Plasmoid Chain Dynamics in Three-Dimensional Kinetic Simulations

POSTER

Abstract

We study the dynamics of a plasmoid chain with three dimensional Particle-in-Cell simulations. The evolution of the system with and without a uniform guide field, whose strength is 1/3 the asymptotic magnetic field, is investigated. The plasmoid chain forms by spontaneous magnetic reconnection: the tearing instability rapidly disrupts the initial current sheet generating several small-scale plasmoids, that rapidly grow in size coalescing and kinking. The plasmoid kink is mainly driven by the coalescence process. The presence of guide field strongly influences the evolution of the plasmoid chain. Without a guide field, a main reconnection site dominates and smaller reconnection regions are included in larger ones, leading to an hierarchical structure of the plasmoid-dominated current sheet. On the contrary in presence of a guide field, plasmoids have approximately the same size and the hierarchical structure does not emerge, a strong core magnetic field develops in the center of the plasmoid in the direction of the existing guide field, and bump-on-tail instability, leading to the formation of electron holes, is detected in proximity of the plasmoids.

*The present work is supported by NASA MMS Grant NNX08AO84G. Additional support rom the European Commission's Seventh Framework Programme under the grant agreement no. 287703 (CRESTA, cresta-project.eu).

Authors

  • Stefano Markidis

    • KTH Royal Institute of Technology
    • HPCViz Department, KTH Royal Institute of Technology, Stockholm, Sweden
  • P. Henri

    • Universit\'e de Nice Sophia Antipolis, CNRS, Observatoire de la C\^ote d'Azur
  • G. Lapenta

    • Katholieke Universiteit Leuven
  • A. Divin

    • Swedish Institute of Space Physics, Uppsala
  • M. Goldman

    • University of Colorado
  • D. Newman

    • University of Colorado
  • E. Laure

    • KTH Royal Institute of Technology