EVIDENCE OF MAGNETIC FIELD SWITCH-OFF IN COLLISIONLESS MAGNETIC RECONNECTION

The long-term evolution of large domain particle-in-cell simulations of collisionless magnetic reconnection is investigated following observations that show two possible outcomes for collisionless reconnection: toward a Petschek-like configuration or toward multiple X points. In the present simulation, a mixed scenario develops. At earlier time, plasmoids are emitted, disrupting the formation of Petschek-like structures. Later, an almost stationary monster plasmoid forms, preventing the emission of other plasmoids. A situation reminiscent of Petschek’s switch-off then ensues. Switch-off is obtained through a slow shock/rotational discontinuity compound structure. Two external slow shocks (SS) located at the separatrices reduce the in-plane tangential component of the magnetic field, but not to zero. Two transitions reminiscent of rotational discontinuities (RD) in the internal part of the exhaust then perform the final switch-off. Both the SS and the RD are characterized through analysis of their Rankine–Hugoniot jump conditions. A moderate guide field is used to suppress the development of the firehose instability in the exhaust.

[1]  Stefano Markidis,et al.  Introduction of temporal sub-stepping in the Multi-Level Multi-Domain semi-implicit Particle-In-Cell code Parsek2D-MLMD , 2015, Comput. Phys. Commun..

[2]  James F. Drake,et al.  Fast reconnection in high temperature plasmas , 1995 .

[3]  V. Angelopoulos,et al.  On the signatures of magnetic islands and multiple X-lines in the solar wind as observed by ARTEMIS and WIND , 2014 .

[4]  William Daughton,et al.  Fully kinetic simulations of undriven magnetic reconnection with open boundary conditions , 2006 .

[5]  M. Shay,et al.  Formation of Electron Holes and Particle Energization During Magnetic Reconnection , 2003, Science.

[6]  G. Lapenta,et al.  Bipolar electric field signatures of reconnection separatrices for a hydrogen plasma at realistic guide fields , 2011, 1108.2492.

[7]  Takaya Hayashi,et al.  Externally driven magnetic reconnection and a powerful magnetic energy converter , 1979 .

[8]  J. Drake,et al.  The structure of the magnetic reconnection exhaust boundary , 2011, 1111.7039.

[9]  E. G. Harris On a plasma sheath separating regions of oppositely directed magnetic field , 1962 .

[10]  Michael Hesse,et al.  Geospace Environmental Modeling (GEM) magnetic reconnection challenge , 2001 .

[11]  K. Arzner,et al.  Kinetic structure of the post plasmoid plasma sheet during magnetotail reconnection , 2001 .

[12]  S. Markidis,et al.  Kinetic simulations of plasmoid chain dynamics , 2013, 1306.1050.

[13]  Stefano Markidis,et al.  Multi-level multi-domain algorithm implementation for two-dimensional multiscale particle in cell simulations , 2014, J. Comput. Phys..

[14]  J. Gosling Observations of Magnetic Reconnection in the Turbulent High-Speed Solar Wind , 2007 .

[15]  A. Schekochihin,et al.  Fast magnetic reconnection in the plasmoid-dominated regime. , 2010, Physical review letters.

[16]  H. Karimabadi,et al.  Current sheets and pressure anisotropy in the reconnection exhaust , 2014 .

[17]  M. Fujimoto,et al.  Ion dynamics and resultant velocity space distributions in the course of magnetotail reconnection , 1998 .

[18]  C. Farrugia,et al.  Plasmoids in reconnecting current sheets: Solar and terrestrial contexts compared , 2008, 0809.3755.

[19]  M. Scholer,et al.  Ion kinetic effects in magnetic reconnection: Hybrid simulations , 1998 .

[20]  B. Rogers,et al.  Formation of secondary islands during magnetic reconnection , 2006 .

[21]  Masahiro Hoshino,et al.  The relation between ion temperature anisotropy and formation of slow shocks in collisionless magnetic reconnection , 2012, 1201.4213.

[22]  A. A. Schekochihin,et al.  Instability of current sheets and formation of plasmoid chains , 2007 .

[23]  H. Karimabadi,et al.  Regimes of the electron diffusion region in magnetic reconnection. , 2013, Physical review letters.

[24]  P. Daly,et al.  Analysis methods for multi-spacecraft data , 1998 .

[25]  H. Ji,et al.  Phase Diagram for Magnetic Reconnection in Heliophysical, Astrophysical and Laboratory Plasmas , 2011, 1109.0756.

[26]  Stefano Markidis,et al.  Multi-scale simulations of plasma with iPIC3D , 2010, Math. Comput. Simul..

[27]  Stefano Markidis,et al.  A Multi Level Multi Domain Method for Particle In Cell plasma simulations , 2012, J. Comput. Phys..

[28]  Christopher T. Russell,et al.  Generalized Walén tests through Alfvén waves and rotational discontinuities using electron flow velocities , 1999 .

[29]  S. Markidis,et al.  Numerical simulations of separatrix instabilities in collisionless magnetic reconnection , 2012 .

[30]  A. Vaivads,et al.  Cluster multispacecraft observations at the high-latitude duskside magnetopause: implications for continuous and component magnetic reconnection , 2005 .

[31]  R. Samtaney,et al.  Magnetic reconnection and stochastic plasmoid chains in high-Lundquist-number plasmas , 2011, 1108.4040.

[32]  V. Vasyliūnas Theoretical models of magnetic field line merging , 1975 .

[33]  Y. Lin,et al.  A two-dimensional hybrid simulation of the magnetotail reconnection layer , 1996 .

[34]  N. Omidi,et al.  Magnetic structure of the reconnection layer and core field generation in plasmoids , 1999 .

[35]  E. W. Hones,et al.  Structure of the magnetotail at 220 RE and its response to geomagnetic activity , 1984 .

[36]  S. Markidis,et al.  Separatrices: The crux of reconnection , 2014, Journal of Plasma Physics.

[37]  Stefaan Poedts,et al.  Principles of Magnetohydrodynamics: With Applications to Laboratory and Astrophysical Plasmas , 2004 .

[38]  G. Lapenta,et al.  Resistive magnetohydrodynamic reconnection: Resolving long-term, chaotic dynamics , 2013 .

[39]  M. Shay,et al.  Electron acceleration from contracting magnetic islands during reconnection , 2006, Nature.

[40]  Paolo Ricci,et al.  Collisionless magnetic reconnection in the presence of a guide field , 2004 .