takes place at locations where the magnetic field strength becomes zero and has an x-point topology. The x-point topology can collapse into two y-points connected by a current sheet when the advection of magnetic flux into the x-point is larger than the dissipation of magnetic flux at the x-point. In three dimensions magnetic fields may also contain singularities in the form of three-dimensional null points. Three-dimensional nulls are created in pairs and are therefore, at least in the initial stages, always connected by at least one field line – the separator. The separator line is defined by the intersection of the fan planes of the two nulls. In the plane perpendicular to a single separator the field line topology locally has a two dimensional x-point structure. Using a numerical approach we find that the collapse of the separator can be initiated at the two nulls by a velocity shear across the fan plane. It is found that for a current concentration to connect the two nulls along the separator, the current sheet can only obtain two different orientations relative to the field line structure of the nulls. The sheet has to have an orientation midway between the fan plane and the spine axis of each null. As part of this process the spine axes are found to lose their identity by transforming into an integrated part of the separator surfaces that divide space into four magnetically independent regions around the current sheet.
引用
收藏
页码:1 / 16
页数:15
相关论文
共 50 条
  • [1] Three-dimensional separator reconnection -: How does it occur?
    Galsgaard, K
    Priest, ER
    Nordlund, Å
    SOLAR PHYSICS, 2000, 193 (1-2) : 1 - 16
  • [2] Particle acceleration in three-dimensional separator reconnection
    Akbari, Z.
    Hosseinpour, M.
    Mohammadi, M. A.
    ADVANCES IN SPACE RESEARCH, 2023, 72 (08) : 3454 - 3463
  • [3] Dynamic three-dimensional reconnection in a separator geometry with two null points
    Pontin, DI
    Craig, IJD
    ASTROPHYSICAL JOURNAL, 2006, 642 (01): : 568 - 578
  • [4] Satellite observations of separator-line geometry of three-dimensional magnetic reconnection
    Xiao, C. J.
    Wang, X. G.
    Pu, Z. Y.
    Ma, Z. W.
    Zhao, H.
    Zhou, G. P.
    Wang, J. X.
    Kivelson, M. G.
    Fu, S. Y.
    Liu, Z. X.
    Zong, Q. G.
    Dunlop, M. W.
    Glassmeier, K.-H.
    Lucek, E.
    Reme, H.
    Dandouras, I.
    Escoubet, C. P.
    NATURE PHYSICS, 2007, 3 (09) : 609 - 613
  • [5] Satellite observations of separator-line geometry of three-dimensional magnetic reconnection
    C. J. Xiao
    X. G. Wang
    Z. Y. Pu
    Z. W. Ma
    H. Zhao
    G. P. Zhou
    J. X. Wang
    M. G. Kivelson
    S. Y. Fu
    Z. X. Liu
    Q. G. Zong
    M. W. Dunlop
    K.-H. Glassmeier
    E. Lucek
    H. Reme
    I. Dandouras
    C. P. Escoubet
    Nature Physics, 2007, 3 : 609 - 613
  • [6] Three-dimensional reconnection on the Sun
    Priest, ER
    EARTH PLANETS AND SPACE, 2001, 53 (06): : 483 - 490
  • [7] Three-dimensional reconnection on the Sun
    Eric R. Priest
    Earth, Planets and Space, 2001, 53 : 483 - 490
  • [8] On the nature of three-dimensional magnetic reconnection
    Priest, E. R.
    Hornig, G.
    Pontin, D. I.
    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2003, 108 (A7)
  • [9] Aspects of three-dimensional magnetic reconnection
    Borgogno, D
    Grasso, D
    Porcelli, F
    Califano, F
    Pegoraro, F
    Farina, D
    PHYSICS OF PLASMAS, 2005, 12 (03) : 1 - 15
  • [10] Three-dimensional Hall magnetic reconnection
    Huba, JD
    Rudakov, LI
    PHYSICS OF PLASMAS, 2002, 9 (11) : 4435 - 4438