Numerical modeling of magnetohydrodynamic activity in the Swarthmore Spheromak Experiment

被引:16
作者
Lukin, VS [1 ]
Qin, G
Matthaeus, WH
Brown, MR
机构
[1] Swarthmore Coll, Dept Phys & Astron, Swarthmore, PA 19081 USA
[2] Univ Delaware, Bartol Res Inst, Newark, DE 19716 USA
关键词
D O I
10.1063/1.1362294
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
Results from a three-dimensional axisymmetric resistive magnetohydrodynamic (MHD) simulation are compared to experimental data from the Swarthmore Spheromak Experiment (SSX) [M. R. Brown, Phys. Plasmas 6, 1717 (1999)]. The MHD simulation is run under conditions and with dimensionless parameters similar to the experiment (Lundquist number S=1000, plasma beta beta =0.1). The simulation is shown to reproduce global equilibrium magnetic field profiles of the spheromaks as well as much of the detailed reconnection dynamics measured when two spheromaks are merged. It is concluded that SSX merger dynamics may be characterized as MHD reconnection, with the likelihood that extensions are needed to account for kinetic effects in the associated current sheet. High spatial and temporal resolution MHD simulation data will be used as input for a particle orbit and energization code. (C) 2001 American Institute of Physics.
引用
收藏
页码:1600 / 1606
页数:7
相关论文
共 24 条
  • [1] TEST PARTICLE-ACCELERATION IN TURBULENT RECONNECTING MAGNETIC-FIELDS
    AMBROSIANO, J
    MATTHAEUS, WH
    GOLDSTEIN, ML
    PLANTE, D
    [J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1988, 93 (A12): : 14383 - 14400
  • [2] Experimental studies of magnetic reconnection
    Brown, MR
    [J]. PHYSICS OF PLASMAS, 1999, 6 (05) : 1717 - 1724
  • [3] Scaling studies of spheromak formation and equilibrium
    Geddes, CGR
    Kornack, TW
    Brown, MR
    [J]. PHYSICS OF PLASMAS, 1998, 5 (04) : 1027 - 1034
  • [4] ACCELERATION OF CHARGED-PARTICLES IN MAGNETIC RECONNECTION - SOLAR-FLARES, THE MAGNETOSPHERE, AND SOLAR-WIND
    GOLDSTEIN, ML
    MATTHAEUS, WH
    AMBROSIANO, JJ
    [J]. GEOPHYSICAL RESEARCH LETTERS, 1986, 13 (03) : 205 - 208
  • [5] THE ROOTS OF CORONAL STRUCTURE IN THE SUNS SURFACE
    GOLUB, L
    ZIRIN, H
    WANG, HM
    [J]. SOLAR PHYSICS, 1994, 153 (1-2) : 179 - 198
  • [6] HSU SC, 2000, PHYS REV LETT, V80, P3256
  • [7] Bi-directional plasma jets produced by magnetic reconnection on the Sun
    Innes, DE
    Inhester, B
    Axford, WI
    Wilhelm, K
    [J]. NATURE, 1997, 386 (6627) : 811 - 813
  • [8] Experimental test of the Sweet-Parker model of magnetic reconnection
    Ji, HT
    Yamada, M
    Hsu, S
    Kulsrud, R
    [J]. PHYSICAL REVIEW LETTERS, 1998, 80 (15) : 3256 - 3259
  • [9] Experimental observation of correlated magnetic reconnection and Alfvenic ion jets
    Kornack, TW
    Sollins, PK
    Brown, MR
    [J]. PHYSICAL REVIEW E, 1998, 58 (01): : R36 - R39
  • [10] TURBULENT MAGNETIC RECONNECTION
    MATTHAEUS, WH
    LAMKIN, SL
    [J]. PHYSICS OF FLUIDS, 1986, 29 (08) : 2513 - 2534