Objective magnetic vortex detection

被引:8
作者
Rempel, Erico L. [1 ,2 ]
Gomes, Tiago F. P. [2 ]
Silva, Suzana S. A. [1 ]
Chian, Abraham C-L [1 ,2 ,3 ]
机构
[1] WISER, Inst Aeronaut Technol ITA, BR-12228900 Sao Jose Dos Campos, SP, Brazil
[2] Natl Inst Space Res INPE, Box 515, BR-12227010 Sao Jose Dos Campos, SP, Brazil
[3] Univ Adelaide, Sch Math Sci, Adelaide, SA 5005, Australia
基金
巴西圣保罗研究基金会;
关键词
VISCO-RESISTIVE DISSIPATION; COHERENT STRUCTURES; DYNAMICS; DRIVEN;
D O I
10.1103/PhysRevE.99.043206
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
Magnetic coherent vortical structures are ubiquitous in space and astrophysical plasmas and their detection is key to understanding the nature of the intrinsic turbulence in those conducting fluids. A recently developed method to detect magnetic vortices is explored in problems of two- and three-dimensional magnetohydrodynamic simulations. The integrated averaged current deviation, the normed difference of the current density at a point and the mean current density in the domain, integrated along a magnetic field line, is proved to be objective, i.e., invariant under rotations and translations of the observer. The method is shown to detect accurately the boundary of magnetic vortices in two-dimensional simulations, as well as magnetic flux ropes in three dimensions.
引用
收藏
页数:15
相关论文
共 42 条
  • [1] [Anonymous], 2004, NONLINEAR FIELD THEO
  • [2] Visco-Resistive Dissipation in Strongly Driven Transient Reconnection
    Armstrong, C. K.
    Craig, I. J. D.
    [J]. SOLAR PHYSICS, 2014, 289 (03) : 869 - 877
  • [3] Visco-Resistive Dissipation in Transient Reconnection Driven by the Orszag-Tang Vortex
    Armstrong, C. K.
    Craig, I. J. D.
    [J]. SOLAR PHYSICS, 2013, 283 (02) : 463 - 471
  • [4] Coherent Lagrangian swirls among submesoscale motions
    Beron-Vera, F. J.
    Hadjighasem, A.
    Xia, Q.
    Olascoaga, M. J.
    Haller, G.
    [J]. PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA, 2019, 116 (37) : 18251 - 18256
  • [5] DYNAMICS OF DECAYING TWO-DIMENSIONAL MAGNETOHYDRODYNAMIC TURBULENCE
    BISKAMP, D
    WELTER, H
    [J]. PHYSICS OF FLUIDS B-PLASMA PHYSICS, 1989, 1 (10): : 1964 - 1979
  • [6] GENESIS OF INTERPLANETARY INTERMITTENT TURBULENCE: A CASE STUDY OF ROPE-ROPE MAGNETIC RECONNECTION
    Chian, Abraham C. -L.
    Feng, Heng Q.
    Hu, Qiang
    Loew, Murray H.
    Miranda, Rodrigo A.
    Munoz, Pablo R.
    Sibeck, David G.
    Wu, De J.
    [J]. ASTROPHYSICAL JOURNAL, 2016, 832 (02)
  • [7] DETECTION OF COHERENT STRUCTURES IN PHOTOSPHERIC TURBULENT FLOWS
    Chian, Abraham C. -L.
    Rempel, Erico L.
    Aulanier, Guillaume
    Schmieder, Brigitte
    Shadden, Shawn C.
    Welsch, Brian T.
    Yeates, Anthony R.
    [J]. ASTROPHYSICAL JOURNAL, 2014, 786 (01)
  • [8] Objective Lagrangian Vortex Detection in the Solar Photosphere
    de Souza e Almeida Silva, Suzana
    Rempel, Erico Luiz
    Pinheiro Gomes, Tiago Francisco
    Requerey, Iker S.
    Chian, Abrahamm C. -L.
    [J]. ASTROPHYSICAL JOURNAL LETTERS, 2018, 863 (01)
  • [9] Magnetic-field decay of three interlocked flux rings with zero linking number
    Del Sordo, Fabio
    Candelaresi, Simon
    Brandenburg, Axel
    [J]. PHYSICAL REVIEW E, 2010, 81 (03):
  • [10] Fang C., 2019, INTRO FLUID MECH