Two-way coupled MHD-PIC simulations of magnetic reconnection in magnetic island coalescence

被引:8
|
作者
Makwana, Kirit [1 ]
Keppens, Rony [1 ]
Lapenta, Giovanni [1 ]
机构
[1] Katholieke Univ Leuven, Dept Math, Ctr Math Plasma Astrophys, Celestijnenlaan 200B, B-3001 Heverlee, Belgium
关键词
PARTICLE; MAGNETOHYDRODYNAMICS; SOLAR; MODEL;
D O I
10.1088/1742-6596/1031/1/012019
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present simulations of magnetic reconnection with a newly developed coupled MHD-PIC code. In this work a global magnetohydrodynamic (MHD) simulation receives kinetic feedback within an embedded region that is modeled by a kinetic particle-in-cell (PIC) code. The PIC code receives initial and boundary conditions from the MHD simulation, while the MHD solution is updated with the PIC state. We briefly describe this coupling mechanism. This method is suitable for simulating magnetic reconnection problems, as we show with the example of reconnection in the coalescence of magnetic islands. We compare the MHD, Hall-MHD, fully PIC and coupled MHD-PIC simulations of the magnetic island coalescence. We find that the kinetic simulations are very different from the MHD and Hall-MHD results, while the coupled MHD-PIC simulations can remedy this discrepancy while saving computing time. The diffusion region is well resolved in the kinetic simulations, which is also captured by the coupled MHD-PIC model. The coupled simulation also reproduces the kinetic Hall magnetic fields correctly. We calculate the reconnection rates and find differences between the MHD and kinetic results. We find that the coupled MHD-PIC code can reasonably reproduce the kinetic reconnection rate when a larger PIC feedback region is used, while still saving significant computing time.
引用
收藏
页数:10
相关论文
共 50 条
  • [41] Dynamics of the solar magnetic network: Two-dimensional MHD simulations
    Hasan, SS
    van Ballegooijen, AA
    Kalkofen, W
    Steiner, O
    ASTROPHYSICAL JOURNAL, 2005, 631 (02): : 1270 - 1280
  • [42] Numerical MHD Simulations of Reconnection in Solar Flares: Effects of the Magnetic-Field Strength in the Current Sheet
    Izquierdo-Guzman, I.
    Gonzalez-Aviles, J. J.
    Guzman, F. S.
    SOLAR PHYSICS, 2023, 298 (09)
  • [43] TIME-DEPENDENT MAGNETIC RECONNECTION - 2-DIMENSIONAL AND 3-DIMENSIONAL MHD SIMULATIONS
    LEE, LC
    COMPUTER PHYSICS COMMUNICATIONS, 1990, 59 (01) : 163 - 174
  • [44] Numerical MHD Simulations of Reconnection in Solar Flares: Effects of the Magnetic-Field Strength in the Current Sheet
    I. Izquierdo-Guzmán
    J. J. González-Avilés
    F. S. Guzmán
    Solar Physics, 2023, 298
  • [45] 3D RESISTIVE MHD SIMULATIONS OF MAGNETIC RECONNECTION AND THE TEARING MODE INSTABILITY IN CURRENT SHEETS
    Murphy, G. C.
    Ouyed, R.
    Pelletier, G.
    INTERNATIONAL JOURNAL OF MODERN PHYSICS D, 2008, 17 (10): : 1715 - 1721
  • [46] Application of parallel programming method for 3D MHD computer simulations of magnetic reconnection in plasma
    Kostomarov, DP
    Inovenkov, IN
    Echkina, EY
    Leonenko, AV
    Pavlova, OA
    Bulanov, SV
    PARALLEL COMPUTATIONAL FLUID DYNAMICS: ADVANCED NUMERICAL METHODS SOFTWARE AND APPLICATIONS, 2004, : 373 - 379
  • [47] Chromospheric magnetic reconnection: two-fluid simulations of coalescing current loops
    Smith, P. D.
    Sakai, J. I.
    ASTRONOMY & ASTROPHYSICS, 2008, 486 (02) : 569 - 575
  • [48] Quantification of fluid migration via faults requires two-way coupled hydromechanical simulations
    Chabab, Elena
    Kempka, Thomas
    EUROPEAN GEOSCIENCES UNION GENERAL ASSEMBLY 2016, 2016, 97 : 372 - 378
  • [49] Two-way coupled simulations of stagnation-point ablation with transient material response
    Schrooyen, Pierre
    Turchi, Alessandro
    Hillewaert, Koen
    Chatelain, Philippe
    Magin, Thierry E.
    INTERNATIONAL JOURNAL OF THERMAL SCIENCES, 2018, 134 : 639 - 652
  • [50] A correction scheme for two-way coupled point-particle simulations on anisotropic grids
    Esmaily, M.
    Horwitz, J. A. K.
    JOURNAL OF COMPUTATIONAL PHYSICS, 2018, 375 : 960 - 982