[Table of Contents]

Plasma and Fusion Research

Volume 4, 024 (2009)

Regular Articles


Open Boundary Condition for Particle Simulation in Magnetic Reconnection Research
Hiroaki OHTANI1,2) and Ritoku HORIUCHI1,2)
1)
Department of Simulation Science, National Institute for Fusion Science, Toki 509-5292, Japan
2)
Graduate University of Advanced Studies (SOKENDAI), Toki 509-5292, Japan
(Received 22 December 2008 / Accepted 1 April 2009 / Published 4 June 2009)

Abstract

We develop a three-dimensional electromagnetic PArticle Simulation code for investigating driven Magnetic reconnection in an Open system from the kinetic view-point (PASMO). In this paper, we advance a new model for the upstream and downstream boundaries. We succeed in achieving the frozen-in condition for both electrons and ions with high accuracy at the upstream boundary, while we can decrease unphysical noise at the downstream boundary. We compare the simulation results of long and short-simulation boxes to check whether the downstream boundary model fulfills its function. The results of the short-simulation box effectively mimic those of the long-simulation box. Using the new boundary model, we succeed in increasing the accuracy of simulation.


Keywords

electromagnetic PIC simulation code, open boundary condition, magnetic reconnection

DOI: 10.1585/pfr.4.024


References

  • [1] V.A. Sergeev, V. Angelopoulos, D.G. Mitchell and C.T. Russell, J. Geophys. Res. 100, 19121 (1995).
  • [2] A.T.Y. Lui, IEEE Trans. Plasma Sci. 28, 1854 (2000).
  • [3] Y. Ono, M. Inomoto, T. Okazaki and Y. Ueda, Phys. Plasmas 4, 1953 (1997).
  • [4] M. Yamada, Phys. Plasmas 14, 058102 (2007).
  • [5] D. Biskamp, Magnetic Reconnection in Plasmas (Cambridge University Press, Cambridge, 2000).
  • [6] E. Priest and T. Forbes, Magnetic Reconnection MHD Theory and Application (Cambridge University Press, Cambridge, 2000).
  • [7] H.P. Furth, J. Killeen and M.N. Rosenbluth, Phys. Fluids 6, 459 (1963).
  • [8] B. Coppi, G. Laval and R. Pellat, Phys. Rev. Lett. 16, 1207 (1966).
  • [9] J.F. Drake and Y.C. Lee, Phys. Fluids 20, 1341 (1977).
  • [10] I. Katanuma and T. Kamimura, Phys. Fluids 23, 2500 (1980).
  • [11] W. Zwingmann, J. Wallance, K. Schindler and J. Birn, J. Geophys. Res. 95, 20877 (1990).
  • [12] P.L. Pritchett, F.V. Coroniti, R. Pellat and H. Karimabadi, J. Geophys. Res. 96, 11523 (1991).
  • [13] X. Wang and A. Bhattacharjee, J. Geophys. Res. 98, 19419 (1993).
  • [14] M. Scholer, J. Geophys. Res. 94, 8805 (1989).
  • [15] T.G. Forbes and E.R. Priest, Rev. Geophys. 25, 1583 (1987).
  • [16] J.D. Huba and L.I. Rudakov, Phys. Rev. Lett. 93, 175003 (2004), hall MHD simulation in open system.
  • [17] J.D. Huba, Phys. Plasmas 12, 012322 (2005).
  • [18] R. Horiuchi, K. Nishimura, T.H. Watanabe and T. Sato, Nucl. Fusion 39, 2083 (1999).
  • [19] M. Hesse, K. Schindler, J. Birn and M. Kuznetsova, Phys. Plasmas 6, 1781 (1999).
  • [20] M. Hesse, J. Birn and M. Kuznetsova, J. Geophys. Res. 106, 3721 (2001).
  • [21] P. Ricci, J.U. Brackbill, W. Daughton and G. Lapenta, Phys. Plasmas 11, 4102 (2004).
  • [22] M.A. Shay, J.F. Drake and M. Swisdak, Phys. Rev. Lett. 99, 155002 (2007).
  • [23] K. Fujimoto and S. Machida, J. Comp. Phys. 214, 550 (2006).
  • [24] K. Fujimoto, Phys. Plasmas 13, 072904 (2006).
  • [25] R. Horiuchi, W. Pei and T. Sato, Earth, Planets and Space 53, 439 (2001).
  • [26] W. Pei, R. Horiuchi and T. Sato, Phys. Plasmas 8, 3251 (2001).
  • [27] W. Pei, R. Horiuchi and T. Sato, Phys. Rev. Lett. 87, 235003 (2001).
  • [28] R. Horiuchi, H. Ohtani and A. Ishizawa, Comp. Phys. Comm. 164, 17 (2004).
  • [29] A. Ishizawa, R. Horiuchi and H. Ohtani, Phys. Plasmas 11, 3579 (2004).
  • [30] A. Ishizawa and R. Horiuchi, Phys. Rev. Lett. 95, 045003 (2005).
  • [31] R. Horiuchi, H. Ohtani and A. Ishizawa, J. Plsama Phys. 72, 953 (2006).
  • [32] H. Ohtani, R. Horiuchi and A. Ishizawa, J. Plasma Phys. 72, 929 (2006).
  • [33] A. Ishizawa and R. Horiuchi, J. Plasma Phys. 72, 787 (2006).
  • [34] D. Ding, L. Lee and D. Swift, J. Geophys. Res. 97, 8453 (1992).
  • [35] D. Krauss-Varban and N. Omidi, Geophys. Res. Lett 22, 3271 (1995).
  • [36] P.L. Pritchett, J. Geophys. Res. 106, 3783 (2001).
  • [37] W. Daughton, J. Scudder and H. Karimabadi, Phys. Plasmas 13, 072101 (2006).
  • [38] A. Klimas, M. Hesse and S. Zenitani, Phys. Plasmas 15, 082102 (2008).
  • [39] H. Ohtani et al., Lecture Notes in Computer Science 4759, 329 (2008).
  • [40] C.K. Birdsall and A.B. Langdon, Plasma Physics Via Computer Simulation (McGraw-Hill, New York, 1985).
  • [41] E.G. Harris, Nuovo Cimento 23, 115 (1962).
  • [42] I. Shinohara, H. Suzuki, M. Fujimoto and M. Hoshino, Phys. Rev. Lett. 87, 095001 (2001).
  • [43] W. Daughton, Phys. Plasmas 6, 1329 (1999).
  • [44] B.D. Martino, S. Briguglio, G. Vladb and P. Sguazzeroc, Parallel Computing 27, 295 (2001).
  • [45] P.L. Pritchett, J. Geophys. Res. 110, A10213 (2005).

This paper may be cited as follows:

Hiroaki OHTANI and Ritoku HORIUCHI, Plasma Fusion Res. 4, 024 (2009).